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bulge.","sources":["nasa"]},{"id":"galaxy:messier-105","type":"galaxy","name":"Messier 105","domain":"science","description":"An elliptical galaxy in Leo and a member of the Leo I group.","sources":["nasa"]},{"id":"galaxy:messier-106","type":"galaxy","name":"Messier 106","domain":"science","description":"A spiral galaxy in Canes Venatici with an active galactic nucleus.","sources":["nasa"]},{"id":"star_cluster:messier-107","type":"star_cluster","name":"Messier 107","domain":"science","description":"A globular cluster in the constellation Ophiuchus.","sources":["nasa"]},{"id":"galaxy:messier-108","type":"galaxy","name":"Messier 108","domain":"science","description":"An edge-on barred spiral galaxy in the constellation Ursa Major.","sources":["nasa"]},{"id":"galaxy:messier-109","type":"galaxy","name":"Messier 109","domain":"science","description":"A barred spiral galaxy in the constellation Ursa Major.","sources":["nasa"]},{"id":"galaxy:messier-110","type":"galaxy","name":"Messier 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crater.","sources":["nasa","jpl"]},{"id":"moon:mimas","type":"moon","name":"Mimas","domain":"science","description":"Mimas is an inner moon of Saturn dominated by the huge impact crater Herschel.","sources":["nasa","jpl"]},{"id":"moon:titania","type":"moon","name":"Titania","domain":"science","description":"Titania is the largest moon of Uranus.","sources":["nasa","jpl"]},{"id":"moon:oberon","type":"moon","name":"Oberon","domain":"science","description":"Oberon is the outermost of the large moons of Uranus and is heavily cratered.","sources":["nasa","jpl"]},{"id":"moon:miranda","type":"moon","name":"Miranda","domain":"science","description":"Miranda is the smallest of the five major moons of Uranus and has an unusually jumbled, varied surface.","sources":["nasa","jpl"]},{"id":"moon:ariel","type":"moon","name":"Ariel","domain":"science","description":"Ariel is a moon of Uranus and the brightest of its major satellites.","sources":["nasa","jpl"]},{"id":"moon:umbriel","type":"moon","name":"Umbriel","domain":"science","description":"Umbriel is a moon of Uranus and the darkest of its major satellites.","sources":["nasa","jpl"]},{"id":"moon:nereid","type":"moon","name":"Nereid","domain":"science","description":"Nereid is a moon of Neptune with one of the most eccentric orbits of any known moon in the Solar System.","sources":["nasa","jpl"]},{"id":"moon:proteus","type":"moon","name":"Proteus","domain":"science","description":"Proteus is one of the larger inner moons of Neptune and one of the darkest objects in the Solar System.","sources":["nasa","jpl"]},{"id":"moon:amalthea","type":"moon","name":"Amalthea","domain":"science","description":"Amalthea is a small, reddish inner moon of Jupiter orbiting closer to the planet than the Galilean moons.","sources":["nasa","jpl"]},{"id":"moon:charon","type":"moon","name":"Charon","domain":"science","description":"Charon is the largest moon of the dwarf 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heavens.","sources":["iau"]},{"id":"astronomer:ptolemy","entryPath":"/history/ptolemy","type":"astronomer","name":"Ptolemy","domain":"science","description":"A Greco-Roman astronomer whose Almagest codified the geocentric model that dominated astronomy for over a millennium.","sources":["iau"]},{"id":"astronomer:hipparchus","entryPath":"/history/hipparchus","type":"astronomer","name":"Hipparchus","domain":"science","description":"An ancient Greek astronomer credited with compiling an early star catalogue and discovering the precession of the equinoxes.","sources":["iau"]},{"id":"astronomer:caroline-herschel","entryPath":"/history/caroline-herschel","type":"astronomer","name":"Caroline Herschel","domain":"science","description":"A German-British astronomer who discovered several comets and was among the first women paid for scientific work.","sources":["iau"]},{"id":"astronomer:henrietta-leavitt","entryPath":"/history/henrietta-leavitt","type":"astronomer","name":"Henrietta Swan 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public.","sources":["nasa"]},{"id":"astronomer:nancy-grace-roman","entryPath":"/history/nancy-grace-roman","type":"astronomer","name":"Nancy Grace Roman","domain":"science","description":"An American astronomer and NASA's first chief of astronomy, often called the 'Mother of Hubble' for her role in space-based astronomy.","sources":["nasa"]},{"id":"catalog:ngc","type":"catalog","name":"New General Catalogue (NGC)","domain":"science","description":"A catalogue of nearly 8,000 deep-sky objects.","sources":["iau"]},{"id":"nebula:ngc-7000","type":"nebula","name":"North America Nebula (NGC 7000)","domain":"science","description":"A large emission nebula in Cygnus whose shape resembles the continent of North America.","sources":["nasa","esa"]},{"id":"nebula:ngc-2024","type":"nebula","name":"Flame Nebula (NGC 2024)","domain":"science","description":"An emission nebula and star-forming region in Orion, near the star Alnitak.","sources":["nasa","esa"]},{"id":"nebula:ngc-6960","type":"nebula","name":"Western Veil Nebula (NGC 6960)","domain":"science","description":"Part of the Veil Nebula, a supernova remnant in Cygnus also known as the Witch's Broom Nebula.","sources":["nasa","esa"]},{"id":"nebula:ngc-6302","type":"nebula","name":"Butterfly Nebula (NGC 6302)","domain":"science","description":"A bipolar planetary nebula in Scorpius with one of the hottest known central stars.","sources":["nasa","esa"]},{"id":"nebula:ngc-6543","type":"nebula","name":"Cat's Eye Nebula (NGC 6543)","domain":"science","description":"A complex planetary nebula in the constellation Draco, one of the first to be studied with a spectroscope.","sources":["nasa","esa"]},{"id":"nebula:ngc-2237","type":"nebula","name":"Rosette Nebula (NGC 2237)","domain":"science","description":"A large emission nebula in the constellation Monoceros surrounding a young open star cluster.","sources":["nasa","esa"]},{"id":"galaxy:ngc-4486","type":"galaxy","name":"Messier 87 (NGC 4486)","domain":"science","description":"A giant elliptical galaxy in Virgo whose supermassive black hole was the first to be directly imaged.","sources":["nasa","esa"]},{"id":"galaxy:ngc-253","type":"galaxy","name":"Sculptor Galaxy (NGC 253)","domain":"science","description":"A bright barred spiral starburst galaxy in the constellation Sculptor.","sources":["nasa","esa"]},{"id":"galaxy:ngc-4565","type":"galaxy","name":"Needle Galaxy (NGC 4565)","domain":"science","description":"An edge-on spiral galaxy in Coma Berenices noted for its slender, needle-like profile.","sources":["nasa","esa"]},{"id":"galaxy:ngc-5128","type":"galaxy","name":"Centaurus A (NGC 5128)","domain":"science","description":"A prominent radio galaxy in Centaurus, one of the closest active galaxies to Earth.","sources":["nasa","esa"]},{"id":"galaxy:ngc-1300","type":"galaxy","name":"NGC 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Canopus.","sources":["iau"]},{"id":"constellation:eridanus","entryPath":"/constellations/eridanus","type":"constellation","name":"Eridanus","domain":"science","description":"Eridanus is a long southern constellation representing a celestial river, terminating at the bright star Achernar.","sources":["iau"]},{"id":"constellation:centaurus","entryPath":"/constellations/centaurus","type":"constellation","name":"Centaurus","domain":"science","description":"Centaurus is a bright southern constellation depicting a centaur and containing several of the sky's most luminous stars.","sources":["iau"]},{"id":"constellation:crux","entryPath":"/constellations/crux","type":"constellation","name":"Crux","domain":"science","description":"Crux, the Southern Cross, is the smallest of the 88 modern constellations and a prominent southern-sky asterism.","sources":["iau"]},{"id":"constellation:ursa-major","entryPath":"/constellations/ursa-major","type":"constellation","name":"Ursa 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star.","sources":["iau"]},{"id":"star:canopus","type":"star","name":"Canopus","domain":"science","description":"Canopus is a white supergiant and the second-brightest star in the night sky, the luminary of the constellation Carina.","sources":["iau","nasa"]},{"id":"star:achernar","type":"star","name":"Achernar","domain":"science","description":"Achernar is a hot blue main-sequence star and the brightest star in the constellation Eridanus.","sources":["iau","nasa"]},{"id":"star:hadar","type":"star","name":"Hadar","domain":"science","description":"Hadar (Beta Centauri) is a blue giant multiple star system and the second-brightest star in the constellation Centaurus.","sources":["iau","nasa"]},{"id":"star:acrux","type":"star","name":"Acrux","domain":"science","description":"Acrux (Alpha Crucis) is the brightest star in the constellation Crux and the southernmost first-magnitude star.","sources":["iau","nasa"]},{"id":"star:gacrux","type":"star","name":"Gacrux","domain":"science","description":"Gacrux (Gamma Crucis) is a red giant marking the top of the Southern Cross in the constellation Crux.","sources":["iau","nasa"]},{"id":"star:bellatrix","type":"star","name":"Bellatrix","domain":"science","description":"Bellatrix is a blue giant marking the left shoulder of the hunter in the constellation Orion.","sources":["iau","nasa"]},{"id":"star:mintaka","type":"star","name":"Mintaka","domain":"science","description":"Mintaka is a multiple star system forming the westernmost star of Orion's Belt in the constellation Orion.","sources":["iau","nasa"]},{"id":"star:alnilam","type":"star","name":"Alnilam","domain":"science","description":"Alnilam is a blue supergiant forming the central star of Orion's Belt in the constellation Orion.","sources":["iau","nasa"]},{"id":"star:alnitak","type":"star","name":"Alnitak","domain":"science","description":"Alnitak is a hot blue 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the brightest star in the constellation Perseus.","sources":["iau","nasa"]},{"id":"star:rasalhague","type":"star","name":"Rasalhague","domain":"science","description":"Rasalhague is a white binary star and the brightest star in the constellation Ophiuchus.","sources":["iau","nasa"]},{"id":"star:vindemiatrix","type":"star","name":"Vindemiatrix","domain":"science","description":"Vindemiatrix is a yellow giant and one of the brighter stars in the constellation Virgo.","sources":["iau","nasa"]},{"id":"star:sadr","type":"star","name":"Sadr","domain":"science","description":"Sadr is a yellow-white supergiant marking the heart of the swan in the constellation Cygnus.","sources":["iau","nasa"]},{"id":"star:albireo","type":"star","name":"Albireo","domain":"science","description":"Albireo is a celebrated colorful double star marking the head of the swan in the constellation Cygnus.","sources":["iau","nasa"]},{"id":"star:deneb-algedi","type":"star","name":"Deneb 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constellations.","sources":["iau"]},{"id":"constellation:libra","entryPath":"/constellations/libra","type":"constellation","name":"Libra","domain":"science","description":"A southern zodiacal constellation, one of the 88 modern constellations.","sources":["iau"]},{"id":"constellation:cetus-constellation","entryPath":"/constellations/cetus-constellation","type":"constellation","name":"Cetus","domain":"science","description":"A large constellation in the southern sky, one of the 88 modern constellations, often called the Whale or Sea Monster.","sources":["iau"]},{"id":"star:trappist-1","type":"star","name":"TRAPPIST-1","domain":"science","description":"An ultra-cool red dwarf star about 40 light-years away that hosts seven known terrestrial planets.","sources":["nasa","esa"]},{"id":"star:kepler-22","type":"star","name":"Kepler-22","domain":"science","description":"A Sun-like star in Cygnus hosting Kepler-22b, the first habitable-zone planet found by the Kepler mission.","sources":["nasa"]},{"id":"star:kepler-186","type":"star","name":"Kepler-186","domain":"science","description":"A red dwarf star in Cygnus hosting Kepler-186f, the first Earth-size planet found in a habitable zone.","sources":["nasa"]},{"id":"star:hd-209458","type":"star","name":"HD 209458","domain":"science","description":"A Sun-like star in Pegasus whose planet HD 209458 b was the first exoplanet observed transiting its star.","sources":["nasa","esa"]},{"id":"star:gliese-581","type":"star","name":"Gliese 581","domain":"science","description":"A red dwarf star in Libra hosting a system of confirmed super-Earth and Neptune-mass planets.","sources":["nasa","esa"]},{"id":"star:tabby-s-star","type":"star","name":"Tabby's Star (KIC 8462852)","domain":"science","description":"An F-type main-sequence star in Cygnus noted for unusual, irregular dimming events detected by Kepler.","sources":["nasa"]},{"id":"exoplanet:proxima-centauri-b","type":"exoplanet","name":"Proxima Centauri 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Earth.","sources":["nasa","esa"]},{"id":"exoplanet:trappist-1-f","type":"exoplanet","name":"TRAPPIST-1 f","domain":"science","description":"A habitable-zone terrestrial planet orbiting TRAPPIST-1.","sources":["nasa","esa"]},{"id":"exoplanet:trappist-1-g","type":"exoplanet","name":"TRAPPIST-1 g","domain":"science","description":"The sixth of the seven known terrestrial planets orbiting TRAPPIST-1.","sources":["nasa","esa"]},{"id":"exoplanet:trappist-1-h","type":"exoplanet","name":"TRAPPIST-1 h","domain":"science","description":"The outermost of the seven known terrestrial planets orbiting TRAPPIST-1.","sources":["nasa","esa"]},{"id":"exoplanet:51-pegasi-b","type":"exoplanet","name":"51 Pegasi b","domain":"science","description":"A hot Jupiter and the first exoplanet discovered orbiting a Sun-like star, announced in 1995.","sources":["nasa","esa"]},{"id":"exoplanet:kepler-22b","type":"exoplanet","name":"Kepler-22b","domain":"science","description":"A super-Earth-to-Neptune-size planet in the habitable zone of the Sun-like star Kepler-22.","sources":["nasa"]},{"id":"exoplanet:kepler-186f","type":"exoplanet","name":"Kepler-186f","domain":"science","description":"The first validated Earth-size planet found orbiting in the habitable zone of another star.","sources":["nasa"]},{"id":"exoplanet:hd-209458-b","type":"exoplanet","name":"HD 209458 b","domain":"science","description":"A hot Jupiter and the first exoplanet observed transiting its host star and to have its atmosphere detected.","sources":["nasa","esa"]},{"id":"exoplanet:55-cancri-e","type":"exoplanet","name":"55 Cancri e","domain":"science","description":"A super-Earth orbiting very close to 55 Cancri, with a likely scorching, possibly molten surface.","sources":["nasa","esa"]},{"id":"exoplanet:gliese-581c","type":"exoplanet","name":"Gliese 581 c","domain":"science","description":"A confirmed super-Earth orbiting the red dwarf Gliese 581, one of the earliest low-mass planets found near a habitable zone.","sources":["esa","nasa"]},{"id":"asteroid:vesta","type":"asteroid","name":"4 Vesta","domain":"science","description":"One of the largest objects in the asteroid belt, visited by NASA's Dawn.","sources":["nasa","jpl"]},{"id":"asteroid:pallas","type":"asteroid","name":"2 Pallas","domain":"science","description":"One of the most massive asteroids in the main belt.","sources":["jpl"]},{"id":"asteroid:hygiea","type":"asteroid","name":"10 Hygiea","domain":"science","description":"A large, dark asteroid in the outer main belt.","sources":["jpl"]},{"id":"asteroid:bennu","type":"asteroid","name":"101955 Bennu","domain":"science","description":"A near-Earth asteroid sampled by NASA's OSIRIS-REx.","sources":["nasa","jpl"]},{"id":"asteroid:ryugu","type":"asteroid","name":"162173 Ryugu","domain":"science","description":"A near-Earth asteroid sampled by Japan's Hayabusa2.","sources":["jpl"]},{"id":"asteroid:eros","type":"asteroid","name":"433 Eros","domain":"science","description":"A near-Earth asteroid orbited by NASA's NEAR Shoemaker.","sources":["nasa","jpl"]},{"id":"asteroid:itokawa","type":"asteroid","name":"25143 Itokawa","domain":"science","description":"A near-Earth asteroid sampled by Japan's Hayabusa.","sources":["jpl"]},{"id":"asteroid:psyche","type":"asteroid","name":"16 Psyche","domain":"science","description":"A metal-rich main-belt asteroid and NASA mission target.","sources":["nasa","jpl"]},{"id":"asteroid:apophis","type":"asteroid","name":"99942 Apophis","domain":"science","description":"A near-Earth asteroid studied for its close approaches to Earth.","sources":["jpl"]},{"id":"comet:hale-bopp","type":"comet","name":"Comet Hale–Bopp","domain":"science","description":"A long-period comet that was widely visible to the naked eye in 1997.","sources":["nasa"]},{"id":"comet:hyakutake","type":"comet","name":"Comet Hyakutake","domain":"science","description":"A comet that passed very close to Earth in 1996.","sources":["nasa"]},{"id":"comet:churyumov-gerasimenko","type":"comet","name":"67P/Churyumov–Gerasimenko","domain":"science","description":"A periodic comet orbited and landed on by ESA's Rosetta mission.","sources":["esa"]},{"id":"comet:shoemaker-levy-9","type":"comet","name":"Comet Shoemaker–Levy 9","domain":"science","description":"A comet that broke apart and collided with Jupiter in 1994.","sources":["nasa"]},{"id":"constellation:antlia","type":"constellation","name":"Antlia","domain":"science","entryPath":"/constellations/antlia","description":"The constellation Antlia (Antliae) — 10 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:apus","type":"constellation","name":"Apus","domain":"science","entryPath":"/constellations/apus","description":"The constellation Apus (Apodis) — 13 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:ara","type":"constellation","name":"Ara","domain":"science","entryPath":"/constellations/ara","description":"The constellation Ara (Arae) — 18 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:caelum","type":"constellation","name":"Caelum","domain":"science","entryPath":"/constellations/caelum","description":"The constellation Caelum (Caeli) — 4 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:camelopardalis","type":"constellation","name":"Camelopardalis","domain":"science","entryPath":"/constellations/camelopardalis","description":"The constellation Camelopardalis (Camelopardalis) — 45 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:canes-venatici","type":"constellation","name":"Canes Venatici","domain":"science","entryPath":"/constellations/canes-venatici","description":"The constellation Canes Venatici (Canum Venaticorum) — 16 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:cepheus","type":"constellation","name":"Cepheus","domain":"science","entryPath":"/constellations/cepheus","description":"The constellation Cepheus (Cephei) — 48 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:chamaeleon","type":"constellation","name":"Chamaeleon","domain":"science","entryPath":"/constellations/chamaeleon","description":"The constellation Chamaeleon (Chamaeleontis) — 13 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:circinus","type":"constellation","name":"Circinus","domain":"science","entryPath":"/constellations/circinus","description":"The constellation Circinus (Circini) — 10 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:columba","type":"constellation","name":"Columba","domain":"science","entryPath":"/constellations/columba","description":"The constellation Columba (Columbae) — 19 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:coma-berenices","type":"constellation","name":"Coma Berenices","domain":"science","entryPath":"/constellations/coma-berenices","description":"The constellation Coma Berenices (Comae Berenices) — 24 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:corona-australis","type":"constellation","name":"Corona Australis","domain":"science","entryPath":"/constellations/corona-australis","description":"The constellation Corona Australis (Coronae Australis) — 21 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:corona-borealis","type":"constellation","name":"Corona Borealis","domain":"science","entryPath":"/constellations/corona-borealis","description":"The constellation Corona Borealis (Coronae Borealis) — 19 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:corvus","type":"constellation","name":"Corvus","domain":"science","entryPath":"/constellations/corvus","description":"The constellation Corvus (Corvi) — 11 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:crater","type":"constellation","name":"Crater","domain":"science","entryPath":"/constellations/crater","description":"The constellation Crater (Crateris) — 11 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:delphinus","type":"constellation","name":"Delphinus","domain":"science","entryPath":"/constellations/delphinus","description":"The constellation Delphinus (Delphini) — 12 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:dorado","type":"constellation","name":"Dorado","domain":"science","entryPath":"/constellations/dorado","description":"The constellation Dorado (Doradus) — 15 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:draco","type":"constellation","name":"Draco","domain":"science","entryPath":"/constellations/draco","description":"The constellation Draco (Draconis) — 79 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:equuleus","type":"constellation","name":"Equuleus","domain":"science","entryPath":"/constellations/equuleus","description":"The constellation Equuleus (Equulei) — 6 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:fornax","type":"constellation","name":"Fornax","domain":"science","entryPath":"/constellations/fornax","description":"The constellation Fornax (Fornacis) — 12 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:grus","type":"constellation","name":"Grus","domain":"science","entryPath":"/constellations/grus","description":"The constellation Grus (Gruis) — 22 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:hercules","type":"constellation","name":"Hercules","domain":"science","entryPath":"/constellations/hercules","description":"The constellation Hercules (Herculis) — 77 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:horologium","type":"constellation","name":"Horologium","domain":"science","entryPath":"/constellations/horologium","description":"The constellation Horologium (Horologii) — 10 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:hydra","type":"constellation","name":"Hydra","domain":"science","entryPath":"/constellations/hydra","description":"The constellation Hydra (Hydrae) — 71 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:hydrus","type":"constellation","name":"Hydrus","domain":"science","entryPath":"/constellations/hydrus","description":"The constellation Hydrus (Hydri) — 10 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:indus","type":"constellation","name":"Indus","domain":"science","entryPath":"/constellations/indus","description":"The constellation Indus (Indi) — 10 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:lacerta","type":"constellation","name":"Lacerta","domain":"science","entryPath":"/constellations/lacerta","description":"The constellation Lacerta (Lacertae) — 21 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:leo-minor","type":"constellation","name":"Leo Minor","domain":"science","entryPath":"/constellations/leo-minor","description":"The constellation Leo Minor (Leonis Minoris) — 14 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:lepus","type":"constellation","name":"Lepus","domain":"science","entryPath":"/constellations/lepus","description":"The constellation Lepus (Leporis) — 26 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:lupus","type":"constellation","name":"Lupus","domain":"science","entryPath":"/constellations/lupus","description":"The constellation Lupus (Lupi) — 48 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:lynx","type":"constellation","name":"Lynx","domain":"science","entryPath":"/constellations/lynx","description":"The constellation Lynx (Lyncis) — 29 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:mensa","type":"constellation","name":"Mensa","domain":"science","entryPath":"/constellations/mensa","description":"The constellation Mensa (Mensae) — 7 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:microscopium","type":"constellation","name":"Microscopium","domain":"science","entryPath":"/constellations/microscopium","description":"The constellation Microscopium (Microscopii) — 15 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:monoceros","type":"constellation","name":"Monoceros","domain":"science","entryPath":"/constellations/monoceros","description":"The constellation Monoceros (Monocerotis) — 37 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:musca","type":"constellation","name":"Musca","domain":"science","entryPath":"/constellations/musca","description":"The constellation Musca (Muscae) — 18 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:norma","type":"constellation","name":"Norma","domain":"science","entryPath":"/constellations/norma","description":"The constellation Norma (Normae) — 14 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:octans","type":"constellation","name":"Octans","domain":"science","entryPath":"/constellations/octans","description":"The constellation Octans (Octantis) — 17 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:pavo","type":"constellation","name":"Pavo","domain":"science","entryPath":"/constellations/pavo","description":"The constellation Pavo (Pavonis) — 28 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:phoenix","type":"constellation","name":"Phoenix","domain":"science","entryPath":"/constellations/phoenix","description":"The constellation Phoenix (Phoenicis) — 26 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:pictor","type":"constellation","name":"Pictor","domain":"science","entryPath":"/constellations/pictor","description":"The constellation Pictor (Pictoris) — 15 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:pisces","type":"constellation","name":"Pisces","domain":"science","entryPath":"/constellations/pisces","description":"The constellation Pisces (Piscium) — 50 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:puppis","type":"constellation","name":"Puppis","domain":"science","entryPath":"/constellations/puppis","description":"The constellation Puppis (Puppis) — 89 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:pyxis","type":"constellation","name":"Pyxis","domain":"science","entryPath":"/constellations/pyxis","description":"The constellation Pyxis (Pyxidis) — 12 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:reticulum","type":"constellation","name":"Reticulum","domain":"science","entryPath":"/constellations/reticulum","description":"The constellation Reticulum (Reticuli) — 11 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:sagitta","type":"constellation","name":"Sagitta","domain":"science","entryPath":"/constellations/sagitta","description":"The constellation Sagitta (Sagittae) — 8 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:sagittarius","type":"constellation","name":"Sagittarius","domain":"science","entryPath":"/constellations/sagittarius","description":"The constellation Sagittarius (Sagittarii) — 69 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:sculptor","type":"constellation","name":"Sculptor","domain":"science","entryPath":"/constellations/sculptor","description":"The constellation Sculptor (Sculptoris) — 17 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:scutum","type":"constellation","name":"Scutum","domain":"science","entryPath":"/constellations/scutum","description":"The constellation Scutum (Scuti) — 11 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:serpens","type":"constellation","name":"Serpens","domain":"science","entryPath":"/constellations/serpens","description":"The constellation Serpens (Serpentis) — 37 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:sextans","type":"constellation","name":"Sextans","domain":"science","entryPath":"/constellations/sextans","description":"The constellation Sextans (Sextantis) — 6 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:telescopium","type":"constellation","name":"Telescopium","domain":"science","entryPath":"/constellations/telescopium","description":"The constellation Telescopium (Telescopii) — 15 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:triangulum","type":"constellation","name":"Triangulum","domain":"science","entryPath":"/constellations/triangulum","description":"The constellation Triangulum (Trianguli) — 11 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:triangulum-australe","type":"constellation","name":"Triangulum Australe","domain":"science","entryPath":"/constellations/triangulum-australe","description":"The constellation Triangulum Australe (Trianguli Australis) — 11 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:tucana","type":"constellation","name":"Tucana","domain":"science","entryPath":"/constellations/tucana","description":"The constellation Tucana (Tucanae) — 19 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:vela","type":"constellation","name":"Vela","domain":"science","entryPath":"/constellations/vela","description":"The constellation Vela (Velorum) — 75 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:volans","type":"constellation","name":"Volans","domain":"science","entryPath":"/constellations/volans","description":"The constellation Volans (Volantis) — 14 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"constellation:vulpecula","type":"constellation","name":"Vulpecula","domain":"science","entryPath":"/constellations/vulpecula","description":"The constellation Vulpecula (Vulpeculae) — 25 catalogued stars in this encyclopedia.","sources":["iau"]},{"id":"star:rigil-kentaurus","type":"star","name":"Rigil Kentaurus","domain":"science","entryPath":"/stars/rigil-kentaurus","description":"Yellow dwarf in Centaurus, about 4.3 light-years from Earth.","aliases":["HR 5459","HD 128620","HIP 71683","Gl 559A"],"sources":["hyg","hipparcos"],"catalogNumbers":["HR 5459","HD 128620","HIP 71683","Gl 559A"]},{"id":"star:mimosa","type":"star","name":"Mimosa","domain":"science","entryPath":"/stars/mimosa","description":"Blue giant in Crux, about 279 light-years from Earth.","aliases":["Beta Crucis","Beta Cru","HR 4853","HD 111123","HIP 62434"],"sources":["hyg","hipparcos"],"scientificName":"Beta Crucis","catalogNumbers":["Beta Cru","HR 4853","HD 111123","HIP 62434"]},{"id":"star:toliman","type":"star","name":"Toliman","domain":"science","entryPath":"/stars/toliman","description":"Main-sequence star in Centaurus, about 4.3 light-years from Earth.","aliases":["HR 5460","HD 128621","HIP 71681","Gl 559B"],"sources":["hyg","hipparcos"],"catalogNumbers":["HR 5460","HD 128621","HIP 71681","Gl 559B"]},{"id":"star:adhara","type":"star","name":"Adhara","domain":"science","entryPath":"/stars/adhara","description":"Blue giant in Canis Major, about 405 light-years from Earth.","aliases":["Epsilon Canis Majoris","Epsilon CMa","21 CMa","HR 2618","HD 52089","HIP 33579"],"sources":["hyg","hipparcos"],"scientificName":"Epsilon Canis Majoris","catalogNumbers":["Epsilon CMa","21 CMa","HR 2618","HD 52089","HIP 33579"]},{"id":"star:shaula","type":"star","name":"Shaula","domain":"science","entryPath":"/stars/shaula","description":"Subgiant in Scorpius, about 571 light-years from Earth.","aliases":["Lambda Scorpii","Lambda Sco","35 Sco","HR 6527","HD 158926","HIP 85927"],"sources":["hyg","hipparcos"],"scientificName":"Lambda Scorpii","catalogNumbers":["Lambda Sco","35 Sco","HR 6527","HD 158926","HIP 85927"]},{"id":"star:elnath","type":"star","name":"Elnath","domain":"science","entryPath":"/stars/elnath","description":"Blue giant in Taurus, about 134 light-years from Earth.","aliases":["Beta Tauri","Beta Tau","112 Tau","HR 1791","HD 35497","HIP 25428"],"sources":["hyg","hipparcos"],"scientificName":"Beta Tauri","catalogNumbers":["Beta Tau","112 Tau","HR 1791","HD 35497","HIP 25428"]},{"id":"star:miaplacidus","type":"star","name":"Miaplacidus","domain":"science","entryPath":"/stars/miaplacidus","description":"Subgiant in Carina, about 113 light-years from Earth.","aliases":["Beta Carinae","Beta Car","HR 3685","HD 80007","HIP 45238"],"sources":["hyg","hipparcos"],"scientificName":"Beta Carinae","catalogNumbers":["Beta Car","HR 3685","HD 80007","HIP 45238"]},{"id":"star:alnair","type":"star","name":"Alnair","domain":"science","entryPath":"/stars/alnair","description":"Subgiant in Grus, about 101 light-years from Earth.","aliases":["Alpha Gruis","Alpha Gru","HR 8425","HD 209952","HIP 109268","Gl 848.2"],"sources":["hyg","hipparcos"],"scientificName":"Alpha Gruis","catalogNumbers":["Alpha Gru","HR 8425","HD 209952","HIP 109268","Gl 848.2"]},{"id":"star:hr-3207","type":"star","name":"HR 3207","domain":"science","entryPath":"/stars/hr-3207","description":"Wolf-Rayet star in Vela, about 1,117 light-years from Earth.","aliases":["HR 3207","HD 68273","HIP 39953"],"sources":["hyg","hipparcos"],"catalogNumbers":["HR 3207","HD 68273","HIP 39953"]},{"id":"star:kaus-australis","type":"star","name":"Kaus Australis","domain":"science","entryPath":"/stars/kaus-australis","description":"Blue giant in Sagittarius, about 143 light-years from Earth.","aliases":["Epsilon Sagittarii","Epsilon Sgr","20 Sgr","HR 6879","HD 169022","HIP 90185"],"sources":["hyg","hipparcos"],"scientificName":"Epsilon Sagittarii","catalogNumbers":["Epsilon Sgr","20 Sgr","HR 6879","HD 169022","HIP 90185"]},{"id":"star:wezen","type":"star","name":"Wezen","domain":"science","entryPath":"/stars/wezen","description":"Star in Canis Major, about 1,607 light-years from Earth.","aliases":["Delta Canis Majoris","Delta CMa","25 CMa","HR 2693","HD 54605","HIP 34444"],"sources":["hyg","hipparcos"],"scientificName":"Delta Canis Majoris","catalogNumbers":["Delta CMa","25 CMa","HR 2693","HD 54605","HIP 34444"]},{"id":"star:avior","type":"star","name":"Avior","domain":"science","entryPath":"/stars/avior","description":"Red giant in Carina, about 605 light-years from Earth.","aliases":["Epsilon Carinae","Epsilon Car","HR 3307","HD 71129","HIP 41037"],"sources":["hyg","hipparcos"],"scientificName":"Epsilon Carinae","catalogNumbers":["Epsilon Car","HR 3307","HD 71129","HIP 41037"]},{"id":"star:sargas","type":"star","name":"Sargas","domain":"science","entryPath":"/stars/sargas","description":"Star in Scorpius, about 300 light-years from Earth.","aliases":["Theta Scorpii","Theta Sco","HR 6553","HD 159532","HIP 86228"],"sources":["hyg","hipparcos"],"scientificName":"Theta Scorpii","catalogNumbers":["Theta Sco","HR 6553","HD 159532","HIP 86228"]},{"id":"star:menkalinan","type":"star","name":"Menkalinan","domain":"science","entryPath":"/stars/menkalinan","description":"Main-sequence star in Auriga, about 81.1 light-years from Earth.","aliases":["Beta Aurigae","Beta Aur","34 Aur","HR 2088","HD 40183","HIP 28360","GJ 3375"],"sources":["hyg","hipparcos"],"scientificName":"Beta Aurigae","catalogNumbers":["Beta Aur","34 Aur","HR 2088","HD 40183","HIP 28360","GJ 3375"]},{"id":"star:atria","type":"star","name":"Atria","domain":"science","entryPath":"/stars/atria","description":"Red supergiant in Triangulum Australe, about 391 light-years from Earth.","aliases":["Alpha Trianguli Australis","Alpha TrA","HR 6217","HD 150798","HIP 82273"],"sources":["hyg","hipparcos"],"scientificName":"Alpha Trianguli Australis","catalogNumbers":["Alpha TrA","HR 6217","HD 150798","HIP 82273"]},{"id":"star:alhena","type":"star","name":"Alhena","domain":"science","entryPath":"/stars/alhena","description":"Subgiant in Gemini, about 109 light-years from Earth.","aliases":["Gamma Geminorum","Gamma Gem","24 Gem","HR 2421","HD 47105","HIP 31681"],"sources":["hyg","hipparcos"],"scientificName":"Gamma Geminorum","catalogNumbers":["Gamma Gem","24 Gem","HR 2421","HD 47105","HIP 31681"]},{"id":"star:alsephina","type":"star","name":"Alsephina","domain":"science","entryPath":"/stars/alsephina","description":"Main-sequence star in Vela, about 80.5 light-years from Earth.","aliases":["Delta Velorum","Delta Vel","HR 3485","HD 74956","HIP 42913","Gl 321.3A"],"sources":["hyg","hipparcos"],"scientificName":"Delta Velorum","catalogNumbers":["Delta Vel","HR 3485","HD 74956","HIP 42913","Gl 321.3A"]},{"id":"star:peacock","type":"star","name":"Peacock","domain":"science","entryPath":"/stars/peacock","description":"Subgiant in Pavo, about 179 light-years from Earth.","aliases":["Alpha Pavonis","Alpha Pav","HR 7790","HD 193924","HIP 100751"],"sources":["hyg","hipparcos"],"scientificName":"Alpha Pavonis","catalogNumbers":["Alpha Pav","HR 7790","HD 193924","HIP 100751"]},{"id":"star:mirzam","type":"star","name":"Mirzam","domain":"science","entryPath":"/stars/mirzam","description":"Blue giant in Canis Major, about 493 light-years from Earth.","aliases":["Beta Canis Majoris","Beta CMa","2 CMa","HR 2294","HD 44743","HIP 30324"],"sources":["hyg","hipparcos"],"scientificName":"Beta Canis Majoris","catalogNumbers":["Beta CMa","2 CMa","HR 2294","HD 44743","HIP 30324"]},{"id":"star:alphard","type":"star","name":"Alphard","domain":"science","entryPath":"/stars/alphard","description":"Red giant in Hydra, about 180 light-years from Earth.","aliases":["Alpha Hydrae","Alpha Hya","30 Hya","HR 3748","HD 81797","HIP 46390"],"sources":["hyg","hipparcos"],"scientificName":"Alpha Hydrae","catalogNumbers":["Alpha Hya","30 Hya","HR 3748","HD 81797","HIP 46390"]},{"id":"star:algieba","type":"star","name":"Algieba","domain":"science","entryPath":"/stars/algieba","description":"Red giant in Leo, about 130 light-years from Earth.","aliases":["41 Leonis","41 Leo","HR 4057","HD 89484","HIP 50583"],"sources":["hyg","hipparcos"],"scientificName":"41 Leonis","catalogNumbers":["41 Leo","HR 4057","HD 89484","HIP 50583"]},{"id":"star:diphda","type":"star","name":"Diphda","domain":"science","entryPath":"/stars/diphda","description":"Red giant in Cetus, about 96.3 light-years from Earth.","aliases":["Beta Ceti","Beta Cet","16 Cet","HR 188","HD 4128","HIP 3419","Gl 31"],"sources":["hyg","hipparcos"],"scientificName":"Beta Ceti","catalogNumbers":["Beta Cet","16 Cet","HR 188","HD 4128","HIP 3419","Gl 31"]},{"id":"star:nunki","type":"star","name":"Nunki","domain":"science","entryPath":"/stars/nunki","description":"Main-sequence star in Sagittarius, about 228 light-years from Earth.","aliases":["Sigma Sagittarii","Sigma Sgr","34 Sgr","HR 7121","HD 175191","HIP 92855"],"sources":["hyg","hipparcos"],"scientificName":"Sigma Sagittarii","catalogNumbers":["Sigma Sgr","34 Sgr","HR 7121","HD 175191","HIP 92855"]},{"id":"star:menkent","type":"star","name":"Menkent","domain":"science","entryPath":"/stars/menkent","description":"Red supergiant in Centaurus, about 58.8 light-years from Earth.","aliases":["Theta Centauri","Theta Cen","5 Cen","HR 5288","HD 123139","HIP 68933","Gl 539"],"sources":["hyg","hipparcos"],"scientificName":"Theta Centauri","catalogNumbers":["Theta Cen","5 Cen","HR 5288","HD 123139","HIP 68933","Gl 539"]},{"id":"star:kochab","type":"star","name":"Kochab","domain":"science","entryPath":"/stars/kochab","description":"Red giant in Ursa Minor, about 131 light-years from Earth.","aliases":["Beta Ursae Minoris","Beta UMi","7 UMi","HR 5563","HD 131873","HIP 72607"],"sources":["hyg","hipparcos"],"scientificName":"Beta Ursae Minoris","catalogNumbers":["Beta UMi","7 UMi","HR 5563","HD 131873","HIP 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super-earth orbiting GJ 676 A, discovered in 2012 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-676-a-e","type":"exoplanet","name":"GJ 676 A e","domain":"science","entryPath":"/exoplanets/gj-676-a-e","description":"GJ 676 A e is a mini-neptune orbiting GJ 676 A, discovered in 2012 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-680-b","type":"exoplanet","name":"GJ 680 b","domain":"science","entryPath":"/exoplanets/gj-680-b","description":"GJ 680 b is a gas giant orbiting GJ 680, discovered in 2022 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-682-b","type":"exoplanet","name":"GJ 682 b","domain":"science","entryPath":"/exoplanets/gj-682-b","description":"GJ 682 b is a super-earth orbiting GJ 682, discovered in 2014 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-682-c","type":"exoplanet","name":"GJ 682 c","domain":"science","entryPath":"/exoplanets/gj-682-c","description":"GJ 682 c is a mini-neptune orbiting GJ 682, discovered in 2014 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-685-b","type":"exoplanet","name":"GJ 685 b","domain":"science","entryPath":"/exoplanets/gj-685-b","description":"GJ 685 b is a mini-neptune orbiting GJ 685, discovered in 2019 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-687-b","type":"exoplanet","name":"GJ 687 b","domain":"science","entryPath":"/exoplanets/gj-687-b","description":"GJ 687 b is a mini-neptune orbiting GJ 687, discovered in 2014 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-687-c","type":"exoplanet","name":"GJ 687 c","domain":"science","entryPath":"/exoplanets/gj-687-c","description":"GJ 687 c is a mini-neptune orbiting GJ 687, discovered in 2020 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-740-b","type":"exoplanet","name":"GJ 740 b","domain":"science","entryPath":"/exoplanets/gj-740-b","description":"GJ 740 b is a terrestrial planet orbiting GJ 740, discovered in 2021 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-806-b","type":"exoplanet","name":"GJ 806 b","domain":"science","entryPath":"/exoplanets/gj-806-b","description":"GJ 806 b is a terrestrial planet orbiting GJ 806, discovered in 2023 by the transit method.","sources":["nasa"]},{"id":"exoplanet:gj-806-c","type":"exoplanet","name":"GJ 806 c","domain":"science","entryPath":"/exoplanets/gj-806-c","description":"GJ 806 c is a super-earth orbiting GJ 806, discovered in 2023 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-832-b","type":"exoplanet","name":"GJ 832 b","domain":"science","entryPath":"/exoplanets/gj-832-b","description":"GJ 832 b is a gas giant orbiting GJ 832, discovered in 2008 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-849-b","type":"exoplanet","name":"GJ 849 b","domain":"science","entryPath":"/exoplanets/gj-849-b","description":"GJ 849 b is a gas 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discovered in 2000 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-876-d","type":"exoplanet","name":"GJ 876 d","domain":"science","entryPath":"/exoplanets/gj-876-d","description":"GJ 876 d is a mini-neptune orbiting GJ 876, discovered in 2005 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-876-e","type":"exoplanet","name":"GJ 876 e","domain":"science","entryPath":"/exoplanets/gj-876-e","description":"GJ 876 e is a mini-neptune orbiting GJ 876, discovered in 2010 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-887-b","type":"exoplanet","name":"GJ 887 b","domain":"science","entryPath":"/exoplanets/gj-887-b","description":"GJ 887 b is a super-earth orbiting GJ 887, discovered in 2020 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-887-c","type":"exoplanet","name":"GJ 887 c","domain":"science","entryPath":"/exoplanets/gj-887-c","description":"GJ 887 c is a mini-neptune orbiting GJ 887, 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discovered in 2024 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:gj-9066-c","type":"exoplanet","name":"GJ 9066 c","domain":"science","entryPath":"/exoplanets/gj-9066-c","description":"GJ 9066 c is a gas giant orbiting GJ 9066, discovered in 2020 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-96-b","type":"exoplanet","name":"GJ 96 b","domain":"science","entryPath":"/exoplanets/gj-96-b","description":"GJ 96 b is a mini-neptune orbiting GJ 96, discovered in 2018 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gj-9827-b","type":"exoplanet","name":"GJ 9827 b","domain":"science","entryPath":"/exoplanets/gj-9827-b","description":"GJ 9827 b is a terrestrial planet orbiting GJ 9827, discovered in 2017 by the transit method.","sources":["nasa"]},{"id":"exoplanet:gj-9827-c","type":"exoplanet","name":"GJ 9827 c","domain":"science","entryPath":"/exoplanets/gj-9827-c","description":"GJ 9827 c is a terrestrial planet orbiting GJ 9827, discovered in 2017 by the transit method.","sources":["nasa"]},{"id":"exoplanet:gj-9827-d","type":"exoplanet","name":"GJ 9827 d","domain":"science","entryPath":"/exoplanets/gj-9827-d","description":"GJ 9827 d is a super-earth orbiting GJ 9827, discovered in 2017 by the transit method.","sources":["nasa"]},{"id":"exoplanet:gl-378-b","type":"exoplanet","name":"Gl 378 b","domain":"science","entryPath":"/exoplanets/gl-378-b","description":"Gl 378 b is a mini-neptune orbiting Gl 378, discovered in 2019 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gl-410-b","type":"exoplanet","name":"Gl 410 b","domain":"science","entryPath":"/exoplanets/gl-410-b","description":"Gl 410 b is a mini-neptune orbiting Gl 410, discovered in 2025 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gl-49-b","type":"exoplanet","name":"Gl 49 b","domain":"science","entryPath":"/exoplanets/gl-49-b","description":"Gl 49 b is a super-earth orbiting Gl 49, discovered in 2019 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gl-686-b","type":"exoplanet","name":"Gl 686 b","domain":"science","entryPath":"/exoplanets/gl-686-b","description":"Gl 686 b is a mini-neptune orbiting Gl 686, discovered in 2018 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gl-725-a-b","type":"exoplanet","name":"Gl 725 A b","domain":"science","entryPath":"/exoplanets/gl-725-a-b","description":"Gl 725 A b is a terrestrial planet orbiting Gl 725 A, discovered in 2025 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:gliese-12-b","type":"exoplanet","name":"Gliese 12 b","domain":"science","entryPath":"/exoplanets/gliese-12-b","description":"Gliese 12 b is a terrestrial planet orbiting Gliese 12, discovered in 2024 by the transit method.","sources":["nasa"]},{"id":"exoplanet:gq-lup-b","type":"exoplanet","name":"GQ Lup b","domain":"science","entryPath":"/exoplanets/gq-lup-b","description":"GQ Lup b is a gas giant orbiting GQ Lup, discovered in 2004 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:gsc-06214-00210-b","type":"exoplanet","name":"GSC 06214-00210 b","domain":"science","entryPath":"/exoplanets/gsc-06214-00210-b","description":"GSC 06214-00210 b is a gas giant orbiting GSC 06214-00210, discovered in 2010 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:gu-psc-b","type":"exoplanet","name":"GU Psc b","domain":"science","entryPath":"/exoplanets/gu-psc-b","description":"GU Psc b is a gas giant orbiting GU Psc, discovered in 2014 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:hd-100546-b","type":"exoplanet","name":"HD 100546 b","domain":"science","entryPath":"/exoplanets/hd-100546-b","description":"HD 100546 b is a gas giant orbiting HD 100546, discovered in 2014 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:hd-100655-b","type":"exoplanet","name":"HD 100655 b","domain":"science","entryPath":"/exoplanets/hd-100655-b","description":"HD 100655 b is a gas 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discovered in 2010 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-113538-c","type":"exoplanet","name":"HD 113538 c","domain":"science","entryPath":"/exoplanets/hd-113538-c","description":"HD 113538 c is a gas giant orbiting HD 113538, discovered in 2010 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-113996-b","type":"exoplanet","name":"HD 113996 b","domain":"science","entryPath":"/exoplanets/hd-113996-b","description":"HD 113996 b is a gas giant orbiting HD 113996, discovered in 2017 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-114386-b","type":"exoplanet","name":"HD 114386 b","domain":"science","entryPath":"/exoplanets/hd-114386-b","description":"HD 114386 b is a gas giant orbiting HD 114386, discovered in 2003 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-114386-c","type":"exoplanet","name":"HD 114386 c","domain":"science","entryPath":"/exoplanets/hd-114386-c","description":"HD 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discovered in 2005 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-125612-b","type":"exoplanet","name":"HD 125612 b","domain":"science","entryPath":"/exoplanets/hd-125612-b","description":"HD 125612 b is a gas giant orbiting HD 125612, discovered in 2007 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-125612-c","type":"exoplanet","name":"HD 125612 c","domain":"science","entryPath":"/exoplanets/hd-125612-c","description":"HD 125612 c is a mini-neptune orbiting HD 125612, discovered in 2009 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-125612-d","type":"exoplanet","name":"HD 125612 d","domain":"science","entryPath":"/exoplanets/hd-125612-d","description":"HD 125612 d is a gas giant orbiting HD 125612, discovered in 2009 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-128311-b","type":"exoplanet","name":"HD 128311 b","domain":"science","entryPath":"/exoplanets/hd-128311-b","description":"HD 128311 b is a gas giant orbiting HD 128311, discovered in 2002 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-128311-c","type":"exoplanet","name":"HD 128311 c","domain":"science","entryPath":"/exoplanets/hd-128311-c","description":"HD 128311 c is a gas giant orbiting HD 128311, discovered in 2005 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-128717-b","type":"exoplanet","name":"HD 128717 b","domain":"science","entryPath":"/exoplanets/hd-128717-b","description":"HD 128717 b is a gas giant orbiting HD 128717, discovered in 2025 by the astrometry.","sources":["nasa"]},{"id":"exoplanet:hd-130322-b","type":"exoplanet","name":"HD 130322 b","domain":"science","entryPath":"/exoplanets/hd-130322-b","description":"HD 130322 b is a gas giant orbiting HD 130322, discovered in 1999 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-131496-b","type":"exoplanet","name":"HD 131496 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method.","sources":["nasa"]},{"id":"exoplanet:hd-134606-c","type":"exoplanet","name":"HD 134606 c","domain":"science","entryPath":"/exoplanets/hd-134606-c","description":"HD 134606 c is a mini-neptune orbiting HD 134606, discovered in 2024 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-134606-d","type":"exoplanet","name":"HD 134606 d","domain":"science","entryPath":"/exoplanets/hd-134606-d","description":"HD 134606 d is a gas giant orbiting HD 134606, discovered in 2024 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-134606-e","type":"exoplanet","name":"HD 134606 e","domain":"science","entryPath":"/exoplanets/hd-134606-e","description":"HD 134606 e is a terrestrial planet orbiting HD 134606, discovered in 2024 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-134606-f","type":"exoplanet","name":"HD 134606 f","domain":"science","entryPath":"/exoplanets/hd-134606-f","description":"HD 134606 f is a super-earth orbiting HD 134606, discovered in 2024 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-134987-b","type":"exoplanet","name":"HD 134987 b","domain":"science","entryPath":"/exoplanets/hd-134987-b","description":"HD 134987 b is a gas giant orbiting HD 134987, discovered in 1999 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-134987-c","type":"exoplanet","name":"HD 134987 c","domain":"science","entryPath":"/exoplanets/hd-134987-c","description":"HD 134987 c is a gas giant orbiting HD 134987, discovered in 2009 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-135344-a-b","type":"exoplanet","name":"HD 135344 A b","domain":"science","entryPath":"/exoplanets/hd-135344-a-b","description":"HD 135344 A b is a gas giant orbiting HD 135344 A, discovered in 2025 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:hd-136352-b","type":"exoplanet","name":"HD 136352 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discovered in 2021 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-141399-b","type":"exoplanet","name":"HD 141399 b","domain":"science","entryPath":"/exoplanets/hd-141399-b","description":"HD 141399 b is a gas giant orbiting HD 141399, discovered in 2014 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-141399-c","type":"exoplanet","name":"HD 141399 c","domain":"science","entryPath":"/exoplanets/hd-141399-c","description":"HD 141399 c is a gas giant orbiting HD 141399, discovered in 2014 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-141399-d","type":"exoplanet","name":"HD 141399 d","domain":"science","entryPath":"/exoplanets/hd-141399-d","description":"HD 141399 d is a gas giant orbiting HD 141399, discovered in 2014 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-141399-e","type":"exoplanet","name":"HD 141399 e","domain":"science","entryPath":"/exoplanets/hd-141399-e","description":"HD 141399 e is a gas giant orbiting HD 141399, discovered in 2014 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-142-a-d","type":"exoplanet","name":"HD 142 A d","domain":"science","entryPath":"/exoplanets/hd-142-a-d","description":"HD 142 A d is a gas giant orbiting HD 142, discovered in 2022 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-142-b","type":"exoplanet","name":"HD 142 b","domain":"science","entryPath":"/exoplanets/hd-142-b","description":"HD 142 b is a gas giant orbiting HD 142, discovered in 2001 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-142-c","type":"exoplanet","name":"HD 142 c","domain":"science","entryPath":"/exoplanets/hd-142-c","description":"HD 142 c is a gas giant orbiting HD 142, discovered in 2012 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-143811-ab-b","type":"exoplanet","name":"HD 143811 AB 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149026, discovered in 2005 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-149143-b","type":"exoplanet","name":"HD 149143 b","domain":"science","entryPath":"/exoplanets/hd-149143-b","description":"HD 149143 b is a hot jupiter orbiting HD 149143, discovered in 2005 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-1502-b","type":"exoplanet","name":"HD 1502 b","domain":"science","entryPath":"/exoplanets/hd-1502-b","description":"HD 1502 b is a gas giant orbiting HD 1502, discovered in 2011 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-152581-b","type":"exoplanet","name":"HD 152581 b","domain":"science","entryPath":"/exoplanets/hd-152581-b","description":"HD 152581 b is a gas giant orbiting HD 152581, discovered in 2011 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-153557-b","type":"exoplanet","name":"HD 153557 b","domain":"science","entryPath":"/exoplanets/hd-153557-b","description":"HD 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orbiting HD 158259, discovered in 2020 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-158259-f","type":"exoplanet","name":"HD 158259 f","domain":"science","entryPath":"/exoplanets/hd-158259-f","description":"HD 158259 f is a super-earth orbiting HD 158259, discovered in 2020 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-160691-b","type":"exoplanet","name":"HD 160691 b","domain":"science","entryPath":"/exoplanets/hd-160691-b","description":"HD 160691 b is an exoplanet orbiting HD 160691, discovered in 2000 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-160691-c","type":"exoplanet","name":"HD 160691 c","domain":"science","entryPath":"/exoplanets/hd-160691-c","description":"HD 160691 c is an exoplanet orbiting HD 160691, discovered in 2004 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-160691-d","type":"exoplanet","name":"HD 160691 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164922, discovered in 2020 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-164922-e","type":"exoplanet","name":"HD 164922 e","domain":"science","entryPath":"/exoplanets/hd-164922-e","description":"HD 164922 e is a mini-neptune orbiting HD 164922, discovered in 2021 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-168746-b","type":"exoplanet","name":"HD 168746 b","domain":"science","entryPath":"/exoplanets/hd-168746-b","description":"HD 168746 b is a hot jupiter orbiting HD 168746, discovered in 2002 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-169142-b","type":"exoplanet","name":"HD 169142 b","domain":"science","entryPath":"/exoplanets/hd-169142-b","description":"HD 169142 b is a gas giant orbiting HD 169142, discovered in 2023 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:hd-17156-b","type":"exoplanet","name":"HD 17156 b","domain":"science","entryPath":"/exoplanets/hd-17156-b","description":"HD 17156 b is a gas giant orbiting HD 17156, discovered in 2007 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-173416-b","type":"exoplanet","name":"HD 173416 b","domain":"science","entryPath":"/exoplanets/hd-173416-b","description":"HD 173416 b is a gas giant orbiting HD 173416, discovered in 2008 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-175541-b","type":"exoplanet","name":"HD 175541 b","domain":"science","entryPath":"/exoplanets/hd-175541-b","description":"HD 175541 b is a gas giant orbiting HD 175541, discovered in 2007 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-176986-b","type":"exoplanet","name":"HD 176986 b","domain":"science","entryPath":"/exoplanets/hd-176986-b","description":"HD 176986 b is an exoplanet orbiting HD 176986, discovered in 2017 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-176986-c","type":"exoplanet","name":"HD 176986 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discovered in 2022 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-192263-b","type":"exoplanet","name":"HD 192263 b","domain":"science","entryPath":"/exoplanets/hd-192263-b","description":"HD 192263 b is a gas giant orbiting HD 192263, discovered in 1999 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-192310-b","type":"exoplanet","name":"HD 192310 b","domain":"science","entryPath":"/exoplanets/hd-192310-b","description":"HD 192310 b is a mini-neptune orbiting HD 192310, discovered in 2011 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-192310-c","type":"exoplanet","name":"HD 192310 c","domain":"science","entryPath":"/exoplanets/hd-192310-c","description":"HD 192310 c is a mini-neptune orbiting HD 192310, discovered in 2011 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-192699-b","type":"exoplanet","name":"HD 192699 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discovered in 2009 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-206893-b","type":"exoplanet","name":"HD 206893 b","domain":"science","entryPath":"/exoplanets/hd-206893-b","description":"HD 206893 b is a gas giant orbiting HD 206893, discovered in 2021 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:hd-206893-c","type":"exoplanet","name":"HD 206893 c","domain":"science","entryPath":"/exoplanets/hd-206893-c","description":"HD 206893 c is a gas giant orbiting HD 206893, discovered in 2022 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:hd-20781-b","type":"exoplanet","name":"HD 20781 b","domain":"science","entryPath":"/exoplanets/hd-20781-b","description":"HD 20781 b is a terrestrial planet orbiting HD 20781, discovered in 2019 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-20781-c","type":"exoplanet","name":"HD 20781 c","domain":"science","entryPath":"/exoplanets/hd-20781-c","description":"HD 20781 c is a 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discovered in 2019 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-212771-b","type":"exoplanet","name":"HD 212771 b","domain":"science","entryPath":"/exoplanets/hd-212771-b","description":"HD 212771 b is a gas giant orbiting HD 212771, discovered in 2009 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-215152-b","type":"exoplanet","name":"HD 215152 b","domain":"science","entryPath":"/exoplanets/hd-215152-b","description":"HD 215152 b is an exoplanet orbiting HD 215152, discovered in 2018 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-215152-c","type":"exoplanet","name":"HD 215152 c","domain":"science","entryPath":"/exoplanets/hd-215152-c","description":"HD 215152 c is an exoplanet orbiting HD 215152, discovered in 2018 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-215152-d","type":"exoplanet","name":"HD 215152 d","domain":"science","entryPath":"/exoplanets/hd-215152-d","description":"HD 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HD 219134, discovered in 2015 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-221287-b","type":"exoplanet","name":"HD 221287 b","domain":"science","entryPath":"/exoplanets/hd-221287-b","description":"HD 221287 b is a gas giant orbiting HD 221287, discovered in 2007 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-222237-b","type":"exoplanet","name":"HD 222237 b","domain":"science","entryPath":"/exoplanets/hd-222237-b","description":"HD 222237 b is a gas giant orbiting HD 222237, discovered in 2024 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-224693-b","type":"exoplanet","name":"HD 224693 b","domain":"science","entryPath":"/exoplanets/hd-224693-b","description":"HD 224693 b is a gas giant orbiting HD 224693, discovered in 2006 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-22496-b","type":"exoplanet","name":"HD 22496 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in 2005 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-27894-c","type":"exoplanet","name":"HD 27894 c","domain":"science","entryPath":"/exoplanets/hd-27894-c","description":"HD 27894 c is a gas giant orbiting HD 27894, discovered in 2017 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-27894-d","type":"exoplanet","name":"HD 27894 d","domain":"science","entryPath":"/exoplanets/hd-27894-d","description":"HD 27894 d is a gas giant orbiting HD 27894, discovered in 2017 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-284149-ab-b","type":"exoplanet","name":"HD 284149 AB b","domain":"science","entryPath":"/exoplanets/hd-284149-ab-b","description":"HD 284149 AB b is a gas giant orbiting HD 284149 A, discovered in 2017 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:hd-285968-b","type":"exoplanet","name":"HD 285968 b","domain":"science","entryPath":"/exoplanets/hd-285968-b","description":"HD 285968 b is a 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46375, discovered in 2000 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-47536-b","type":"exoplanet","name":"HD 47536 b","domain":"science","entryPath":"/exoplanets/hd-47536-b","description":"HD 47536 b is a gas giant orbiting HD 47536, discovered in 2002 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-48265-b","type":"exoplanet","name":"HD 48265 b","domain":"science","entryPath":"/exoplanets/hd-48265-b","description":"HD 48265 b is a gas giant orbiting HD 48265, discovered in 2008 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-48265-c","type":"exoplanet","name":"HD 48265 c","domain":"science","entryPath":"/exoplanets/hd-48265-c","description":"HD 48265 c is a gas giant orbiting HD 48265, discovered in 2026 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-48948-b","type":"exoplanet","name":"HD 48948 b","domain":"science","entryPath":"/exoplanets/hd-48948-b","description":"HD 48948 b is a super-earth orbiting HD 48948, discovered in 2024 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-48948-c","type":"exoplanet","name":"HD 48948 c","domain":"science","entryPath":"/exoplanets/hd-48948-c","description":"HD 48948 c is a mini-neptune orbiting HD 48948, discovered in 2024 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-48948-d","type":"exoplanet","name":"HD 48948 d","domain":"science","entryPath":"/exoplanets/hd-48948-d","description":"HD 48948 d is a mini-neptune orbiting HD 48948, discovered in 2024 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-49674-b","type":"exoplanet","name":"HD 49674 b","domain":"science","entryPath":"/exoplanets/hd-49674-b","description":"HD 49674 b is a hot jupiter orbiting HD 49674, discovered in 2002 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:hd-52265-b","type":"exoplanet","name":"HD 52265 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orbiting WD 0806-661, discovered in 2011 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:wise-j033605-05-014350-4-b","type":"exoplanet","name":"WISE J033605.05-014350.4 b","domain":"science","entryPath":"/exoplanets/wise-j033605-05-014350-4-b","description":"WISE J033605.05-014350.4 b is a gas giant orbiting WISE J033605.05-014350.4, discovered in 2023 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:wisep-j121756-91-162640-2-a-b","type":"exoplanet","name":"WISEP J121756.91+162640.2 A b","domain":"science","entryPath":"/exoplanets/wisep-j121756-91-162640-2-a-b","description":"WISEP J121756.91+162640.2 A b is a gas giant orbiting WISEP J121756.91+162640.2 A, discovered in 2012 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:wispit-1-b","type":"exoplanet","name":"WISPIT 1 b","domain":"science","entryPath":"/exoplanets/wispit-1-b","description":"WISPIT 1 b is a gas giant orbiting WISPIT 1, discovered in 2025 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:wispit-1-c","type":"exoplanet","name":"WISPIT 1 c","domain":"science","entryPath":"/exoplanets/wispit-1-c","description":"WISPIT 1 c is a gas giant orbiting WISPIT 1, discovered in 2025 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:wispit-2-b","type":"exoplanet","name":"WISPIT 2 b","domain":"science","entryPath":"/exoplanets/wispit-2-b","description":"WISPIT 2 b is a gas giant orbiting WISPIT 2, discovered in 2025 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:wispit-2-c","type":"exoplanet","name":"WISPIT 2 c","domain":"science","entryPath":"/exoplanets/wispit-2-c","description":"WISPIT 2 c is a gas giant orbiting WISPIT 2, discovered in 2026 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:wolf-1061-b","type":"exoplanet","name":"Wolf 1061 b","domain":"science","entryPath":"/exoplanets/wolf-1061-b","description":"Wolf 1061 b is a terrestrial planet orbiting Wolf 1061, discovered in 2015 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:wolf-1061-c","type":"exoplanet","name":"Wolf 1061 c","domain":"science","entryPath":"/exoplanets/wolf-1061-c","description":"Wolf 1061 c is a super-earth orbiting Wolf 1061, discovered in 2015 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:wolf-1061-d","type":"exoplanet","name":"Wolf 1061 d","domain":"science","entryPath":"/exoplanets/wolf-1061-d","description":"Wolf 1061 d is a mini-neptune orbiting Wolf 1061, discovered in 2015 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:wolf-1069-b","type":"exoplanet","name":"Wolf 1069 b","domain":"science","entryPath":"/exoplanets/wolf-1069-b","description":"Wolf 1069 b is a terrestrial planet orbiting Wolf 1069, discovered in 2023 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:kointreau-1-b","type":"exoplanet","name":"KOINTREAU-1 b","domain":"science","entryPath":"/exoplanets/kointreau-1-b","description":"KOINTREAU-1 b is a gas giant orbiting XEST 17-036, discovered in 2026 by the direct imaging.","sources":["nasa"]},{"id":"exoplanet:xi-aql-b","type":"exoplanet","name":"xi Aql b","domain":"science","entryPath":"/exoplanets/xi-aql-b","description":"xi Aql b is a gas giant orbiting xi Aql, discovered in 2007 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:xo-2-s-b","type":"exoplanet","name":"XO-2 S b","domain":"science","entryPath":"/exoplanets/xo-2-s-b","description":"XO-2 S b is a gas giant orbiting XO-2 S, discovered in 2014 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:xo-2-s-c","type":"exoplanet","name":"XO-2 S c","domain":"science","entryPath":"/exoplanets/xo-2-s-c","description":"XO-2 S c is a gas giant orbiting XO-2 S, discovered in 2014 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:xo-2-s-d","type":"exoplanet","name":"XO-2 S d","domain":"science","entryPath":"/exoplanets/xo-2-s-d","description":"XO-2 S d is a gas giant orbiting XO-2 S, discovered in 2024 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:yz-cet-b","type":"exoplanet","name":"YZ Cet b","domain":"science","entryPath":"/exoplanets/yz-cet-b","description":"YZ Cet b is a terrestrial planet orbiting YZ Cet, discovered in 2017 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:yz-cet-c","type":"exoplanet","name":"YZ Cet c","domain":"science","entryPath":"/exoplanets/yz-cet-c","description":"YZ Cet c is a terrestrial planet orbiting YZ Cet, discovered in 2017 by the radial velocity method.","sources":["nasa"]},{"id":"exoplanet:yz-cet-d","type":"exoplanet","name":"YZ Cet d","domain":"science","entryPath":"/exoplanets/yz-cet-d","description":"YZ Cet d is a terrestrial planet orbiting YZ Cet, discovered in 2017 by the radial velocity method.","sources":["nasa"]},{"id":"host_star:14-her","type":"host_star","name":"14 Her","domain":"science","entryPath":"/exoplanets/14-her","description":"14 Her is a K0 star that hosts 2 known exoplanets in this catalogue, about 58 light-years away.","aliases":["K0"],"sources":["nasa"]},{"id":"host_star:1rxs-j160929-1-210524","type":"host_star","name":"1RXS J160929.1-210524","domain":"science","entryPath":"/exoplanets/1rxs-j160929-1-210524","description":"1RXS J160929.1-210524 is a K7 V star that hosts 1 known exoplanet in this catalogue, about 454 light-years away.","aliases":["K7 V"],"sources":["nasa"]},{"id":"host_star:2mass-j01033563-5515561-a-star","type":"host_star","name":"2MASS J01033563-5515561 A","domain":"science","entryPath":"/exoplanets/2mass-j01033563-5515561-a-star","description":"2MASS J01033563-5515561 A is a M5.5/M6 star that hosts 1 known exoplanet in this catalogue, about 154 light-years away.","aliases":["M5.5/M6"],"sources":["nasa"]},{"id":"host_star:2mass-j01225093-2439505","type":"host_star","name":"2MASS J01225093-2439505","domain":"science","entryPath":"/exoplanets/2mass-j01225093-2439505","description":"2MASS J01225093-2439505 is a M3.5 V star that hosts 1 known exoplanet in this catalogue, about 110 light-years away.","aliases":["M3.5 V"],"sources":["nasa"]},{"id":"host_star:2mass-j02192210-3925225","type":"host_star","name":"2MASS J02192210-3925225","domain":"science","entryPath":"/exoplanets/2mass-j02192210-3925225","description":"2MASS J02192210-3925225 is a M6 star that hosts 1 known exoplanet in this catalogue, about 131 light-years away.","aliases":["M6"],"sources":["nasa"]},{"id":"host_star:2mass-j0249-0557-a-star","type":"host_star","name":"2MASS J0249-0557 A","domain":"science","entryPath":"/exoplanets/2mass-j0249-0557-a-star","description":"2MASS J0249-0557 A is a M6 V star that hosts 1 known exoplanet in this catalogue, about 215 light-years away.","aliases":["M6 V"],"sources":["nasa"]},{"id":"host_star:2mass-j03590986-2009361","type":"host_star","name":"2MASS J03590986+2009361","domain":"science","entryPath":"/exoplanets/2mass-j03590986-2009361","description":"2MASS J03590986+2009361 is a star that hosts 1 known exoplanet in this catalogue, about 383 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:2mass-j04372171-2651014","type":"host_star","name":"2MASS J04372171+2651014","domain":"science","entryPath":"/exoplanets/2mass-j04372171-2651014","description":"2MASS J04372171+2651014 is a M V star that hosts 1 known exoplanet in this catalogue, about 419 light-years away.","aliases":["M V"],"sources":["nasa"]},{"id":"host_star:2mass-j04414489-2301513","type":"host_star","name":"2MASS J04414489+2301513","domain":"science","entryPath":"/exoplanets/2mass-j04414489-2301513","description":"2MASS J04414489+2301513 is a M8.5 star that hosts 1 known exoplanet in this catalogue, about 393 light-years away.","aliases":["M8.5"],"sources":["nasa"]},{"id":"host_star:2mass-j11011926-7732383","type":"host_star","name":"2MASS J11011926-7732383","domain":"science","entryPath":"/exoplanets/2mass-j11011926-7732383","description":"2MASS J11011926-7732383 is a star that hosts 1 known exoplanet in this catalogue.","aliases":[],"sources":["nasa"]},{"id":"host_star:2mass-j11550485-7919108","type":"host_star","name":"2MASS J11550485-7919108","domain":"science","entryPath":"/exoplanets/2mass-j11550485-7919108","description":"2MASS J11550485-7919108 is a star that hosts 1 known exoplanet in this catalogue, about 329 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:2mass-j12073346-3932539","type":"host_star","name":"2MASS J12073346-3932539","domain":"science","entryPath":"/exoplanets/2mass-j12073346-3932539","description":"2MASS J12073346-3932539 is a M8 star that hosts 1 known exoplanet in this catalogue, about 210 light-years away.","aliases":["M8"],"sources":["nasa"]},{"id":"host_star:2mass-j16262785-2625152","type":"host_star","name":"2MASS J16262785-2625152","domain":"science","entryPath":"/exoplanets/2mass-j16262785-2625152","description":"2MASS J16262785-2625152 is a M4.5 star that hosts 1 known exoplanet in this catalogue, about 474 light-years away.","aliases":["M4.5"],"sources":["nasa"]},{"id":"host_star:2mass-j19383260-4603591","type":"host_star","name":"2MASS J19383260+4603591","domain":"science","entryPath":"/exoplanets/2mass-j19383260-4603591","description":"2MASS J19383260+4603591 is a star that hosts 3 known exoplanets in this catalogue, about 1293 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:2mass-j21252752-8138278","type":"host_star","name":"2MASS J21252752-8138278","domain":"science","entryPath":"/exoplanets/2mass-j21252752-8138278","description":"2MASS J21252752-8138278 is a star that hosts 1 known exoplanet in this catalogue, about 111 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:2mass-j22362452-4751425","type":"host_star","name":"2MASS J22362452+4751425","domain":"science","entryPath":"/exoplanets/2mass-j22362452-4751425","description":"2MASS J22362452+4751425 is a K7 V star that hosts 1 known exoplanet in this catalogue, about 227 light-years away.","aliases":["K7 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Pic","domain":"science","entryPath":"/exoplanets/ab-pic","description":"AB Pic is a K2 V star that hosts 1 known exoplanet in this catalogue, about 163 light-years away.","aliases":["K2 V"],"sources":["nasa"]},{"id":"host_star:af-lep","type":"host_star","name":"AF Lep","domain":"science","entryPath":"/exoplanets/af-lep","description":"AF Lep is a F8 star that hosts 1 known exoplanet in this catalogue, about 88 light-years away.","aliases":["F8"],"sources":["nasa"]},{"id":"host_star:au-mic","type":"host_star","name":"AU Mic","domain":"science","entryPath":"/exoplanets/au-mic","description":"AU Mic is a M1 V star that hosts 4 known exoplanets in this catalogue, about 32 light-years away.","aliases":["M1 V"],"sources":["nasa"]},{"id":"host_star:b-cen-a-star","type":"host_star","name":"b Cen A","domain":"science","entryPath":"/exoplanets/b-cen-a-star","description":"b Cen A is a B2.5 V star that hosts 1 known exoplanet in this catalogue, about 320 light-years away.","aliases":["B2.5 V"],"sources":["nasa"]},{"id":"host_star:bd-06-1339","type":"host_star","name":"BD-06 1339","domain":"science","entryPath":"/exoplanets/bd-06-1339","description":"BD-06 1339 is a K7/M0 V star that hosts 2 known exoplanets in this catalogue, about 66 light-years away.","aliases":["K7/M0 V"],"sources":["nasa"]},{"id":"host_star:bd-11-4672","type":"host_star","name":"BD-11 4672","domain":"science","entryPath":"/exoplanets/bd-11-4672","description":"BD-11 4672 is a K7V star that hosts 2 known exoplanets in this catalogue, about 89 light-years away.","aliases":["K7V"],"sources":["nasa"]},{"id":"host_star:bd-210397","type":"host_star","name":"BD-210397","domain":"science","entryPath":"/exoplanets/bd-210397","description":"BD-210397 is a K7 V star that hosts 2 known exoplanets in this catalogue, about 77 light-years away.","aliases":["K7 V"],"sources":["nasa"]},{"id":"host_star:bd-60-1417","type":"host_star","name":"BD+60 1417","domain":"science","entryPath":"/exoplanets/bd-60-1417","description":"BD+60 1417 is a K0 star that hosts 1 known exoplanet in this catalogue, about 147 light-years away.","aliases":["K0"],"sources":["nasa"]},{"id":"host_star:bet-pic","type":"host_star","name":"bet Pic","domain":"science","entryPath":"/exoplanets/bet-pic","description":"bet Pic is a A5V star that hosts 2 known exoplanets in this catalogue, about 64 light-years away.","aliases":["A5V"],"sources":["nasa"]},{"id":"host_star:cd-cet","type":"host_star","name":"CD Cet","domain":"science","entryPath":"/exoplanets/cd-cet","description":"CD Cet is a M5.0 V star that hosts 1 known exoplanet in this catalogue, about 28 light-years away.","aliases":["M5.0 V"],"sources":["nasa"]},{"id":"host_star:cd-35-2722","type":"host_star","name":"CD-35 2722","domain":"science","entryPath":"/exoplanets/cd-35-2722","description":"CD-35 2722 is a M1 V star that hosts 1 known exoplanet in this catalogue, about 73 light-years away.","aliases":["M1 V"],"sources":["nasa"]},{"id":"host_star:cfbdsir-j145829-101343","type":"host_star","name":"CFBDSIR J145829+101343","domain":"science","entryPath":"/exoplanets/cfbdsir-j145829-101343","description":"CFBDSIR J145829+101343 is a star that hosts 1 known exoplanet in this catalogue, about 75 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:cfhtwir-oph-98-a-star","type":"host_star","name":"CFHTWIR-Oph 98 A","domain":"science","entryPath":"/exoplanets/cfhtwir-oph-98-a-star","description":"CFHTWIR-Oph 98 A is a M9-L1 star that hosts 1 known exoplanet in this catalogue.","aliases":["M9-L1"],"sources":["nasa"]},{"id":"host_star:chxr-73","type":"host_star","name":"CHXR 73","domain":"science","entryPath":"/exoplanets/chxr-73","description":"CHXR 73 is a M3.5 star that hosts 1 known exoplanet in this catalogue, about 621 light-years away.","aliases":["M3.5"],"sources":["nasa"]},{"id":"host_star:coconuts-2-a-star","type":"host_star","name":"COCONUTS-2 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J082303.1-491201","domain":"science","entryPath":"/exoplanets/denis-p-j082303-1-491201","description":"DENIS-P J082303.1-491201 is a L1.5 star that hosts 1 known exoplanet in this catalogue, about 68 light-years away.","aliases":["L1.5"],"sources":["nasa"]},{"id":"host_star:dh-tau","type":"host_star","name":"DH Tau","domain":"science","entryPath":"/exoplanets/dh-tau","description":"DH Tau is a M0.5 star that hosts 1 known exoplanet in this catalogue, about 440 light-years away.","aliases":["M0.5"],"sources":["nasa"]},{"id":"host_star:dmpp-1","type":"host_star","name":"DMPP-1","domain":"science","entryPath":"/exoplanets/dmpp-1","description":"DMPP-1 is a F8 V star that hosts 4 known exoplanets in this catalogue, about 204 light-years away.","aliases":["F8 V"],"sources":["nasa"]},{"id":"host_star:dp-leo","type":"host_star","name":"DP Leo","domain":"science","entryPath":"/exoplanets/dp-leo","description":"DP Leo is a star that hosts 1 known exoplanet in this catalogue, about 997 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:eps-eri","type":"host_star","name":"eps Eri","domain":"science","entryPath":"/exoplanets/eps-eri","description":"eps Eri is a K2 V star that hosts 1 known exoplanet in this catalogue, about 10 light-years away.","aliases":["K2 V"],"sources":["nasa"]},{"id":"host_star:eps-ind-a-star","type":"host_star","name":"eps Ind A","domain":"science","entryPath":"/exoplanets/eps-ind-a-star","description":"eps Ind A is a K5 V star that hosts 1 known exoplanet in this catalogue, about 12 light-years away.","aliases":["K5 V"],"sources":["nasa"]},{"id":"host_star:fu-tau","type":"host_star","name":"FU Tau","domain":"science","entryPath":"/exoplanets/fu-tau","description":"FU Tau is a M7.25 star that hosts 1 known exoplanet in this catalogue, about 435 light-years away.","aliases":["M7.25"],"sources":["nasa"]},{"id":"host_star:g-192-15","type":"host_star","name":"G 192-15","domain":"science","entryPath":"/exoplanets/g-192-15","description":"G 192-15 is a M5.0 V star that hosts 2 known exoplanets in this catalogue, about 31 light-years away.","aliases":["M5.0 V"],"sources":["nasa"]},{"id":"host_star:g-196-3","type":"host_star","name":"G 196-3","domain":"science","entryPath":"/exoplanets/g-196-3","description":"G 196-3 is a star that hosts 1 known exoplanet in this catalogue, about 71 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:g-261-6","type":"host_star","name":"G 261-6","domain":"science","entryPath":"/exoplanets/g-261-6","description":"G 261-6 is a M5.5 V star that hosts 1 known exoplanet in this catalogue, about 35 light-years away.","aliases":["M5.5 V"],"sources":["nasa"]},{"id":"host_star:gaia-4","type":"host_star","name":"Gaia-4","domain":"science","entryPath":"/exoplanets/gaia-4","description":"Gaia-4 is a star that hosts 1 known exoplanet in this catalogue, about 240 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:gaia-5","type":"host_star","name":"Gaia-5","domain":"science","entryPath":"/exoplanets/gaia-5","description":"Gaia-5 is a star that hosts 1 known exoplanet in this catalogue, about 134 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:gam-cep","type":"host_star","name":"gam Cep","domain":"science","entryPath":"/exoplanets/gam-cep","description":"gam Cep is a K1 III-IV star that hosts 1 known exoplanet in this catalogue, about 46 light-years away.","aliases":["K1 III-IV"],"sources":["nasa"]},{"id":"host_star:gj-1002","type":"host_star","name":"GJ 1002","domain":"science","entryPath":"/exoplanets/gj-1002","description":"GJ 1002 is a M5.5 V star that hosts 2 known exoplanets in this catalogue, about 16 light-years away.","aliases":["M5.5 V"],"sources":["nasa"]},{"id":"host_star:gj-1061","type":"host_star","name":"GJ 1061","domain":"science","entryPath":"/exoplanets/gj-1061","description":"GJ 1061 is a M5.5 V star that hosts 3 known exoplanets in this catalogue, about 12 light-years away.","aliases":["M5.5 V"],"sources":["nasa"]},{"id":"host_star:gj-1132","type":"host_star","name":"GJ 1132","domain":"science","entryPath":"/exoplanets/gj-1132","description":"GJ 1132 is a M4.5 V star that hosts 2 known exoplanets in this catalogue, about 41 light-years away.","aliases":["M4.5 V"],"sources":["nasa"]},{"id":"host_star:gj-1148","type":"host_star","name":"GJ 1148","domain":"science","entryPath":"/exoplanets/gj-1148","description":"GJ 1148 is a M5 star that hosts 2 known exoplanets in this catalogue, about 36 light-years away.","aliases":["M5"],"sources":["nasa"]},{"id":"host_star:gj-1151","type":"host_star","name":"GJ 1151","domain":"science","entryPath":"/exoplanets/gj-1151","description":"GJ 1151 is a M 4.5V star that hosts 1 known exoplanet in this catalogue, about 26 light-years away.","aliases":["M 4.5V"],"sources":["nasa"]},{"id":"host_star:gj-1265","type":"host_star","name":"GJ 1265","domain":"science","entryPath":"/exoplanets/gj-1265","description":"GJ 1265 is a M4.5 V star that hosts 1 known exoplanet in this catalogue, about 33 light-years away.","aliases":["M4.5 V"],"sources":["nasa"]},{"id":"host_star:gj-1289","type":"host_star","name":"GJ 1289","domain":"science","entryPath":"/exoplanets/gj-1289","description":"GJ 1289 is a M4.5 Ve star that hosts 1 known exoplanet in this catalogue, about 27 light-years away.","aliases":["M4.5 Ve"],"sources":["nasa"]},{"id":"host_star:gj-15-a-star","type":"host_star","name":"GJ 15 A","domain":"science","entryPath":"/exoplanets/gj-15-a-star","description":"GJ 15 A is a M1 star that hosts 2 known exoplanets in this catalogue, about 12 light-years away.","aliases":["M1"],"sources":["nasa"]},{"id":"host_star:gj-163","type":"host_star","name":"GJ 163","domain":"science","entryPath":"/exoplanets/gj-163","description":"GJ 163 is a M star that hosts 3 known exoplanets in this catalogue, about 49 light-years away.","aliases":["M"],"sources":["nasa"]},{"id":"host_star:gj-179","type":"host_star","name":"GJ 179","domain":"science","entryPath":"/exoplanets/gj-179","description":"GJ 179 is a M3.5 V star that hosts 1 known exoplanet in this catalogue, about 40 light-years away.","aliases":["M3.5 V"],"sources":["nasa"]},{"id":"host_star:gj-180","type":"host_star","name":"GJ 180","domain":"science","entryPath":"/exoplanets/gj-180","description":"GJ 180 is a M3 star that hosts 3 known exoplanets in this catalogue, about 39 light-years away.","aliases":["M3"],"sources":["nasa"]},{"id":"host_star:gj-229","type":"host_star","name":"GJ 229","domain":"science","entryPath":"/exoplanets/gj-229","description":"GJ 229 is a M1.5V star that hosts 2 known exoplanets in this catalogue, about 19 light-years away.","aliases":["M1.5V"],"sources":["nasa"]},{"id":"host_star:gj-251","type":"host_star","name":"GJ 251","domain":"science","entryPath":"/exoplanets/gj-251","description":"GJ 251 is a M3.0 V star that hosts 2 known exoplanets in this catalogue, about 18 light-years away.","aliases":["M3.0 V"],"sources":["nasa"]},{"id":"host_star:gj-273","type":"host_star","name":"GJ 273","domain":"science","entryPath":"/exoplanets/gj-273","description":"GJ 273 is a M3.5 star that hosts 2 known exoplanets in this catalogue, about 19 light-years away.","aliases":["M3.5"],"sources":["nasa"]},{"id":"host_star:gj-3021","type":"host_star","name":"GJ 3021","domain":"science","entryPath":"/exoplanets/gj-3021","description":"GJ 3021 is a G6 V star that hosts 1 known exoplanet in this catalogue, about 57 light-years away.","aliases":["G6 V"],"sources":["nasa"]},{"id":"host_star:gj-3138","type":"host_star","name":"GJ 3138","domain":"science","entryPath":"/exoplanets/gj-3138","description":"GJ 3138 is a M0 star that hosts 3 known exoplanets in this catalogue, about 93 light-years away.","aliases":["M0"],"sources":["nasa"]},{"id":"host_star:gj-317","type":"host_star","name":"GJ 317","domain":"science","entryPath":"/exoplanets/gj-317","description":"GJ 317 is a M3.5 V star that hosts 2 known exoplanets in this catalogue, about 50 light-years away.","aliases":["M3.5 V"],"sources":["nasa"]},{"id":"host_star:gj-328","type":"host_star","name":"GJ 328","domain":"science","entryPath":"/exoplanets/gj-328","description":"GJ 328 is a M0.0 star that hosts 2 known exoplanets in this catalogue, about 67 light-years away.","aliases":["M0.0"],"sources":["nasa"]},{"id":"host_star:gj-3293","type":"host_star","name":"GJ 3293","domain":"science","entryPath":"/exoplanets/gj-3293","description":"GJ 3293 is a M2.5 star that hosts 4 known exoplanets in this catalogue, about 66 light-years away.","aliases":["M2.5"],"sources":["nasa"]},{"id":"host_star:gj-3323","type":"host_star","name":"GJ 3323","domain":"science","entryPath":"/exoplanets/gj-3323","description":"GJ 3323 is a M4 star that hosts 2 known exoplanets in this catalogue, about 18 light-years away.","aliases":["M4"],"sources":["nasa"]},{"id":"host_star:gj-3378","type":"host_star","name":"GJ 3378","domain":"science","entryPath":"/exoplanets/gj-3378","description":"GJ 3378 is a M4 V star that hosts 1 known exoplanet in this catalogue, about 25 light-years away.","aliases":["M4 V"],"sources":["nasa"]},{"id":"host_star:gj-338-b-star","type":"host_star","name":"GJ 338 B","domain":"science","entryPath":"/exoplanets/gj-338-b-star","description":"GJ 338 B is a M0 V star that hosts 1 known exoplanet in this catalogue, about 21 light-years away.","aliases":["M0 V"],"sources":["nasa"]},{"id":"host_star:gj-341","type":"host_star","name":"GJ 341","domain":"science","entryPath":"/exoplanets/gj-341","description":"GJ 341 is a M1 star that hosts 1 known exoplanet in this catalogue, about 34 light-years away.","aliases":["M1"],"sources":["nasa"]},{"id":"host_star:gj-3512","type":"host_star","name":"GJ 3512","domain":"science","entryPath":"/exoplanets/gj-3512","description":"GJ 3512 is a M5.5 V star that hosts 2 known exoplanets in this catalogue, about 31 light-years away.","aliases":["M5.5 V"],"sources":["nasa"]},{"id":"host_star:gj-357","type":"host_star","name":"GJ 357","domain":"science","entryPath":"/exoplanets/gj-357","description":"GJ 357 is a M2.5 V star that hosts 3 known exoplanets in this catalogue, about 31 light-years away.","aliases":["M2.5 V"],"sources":["nasa"]},{"id":"host_star:gj-3634","type":"host_star","name":"GJ 3634","domain":"science","entryPath":"/exoplanets/gj-3634","description":"GJ 3634 is a M2.5 star that hosts 1 known exoplanet in this catalogue, about 66 light-years away.","aliases":["M2.5"],"sources":["nasa"]},{"id":"host_star:gj-367","type":"host_star","name":"GJ 367","domain":"science","entryPath":"/exoplanets/gj-367","description":"GJ 367 is a M1.0 V star that hosts 3 known exoplanets in this catalogue, about 31 light-years away.","aliases":["M1.0 V"],"sources":["nasa"]},{"id":"host_star:gj-3779","type":"host_star","name":"GJ 3779","domain":"science","entryPath":"/exoplanets/gj-3779","description":"GJ 3779 is a M4.0 V star that hosts 1 known exoplanet in this catalogue, about 45 light-years away.","aliases":["M4.0 V"],"sources":["nasa"]},{"id":"host_star:gj-393","type":"host_star","name":"GJ 393","domain":"science","entryPath":"/exoplanets/gj-393","description":"GJ 393 is a M2.0 V star that hosts 1 known exoplanet in this catalogue, about 23 light-years away.","aliases":["M2.0 V"],"sources":["nasa"]},{"id":"host_star:gj-3988","type":"host_star","name":"GJ 3988","domain":"science","entryPath":"/exoplanets/gj-3988","description":"GJ 3988 is a M4.5 V star that hosts 1 known exoplanet in this catalogue, about 32 light-years away.","aliases":["M4.5 V"],"sources":["nasa"]},{"id":"host_star:gj-3998","type":"host_star","name":"GJ 3998","domain":"science","entryPath":"/exoplanets/gj-3998","description":"GJ 3998 is a M1 star that hosts 3 known exoplanets in this catalogue, about 59 light-years away.","aliases":["M1"],"sources":["nasa"]},{"id":"host_star:gj-411","type":"host_star","name":"GJ 411","domain":"science","entryPath":"/exoplanets/gj-411","description":"GJ 411 is a M1.5 V star that hosts 2 known exoplanets in this catalogue, about 19 light-years away.","aliases":["M1.5 V"],"sources":["nasa"]},{"id":"host_star:gj-414-a-star","type":"host_star","name":"GJ 414 A","domain":"science","entryPath":"/exoplanets/gj-414-a-star","description":"GJ 414 A is a K7 V star that hosts 2 known exoplanets in this catalogue, about 39 light-years away.","aliases":["K7 V"],"sources":["nasa"]},{"id":"host_star:gj-422","type":"host_star","name":"GJ 422","domain":"science","entryPath":"/exoplanets/gj-422","description":"GJ 422 is a M3.5 V star that hosts 1 known exoplanet in this catalogue, about 41 light-years away.","aliases":["M3.5 V"],"sources":["nasa"]},{"id":"host_star:gj-4274","type":"host_star","name":"GJ 4274","domain":"science","entryPath":"/exoplanets/gj-4274","description":"GJ 4274 is a M4.5 V star that hosts 2 known exoplanets in this catalogue, about 24 light-years away.","aliases":["M4.5 V"],"sources":["nasa"]},{"id":"host_star:gj-433","type":"host_star","name":"GJ 433","domain":"science","entryPath":"/exoplanets/gj-433","description":"GJ 433 is a M2V star that hosts 3 known exoplanets in this catalogue, about 30 light-years away.","aliases":["M2V"],"sources":["nasa"]},{"id":"host_star:gj-436","type":"host_star","name":"GJ 436","domain":"science","entryPath":"/exoplanets/gj-436","description":"GJ 436 is a M2.5 V star that hosts 1 known exoplanet in this catalogue, about 32 light-years away.","aliases":["M2.5 V"],"sources":["nasa"]},{"id":"host_star:gj-480","type":"host_star","name":"GJ 480","domain":"science","entryPath":"/exoplanets/gj-480","description":"GJ 480 is a M3.5 Ve star that hosts 1 known exoplanet in this catalogue, about 46 light-years away.","aliases":["M3.5 Ve"],"sources":["nasa"]},{"id":"host_star:gj-486","type":"host_star","name":"GJ 486","domain":"science","entryPath":"/exoplanets/gj-486","description":"GJ 486 is a M3.5 V star that hosts 1 known exoplanet in this catalogue, about 26 light-years away.","aliases":["M3.5 V"],"sources":["nasa"]},{"id":"host_star:gj-504","type":"host_star","name":"GJ 504","domain":"science","entryPath":"/exoplanets/gj-504","description":"GJ 504 is a G0 V star that hosts 1 known exoplanet in this catalogue, about 57 light-years away.","aliases":["G0 V"],"sources":["nasa"]},{"id":"host_star:gj-514","type":"host_star","name":"GJ 514","domain":"science","entryPath":"/exoplanets/gj-514","description":"GJ 514 is a M0.5-1.0 V star that hosts 1 known exoplanet in this catalogue, about 25 light-years away.","aliases":["M0.5-1.0 V"],"sources":["nasa"]},{"id":"host_star:gj-536","type":"host_star","name":"GJ 536","domain":"science","entryPath":"/exoplanets/gj-536","description":"GJ 536 is a M1 V star that hosts 2 known exoplanets in this catalogue, about 34 light-years away.","aliases":["M1 V"],"sources":["nasa"]},{"id":"host_star:gj-625","type":"host_star","name":"GJ 625","domain":"science","entryPath":"/exoplanets/gj-625","description":"GJ 625 is a M2 star that hosts 1 known exoplanet in this catalogue, about 21 light-years away.","aliases":["M2"],"sources":["nasa"]},{"id":"host_star:gj-649","type":"host_star","name":"GJ 649","domain":"science","entryPath":"/exoplanets/gj-649","description":"GJ 649 is a M1.0 star that hosts 1 known exoplanet in this catalogue, about 34 light-years away.","aliases":["M1.0"],"sources":["nasa"]},{"id":"host_star:gj-667-c-star","type":"host_star","name":"GJ 667 C","domain":"science","entryPath":"/exoplanets/gj-667-c-star","description":"GJ 667 C is a M1.5 V star that hosts 5 known exoplanets in this catalogue, about 24 light-years away.","aliases":["M1.5 V"],"sources":["nasa"]},{"id":"host_star:gj-674","type":"host_star","name":"GJ 674","domain":"science","entryPath":"/exoplanets/gj-674","description":"GJ 674 is a M2.5 star that hosts 1 known exoplanet in this catalogue, about 15 light-years away.","aliases":["M2.5"],"sources":["nasa"]},{"id":"host_star:gj-676-a-star","type":"host_star","name":"GJ 676 A","domain":"science","entryPath":"/exoplanets/gj-676-a-star","description":"GJ 676 A is a M0 star that hosts 4 known exoplanets in this catalogue, about 52 light-years away.","aliases":["M0"],"sources":["nasa"]},{"id":"host_star:gj-680","type":"host_star","name":"GJ 680","domain":"science","entryPath":"/exoplanets/gj-680","description":"GJ 680 is a K5 star that hosts 1 known exoplanet in this catalogue, about 32 light-years away.","aliases":["K5"],"sources":["nasa"]},{"id":"host_star:gj-682","type":"host_star","name":"GJ 682","domain":"science","entryPath":"/exoplanets/gj-682","description":"GJ 682 is a M3.5 V star that hosts 2 known exoplanets in this catalogue, about 16 light-years away.","aliases":["M3.5 V"],"sources":["nasa"]},{"id":"host_star:gj-685","type":"host_star","name":"GJ 685","domain":"science","entryPath":"/exoplanets/gj-685","description":"GJ 685 is a M0.5 star that hosts 1 known exoplanet in this catalogue, about 47 light-years away.","aliases":["M0.5"],"sources":["nasa"]},{"id":"host_star:gj-687","type":"host_star","name":"GJ 687","domain":"science","entryPath":"/exoplanets/gj-687","description":"GJ 687 is a M3.0V star that hosts 2 known exoplanets in this catalogue, about 15 light-years away.","aliases":["M3.0V"],"sources":["nasa"]},{"id":"host_star:gj-740","type":"host_star","name":"GJ 740","domain":"science","entryPath":"/exoplanets/gj-740","description":"GJ 740 is a M1.0 V star that hosts 1 known exoplanet in this catalogue, about 36 light-years away.","aliases":["M1.0 V"],"sources":["nasa"]},{"id":"host_star:gj-806","type":"host_star","name":"GJ 806","domain":"science","entryPath":"/exoplanets/gj-806","description":"GJ 806 is a M1.5 V star that hosts 2 known exoplanets in this catalogue, about 39 light-years away.","aliases":["M1.5 V"],"sources":["nasa"]},{"id":"host_star:gj-832","type":"host_star","name":"GJ 832","domain":"science","entryPath":"/exoplanets/gj-832","description":"GJ 832 is a M2/3 V star that hosts 1 known exoplanet in this catalogue, about 16 light-years away.","aliases":["M2/3 V"],"sources":["nasa"]},{"id":"host_star:gj-849","type":"host_star","name":"GJ 849","domain":"science","entryPath":"/exoplanets/gj-849","description":"GJ 849 is a M3.5 star that hosts 2 known exoplanets in this catalogue, about 29 light-years away.","aliases":["M3.5"],"sources":["nasa"]},{"id":"host_star:gj-86","type":"host_star","name":"GJ 86","domain":"science","entryPath":"/exoplanets/gj-86","description":"GJ 86 is a K1V star that hosts 1 known exoplanet in this catalogue, about 35 light-years away.","aliases":["K1V"],"sources":["nasa"]},{"id":"host_star:gj-876","type":"host_star","name":"GJ 876","domain":"science","entryPath":"/exoplanets/gj-876","description":"GJ 876 is a M2.5V star that hosts 4 known exoplanets in this catalogue, about 15 light-years away.","aliases":["M2.5V"],"sources":["nasa"]},{"id":"host_star:gj-887","type":"host_star","name":"GJ 887","domain":"science","entryPath":"/exoplanets/gj-887","description":"GJ 887 is a M1 V star that hosts 4 known exoplanets in this catalogue, about 11 light-years away.","aliases":["M1 V"],"sources":["nasa"]},{"id":"host_star:gj-896-a-star","type":"host_star","name":"GJ 896 A","domain":"science","entryPath":"/exoplanets/gj-896-a-star","description":"GJ 896 A is a M3.5 V star that hosts 1 known exoplanet in this catalogue, about 20 light-years away.","aliases":["M3.5 V"],"sources":["nasa"]},{"id":"host_star:gj-900-a-star","type":"host_star","name":"GJ 900 A","domain":"science","entryPath":"/exoplanets/gj-900-a-star","description":"GJ 900 A is a K7 star that hosts 1 known exoplanet in this catalogue, about 68 light-years away.","aliases":["K7"],"sources":["nasa"]},{"id":"host_star:gj-9066","type":"host_star","name":"GJ 9066","domain":"science","entryPath":"/exoplanets/gj-9066","description":"GJ 9066 is a M5.0 V star that hosts 1 known exoplanet in this catalogue, about 15 light-years away.","aliases":["M5.0 V"],"sources":["nasa"]},{"id":"host_star:gj-96","type":"host_star","name":"GJ 96","domain":"science","entryPath":"/exoplanets/gj-96","description":"GJ 96 is a M2 star that hosts 1 known exoplanet in this catalogue, about 39 light-years away.","aliases":["M2"],"sources":["nasa"]},{"id":"host_star:gj-9827","type":"host_star","name":"GJ 9827","domain":"science","entryPath":"/exoplanets/gj-9827","description":"GJ 9827 is a K7 V star that hosts 3 known exoplanets in this catalogue, about 97 light-years away.","aliases":["K7 V"],"sources":["nasa"]},{"id":"host_star:gl-378","type":"host_star","name":"Gl 378","domain":"science","entryPath":"/exoplanets/gl-378","description":"Gl 378 is a M1 star that hosts 1 known exoplanet in this catalogue, about 49 light-years away.","aliases":["M1"],"sources":["nasa"]},{"id":"host_star:gl-410","type":"host_star","name":"Gl 410","domain":"science","entryPath":"/exoplanets/gl-410","description":"Gl 410 is a K star that hosts 1 known exoplanet in this catalogue, about 39 light-years away.","aliases":["K"],"sources":["nasa"]},{"id":"host_star:gl-49","type":"host_star","name":"Gl 49","domain":"science","entryPath":"/exoplanets/gl-49","description":"Gl 49 is a M1.5 V star that hosts 1 known exoplanet in this catalogue, about 32 light-years away.","aliases":["M1.5 V"],"sources":["nasa"]},{"id":"host_star:gl-686","type":"host_star","name":"Gl 686","domain":"science","entryPath":"/exoplanets/gl-686","description":"Gl 686 is a M1.0 V star that hosts 1 known exoplanet in this catalogue, about 27 light-years away.","aliases":["M1.0 V"],"sources":["nasa"]},{"id":"host_star:gliese-12","type":"host_star","name":"Gliese 12","domain":"science","entryPath":"/exoplanets/gliese-12","description":"Gliese 12 is a M4 V star that hosts 1 known exoplanet in this catalogue, about 40 light-years away.","aliases":["M4 V"],"sources":["nasa"]},{"id":"host_star:gq-lup","type":"host_star","name":"GQ Lup","domain":"science","entryPath":"/exoplanets/gq-lup","description":"GQ Lup is a K7e V star that hosts 1 known exoplanet in this catalogue, about 493 light-years away.","aliases":["K7e V"],"sources":["nasa"]},{"id":"host_star:gsc-06214-00210","type":"host_star","name":"GSC 06214-00210","domain":"science","entryPath":"/exoplanets/gsc-06214-00210","description":"GSC 06214-00210 is a K7 star that hosts 1 known exoplanet in this catalogue, about 354 light-years away.","aliases":["K7"],"sources":["nasa"]},{"id":"host_star:gu-psc","type":"host_star","name":"GU Psc","domain":"science","entryPath":"/exoplanets/gu-psc","description":"GU Psc is a M3 star that hosts 1 known exoplanet in this catalogue, about 155 light-years away.","aliases":["M3"],"sources":["nasa"]},{"id":"host_star:hd-100546","type":"host_star","name":"HD 100546","domain":"science","entryPath":"/exoplanets/hd-100546","description":"HD 100546 is a B9 Vne star that hosts 1 known exoplanet in this catalogue, about 358 light-years away.","aliases":["B9 Vne"],"sources":["nasa"]},{"id":"host_star:hd-10180","type":"host_star","name":"HD 10180","domain":"science","entryPath":"/exoplanets/hd-10180","description":"HD 10180 is a G1 V star that hosts 6 known exoplanets in this catalogue, about 127 light-years away.","aliases":["G1 V"],"sources":["nasa"]},{"id":"host_star:hd-104067","type":"host_star","name":"HD 104067","domain":"science","entryPath":"/exoplanets/hd-104067","description":"HD 104067 is a K2V star that hosts 2 known exoplanets in this catalogue, about 66 light-years away.","aliases":["K2V"],"sources":["nasa"]},{"id":"host_star:hd-10647","type":"host_star","name":"HD 10647","domain":"science","entryPath":"/exoplanets/hd-10647","description":"HD 10647 is a F9 V star that hosts 1 known exoplanet in this catalogue, about 57 light-years away.","aliases":["F9 V"],"sources":["nasa"]},{"id":"host_star:hd-106906","type":"host_star","name":"HD 106906","domain":"science","entryPath":"/exoplanets/hd-106906","description":"HD 106906 is a F5 V star that hosts 1 known exoplanet in this catalogue, about 336 light-years away.","aliases":["F5 V"],"sources":["nasa"]},{"id":"host_star:hd-111232","type":"host_star","name":"HD 111232","domain":"science","entryPath":"/exoplanets/hd-111232","description":"HD 111232 is a G8 V star that hosts 2 known exoplanets in this catalogue, about 94 light-years away.","aliases":["G8 V"],"sources":["nasa"]},{"id":"host_star:hd-113538","type":"host_star","name":"HD 113538","domain":"science","entryPath":"/exoplanets/hd-113538","description":"HD 113538 is a K9 V star that hosts 2 known exoplanets in this catalogue, about 53 light-years away.","aliases":["K9 V"],"sources":["nasa"]},{"id":"host_star:hd-114386","type":"host_star","name":"HD 114386","domain":"science","entryPath":"/exoplanets/hd-114386","description":"HD 114386 is a K3 VC star that hosts 2 known exoplanets in this catalogue, about 91 light-years away.","aliases":["K3 VC"],"sources":["nasa"]},{"id":"host_star:hd-114783","type":"host_star","name":"HD 114783","domain":"science","entryPath":"/exoplanets/hd-114783","description":"HD 114783 is a K0 star that hosts 2 known exoplanets in this catalogue, about 69 light-years away.","aliases":["K0"],"sources":["nasa"]},{"id":"host_star:hd-11506","type":"host_star","name":"HD 11506","domain":"science","entryPath":"/exoplanets/hd-11506","description":"HD 11506 is a G0 V star that hosts 3 known exoplanets in this catalogue, about 167 light-years away.","aliases":["G0 V"],"sources":["nasa"]},{"id":"host_star:hd-115404-a-star","type":"host_star","name":"HD 115404 A","domain":"science","entryPath":"/exoplanets/hd-115404-a-star","description":"HD 115404 A is a K2V star that hosts 2 known exoplanets in this catalogue, about 36 light-years away.","aliases":["K2V"],"sources":["nasa"]},{"id":"host_star:hd-125612","type":"host_star","name":"HD 125612","domain":"science","entryPath":"/exoplanets/hd-125612","description":"HD 125612 is a G3 V star that hosts 3 known exoplanets in this catalogue, about 188 light-years away.","aliases":["G3 V"],"sources":["nasa"]},{"id":"host_star:hd-128311","type":"host_star","name":"HD 128311","domain":"science","entryPath":"/exoplanets/hd-128311","description":"HD 128311 is a K0 star that hosts 2 known exoplanets in this catalogue, about 53 light-years away.","aliases":["K0"],"sources":["nasa"]},{"id":"host_star:hd-128717","type":"host_star","name":"HD 128717","domain":"science","entryPath":"/exoplanets/hd-128717","description":"HD 128717 is a star that hosts 1 known exoplanet in this catalogue, about 240 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:hd-134060","type":"host_star","name":"HD 134060","domain":"science","entryPath":"/exoplanets/hd-134060","description":"HD 134060 is a G3 IV star that hosts 2 known exoplanets in this catalogue, about 78 light-years away.","aliases":["G3 IV"],"sources":["nasa"]},{"id":"host_star:hd-134606","type":"host_star","name":"HD 134606","domain":"science","entryPath":"/exoplanets/hd-134606","description":"HD 134606 is a G5IV star that hosts 5 known exoplanets in this catalogue, about 87 light-years away.","aliases":["G5IV"],"sources":["nasa"]},{"id":"host_star:hd-134987","type":"host_star","name":"HD 134987","domain":"science","entryPath":"/exoplanets/hd-134987","description":"HD 134987 is a G5 V star that hosts 2 known exoplanets in this catalogue, about 85 light-years away.","aliases":["G5 V"],"sources":["nasa"]},{"id":"host_star:hd-135344-a-star","type":"host_star","name":"HD 135344 A","domain":"science","entryPath":"/exoplanets/hd-135344-a-star","description":"HD 135344 A is a A0 V star that hosts 1 known exoplanet in this catalogue, about 462 light-years away.","aliases":["A0 V"],"sources":["nasa"]},{"id":"host_star:hd-136352","type":"host_star","name":"HD 136352","domain":"science","entryPath":"/exoplanets/hd-136352","description":"HD 136352 is a G4 V star that hosts 3 known exoplanets in this catalogue, about 48 light-years away.","aliases":["G4 V"],"sources":["nasa"]},{"id":"host_star:hd-13808","type":"host_star","name":"HD 13808","domain":"science","entryPath":"/exoplanets/hd-13808","description":"HD 13808 is a K2 V star that hosts 2 known exoplanets in this catalogue, about 92 light-years away.","aliases":["K2 V"],"sources":["nasa"]},{"id":"host_star:hd-141399","type":"host_star","name":"HD 141399","domain":"science","entryPath":"/exoplanets/hd-141399","description":"HD 141399 is a K0 star that hosts 4 known exoplanets in this catalogue, about 121 light-years away.","aliases":["K0"],"sources":["nasa"]},{"id":"host_star:hd-142","type":"host_star","name":"HD 142","domain":"science","entryPath":"/exoplanets/hd-142","description":"HD 142 is a F7V star that hosts 3 known exoplanets in this catalogue, about 85 light-years away.","aliases":["F7V"],"sources":["nasa"]},{"id":"host_star:hd-143811-a-star","type":"host_star","name":"HD 143811 A","domain":"science","entryPath":"/exoplanets/hd-143811-a-star","description":"HD 143811 A is a star that hosts 1 known exoplanet in this catalogue, about 446 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:hd-1461","type":"host_star","name":"HD 1461","domain":"science","entryPath":"/exoplanets/hd-1461","description":"HD 1461 is a G0 V star that hosts 2 known exoplanets in this catalogue, about 76 light-years away.","aliases":["G0 V"],"sources":["nasa"]},{"id":"host_star:hd-147379","type":"host_star","name":"HD 147379","domain":"science","entryPath":"/exoplanets/hd-147379","description":"HD 147379 is a M0.0 V star that hosts 1 known exoplanet in this catalogue, about 35 light-years away.","aliases":["M0.0 V"],"sources":["nasa"]},{"id":"host_star:hd-153557","type":"host_star","name":"HD 153557","domain":"science","entryPath":"/exoplanets/hd-153557","description":"HD 153557 is a K0 star that hosts 3 known exoplanets in this catalogue, about 59 light-years away.","aliases":["K0"],"sources":["nasa"]},{"id":"host_star:hd-154345","type":"host_star","name":"HD 154345","domain":"science","entryPath":"/exoplanets/hd-154345","description":"HD 154345 is a G8 star that hosts 1 known exoplanet in this catalogue, about 60 light-years away.","aliases":["G8"],"sources":["nasa"]},{"id":"host_star:hd-156668","type":"host_star","name":"HD 156668","domain":"science","entryPath":"/exoplanets/hd-156668","description":"HD 156668 is a K2 star that hosts 2 known exoplanets in this catalogue, about 79 light-years away.","aliases":["K2"],"sources":["nasa"]},{"id":"host_star:hd-158259","type":"host_star","name":"HD 158259","domain":"science","entryPath":"/exoplanets/hd-158259","description":"HD 158259 is a G0 star that hosts 5 known exoplanets in this catalogue, about 88 light-years away.","aliases":["G0"],"sources":["nasa"]},{"id":"host_star:hd-164922","type":"host_star","name":"HD 164922","domain":"science","entryPath":"/exoplanets/hd-164922","description":"HD 164922 is a G9 V star that hosts 4 known exoplanets in this catalogue, about 72 light-years away.","aliases":["G9 V"],"sources":["nasa"]},{"id":"host_star:hd-169142","type":"host_star","name":"HD 169142","domain":"science","entryPath":"/exoplanets/hd-169142","description":"HD 169142 is a star that hosts 1 known exoplanet in this catalogue, about 371 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:hd-176986","type":"host_star","name":"HD 176986","domain":"science","entryPath":"/exoplanets/hd-176986","description":"HD 176986 is a K2.5 V star that hosts 3 known exoplanets in this catalogue, about 91 light-years away.","aliases":["K2.5 V"],"sources":["nasa"]},{"id":"host_star:hd-180617","type":"host_star","name":"HD 180617","domain":"science","entryPath":"/exoplanets/hd-180617","description":"HD 180617 is a M2.5 V star that hosts 1 known exoplanet in this catalogue, about 19 light-years away.","aliases":["M2.5 V"],"sources":["nasa"]},{"id":"host_star:hd-181433","type":"host_star","name":"HD 181433","domain":"science","entryPath":"/exoplanets/hd-181433","description":"HD 181433 is a K3 IV star that hosts 3 known exoplanets in this catalogue, about 88 light-years away.","aliases":["K3 IV"],"sources":["nasa"]},{"id":"host_star:hd-189567","type":"host_star","name":"HD 189567","domain":"science","entryPath":"/exoplanets/hd-189567","description":"HD 189567 is a G3 V star that hosts 2 known exoplanets in this catalogue, about 58 light-years away.","aliases":["G3 V"],"sources":["nasa"]},{"id":"host_star:hd-189733","type":"host_star","name":"HD 189733","domain":"science","entryPath":"/exoplanets/hd-189733","description":"HD 189733 is a K2 V star that hosts 1 known exoplanet in this catalogue, about 64 light-years away.","aliases":["K2 V"],"sources":["nasa"]},{"id":"host_star:hd-190007","type":"host_star","name":"HD 190007","domain":"science","entryPath":"/exoplanets/hd-190007","description":"HD 190007 is a K4 V star that hosts 1 known exoplanet in this catalogue, about 41 light-years away.","aliases":["K4 V"],"sources":["nasa"]},{"id":"host_star:hd-190360","type":"host_star","name":"HD 190360","domain":"science","entryPath":"/exoplanets/hd-190360","description":"HD 190360 is a G star that hosts 2 known exoplanets in this catalogue, about 52 light-years away.","aliases":["G"],"sources":["nasa"]},{"id":"host_star:hd-191939","type":"host_star","name":"HD 191939","domain":"science","entryPath":"/exoplanets/hd-191939","description":"HD 191939 is a G9 V star that hosts 6 known exoplanets in this catalogue, about 175 light-years away.","aliases":["G9 V"],"sources":["nasa"]},{"id":"host_star:hd-192263","type":"host_star","name":"HD 192263","domain":"science","entryPath":"/exoplanets/hd-192263","description":"HD 192263 is a K2 V star that hosts 1 known exoplanet in this catalogue, about 64 light-years away.","aliases":["K2 V"],"sources":["nasa"]},{"id":"host_star:hd-192310","type":"host_star","name":"HD 192310","domain":"science","entryPath":"/exoplanets/hd-192310","description":"HD 192310 is a K3V star that hosts 2 known exoplanets in this catalogue, about 29 light-years away.","aliases":["K3V"],"sources":["nasa"]},{"id":"host_star:hd-203030","type":"host_star","name":"HD 203030","domain":"science","entryPath":"/exoplanets/hd-203030","description":"HD 203030 is a G8 V star that hosts 1 known exoplanet in this catalogue, about 128 light-years away.","aliases":["G8 V"],"sources":["nasa"]},{"id":"host_star:hd-204941","type":"host_star","name":"HD 204941","domain":"science","entryPath":"/exoplanets/hd-204941","description":"HD 204941 is a K1/2V star that hosts 1 known exoplanet in this catalogue, about 94 light-years away.","aliases":["K1/2V"],"sources":["nasa"]},{"id":"host_star:hd-206893","type":"host_star","name":"HD 206893","domain":"science","entryPath":"/exoplanets/hd-206893","description":"HD 206893 is a F5 V star that hosts 2 known exoplanets in this catalogue, about 133 light-years away.","aliases":["F5 V"],"sources":["nasa"]},{"id":"host_star:hd-20781","type":"host_star","name":"HD 20781","domain":"science","entryPath":"/exoplanets/hd-20781","description":"HD 20781 is a K0 V star that hosts 4 known exoplanets in this catalogue, about 117 light-years away.","aliases":["K0 V"],"sources":["nasa"]},{"id":"host_star:hd-20782","type":"host_star","name":"HD 20782","domain":"science","entryPath":"/exoplanets/hd-20782","description":"HD 20782 is a G1.5 V star that hosts 1 known exoplanet in this catalogue, about 117 light-years away.","aliases":["G1.5 V"],"sources":["nasa"]},{"id":"host_star:hd-210277","type":"host_star","name":"HD 210277","domain":"science","entryPath":"/exoplanets/hd-210277","description":"HD 210277 is a G0 V star that hosts 1 known exoplanet in this catalogue, about 69 light-years away.","aliases":["G0 V"],"sources":["nasa"]},{"id":"host_star:hd-211970","type":"host_star","name":"HD 211970","domain":"science","entryPath":"/exoplanets/hd-211970","description":"HD 211970 is a K7 V star that hosts 1 known exoplanet in this catalogue, about 43 light-years away.","aliases":["K7 V"],"sources":["nasa"]},{"id":"host_star:hd-215152","type":"host_star","name":"HD 215152","domain":"science","entryPath":"/exoplanets/hd-215152","description":"HD 215152 is a K3 V star that hosts 4 known exoplanets in this catalogue, about 70 light-years away.","aliases":["K3 V"],"sources":["nasa"]},{"id":"host_star:hd-217107","type":"host_star","name":"HD 217107","domain":"science","entryPath":"/exoplanets/hd-217107","description":"HD 217107 is a G star that hosts 2 known exoplanets in this catalogue, about 65 light-years away.","aliases":["G"],"sources":["nasa"]},{"id":"host_star:hd-219077","type":"host_star","name":"HD 219077","domain":"science","entryPath":"/exoplanets/hd-219077","description":"HD 219077 is a G8 V+ star that hosts 1 known exoplanet in this catalogue, about 95 light-years away.","aliases":["G8 V+"],"sources":["nasa"]},{"id":"host_star:hd-219134","type":"host_star","name":"HD 219134","domain":"science","entryPath":"/exoplanets/hd-219134","description":"HD 219134 is a K3 V star that hosts 6 known exoplanets in this catalogue, about 21 light-years away.","aliases":["K3 V"],"sources":["nasa"]},{"id":"host_star:hd-222237","type":"host_star","name":"HD 222237","domain":"science","entryPath":"/exoplanets/hd-222237","description":"HD 222237 is a K3 V star that hosts 1 known exoplanet in this catalogue, about 37 light-years away.","aliases":["K3 V"],"sources":["nasa"]},{"id":"host_star:hd-22496","type":"host_star","name":"HD 22496","domain":"science","entryPath":"/exoplanets/hd-22496","description":"HD 22496 is a K5/M0V star that hosts 1 known exoplanet in this catalogue, about 44 light-years away.","aliases":["K5/M0V"],"sources":["nasa"]},{"id":"host_star:hd-260655","type":"host_star","name":"HD 260655","domain":"science","entryPath":"/exoplanets/hd-260655","description":"HD 260655 is a M0 V star that hosts 2 known exoplanets in this catalogue, about 33 light-years away.","aliases":["M0 V"],"sources":["nasa"]},{"id":"host_star:hd-27894","type":"host_star","name":"HD 27894","domain":"science","entryPath":"/exoplanets/hd-27894","description":"HD 27894 is a K2 V star that hosts 3 known exoplanets in this catalogue, about 143 light-years away.","aliases":["K2 V"],"sources":["nasa"]},{"id":"host_star:hd-284149-a-star","type":"host_star","name":"HD 284149 A","domain":"science","entryPath":"/exoplanets/hd-284149-a-star","description":"HD 284149 A is a star that hosts 1 known exoplanet in this catalogue, about 384 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:hd-285968","type":"host_star","name":"HD 285968","domain":"science","entryPath":"/exoplanets/hd-285968","description":"HD 285968 is a M2 V star that hosts 1 known exoplanet in this catalogue, about 31 light-years away.","aliases":["M2 V"],"sources":["nasa"]},{"id":"host_star:hd-33142","type":"host_star","name":"HD 33142","domain":"science","entryPath":"/exoplanets/hd-33142","description":"HD 33142 is a K0 III star that hosts 3 known exoplanets in this catalogue, about 396 light-years away.","aliases":["K0 III"],"sources":["nasa"]},{"id":"host_star:hd-34445","type":"host_star","name":"HD 34445","domain":"science","entryPath":"/exoplanets/hd-34445","description":"HD 34445 is a G0 V star that hosts 6 known exoplanets in this catalogue, about 150 light-years away.","aliases":["G0 V"],"sources":["nasa"]},{"id":"host_star:hd-3651","type":"host_star","name":"HD 3651","domain":"science","entryPath":"/exoplanets/hd-3651","description":"HD 3651 is a K0 V star that hosts 1 known exoplanet in this catalogue, about 36 light-years away.","aliases":["K0 V"],"sources":["nasa"]},{"id":"host_star:hd-37124","type":"host_star","name":"HD 37124","domain":"science","entryPath":"/exoplanets/hd-37124","description":"HD 37124 is a G4 V star that hosts 3 known exoplanets in this catalogue, about 103 light-years away.","aliases":["G4 V"],"sources":["nasa"]},{"id":"host_star:hd-39091","type":"host_star","name":"HD 39091","domain":"science","entryPath":"/exoplanets/hd-39091","description":"HD 39091 is a G0 V star that hosts 3 known exoplanets in this catalogue, about 60 light-years away.","aliases":["G0 V"],"sources":["nasa"]},{"id":"host_star:hd-39194","type":"host_star","name":"HD 39194","domain":"science","entryPath":"/exoplanets/hd-39194","description":"HD 39194 is a K0 V star that hosts 3 known exoplanets in this catalogue, about 86 light-years away.","aliases":["K0 V"],"sources":["nasa"]},{"id":"host_star:hd-40307","type":"host_star","name":"HD 40307","domain":"science","entryPath":"/exoplanets/hd-40307","description":"HD 40307 is a K2.5 V star that hosts 5 known exoplanets in this catalogue, about 42 light-years away.","aliases":["K2.5 V"],"sources":["nasa"]},{"id":"host_star:hd-4308","type":"host_star","name":"HD 4308","domain":"science","entryPath":"/exoplanets/hd-4308","description":"HD 4308 is a G5V star that hosts 1 known exoplanet in this catalogue, about 72 light-years away.","aliases":["G5V"],"sources":["nasa"]},{"id":"host_star:hd-45184","type":"host_star","name":"HD 45184","domain":"science","entryPath":"/exoplanets/hd-45184","description":"HD 45184 is a G1.5 V star that hosts 2 known exoplanets in this catalogue, about 72 light-years away.","aliases":["G1.5 V"],"sources":["nasa"]},{"id":"host_star:hd-46375","type":"host_star","name":"HD 46375","domain":"science","entryPath":"/exoplanets/hd-46375","description":"HD 46375 is a K1 IV-V star that hosts 1 known exoplanet in this catalogue, about 96 light-years away.","aliases":["K1 IV-V"],"sources":["nasa"]},{"id":"host_star:hd-48948","type":"host_star","name":"HD 48948","domain":"science","entryPath":"/exoplanets/hd-48948","description":"HD 48948 is a K3 V star that hosts 3 known exoplanets in this catalogue, about 55 light-years away.","aliases":["K3 V"],"sources":["nasa"]},{"id":"host_star:hd-62509","type":"host_star","name":"HD 62509","domain":"science","entryPath":"/exoplanets/hd-62509","description":"HD 62509 is a K0IIIvar star that hosts 1 known exoplanet in this catalogue, about 34 light-years away.","aliases":["K0IIIvar"],"sources":["nasa"]},{"id":"host_star:hd-63433","type":"host_star","name":"HD 63433","domain":"science","entryPath":"/exoplanets/hd-63433","description":"HD 63433 is a G5 V star that hosts 3 known exoplanets in this catalogue, about 73 light-years away.","aliases":["G5 V"],"sources":["nasa"]},{"id":"host_star:hd-69830","type":"host_star","name":"HD 69830","domain":"science","entryPath":"/exoplanets/hd-69830","description":"HD 69830 is a K0V star that hosts 3 known exoplanets in this catalogue, about 41 light-years away.","aliases":["K0V"],"sources":["nasa"]},{"id":"host_star:hd-75289","type":"host_star","name":"HD 75289","domain":"science","entryPath":"/exoplanets/hd-75289","description":"HD 75289 is a G0 star that hosts 1 known exoplanet in this catalogue, about 95 light-years away.","aliases":["G0"],"sources":["nasa"]},{"id":"host_star:hd-7924","type":"host_star","name":"HD 7924","domain":"science","entryPath":"/exoplanets/hd-7924","description":"HD 7924 is a K0.5 V star that hosts 3 known exoplanets in this catalogue, about 55 light-years away.","aliases":["K0.5 V"],"sources":["nasa"]},{"id":"host_star:hd-82943","type":"host_star","name":"HD 82943","domain":"science","entryPath":"/exoplanets/hd-82943","description":"HD 82943 is a G2/3V star that hosts 2 known exoplanets in this catalogue, about 90 light-years away.","aliases":["G2/3V"],"sources":["nasa"]},{"id":"host_star:hd-90156","type":"host_star","name":"HD 90156","domain":"science","entryPath":"/exoplanets/hd-90156","description":"HD 90156 is a G5V star that hosts 1 known exoplanet in this catalogue, about 72 light-years away.","aliases":["G5V"],"sources":["nasa"]},{"id":"host_star:hd-96700","type":"host_star","name":"HD 96700","domain":"science","entryPath":"/exoplanets/hd-96700","description":"HD 96700 is a G0 V star that hosts 3 known exoplanets in this catalogue, about 83 light-years away.","aliases":["G0 V"],"sources":["nasa"]},{"id":"host_star:hd-97658","type":"host_star","name":"HD 97658","domain":"science","entryPath":"/exoplanets/hd-97658","description":"HD 97658 is a K1 V star that hosts 1 known exoplanet in this catalogue, about 70 light-years away.","aliases":["K1 V"],"sources":["nasa"]},{"id":"host_star:hd-99492","type":"host_star","name":"HD 99492","domain":"science","entryPath":"/exoplanets/hd-99492","description":"HD 99492 is a K2 V star that hosts 2 known exoplanets in this catalogue, about 59 light-years away.","aliases":["K2 V"],"sources":["nasa"]},{"id":"host_star:hip-14810","type":"host_star","name":"HIP 14810","domain":"science","entryPath":"/exoplanets/hip-14810","description":"HIP 14810 is a G5 star that hosts 3 known exoplanets in this catalogue, about 165 light-years away.","aliases":["G5"],"sources":["nasa"]},{"id":"host_star:hip-21152","type":"host_star","name":"HIP 21152","domain":"science","entryPath":"/exoplanets/hip-21152","description":"HIP 21152 is a F5 V star that hosts 1 known exoplanet in this catalogue, about 142 light-years away.","aliases":["F5 V"],"sources":["nasa"]},{"id":"host_star:hip-39017","type":"host_star","name":"HIP 39017","domain":"science","entryPath":"/exoplanets/hip-39017","description":"HIP 39017 is a A9/F0 star that hosts 1 known exoplanet in this catalogue, about 216 light-years away.","aliases":["A9/F0"],"sources":["nasa"]},{"id":"host_star:hip-41378","type":"host_star","name":"HIP 41378","domain":"science","entryPath":"/exoplanets/hip-41378","description":"HIP 41378 is a F6 star that hosts 6 known exoplanets in this catalogue, about 347 light-years away.","aliases":["F6"],"sources":["nasa"]},{"id":"host_star:hip-48714","type":"host_star","name":"HIP 48714","domain":"science","entryPath":"/exoplanets/hip-48714","description":"HIP 48714 is a M0.5 Ve star that hosts 1 known exoplanet in this catalogue, about 34 light-years away.","aliases":["M0.5 Ve"],"sources":["nasa"]},{"id":"host_star:hip-54515","type":"host_star","name":"HIP 54515","domain":"science","entryPath":"/exoplanets/hip-54515","description":"HIP 54515 is a A5 V star that hosts 1 known exoplanet in this catalogue, about 270 light-years away.","aliases":["A5 V"],"sources":["nasa"]},{"id":"host_star:hip-56998","type":"host_star","name":"HIP 56998","domain":"science","entryPath":"/exoplanets/hip-56998","description":"HIP 56998 is a K4/5V star that hosts 2 known exoplanets in this catalogue, about 42 light-years away.","aliases":["K4/5V"],"sources":["nasa"]},{"id":"host_star:hip-57274","type":"host_star","name":"HIP 57274","domain":"science","entryPath":"/exoplanets/hip-57274","description":"HIP 57274 is a K4 V star that hosts 3 known exoplanets in this catalogue, about 84 light-years away.","aliases":["K4 V"],"sources":["nasa"]},{"id":"host_star:hip-66074","type":"host_star","name":"HIP 66074","domain":"science","entryPath":"/exoplanets/hip-66074","description":"HIP 66074 is a star that hosts 1 known exoplanet in this catalogue, about 116 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:hip-70849","type":"host_star","name":"HIP 70849","domain":"science","entryPath":"/exoplanets/hip-70849","description":"HIP 70849 is a K7 V star that hosts 1 known exoplanet in this catalogue, about 78 light-years away.","aliases":["K7 V"],"sources":["nasa"]},{"id":"host_star:hip-77900","type":"host_star","name":"HIP 77900","domain":"science","entryPath":"/exoplanets/hip-77900","description":"HIP 77900 is a star that hosts 1 known exoplanet in this catalogue, about 492 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:hip-78530","type":"host_star","name":"HIP 78530","domain":"science","entryPath":"/exoplanets/hip-78530","description":"HIP 78530 is a B9 V star that hosts 1 known exoplanet in this catalogue, about 446 light-years away.","aliases":["B9 V"],"sources":["nasa"]},{"id":"host_star:hip-79098-ab","type":"host_star","name":"HIP 79098 AB","domain":"science","entryPath":"/exoplanets/hip-79098-ab","description":"HIP 79098 AB is a B9 V star that hosts 1 known exoplanet in this catalogue, about 476 light-years away.","aliases":["B9 V"],"sources":["nasa"]},{"id":"host_star:hip-81208-c-star","type":"host_star","name":"HIP 81208 C","domain":"science","entryPath":"/exoplanets/hip-81208-c-star","description":"HIP 81208 C is a M star that hosts 1 known exoplanet in this catalogue, about 481 light-years away.","aliases":["M"],"sources":["nasa"]},{"id":"host_star:hn-lib","type":"host_star","name":"HN Lib","domain":"science","entryPath":"/exoplanets/hn-lib","description":"HN Lib is a M4.0 V star that hosts 1 known exoplanet in this catalogue, about 20 light-years away.","aliases":["M4.0 V"],"sources":["nasa"]},{"id":"host_star:hn-peg","type":"host_star","name":"HN Peg","domain":"science","entryPath":"/exoplanets/hn-peg","description":"HN Peg is a G0 V star that hosts 1 known exoplanet in this catalogue, about 59 light-years away.","aliases":["G0 V"],"sources":["nasa"]},{"id":"host_star:hr-2562","type":"host_star","name":"HR 2562","domain":"science","entryPath":"/exoplanets/hr-2562","description":"HR 2562 is a F5 V star that hosts 1 known exoplanet in this catalogue, about 111 light-years away.","aliases":["F5 V"],"sources":["nasa"]},{"id":"host_star:hr-8799","type":"host_star","name":"HR 8799","domain":"science","entryPath":"/exoplanets/hr-8799","description":"HR 8799 is a A5 V star that hosts 4 known exoplanets in this catalogue, about 135 light-years away.","aliases":["A5 V"],"sources":["nasa"]},{"id":"host_star:iso-oph-96","type":"host_star","name":"ISO-Oph 96","domain":"science","entryPath":"/exoplanets/iso-oph-96","description":"ISO-Oph 96 is a K6-M1 star that hosts 1 known exoplanet in this catalogue, about 459 light-years away.","aliases":["K6-M1"],"sources":["nasa"]},{"id":"host_star:itg-15-a-star","type":"host_star","name":"ITG 15 A","domain":"science","entryPath":"/exoplanets/itg-15-a-star","description":"ITG 15 A is a star that hosts 1 known exoplanet in this catalogue, about 445 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:k2-18","type":"host_star","name":"K2-18","domain":"science","entryPath":"/exoplanets/k2-18","description":"K2-18 is a M2.5 V star that hosts 2 known exoplanets in this catalogue, about 124 light-years away.","aliases":["M2.5 V"],"sources":["nasa"]},{"id":"host_star:kap-and","type":"host_star","name":"kap And","domain":"science","entryPath":"/exoplanets/kap-and","description":"kap And is a B9 IVn star that hosts 1 known exoplanet in this catalogue, about 163 light-years away.","aliases":["B9 IVn"],"sources":["nasa"]},{"id":"host_star:kapteyn","type":"host_star","name":"Kapteyn","domain":"science","entryPath":"/exoplanets/kapteyn","description":"Kapteyn is a M2.0V star that hosts 1 known exoplanet in this catalogue, about 13 light-years away.","aliases":["M2.0V"],"sources":["nasa"]},{"id":"host_star:kelt-9","type":"host_star","name":"KELT-9","domain":"science","entryPath":"/exoplanets/kelt-9","description":"KELT-9 is a B9.5-A0 star that hosts 1 known exoplanet in this catalogue, about 667 light-years away.","aliases":["B9.5-A0"],"sources":["nasa"]},{"id":"host_star:kepler-100","type":"host_star","name":"Kepler-100","domain":"science","entryPath":"/exoplanets/kepler-100","description":"Kepler-100 is a star that hosts 4 known exoplanets in this catalogue, about 994 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-11","type":"host_star","name":"Kepler-11","domain":"science","entryPath":"/exoplanets/kepler-11","description":"Kepler-11 is a star that hosts 6 known exoplanets in this catalogue, about 2108 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-122","type":"host_star","name":"Kepler-122","domain":"science","entryPath":"/exoplanets/kepler-122","description":"Kepler-122 is a star that hosts 5 known exoplanets in this catalogue, about 3352 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-138","type":"host_star","name":"Kepler-138","domain":"science","entryPath":"/exoplanets/kepler-138","description":"Kepler-138 is a M1 V star that hosts 4 known exoplanets in this catalogue, about 218 light-years away.","aliases":["M1 V"],"sources":["nasa"]},{"id":"host_star:kepler-139","type":"host_star","name":"Kepler-139","domain":"science","entryPath":"/exoplanets/kepler-139","description":"Kepler-139 is a star that hosts 5 known exoplanets in this catalogue, about 1276 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-16","type":"host_star","name":"Kepler-16","domain":"science","entryPath":"/exoplanets/kepler-16","description":"Kepler-16 is a star that hosts 1 known exoplanet in this catalogue, about 245 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-1649","type":"host_star","name":"Kepler-1649","domain":"science","entryPath":"/exoplanets/kepler-1649","description":"Kepler-1649 is a star that hosts 2 known exoplanets in this catalogue, about 301 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-1660-a-star","type":"host_star","name":"Kepler-1660 A","domain":"science","entryPath":"/exoplanets/kepler-1660-a-star","description":"Kepler-1660 A is a F7 V star that hosts 1 known exoplanet in this catalogue, about 3877 light-years away.","aliases":["F7 V"],"sources":["nasa"]},{"id":"host_star:kepler-19","type":"host_star","name":"Kepler-19","domain":"science","entryPath":"/exoplanets/kepler-19","description":"Kepler-19 is a star that hosts 3 known exoplanets in this catalogue, about 713 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-20","type":"host_star","name":"Kepler-20","domain":"science","entryPath":"/exoplanets/kepler-20","description":"Kepler-20 is a star that hosts 6 known exoplanets in this catalogue, about 922 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-24","type":"host_star","name":"Kepler-24","domain":"science","entryPath":"/exoplanets/kepler-24","description":"Kepler-24 is a star that hosts 4 known exoplanets in this catalogue, about 3774 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-26","type":"host_star","name":"Kepler-26","domain":"science","entryPath":"/exoplanets/kepler-26","description":"Kepler-26 is a M0 V star that hosts 4 known exoplanets in this catalogue, about 1094 light-years away.","aliases":["M0 V"],"sources":["nasa"]},{"id":"host_star:kepler-32","type":"host_star","name":"Kepler-32","domain":"science","entryPath":"/exoplanets/kepler-32","description":"Kepler-32 is a M1 V star that hosts 5 known exoplanets in this catalogue, about 1056 light-years away.","aliases":["M1 V"],"sources":["nasa"]},{"id":"host_star:kepler-33","type":"host_star","name":"Kepler-33","domain":"science","entryPath":"/exoplanets/kepler-33","description":"Kepler-33 is a star that hosts 5 known exoplanets in this catalogue, about 3944 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-338","type":"host_star","name":"Kepler-338","domain":"science","entryPath":"/exoplanets/kepler-338","description":"Kepler-338 is a star that hosts 4 known exoplanets in this catalogue, about 1803 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-37","type":"host_star","name":"Kepler-37","domain":"science","entryPath":"/exoplanets/kepler-37","description":"Kepler-37 is a star that hosts 4 known exoplanets in this catalogue, about 209 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-411","type":"host_star","name":"Kepler-411","domain":"science","entryPath":"/exoplanets/kepler-411","description":"Kepler-411 is a K2 V star that hosts 4 known exoplanets in this catalogue, about 501 light-years away.","aliases":["K2 V"],"sources":["nasa"]},{"id":"host_star:kepler-416","type":"host_star","name":"Kepler-416","domain":"science","entryPath":"/exoplanets/kepler-416","description":"Kepler-416 is a star that hosts 3 known exoplanets in this catalogue, about 2253 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-442","type":"host_star","name":"Kepler-442","domain":"science","entryPath":"/exoplanets/kepler-442","description":"Kepler-442 is a star that hosts 1 known exoplanet in this catalogue, about 1194 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-452","type":"host_star","name":"Kepler-452","domain":"science","entryPath":"/exoplanets/kepler-452","description":"Kepler-452 is a G2 star that hosts 1 known exoplanet in this catalogue, about 1800 light-years away.","aliases":["G2"],"sources":["nasa"]},{"id":"host_star:kepler-46","type":"host_star","name":"Kepler-46","domain":"science","entryPath":"/exoplanets/kepler-46","description":"Kepler-46 is a star that hosts 3 known exoplanets in this catalogue, about 2535 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-48","type":"host_star","name":"Kepler-48","domain":"science","entryPath":"/exoplanets/kepler-48","description":"Kepler-48 is a star that hosts 5 known exoplanets in this catalogue, about 1001 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-49","type":"host_star","name":"Kepler-49","domain":"science","entryPath":"/exoplanets/kepler-49","description":"Kepler-49 is a M1 V star that hosts 4 known exoplanets in this catalogue, about 1015 light-years away.","aliases":["M1 V"],"sources":["nasa"]},{"id":"host_star:kepler-51","type":"host_star","name":"Kepler-51","domain":"science","entryPath":"/exoplanets/kepler-51","description":"Kepler-51 is a star that hosts 4 known exoplanets in this catalogue, about 2557 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-55","type":"host_star","name":"Kepler-55","domain":"science","entryPath":"/exoplanets/kepler-55","description":"Kepler-55 is a star that hosts 5 known exoplanets in this catalogue, about 1888 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-58","type":"host_star","name":"Kepler-58","domain":"science","entryPath":"/exoplanets/kepler-58","description":"Kepler-58 is a star that hosts 4 known exoplanets in this catalogue, about 3162 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-65","type":"host_star","name":"Kepler-65","domain":"science","entryPath":"/exoplanets/kepler-65","description":"Kepler-65 is a star that hosts 4 known exoplanets in this catalogue, about 991 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-68","type":"host_star","name":"Kepler-68","domain":"science","entryPath":"/exoplanets/kepler-68","description":"Kepler-68 is a star that hosts 4 known exoplanets in this catalogue, about 470 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-79","type":"host_star","name":"Kepler-79","domain":"science","entryPath":"/exoplanets/kepler-79","description":"Kepler-79 is a star that hosts 4 known exoplanets in this catalogue, about 3330 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-80","type":"host_star","name":"Kepler-80","domain":"science","entryPath":"/exoplanets/kepler-80","description":"Kepler-80 is a K5 star that hosts 6 known exoplanets in this catalogue, about 1205 light-years away.","aliases":["K5"],"sources":["nasa"]},{"id":"host_star:kepler-82","type":"host_star","name":"Kepler-82","domain":"science","entryPath":"/exoplanets/kepler-82","description":"Kepler-82 is a star that hosts 5 known exoplanets in this catalogue, about 2950 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-84","type":"host_star","name":"Kepler-84","domain":"science","entryPath":"/exoplanets/kepler-84","description":"Kepler-84 is a star that hosts 5 known exoplanets in this catalogue, about 3340 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:kepler-85","type":"host_star","name":"Kepler-85","domain":"science","entryPath":"/exoplanets/kepler-85","description":"Kepler-85 is a star that hosts 4 known exoplanets in this catalogue, about 2496 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:koi-142","type":"host_star","name":"KOI-142","domain":"science","entryPath":"/exoplanets/koi-142","description":"KOI-142 is a G6 V star that hosts 3 known exoplanets in this catalogue, about 1229 light-years away.","aliases":["G6 V"],"sources":["nasa"]},{"id":"host_star:l-363-38","type":"host_star","name":"L 363-38","domain":"science","entryPath":"/exoplanets/l-363-38","description":"L 363-38 is a star that hosts 1 known exoplanet in this catalogue, about 33 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:l-98-59","type":"host_star","name":"L 98-59","domain":"science","entryPath":"/exoplanets/l-98-59","description":"L 98-59 is a M3 V star that hosts 5 known exoplanets in this catalogue, about 35 light-years away.","aliases":["M3 V"],"sources":["nasa"]},{"id":"host_star:lhs-1140","type":"host_star","name":"LHS 1140","domain":"science","entryPath":"/exoplanets/lhs-1140","description":"LHS 1140 is a M4.5 V star that hosts 2 known exoplanets in this catalogue, about 49 light-years away.","aliases":["M4.5 V"],"sources":["nasa"]},{"id":"host_star:lhs-1678","type":"host_star","name":"LHS 1678","domain":"science","entryPath":"/exoplanets/lhs-1678","description":"LHS 1678 is a M2.0 V star that hosts 3 known exoplanets in this catalogue, about 65 light-years away.","aliases":["M2.0 V"],"sources":["nasa"]},{"id":"host_star:lhs-3844","type":"host_star","name":"LHS 3844","domain":"science","entryPath":"/exoplanets/lhs-3844","description":"LHS 3844 is a M4.5-M5.0 star that hosts 1 known exoplanet in this catalogue, about 49 light-years away.","aliases":["M4.5-M5.0"],"sources":["nasa"]},{"id":"host_star:lhs-475","type":"host_star","name":"LHS 475","domain":"science","entryPath":"/exoplanets/lhs-475","description":"LHS 475 is a M3.5 V star that hosts 1 known exoplanet in this catalogue, about 41 light-years away.","aliases":["M3.5 V"],"sources":["nasa"]},{"id":"host_star:lkca-15","type":"host_star","name":"LkCa 15","domain":"science","entryPath":"/exoplanets/lkca-15","description":"LkCa 15 is a star that hosts 2 known exoplanets in this catalogue, about 516 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:lp-261-75-a-star","type":"host_star","name":"LP 261-75 A","domain":"science","entryPath":"/exoplanets/lp-261-75-a-star","description":"LP 261-75 A is a M4.5 V star that hosts 1 known exoplanet in this catalogue, about 111 light-years away.","aliases":["M4.5 V"],"sources":["nasa"]},{"id":"host_star:lp-791-18","type":"host_star","name":"LP 791-18","domain":"science","entryPath":"/exoplanets/lp-791-18","description":"LP 791-18 is a M(6.1 +/- 0.7) V star that hosts 3 known exoplanets in this catalogue, about 86 light-years away.","aliases":["M(6.1 +/- 0.7) V"],"sources":["nasa"]},{"id":"host_star:lp-890-9","type":"host_star","name":"LP 890-9","domain":"science","entryPath":"/exoplanets/lp-890-9","description":"LP 890-9 is a M6 V star that hosts 2 known exoplanets in this catalogue, about 106 light-years away.","aliases":["M6 V"],"sources":["nasa"]},{"id":"host_star:ltt-1445-a-star","type":"host_star","name":"LTT 1445 A","domain":"science","entryPath":"/exoplanets/ltt-1445-a-star","description":"LTT 1445 A is a M3.0 star that hosts 2 known exoplanets in this catalogue, about 22 light-years away.","aliases":["M3.0"],"sources":["nasa"]},{"id":"host_star:luhman-16-a-star","type":"host_star","name":"Luhman 16 A","domain":"science","entryPath":"/exoplanets/luhman-16-a-star","description":"Luhman 16 A is a star that hosts 1 known exoplanet in this catalogue.","aliases":[],"sources":["nasa"]},{"id":"host_star:m62h","type":"host_star","name":"M62H","domain":"science","entryPath":"/exoplanets/m62h","description":"M62H is a star that hosts 1 known exoplanet in this catalogue.","aliases":[],"sources":["nasa"]},{"id":"host_star:moa-2007-blg-192l","type":"host_star","name":"MOA-2007-BLG-192L","domain":"science","entryPath":"/exoplanets/moa-2007-blg-192l","description":"MOA-2007-BLG-192L is a star that hosts 1 known exoplanet in this catalogue, about 7046 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:mu2-sco","type":"host_star","name":"mu2 Sco","domain":"science","entryPath":"/exoplanets/mu2-sco","description":"mu2 Sco is a B2 IV star that hosts 1 known exoplanet in this catalogue.","aliases":["B2 IV"],"sources":["nasa"]},{"id":"host_star:mwc-758","type":"host_star","name":"MWC 758","domain":"science","entryPath":"/exoplanets/mwc-758","description":"MWC 758 is a A8Ve star that hosts 1 known exoplanet in this catalogue, about 520 light-years away.","aliases":["A8Ve"],"sources":["nasa"]},{"id":"host_star:nn-ser","type":"host_star","name":"NN Ser","domain":"science","entryPath":"/exoplanets/nn-ser","description":"NN Ser is a WD star that hosts 2 known exoplanets in this catalogue, about 1683 light-years away.","aliases":["WD"],"sources":["nasa"]},{"id":"host_star:ny-vir","type":"host_star","name":"NY Vir","domain":"science","entryPath":"/exoplanets/ny-vir","description":"NY Vir is a star that hosts 2 known exoplanets in this catalogue, about 1775 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:ogle-2005-blg-071l","type":"host_star","name":"OGLE-2005-BLG-071L","domain":"science","entryPath":"/exoplanets/ogle-2005-blg-071l","description":"OGLE-2005-BLG-071L is a star that hosts 1 known exoplanet in this catalogue, about 10438 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:ogle-2005-blg-390l","type":"host_star","name":"OGLE-2005-BLG-390L","domain":"science","entryPath":"/exoplanets/ogle-2005-blg-390l","description":"OGLE-2005-BLG-390L is a star that hosts 1 known exoplanet in this catalogue, about 21529 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:ogle-2006-blg-109l","type":"host_star","name":"OGLE-2006-BLG-109L","domain":"science","entryPath":"/exoplanets/ogle-2006-blg-109l","description":"OGLE-2006-BLG-109L is a star that hosts 2 known exoplanets in this catalogue, about 4926 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:ogle-2007-blg-368l","type":"host_star","name":"OGLE-2007-BLG-368L","domain":"science","entryPath":"/exoplanets/ogle-2007-blg-368l","description":"OGLE-2007-BLG-368L is a star that hosts 1 known exoplanet in this catalogue, about 19246 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:ogle-2012-blg-0026l","type":"host_star","name":"OGLE-2012-BLG-0026L","domain":"science","entryPath":"/exoplanets/ogle-2012-blg-0026l","description":"OGLE-2012-BLG-0026L is a G5 V star that hosts 2 known exoplanets in this catalogue, about 13110 light-years away.","aliases":["G5 V"],"sources":["nasa"]},{"id":"host_star:oph-11","type":"host_star","name":"Oph 11","domain":"science","entryPath":"/exoplanets/oph-11","description":"Oph 11 is a M9 star that hosts 1 known exoplanet in this catalogue, about 444 light-years away.","aliases":["M9"],"sources":["nasa"]},{"id":"host_star:pds-70","type":"host_star","name":"PDS 70","domain":"science","entryPath":"/exoplanets/pds-70","description":"PDS 70 is a K7 star that hosts 2 known exoplanets in this catalogue, about 369 light-years away.","aliases":["K7"],"sources":["nasa"]},{"id":"host_star:psr-b0329-54","type":"host_star","name":"PSR B0329+54","domain":"science","entryPath":"/exoplanets/psr-b0329-54","description":"PSR B0329+54 is a star that hosts 1 known exoplanet in this catalogue, about 1647 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:psr-b1257-12","type":"host_star","name":"PSR B1257+12","domain":"science","entryPath":"/exoplanets/psr-b1257-12","description":"PSR B1257+12 is a star that hosts 3 known exoplanets in this catalogue, about 1957 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:psr-b1620-26","type":"host_star","name":"PSR B1620-26","domain":"science","entryPath":"/exoplanets/psr-b1620-26","description":"PSR B1620-26 is a star that hosts 1 known exoplanet in this catalogue.","aliases":[],"sources":["nasa"]},{"id":"host_star:psr-j1719-1438","type":"host_star","name":"PSR J1719-1438","domain":"science","entryPath":"/exoplanets/psr-j1719-1438","description":"PSR J1719-1438 is a star that hosts 1 known exoplanet in this catalogue, about 3914 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:psr-j2322-2650","type":"host_star","name":"PSR J2322-2650","domain":"science","entryPath":"/exoplanets/psr-j2322-2650","description":"PSR J2322-2650 is a star that hosts 1 known exoplanet in this catalogue, about 750 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:pz-tel","type":"host_star","name":"PZ Tel","domain":"science","entryPath":"/exoplanets/pz-tel","description":"PZ Tel is a G9 IV star that hosts 1 known exoplanet in this catalogue, about 154 light-years away.","aliases":["G9 IV"],"sources":["nasa"]},{"id":"host_star:ross-458","type":"host_star","name":"Ross 458","domain":"science","entryPath":"/exoplanets/ross-458","description":"Ross 458 is a M2 star that hosts 1 known exoplanet in this catalogue, about 38 light-years away.","aliases":["M2"],"sources":["nasa"]},{"id":"host_star:ross-508","type":"host_star","name":"Ross 508","domain":"science","entryPath":"/exoplanets/ross-508","description":"Ross 508 is a M4.5 V star that hosts 1 known exoplanet in this catalogue, about 37 light-years away.","aliases":["M4.5 V"],"sources":["nasa"]},{"id":"host_star:roxs-12","type":"host_star","name":"ROXs 12","domain":"science","entryPath":"/exoplanets/roxs-12","description":"ROXs 12 is a M0 star that hosts 1 known exoplanet in this catalogue, about 446 light-years away.","aliases":["M0"],"sources":["nasa"]},{"id":"host_star:roxs-42-b-star","type":"host_star","name":"ROXs 42 B","domain":"science","entryPath":"/exoplanets/roxs-42-b-star","description":"ROXs 42 B is a M0 star that hosts 1 known exoplanet in this catalogue, about 468 light-years away.","aliases":["M0"],"sources":["nasa"]},{"id":"host_star:rr-cae","type":"host_star","name":"RR Cae","domain":"science","entryPath":"/exoplanets/rr-cae","description":"RR Cae is a M star that hosts 1 known exoplanet in this catalogue, about 69 light-years away.","aliases":["M"],"sources":["nasa"]},{"id":"host_star:sr-12-ab","type":"host_star","name":"SR 12 AB","domain":"science","entryPath":"/exoplanets/sr-12-ab","description":"SR 12 AB is a star that hosts 1 known exoplanet in this catalogue, about 366 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:teegarden-s-star","type":"host_star","name":"Teegarden's Star","domain":"science","entryPath":"/exoplanets/teegarden-s-star","description":"Teegarden's Star is a M7.0 V star that hosts 3 known exoplanets in this catalogue, about 12 light-years away.","aliases":["M7.0 V"],"sources":["nasa"]},{"id":"host_star:toi-1203","type":"host_star","name":"TOI-1203","domain":"science","entryPath":"/exoplanets/toi-1203","description":"TOI-1203 is a G3 V star that hosts 4 known exoplanets in this catalogue, about 212 light-years away.","aliases":["G3 V"],"sources":["nasa"]},{"id":"host_star:toi-1266","type":"host_star","name":"TOI-1266","domain":"science","entryPath":"/exoplanets/toi-1266","description":"TOI-1266 is a M2 star that hosts 3 known exoplanets in this catalogue, about 117 light-years away.","aliases":["M2"],"sources":["nasa"]},{"id":"host_star:toi-201","type":"host_star","name":"TOI-201","domain":"science","entryPath":"/exoplanets/toi-201","description":"TOI-201 is a F star that hosts 3 known exoplanets in this catalogue, about 371 light-years away.","aliases":["F"],"sources":["nasa"]},{"id":"host_star:toi-2267-a-star","type":"host_star","name":"TOI-2267 A","domain":"science","entryPath":"/exoplanets/toi-2267-a-star","description":"TOI-2267 A is a M5 V star that hosts 2 known exoplanets in this catalogue, about 74 light-years away.","aliases":["M5 V"],"sources":["nasa"]},{"id":"host_star:toi-2267-b-star","type":"host_star","name":"TOI-2267 B","domain":"science","entryPath":"/exoplanets/toi-2267-b-star","description":"TOI-2267 B is a M6 V star that hosts 1 known exoplanet in this catalogue, about 74 light-years away.","aliases":["M6 V"],"sources":["nasa"]},{"id":"host_star:toi-270","type":"host_star","name":"TOI-270","domain":"science","entryPath":"/exoplanets/toi-270","description":"TOI-270 is a M3 V star that hosts 3 known exoplanets in this catalogue, about 73 light-years away.","aliases":["M3 V"],"sources":["nasa"]},{"id":"host_star:toi-4010","type":"host_star","name":"TOI-4010","domain":"science","entryPath":"/exoplanets/toi-4010","description":"TOI-4010 is a K V star that hosts 4 known exoplanets in this catalogue, about 579 light-years away.","aliases":["K V"],"sources":["nasa"]},{"id":"host_star:toi-540","type":"host_star","name":"TOI-540","domain":"science","entryPath":"/exoplanets/toi-540","description":"TOI-540 is a M V star that hosts 1 known exoplanet in this catalogue, about 46 light-years away.","aliases":["M V"],"sources":["nasa"]},{"id":"host_star:toi-5624","type":"host_star","name":"TOI-5624","domain":"science","entryPath":"/exoplanets/toi-5624","description":"TOI-5624 is a star that hosts 5 known exoplanets in this catalogue, about 332 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:toi-5789","type":"host_star","name":"TOI-5789","domain":"science","entryPath":"/exoplanets/toi-5789","description":"TOI-5789 is a K1 V star that hosts 4 known exoplanets in this catalogue, about 67 light-years away.","aliases":["K1 V"],"sources":["nasa"]},{"id":"host_star:toi-700","type":"host_star","name":"TOI-700","domain":"science","entryPath":"/exoplanets/toi-700","description":"TOI-700 is a M2.5 V star that hosts 4 known exoplanets in this catalogue, about 102 light-years away.","aliases":["M2.5 V"],"sources":["nasa"]},{"id":"host_star:toi-771","type":"host_star","name":"TOI-771","domain":"science","entryPath":"/exoplanets/toi-771","description":"TOI-771 is a M3 star that hosts 2 known exoplanets in this catalogue, about 82 light-years away.","aliases":["M3"],"sources":["nasa"]},{"id":"host_star:twa-7","type":"host_star","name":"TWA 7","domain":"science","entryPath":"/exoplanets/twa-7","description":"TWA 7 is a star that hosts 1 known exoplanet in this catalogue, about 111 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:tyc-8998-760-1","type":"host_star","name":"TYC 8998-760-1","domain":"science","entryPath":"/exoplanets/tyc-8998-760-1","description":"TYC 8998-760-1 is a K3 IV star that hosts 2 known exoplanets in this catalogue, about 309 light-years away.","aliases":["K3 IV"],"sources":["nasa"]},{"id":"host_star:ucac3-113-933","type":"host_star","name":"UCAC3 113-933","domain":"science","entryPath":"/exoplanets/ucac3-113-933","description":"UCAC3 113-933 is a M0 star that hosts 1 known exoplanet in this catalogue, about 172 light-years away.","aliases":["M0"],"sources":["nasa"]},{"id":"host_star:ucac4-328-061594","type":"host_star","name":"UCAC4 328-061594","domain":"science","entryPath":"/exoplanets/ucac4-328-061594","description":"UCAC4 328-061594 is a DC star that hosts 1 known exoplanet in this catalogue, about 130 light-years away.","aliases":["DC"],"sources":["nasa"]},{"id":"host_star:ups-and","type":"host_star","name":"ups And","domain":"science","entryPath":"/exoplanets/ups-and","description":"ups And is a F8 V star that hosts 3 known exoplanets in this catalogue, about 44 light-years away.","aliases":["F8 V"],"sources":["nasa"]},{"id":"host_star:usco-ctio-108","type":"host_star","name":"USco CTIO 108","domain":"science","entryPath":"/exoplanets/usco-ctio-108","description":"USco CTIO 108 is a M7 star that hosts 1 known exoplanet in this catalogue, about 470 light-years away.","aliases":["M7"],"sources":["nasa"]},{"id":"host_star:usco1556-a-star","type":"host_star","name":"USco1556 A","domain":"science","entryPath":"/exoplanets/usco1556-a-star","description":"USco1556 A is a M3.0 V star that hosts 1 known exoplanet in this catalogue, about 459 light-years away.","aliases":["M3.0 V"],"sources":["nasa"]},{"id":"host_star:usco1621-a-star","type":"host_star","name":"USco1621 A","domain":"science","entryPath":"/exoplanets/usco1621-a-star","description":"USco1621 A is a M2.5 V star that hosts 1 known exoplanet in this catalogue, about 450 light-years away.","aliases":["M2.5 V"],"sources":["nasa"]},{"id":"host_star:v2376-ori","type":"host_star","name":"V2376 Ori","domain":"science","entryPath":"/exoplanets/v2376-ori","description":"V2376 Ori is a M star that hosts 1 known exoplanet in this catalogue.","aliases":["M"],"sources":["nasa"]},{"id":"host_star:vhs-j125601-92-125723-9","type":"host_star","name":"VHS J125601.92-125723.9","domain":"science","entryPath":"/exoplanets/vhs-j125601-92-125723-9","description":"VHS J125601.92-125723.9 is a M7.5 star that hosts 1 known exoplanet in this catalogue, about 41 light-years away.","aliases":["M7.5"],"sources":["nasa"]},{"id":"host_star:wasp-12","type":"host_star","name":"WASP-12","domain":"science","entryPath":"/exoplanets/wasp-12","description":"WASP-12 is a star that hosts 1 known exoplanet in this catalogue, about 1394 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:wasp-121","type":"host_star","name":"WASP-121","domain":"science","entryPath":"/exoplanets/wasp-121","description":"WASP-121 is a F6 V star that hosts 1 known exoplanet in this catalogue, about 880 light-years away.","aliases":["F6 V"],"sources":["nasa"]},{"id":"host_star:wasp-17","type":"host_star","name":"WASP-17","domain":"science","entryPath":"/exoplanets/wasp-17","description":"WASP-17 is a F4 star that hosts 1 known exoplanet in this catalogue, about 1324 light-years away.","aliases":["F4"],"sources":["nasa"]},{"id":"host_star:wasp-39","type":"host_star","name":"WASP-39","domain":"science","entryPath":"/exoplanets/wasp-39","description":"WASP-39 is a star that hosts 1 known exoplanet in this catalogue, about 698 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:wasp-43","type":"host_star","name":"WASP-43","domain":"science","entryPath":"/exoplanets/wasp-43","description":"WASP-43 is a K7 V star that hosts 1 known exoplanet in this catalogue, about 283 light-years away.","aliases":["K7 V"],"sources":["nasa"]},{"id":"host_star:wasp-76","type":"host_star","name":"WASP-76","domain":"science","entryPath":"/exoplanets/wasp-76","description":"WASP-76 is a F7 star that hosts 1 known exoplanet in this catalogue, about 634 light-years away.","aliases":["F7"],"sources":["nasa"]},{"id":"host_star:wasp-96","type":"host_star","name":"WASP-96","domain":"science","entryPath":"/exoplanets/wasp-96","description":"WASP-96 is a G8 star that hosts 1 known exoplanet in this catalogue, about 1150 light-years away.","aliases":["G8"],"sources":["nasa"]},{"id":"host_star:wd-0806-661","type":"host_star","name":"WD 0806-661","domain":"science","entryPath":"/exoplanets/wd-0806-661","description":"WD 0806-661 is a DQ star that hosts 1 known exoplanet in this catalogue, about 63 light-years away.","aliases":["DQ"],"sources":["nasa"]},{"id":"host_star:wise-j033605-05-014350-4","type":"host_star","name":"WISE J033605.05-014350.4","domain":"science","entryPath":"/exoplanets/wise-j033605-05-014350-4","description":"WISE J033605.05-014350.4 is a star that hosts 1 known exoplanet in this catalogue.","aliases":[],"sources":["nasa"]},{"id":"host_star:wisep-j121756-91-162640-2-a-star","type":"host_star","name":"WISEP J121756.91+162640.2 A","domain":"science","entryPath":"/exoplanets/wisep-j121756-91-162640-2-a-star","description":"WISEP J121756.91+162640.2 A is a T8.5 star that hosts 1 known exoplanet in this catalogue, about 33 light-years away.","aliases":["T8.5"],"sources":["nasa"]},{"id":"host_star:wispit-1","type":"host_star","name":"WISPIT 1","domain":"science","entryPath":"/exoplanets/wispit-1","description":"WISPIT 1 is a K4 V star that hosts 2 known exoplanets in this catalogue, about 750 light-years away.","aliases":["K4 V"],"sources":["nasa"]},{"id":"host_star:wispit-2","type":"host_star","name":"WISPIT 2","domain":"science","entryPath":"/exoplanets/wispit-2","description":"WISPIT 2 is a star that hosts 2 known exoplanets in this catalogue, about 440 light-years away.","aliases":[],"sources":["nasa"]},{"id":"host_star:wolf-1069","type":"host_star","name":"Wolf 1069","domain":"science","entryPath":"/exoplanets/wolf-1069","description":"Wolf 1069 is a M5.0 V star that hosts 1 known exoplanet in this catalogue, about 31 light-years away.","aliases":["M5.0 V"],"sources":["nasa"]},{"id":"host_star:xest-17-036","type":"host_star","name":"XEST 17-036","domain":"science","entryPath":"/exoplanets/xest-17-036","description":"XEST 17-036 is a M4 star that hosts 1 known exoplanet in this catalogue, about 517 light-years away.","aliases":["M4"],"sources":["nasa"]},{"id":"host_star:xo-2-s-star","type":"host_star","name":"XO-2 S","domain":"science","entryPath":"/exoplanets/xo-2-s-star","description":"XO-2 S is a G8 V star that hosts 3 known exoplanets in this catalogue, about 494 light-years away.","aliases":["G8 V"],"sources":["nasa"]},{"id":"host_star:yz-cet","type":"host_star","name":"YZ Cet","domain":"science","entryPath":"/exoplanets/yz-cet","description":"YZ Cet is a M4.5 V star that hosts 3 known exoplanets in this catalogue, about 12 light-years away.","aliases":["M4.5 V"],"sources":["nasa"]},{"id":"planetary_system:14-her-system","type":"planetary_system","name":"14 Her system","domain":"science","entryPath":"/exoplanets/14-her-system","description":"The 14 Her system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:2mass-j19383260-4603591-system","type":"planetary_system","name":"2MASS J19383260+4603591 system","domain":"science","entryPath":"/exoplanets/2mass-j19383260-4603591-system","description":"The 2MASS J19383260+4603591 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:47-uma-system","type":"planetary_system","name":"47 UMa system","domain":"science","entryPath":"/exoplanets/47-uma-system","description":"The 47 UMa system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:55-cnc-system","type":"planetary_system","name":"55 Cnc system","domain":"science","entryPath":"/exoplanets/55-cnc-system","description":"The 55 Cnc system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:55-cnc-b-star-system","type":"planetary_system","name":"55 Cnc B system","domain":"science","entryPath":"/exoplanets/55-cnc-b-star-system","description":"The 55 Cnc B system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:61-vir-system","type":"planetary_system","name":"61 Vir system","domain":"science","entryPath":"/exoplanets/61-vir-system","description":"The 61 Vir system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:7-cma-system","type":"planetary_system","name":"7 CMa system","domain":"science","entryPath":"/exoplanets/7-cma-system","description":"The 7 CMa system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:75-cet-system","type":"planetary_system","name":"75 Cet system","domain":"science","entryPath":"/exoplanets/75-cet-system","description":"The 75 Cet system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:au-mic-system","type":"planetary_system","name":"AU Mic system","domain":"science","entryPath":"/exoplanets/au-mic-system","description":"The AU Mic system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:barnard-s-star-system","type":"planetary_system","name":"Barnard's star system","domain":"science","entryPath":"/exoplanets/barnard-s-star-system","description":"The Barnard's star system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:bd-06-1339-system","type":"planetary_system","name":"BD-06 1339 system","domain":"science","entryPath":"/exoplanets/bd-06-1339-system","description":"The BD-06 1339 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:bd-11-4672-system","type":"planetary_system","name":"BD-11 4672 system","domain":"science","entryPath":"/exoplanets/bd-11-4672-system","description":"The BD-11 4672 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:bd-210397-system","type":"planetary_system","name":"BD-210397 system","domain":"science","entryPath":"/exoplanets/bd-210397-system","description":"The BD-210397 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:bet-pic-system","type":"planetary_system","name":"bet Pic system","domain":"science","entryPath":"/exoplanets/bet-pic-system","description":"The bet Pic system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:dmpp-1-system","type":"planetary_system","name":"DMPP-1 system","domain":"science","entryPath":"/exoplanets/dmpp-1-system","description":"The DMPP-1 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:g-192-15-system","type":"planetary_system","name":"G 192-15 system","domain":"science","entryPath":"/exoplanets/g-192-15-system","description":"The G 192-15 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-1002-system","type":"planetary_system","name":"GJ 1002 system","domain":"science","entryPath":"/exoplanets/gj-1002-system","description":"The GJ 1002 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-1061-system","type":"planetary_system","name":"GJ 1061 system","domain":"science","entryPath":"/exoplanets/gj-1061-system","description":"The GJ 1061 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-1132-system","type":"planetary_system","name":"GJ 1132 system","domain":"science","entryPath":"/exoplanets/gj-1132-system","description":"The GJ 1132 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-1148-system","type":"planetary_system","name":"GJ 1148 system","domain":"science","entryPath":"/exoplanets/gj-1148-system","description":"The GJ 1148 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-15-a-star-system","type":"planetary_system","name":"GJ 15 A system","domain":"science","entryPath":"/exoplanets/gj-15-a-star-system","description":"The GJ 15 A system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-163-system","type":"planetary_system","name":"GJ 163 system","domain":"science","entryPath":"/exoplanets/gj-163-system","description":"The GJ 163 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-180-system","type":"planetary_system","name":"GJ 180 system","domain":"science","entryPath":"/exoplanets/gj-180-system","description":"The GJ 180 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-229-system","type":"planetary_system","name":"GJ 229 system","domain":"science","entryPath":"/exoplanets/gj-229-system","description":"The GJ 229 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-251-system","type":"planetary_system","name":"GJ 251 system","domain":"science","entryPath":"/exoplanets/gj-251-system","description":"The GJ 251 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-273-system","type":"planetary_system","name":"GJ 273 system","domain":"science","entryPath":"/exoplanets/gj-273-system","description":"The GJ 273 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-3138-system","type":"planetary_system","name":"GJ 3138 system","domain":"science","entryPath":"/exoplanets/gj-3138-system","description":"The GJ 3138 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-317-system","type":"planetary_system","name":"GJ 317 system","domain":"science","entryPath":"/exoplanets/gj-317-system","description":"The GJ 317 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-328-system","type":"planetary_system","name":"GJ 328 system","domain":"science","entryPath":"/exoplanets/gj-328-system","description":"The GJ 328 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-3293-system","type":"planetary_system","name":"GJ 3293 system","domain":"science","entryPath":"/exoplanets/gj-3293-system","description":"The GJ 3293 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-3323-system","type":"planetary_system","name":"GJ 3323 system","domain":"science","entryPath":"/exoplanets/gj-3323-system","description":"The GJ 3323 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-3512-system","type":"planetary_system","name":"GJ 3512 system","domain":"science","entryPath":"/exoplanets/gj-3512-system","description":"The GJ 3512 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-357-system","type":"planetary_system","name":"GJ 357 system","domain":"science","entryPath":"/exoplanets/gj-357-system","description":"The GJ 357 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-367-system","type":"planetary_system","name":"GJ 367 system","domain":"science","entryPath":"/exoplanets/gj-367-system","description":"The GJ 367 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-3998-system","type":"planetary_system","name":"GJ 3998 system","domain":"science","entryPath":"/exoplanets/gj-3998-system","description":"The GJ 3998 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-411-system","type":"planetary_system","name":"GJ 411 system","domain":"science","entryPath":"/exoplanets/gj-411-system","description":"The GJ 411 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-414-a-star-system","type":"planetary_system","name":"GJ 414 A system","domain":"science","entryPath":"/exoplanets/gj-414-a-star-system","description":"The GJ 414 A system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-4274-system","type":"planetary_system","name":"GJ 4274 system","domain":"science","entryPath":"/exoplanets/gj-4274-system","description":"The GJ 4274 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-433-system","type":"planetary_system","name":"GJ 433 system","domain":"science","entryPath":"/exoplanets/gj-433-system","description":"The GJ 433 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-536-system","type":"planetary_system","name":"GJ 536 system","domain":"science","entryPath":"/exoplanets/gj-536-system","description":"The GJ 536 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-581-system","type":"planetary_system","name":"GJ 581 system","domain":"science","entryPath":"/exoplanets/gj-581-system","description":"The GJ 581 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-667-c-star-system","type":"planetary_system","name":"GJ 667 C system","domain":"science","entryPath":"/exoplanets/gj-667-c-star-system","description":"The GJ 667 C system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-676-a-star-system","type":"planetary_system","name":"GJ 676 A system","domain":"science","entryPath":"/exoplanets/gj-676-a-star-system","description":"The GJ 676 A system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-682-system","type":"planetary_system","name":"GJ 682 system","domain":"science","entryPath":"/exoplanets/gj-682-system","description":"The GJ 682 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-687-system","type":"planetary_system","name":"GJ 687 system","domain":"science","entryPath":"/exoplanets/gj-687-system","description":"The GJ 687 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-806-system","type":"planetary_system","name":"GJ 806 system","domain":"science","entryPath":"/exoplanets/gj-806-system","description":"The GJ 806 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-849-system","type":"planetary_system","name":"GJ 849 system","domain":"science","entryPath":"/exoplanets/gj-849-system","description":"The GJ 849 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-876-system","type":"planetary_system","name":"GJ 876 system","domain":"science","entryPath":"/exoplanets/gj-876-system","description":"The GJ 876 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-887-system","type":"planetary_system","name":"GJ 887 system","domain":"science","entryPath":"/exoplanets/gj-887-system","description":"The GJ 887 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:gj-9827-system","type":"planetary_system","name":"GJ 9827 system","domain":"science","entryPath":"/exoplanets/gj-9827-system","description":"The GJ 9827 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-10180-system","type":"planetary_system","name":"HD 10180 system","domain":"science","entryPath":"/exoplanets/hd-10180-system","description":"The HD 10180 system is a planetary system with 6 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-104067-system","type":"planetary_system","name":"HD 104067 system","domain":"science","entryPath":"/exoplanets/hd-104067-system","description":"The HD 104067 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-111232-system","type":"planetary_system","name":"HD 111232 system","domain":"science","entryPath":"/exoplanets/hd-111232-system","description":"The HD 111232 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-113538-system","type":"planetary_system","name":"HD 113538 system","domain":"science","entryPath":"/exoplanets/hd-113538-system","description":"The HD 113538 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-114386-system","type":"planetary_system","name":"HD 114386 system","domain":"science","entryPath":"/exoplanets/hd-114386-system","description":"The HD 114386 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-114783-system","type":"planetary_system","name":"HD 114783 system","domain":"science","entryPath":"/exoplanets/hd-114783-system","description":"The HD 114783 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-11506-system","type":"planetary_system","name":"HD 11506 system","domain":"science","entryPath":"/exoplanets/hd-11506-system","description":"The HD 11506 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-115404-a-star-system","type":"planetary_system","name":"HD 115404 A system","domain":"science","entryPath":"/exoplanets/hd-115404-a-star-system","description":"The HD 115404 A system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-118203-system","type":"planetary_system","name":"HD 118203 system","domain":"science","entryPath":"/exoplanets/hd-118203-system","description":"The HD 118203 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-125612-system","type":"planetary_system","name":"HD 125612 system","domain":"science","entryPath":"/exoplanets/hd-125612-system","description":"The HD 125612 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-128311-system","type":"planetary_system","name":"HD 128311 system","domain":"science","entryPath":"/exoplanets/hd-128311-system","description":"The HD 128311 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-134060-system","type":"planetary_system","name":"HD 134060 system","domain":"science","entryPath":"/exoplanets/hd-134060-system","description":"The HD 134060 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-134606-system","type":"planetary_system","name":"HD 134606 system","domain":"science","entryPath":"/exoplanets/hd-134606-system","description":"The HD 134606 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-134987-system","type":"planetary_system","name":"HD 134987 system","domain":"science","entryPath":"/exoplanets/hd-134987-system","description":"The HD 134987 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-136352-system","type":"planetary_system","name":"HD 136352 system","domain":"science","entryPath":"/exoplanets/hd-136352-system","description":"The HD 136352 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-13808-system","type":"planetary_system","name":"HD 13808 system","domain":"science","entryPath":"/exoplanets/hd-13808-system","description":"The HD 13808 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-141399-system","type":"planetary_system","name":"HD 141399 system","domain":"science","entryPath":"/exoplanets/hd-141399-system","description":"The HD 141399 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-142-system","type":"planetary_system","name":"HD 142 system","domain":"science","entryPath":"/exoplanets/hd-142-system","description":"The HD 142 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-1461-system","type":"planetary_system","name":"HD 1461 system","domain":"science","entryPath":"/exoplanets/hd-1461-system","description":"The HD 1461 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-153557-system","type":"planetary_system","name":"HD 153557 system","domain":"science","entryPath":"/exoplanets/hd-153557-system","description":"The HD 153557 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-156668-system","type":"planetary_system","name":"HD 156668 system","domain":"science","entryPath":"/exoplanets/hd-156668-system","description":"The HD 156668 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-158259-system","type":"planetary_system","name":"HD 158259 system","domain":"science","entryPath":"/exoplanets/hd-158259-system","description":"The HD 158259 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-160691-system","type":"planetary_system","name":"HD 160691 system","domain":"science","entryPath":"/exoplanets/hd-160691-system","description":"The HD 160691 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-164604-system","type":"planetary_system","name":"HD 164604 system","domain":"science","entryPath":"/exoplanets/hd-164604-system","description":"The HD 164604 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-164922-system","type":"planetary_system","name":"HD 164922 system","domain":"science","entryPath":"/exoplanets/hd-164922-system","description":"The HD 164922 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-176986-system","type":"planetary_system","name":"HD 176986 system","domain":"science","entryPath":"/exoplanets/hd-176986-system","description":"The HD 176986 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-181433-system","type":"planetary_system","name":"HD 181433 system","domain":"science","entryPath":"/exoplanets/hd-181433-system","description":"The HD 181433 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-189567-system","type":"planetary_system","name":"HD 189567 system","domain":"science","entryPath":"/exoplanets/hd-189567-system","description":"The HD 189567 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-190360-system","type":"planetary_system","name":"HD 190360 system","domain":"science","entryPath":"/exoplanets/hd-190360-system","description":"The HD 190360 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-191939-system","type":"planetary_system","name":"HD 191939 system","domain":"science","entryPath":"/exoplanets/hd-191939-system","description":"The HD 191939 system is a planetary system with 6 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-192310-system","type":"planetary_system","name":"HD 192310 system","domain":"science","entryPath":"/exoplanets/hd-192310-system","description":"The HD 192310 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-203387-system","type":"planetary_system","name":"HD 203387 system","domain":"science","entryPath":"/exoplanets/hd-203387-system","description":"The HD 203387 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-206893-system","type":"planetary_system","name":"HD 206893 system","domain":"science","entryPath":"/exoplanets/hd-206893-system","description":"The HD 206893 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-20781-system","type":"planetary_system","name":"HD 20781 system","domain":"science","entryPath":"/exoplanets/hd-20781-system","description":"The HD 20781 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-20794-system","type":"planetary_system","name":"HD 20794 system","domain":"science","entryPath":"/exoplanets/hd-20794-system","description":"The HD 20794 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-215152-system","type":"planetary_system","name":"HD 215152 system","domain":"science","entryPath":"/exoplanets/hd-215152-system","description":"The HD 215152 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-217107-system","type":"planetary_system","name":"HD 217107 system","domain":"science","entryPath":"/exoplanets/hd-217107-system","description":"The HD 217107 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-219134-system","type":"planetary_system","name":"HD 219134 system","domain":"science","entryPath":"/exoplanets/hd-219134-system","description":"The HD 219134 system is a planetary system with 6 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-23079-system","type":"planetary_system","name":"HD 23079 system","domain":"science","entryPath":"/exoplanets/hd-23079-system","description":"The HD 23079 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-260655-system","type":"planetary_system","name":"HD 260655 system","domain":"science","entryPath":"/exoplanets/hd-260655-system","description":"The HD 260655 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-27894-system","type":"planetary_system","name":"HD 27894 system","domain":"science","entryPath":"/exoplanets/hd-27894-system","description":"The HD 27894 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-33142-system","type":"planetary_system","name":"HD 33142 system","domain":"science","entryPath":"/exoplanets/hd-33142-system","description":"The HD 33142 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-34445-system","type":"planetary_system","name":"HD 34445 system","domain":"science","entryPath":"/exoplanets/hd-34445-system","description":"The HD 34445 system is a planetary system with 6 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-37124-system","type":"planetary_system","name":"HD 37124 system","domain":"science","entryPath":"/exoplanets/hd-37124-system","description":"The HD 37124 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-39091-system","type":"planetary_system","name":"HD 39091 system","domain":"science","entryPath":"/exoplanets/hd-39091-system","description":"The HD 39091 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-39194-system","type":"planetary_system","name":"HD 39194 system","domain":"science","entryPath":"/exoplanets/hd-39194-system","description":"The HD 39194 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-40307-system","type":"planetary_system","name":"HD 40307 system","domain":"science","entryPath":"/exoplanets/hd-40307-system","description":"The HD 40307 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-43197-system","type":"planetary_system","name":"HD 43197 system","domain":"science","entryPath":"/exoplanets/hd-43197-system","description":"The HD 43197 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-45184-system","type":"planetary_system","name":"HD 45184 system","domain":"science","entryPath":"/exoplanets/hd-45184-system","description":"The HD 45184 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-48265-system","type":"planetary_system","name":"HD 48265 system","domain":"science","entryPath":"/exoplanets/hd-48265-system","description":"The HD 48265 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-48948-system","type":"planetary_system","name":"HD 48948 system","domain":"science","entryPath":"/exoplanets/hd-48948-system","description":"The HD 48948 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-60532-system","type":"planetary_system","name":"HD 60532 system","domain":"science","entryPath":"/exoplanets/hd-60532-system","description":"The HD 60532 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-63433-system","type":"planetary_system","name":"HD 63433 system","domain":"science","entryPath":"/exoplanets/hd-63433-system","description":"The HD 63433 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-68988-system","type":"planetary_system","name":"HD 68988 system","domain":"science","entryPath":"/exoplanets/hd-68988-system","description":"The HD 68988 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-69830-system","type":"planetary_system","name":"HD 69830 system","domain":"science","entryPath":"/exoplanets/hd-69830-system","description":"The HD 69830 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-75898-system","type":"planetary_system","name":"HD 75898 system","domain":"science","entryPath":"/exoplanets/hd-75898-system","description":"The HD 75898 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-7924-system","type":"planetary_system","name":"HD 7924 system","domain":"science","entryPath":"/exoplanets/hd-7924-system","description":"The HD 7924 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-81817-system","type":"planetary_system","name":"HD 81817 system","domain":"science","entryPath":"/exoplanets/hd-81817-system","description":"The HD 81817 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-82943-system","type":"planetary_system","name":"HD 82943 system","domain":"science","entryPath":"/exoplanets/hd-82943-system","description":"The HD 82943 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-83443-system","type":"planetary_system","name":"HD 83443 system","domain":"science","entryPath":"/exoplanets/hd-83443-system","description":"The HD 83443 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-93083-system","type":"planetary_system","name":"HD 93083 system","domain":"science","entryPath":"/exoplanets/hd-93083-system","description":"The HD 93083 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-94890-system","type":"planetary_system","name":"HD 94890 system","domain":"science","entryPath":"/exoplanets/hd-94890-system","description":"The HD 94890 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-96700-system","type":"planetary_system","name":"HD 96700 system","domain":"science","entryPath":"/exoplanets/hd-96700-system","description":"The HD 96700 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hd-99492-system","type":"planetary_system","name":"HD 99492 system","domain":"science","entryPath":"/exoplanets/hd-99492-system","description":"The HD 99492 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hip-14810-system","type":"planetary_system","name":"HIP 14810 system","domain":"science","entryPath":"/exoplanets/hip-14810-system","description":"The HIP 14810 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hip-41378-system","type":"planetary_system","name":"HIP 41378 system","domain":"science","entryPath":"/exoplanets/hip-41378-system","description":"The HIP 41378 system is a planetary system with 6 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hip-56998-system","type":"planetary_system","name":"HIP 56998 system","domain":"science","entryPath":"/exoplanets/hip-56998-system","description":"The HIP 56998 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hip-57274-system","type":"planetary_system","name":"HIP 57274 system","domain":"science","entryPath":"/exoplanets/hip-57274-system","description":"The HIP 57274 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:hr-8799-system","type":"planetary_system","name":"HR 8799 system","domain":"science","entryPath":"/exoplanets/hr-8799-system","description":"The HR 8799 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:k2-18-system","type":"planetary_system","name":"K2-18 system","domain":"science","entryPath":"/exoplanets/k2-18-system","description":"The K2-18 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-100-system","type":"planetary_system","name":"Kepler-100 system","domain":"science","entryPath":"/exoplanets/kepler-100-system","description":"The Kepler-100 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-11-system","type":"planetary_system","name":"Kepler-11 system","domain":"science","entryPath":"/exoplanets/kepler-11-system","description":"The Kepler-11 system is a planetary system with 6 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-122-system","type":"planetary_system","name":"Kepler-122 system","domain":"science","entryPath":"/exoplanets/kepler-122-system","description":"The Kepler-122 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-138-system","type":"planetary_system","name":"Kepler-138 system","domain":"science","entryPath":"/exoplanets/kepler-138-system","description":"The Kepler-138 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-139-system","type":"planetary_system","name":"Kepler-139 system","domain":"science","entryPath":"/exoplanets/kepler-139-system","description":"The Kepler-139 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-1649-system","type":"planetary_system","name":"Kepler-1649 system","domain":"science","entryPath":"/exoplanets/kepler-1649-system","description":"The Kepler-1649 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-186-system","type":"planetary_system","name":"Kepler-186 system","domain":"science","entryPath":"/exoplanets/kepler-186-system","description":"The Kepler-186 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-19-system","type":"planetary_system","name":"Kepler-19 system","domain":"science","entryPath":"/exoplanets/kepler-19-system","description":"The Kepler-19 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-20-system","type":"planetary_system","name":"Kepler-20 system","domain":"science","entryPath":"/exoplanets/kepler-20-system","description":"The Kepler-20 system is a planetary system with 6 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-24-system","type":"planetary_system","name":"Kepler-24 system","domain":"science","entryPath":"/exoplanets/kepler-24-system","description":"The Kepler-24 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-26-system","type":"planetary_system","name":"Kepler-26 system","domain":"science","entryPath":"/exoplanets/kepler-26-system","description":"The Kepler-26 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-32-system","type":"planetary_system","name":"Kepler-32 system","domain":"science","entryPath":"/exoplanets/kepler-32-system","description":"The Kepler-32 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-33-system","type":"planetary_system","name":"Kepler-33 system","domain":"science","entryPath":"/exoplanets/kepler-33-system","description":"The Kepler-33 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-338-system","type":"planetary_system","name":"Kepler-338 system","domain":"science","entryPath":"/exoplanets/kepler-338-system","description":"The Kepler-338 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-37-system","type":"planetary_system","name":"Kepler-37 system","domain":"science","entryPath":"/exoplanets/kepler-37-system","description":"The Kepler-37 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-411-system","type":"planetary_system","name":"Kepler-411 system","domain":"science","entryPath":"/exoplanets/kepler-411-system","description":"The Kepler-411 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-416-system","type":"planetary_system","name":"Kepler-416 system","domain":"science","entryPath":"/exoplanets/kepler-416-system","description":"The Kepler-416 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-46-system","type":"planetary_system","name":"Kepler-46 system","domain":"science","entryPath":"/exoplanets/kepler-46-system","description":"The Kepler-46 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-48-system","type":"planetary_system","name":"Kepler-48 system","domain":"science","entryPath":"/exoplanets/kepler-48-system","description":"The Kepler-48 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-49-system","type":"planetary_system","name":"Kepler-49 system","domain":"science","entryPath":"/exoplanets/kepler-49-system","description":"The Kepler-49 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-51-system","type":"planetary_system","name":"Kepler-51 system","domain":"science","entryPath":"/exoplanets/kepler-51-system","description":"The Kepler-51 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-55-system","type":"planetary_system","name":"Kepler-55 system","domain":"science","entryPath":"/exoplanets/kepler-55-system","description":"The Kepler-55 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-58-system","type":"planetary_system","name":"Kepler-58 system","domain":"science","entryPath":"/exoplanets/kepler-58-system","description":"The Kepler-58 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-65-system","type":"planetary_system","name":"Kepler-65 system","domain":"science","entryPath":"/exoplanets/kepler-65-system","description":"The Kepler-65 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-68-system","type":"planetary_system","name":"Kepler-68 system","domain":"science","entryPath":"/exoplanets/kepler-68-system","description":"The Kepler-68 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-79-system","type":"planetary_system","name":"Kepler-79 system","domain":"science","entryPath":"/exoplanets/kepler-79-system","description":"The Kepler-79 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-80-system","type":"planetary_system","name":"Kepler-80 system","domain":"science","entryPath":"/exoplanets/kepler-80-system","description":"The Kepler-80 system is a planetary system with 6 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-82-system","type":"planetary_system","name":"Kepler-82 system","domain":"science","entryPath":"/exoplanets/kepler-82-system","description":"The Kepler-82 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-84-system","type":"planetary_system","name":"Kepler-84 system","domain":"science","entryPath":"/exoplanets/kepler-84-system","description":"The Kepler-84 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:kepler-85-system","type":"planetary_system","name":"Kepler-85 system","domain":"science","entryPath":"/exoplanets/kepler-85-system","description":"The Kepler-85 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:koi-142-system","type":"planetary_system","name":"KOI-142 system","domain":"science","entryPath":"/exoplanets/koi-142-system","description":"The KOI-142 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:l-98-59-system","type":"planetary_system","name":"L 98-59 system","domain":"science","entryPath":"/exoplanets/l-98-59-system","description":"The L 98-59 system is a planetary system with 5 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:lhs-1140-system","type":"planetary_system","name":"LHS 1140 system","domain":"science","entryPath":"/exoplanets/lhs-1140-system","description":"The LHS 1140 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:lhs-1678-system","type":"planetary_system","name":"LHS 1678 system","domain":"science","entryPath":"/exoplanets/lhs-1678-system","description":"The LHS 1678 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:lkca-15-system","type":"planetary_system","name":"LkCa 15 system","domain":"science","entryPath":"/exoplanets/lkca-15-system","description":"The LkCa 15 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:lp-791-18-system","type":"planetary_system","name":"LP 791-18 system","domain":"science","entryPath":"/exoplanets/lp-791-18-system","description":"The LP 791-18 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:lp-890-9-system","type":"planetary_system","name":"LP 890-9 system","domain":"science","entryPath":"/exoplanets/lp-890-9-system","description":"The LP 890-9 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:ltt-1445-a-star-system","type":"planetary_system","name":"LTT 1445 A system","domain":"science","entryPath":"/exoplanets/ltt-1445-a-star-system","description":"The LTT 1445 A system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:nn-ser-system","type":"planetary_system","name":"NN Ser system","domain":"science","entryPath":"/exoplanets/nn-ser-system","description":"The NN Ser system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:nu-oph-system","type":"planetary_system","name":"nu Oph system","domain":"science","entryPath":"/exoplanets/nu-oph-system","description":"The nu Oph system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:ny-vir-system","type":"planetary_system","name":"NY Vir system","domain":"science","entryPath":"/exoplanets/ny-vir-system","description":"The NY Vir system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:ogle-2006-blg-109l-system","type":"planetary_system","name":"OGLE-2006-BLG-109L system","domain":"science","entryPath":"/exoplanets/ogle-2006-blg-109l-system","description":"The OGLE-2006-BLG-109L system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:ogle-2012-blg-0026l-system","type":"planetary_system","name":"OGLE-2012-BLG-0026L system","domain":"science","entryPath":"/exoplanets/ogle-2012-blg-0026l-system","description":"The OGLE-2012-BLG-0026L system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:pds-70-system","type":"planetary_system","name":"PDS 70 system","domain":"science","entryPath":"/exoplanets/pds-70-system","description":"The PDS 70 system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:proxima-cen-system","type":"planetary_system","name":"Proxima Cen system","domain":"science","entryPath":"/exoplanets/proxima-cen-system","description":"The Proxima Cen system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:psr-b1257-12-system","type":"planetary_system","name":"PSR B1257+12 system","domain":"science","entryPath":"/exoplanets/psr-b1257-12-system","description":"The PSR B1257+12 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:rho-crb-system","type":"planetary_system","name":"rho CrB system","domain":"science","entryPath":"/exoplanets/rho-crb-system","description":"The rho CrB system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:tau-cet-system","type":"planetary_system","name":"tau Cet system","domain":"science","entryPath":"/exoplanets/tau-cet-system","description":"The tau Cet system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:teegarden-s-star-system","type":"planetary_system","name":"Teegarden's Star system","domain":"science","entryPath":"/exoplanets/teegarden-s-star-system","description":"The Teegarden's Star system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:toi-1203-system","type":"planetary_system","name":"TOI-1203 system","domain":"science","entryPath":"/exoplanets/toi-1203-system","description":"The TOI-1203 system is a planetary system with 4 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:toi-1266-system","type":"planetary_system","name":"TOI-1266 system","domain":"science","entryPath":"/exoplanets/toi-1266-system","description":"The TOI-1266 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:toi-201-system","type":"planetary_system","name":"TOI-201 system","domain":"science","entryPath":"/exoplanets/toi-201-system","description":"The TOI-201 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:toi-2267-a-star-system","type":"planetary_system","name":"TOI-2267 A system","domain":"science","entryPath":"/exoplanets/toi-2267-a-star-system","description":"The TOI-2267 A system is a planetary system with 2 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:toi-270-system","type":"planetary_system","name":"TOI-270 system","domain":"science","entryPath":"/exoplanets/toi-270-system","description":"The TOI-270 system is a planetary system with 3 known planets in this catalogue.","sources":["nasa"]},{"id":"planetary_system:toi-4010-system","type":"planetary_system","name":"TOI-4010 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Russia.","aliases":["Site 35"],"sources":["gunters"]},{"id":"launch_pad:jiuquan-921","type":"launch_pad","name":"Jiuquan Area 4 (SLS-1)","domain":"science","entryPath":"/rockets/jiuquan-921","description":"The Jiuquan complex for China's human-rated Long March 2F, launching Shenzhou crews to the Tiangong station.","sources":["gunters"]},{"id":"launch_pad:xichang-2","type":"launch_pad","name":"Xichang LC-2","domain":"science","entryPath":"/rockets/xichang-2","description":"A Xichang complex widely used for Long March 3B launches to geostationary transfer orbit.","sources":["gunters"]},{"id":"launch_pad:wenchang-101","type":"launch_pad","name":"Wenchang LC-101","domain":"science","entryPath":"/rockets/wenchang-101","description":"The coastal Wenchang complex for the heavy-lift Long March 5.","sources":["gunters"]},{"id":"launch_pad:wenchang-201","type":"launch_pad","name":"Wenchang LC-201","domain":"science","entryPath":"/rockets/wenchang-201","description":"The Wenchang complex for the 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and Sirius — enclosing much of the northern winter sky.","sources":["britannica"]},{"id":"asterism:great-square-of-pegasus","type":"asterism","name":"The Great Square of Pegasus","domain":"science","entryPath":"/constellations/asterism/great-square-of-pegasus","description":"A large near-square of stars marking the body of Pegasus, with its northeastern corner shared by Andromeda — a key autumn signpost.","sources":["britannica"]},{"id":"asterism:northern-cross","type":"asterism","name":"The Northern Cross","domain":"science","entryPath":"/constellations/asterism/northern-cross","description":"The cross-shaped main pattern of Cygnus, laid along the summer Milky Way with Deneb at its head.","sources":["britannica"]},{"id":"asterism:teapot","type":"asterism","name":"The Teapot","domain":"science","entryPath":"/constellations/asterism/teapot","description":"The brightest stars of Sagittarius form a teapot whose spout points toward the Galactic Center, where the summer Milky Way is richest.","sources":["britannica"]},{"id":"asterism:sickle","type":"asterism","name":"The Sickle of Leo","domain":"science","entryPath":"/constellations/asterism/sickle","description":"A backwards-question-mark of stars marking the head and mane of Leo, anchored by Regulus.","sources":["britannica"]},{"id":"asterism:keystone","type":"asterism","name":"The Keystone","domain":"science","entryPath":"/constellations/asterism/keystone","description":"A lopsided quadrilateral forming the torso of Hercules; the great globular cluster M13 lies along its western side.","sources":["britannica"]},{"id":"asterism:coathanger","type":"asterism","name":"The Coathanger","domain":"science","entryPath":"/constellations/asterism/coathanger","description":"A chance line of six stars with a hook (also called Brocchi's Cluster) in Vulpecula, a fine binocular target.","sources":["britannica"]},{"id":"asterism:false-cross","type":"asterism","name":"The False 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Low latency and easy access make it the busiest orbital regime.","aliases":["LEO"],"sources":["nasa","esa"]},{"id":"orbit_type:meo","type":"orbit_type","name":"Medium Earth Orbit (MEO)","domain":"science","entryPath":"/satellites/orbit/meo","description":"The band of orbits between low Earth orbit and the geostationary altitude. Its multi-hour periods and wide coverage make it ideal for navigation constellations, typically near 20,000 km.","aliases":["MEO"],"sources":["nasa","esa"]},{"id":"orbit_type:geo","type":"orbit_type","name":"Geostationary Orbit (GEO)","domain":"science","entryPath":"/satellites/orbit/geo","description":"A circular orbit 35,786 km above the equator where a satellite's period matches Earth's rotation, so it appears fixed in the sky. The workhorse orbit for communications and weather monitoring.","aliases":["GEO","Geostationary"],"sources":["nasa","esa"]},{"id":"orbit_type:sso","type":"orbit_type","name":"Sun-Synchronous Orbit (SSO)","domain":"science","entryPath":"/satellites/orbit/sso","description":"A near-polar low orbit whose plane precesses to keep a constant angle to the Sun, so a satellite passes over each location at the same local solar time — ideal for consistent-illumination Earth imaging.","aliases":["SSO","Sun-synchronous"],"sources":["nasa","esa"]},{"id":"orbit_type:polar","type":"orbit_type","name":"Polar Orbit","domain":"science","entryPath":"/satellites/orbit/polar","description":"A low orbit inclined close to 90° that passes over (or near) both poles, letting a satellite eventually observe the whole planet as the Earth turns underneath it.","aliases":["Polar"],"sources":["nasa","esa"]},{"id":"orbit_type:heo","type":"orbit_type","name":"Highly Elliptical Orbit (HEO)","domain":"science","entryPath":"/satellites/orbit/heo","description":"An elongated orbit with a low perigee and a very high apogee (as in the Molniya and Tundra orbits). The satellite moves slowly near apogee, dwelling for hours over high latitudes that geostationary orbit cannot serve.","aliases":["HEO","Molniya"],"sources":["nasa","esa"]},{"id":"orbit_type:gto","type":"orbit_type","name":"Geostationary Transfer Orbit (GTO)","domain":"science","entryPath":"/satellites/orbit/gto","description":"An elliptical transfer orbit with perigee in low Earth orbit and apogee at the geostationary altitude, used to carry a satellite most of the way to GEO before its own engine circularises the orbit.","aliases":["GTO"],"sources":["nasa","esa"]},{"id":"organization:noaa","type":"organization","name":"NOAA","domain":"science","entryPath":"/satellites/operator/noaa","description":"The U.S. agency operating the GOES geostationary and JPSS/POES polar weather satellites.","aliases":["National Oceanic and Atmospheric 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commercial GEO comsat, Early Bird.","sources":["gunters"]},{"id":"organization:planet-labs","type":"organization","name":"Planet Labs","domain":"science","entryPath":"/satellites/operator/planet-labs","description":"A commercial Earth-imaging company operating the large Dove (Flock) and SkySat constellations.","aliases":["Planet"],"sources":["gunters"]},{"id":"organization:maxar","type":"organization","name":"Maxar Technologies","domain":"science","entryPath":"/satellites/operator/maxar","description":"A commercial operator of very-high-resolution Earth-imaging satellites, including the WorldView series.","aliases":["DigitalGlobe"],"sources":["gunters"]},{"id":"organization:blacksky","type":"organization","name":"BlackSky","domain":"science","entryPath":"/satellites/operator/blacksky","description":"A commercial operator of a low-Earth-orbit constellation for rapid-revisit Earth imaging.","sources":["gunters"]},{"id":"satellite_constellation:starlink","type":"satellite_constellation","name":"Starlink","domain":"science","entryPath":"/satellites/constellation/starlink","description":"SpaceX's low-Earth-orbit broadband internet constellation, the largest ever built, delivering global high-speed connectivity.","sources":["gunters"]},{"id":"satellite_constellation:oneweb","type":"satellite_constellation","name":"OneWeb","domain":"science","entryPath":"/satellites/constellation/oneweb","description":"A low-Earth-orbit broadband constellation providing global connectivity, focused on enterprise, government, and maritime users.","sources":["gunters"]},{"id":"satellite_constellation:iridium-next","type":"satellite_constellation","name":"Iridium NEXT","domain":"science","entryPath":"/satellites/constellation/iridium-next","description":"The second-generation Iridium constellation of 66 cross-linked low-Earth-orbit satellites providing pole-to-pole voice and data coverage.","aliases":["Iridium"],"sources":["gunters"]},{"id":"satellite_constellation:globalstar","type":"satellite_constellation","name":"Globalstar","domain":"science","entryPath":"/satellites/constellation/globalstar","description":"A low-Earth-orbit satellite-phone and data constellation serving voice, messaging, and IoT connectivity.","sources":["gunters"]},{"id":"satellite_constellation:o3b","type":"satellite_constellation","name":"O3b","domain":"science","entryPath":"/satellites/constellation/o3b","description":"SES's medium-Earth-orbit broadband constellation delivering low-latency connectivity to telecom, maritime, and enterprise customers between the tropics and beyond.","aliases":["O3b mPOWER"],"sources":["gunters"]},{"id":"satellite_constellation:gps","type":"satellite_constellation","name":"GPS (Global Positioning System)","domain":"science","entryPath":"/satellites/constellation/gps","description":"The United States' global navigation satellite system, providing worldwide positioning, navigation, and timing from medium Earth orbit.","aliases":["NAVSTAR GPS","GPS"],"sources":["gunters"]},{"id":"satellite_constellation:galileo-navigation","type":"satellite_constellation","name":"Galileo (navigation system)","domain":"science","entryPath":"/satellites/constellation/galileo-navigation","description":"Europe's civil global navigation satellite system — owned by the EU and operated through EUSPA, with ESA as the design and procurement agent — offering high-accuracy positioning independent of GPS.","aliases":["Galileo GNSS"],"sources":["esa"]},{"id":"satellite_constellation:glonass","type":"satellite_constellation","name":"GLONASS","domain":"science","entryPath":"/satellites/constellation/glonass","description":"Russia's global navigation satellite system, providing worldwide positioning and timing from medium Earth orbit.","sources":["roscosmos"]},{"id":"satellite_constellation:beidou","type":"satellite_constellation","name":"BeiDou","domain":"science","entryPath":"/satellites/constellation/beidou","description":"China's global navigation satellite system, using a mix of medium-Earth, geostationary, and inclined geosynchronous orbits.","aliases":["BDS","Beidou Navigation Satellite System"],"sources":["gunters"]},{"id":"satellite_constellation:planet-dove","type":"satellite_constellation","name":"Planet Dove (Flock)","domain":"science","entryPath":"/satellites/constellation/planet-dove","description":"Planet Labs' fleet of shoebox-sized Dove CubeSats that image the entire land surface of the Earth daily at medium resolution.","aliases":["Flock","Planet"],"sources":["gunters"]},{"id":"satellite_constellation:blacksky-constellation","type":"satellite_constellation","name":"BlackSky Global","domain":"science","entryPath":"/satellites/constellation/blacksky-constellation","description":"A commercial low-Earth-orbit constellation delivering rapid-revisit, high-cadence Earth imagery.","aliases":["BlackSky"],"sources":["gunters"]},{"id":"tracking_network:deep-space-network","type":"tracking_network","name":"Deep Space Network (DSN)","domain":"science","entryPath":"/satellites/network/deep-space-network","description":"NASA's international array of giant radio antennas — at Goldstone (California), Madrid, and Canberra — that communicates with interplanetary spacecraft and distant satellites, spaced around the globe for continuous coverage.","aliases":["DSN"],"sources":["nasa"]},{"id":"tracking_network:near-space-network","type":"tracking_network","name":"Near Space Network","domain":"science","entryPath":"/satellites/network/near-space-network","description":"NASA's network of ground stations and relay satellites (formerly the Space Network's TDRSS and the Ground Network) that supports missions in Earth orbit and near-Earth space.","aliases":["NSN","Space Network","Ground 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Built by JPL and launched by the U.S. Army — NASA did not yet exist.","sources":["nasa"]},{"id":"satellite:vanguard-1","type":"satellite","name":"Vanguard 1","domain":"science","entryPath":"/satellites/vanguard-1","description":"An early U.S. technology and science satellite — the oldest human-made object still in orbit, and the first satellite to use solar cells.","sources":["nasa"]},{"id":"satellite:telstar-1","type":"satellite","name":"Telstar 1","domain":"science","entryPath":"/satellites/telstar-1","description":"The first active communications satellite, which relayed the first transatlantic television signals in 1962.","sources":["nasa"]},{"id":"satellite:tiros-1","type":"satellite","name":"TIROS-1","domain":"science","entryPath":"/satellites/tiros-1","description":"The first successful weather satellite, which returned the first television images of Earth's cloud cover in 1960 and founded operational meteorology from space.","aliases":["TIROS 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program, which began the longest continuous record of Earth's land surface from space.","aliases":["ERTS-1"],"sources":["nasa"]},{"id":"satellite:landsat-8","type":"satellite","name":"Landsat 8","domain":"science","entryPath":"/satellites/landsat-8","description":"A NASA/USGS Landsat satellite carrying the Operational Land Imager and Thermal Infrared Sensor, continuing the multi-decade land-imaging record.","sources":["nasa"]},{"id":"satellite:landsat-9","type":"satellite","name":"Landsat 9","domain":"science","entryPath":"/satellites/landsat-9","description":"The latest Landsat satellite, launched in 2021 to work in tandem with Landsat 8 for an eight-day global revisit of the land surface.","sources":["nasa"]},{"id":"satellite:sentinel-1","type":"satellite","name":"Sentinel-1","domain":"science","entryPath":"/satellites/sentinel-1","description":"A Copernicus radar-imaging mission providing all-weather, day-and-night synthetic-aperture radar imagery of land and ocean.","sources":["esa"]},{"id":"satellite:sentinel-2","type":"satellite","name":"Sentinel-2","domain":"science","entryPath":"/satellites/sentinel-2","description":"A Copernicus optical-imaging mission delivering high-resolution multispectral imagery for land monitoring, agriculture, and disaster response.","sources":["esa"]},{"id":"satellite:sentinel-3","type":"satellite","name":"Sentinel-3","domain":"science","entryPath":"/satellites/sentinel-3","description":"A Copernicus mission monitoring ocean and land surface temperature, colour, and topography for climate and marine services.","sources":["esa"]},{"id":"satellite:terra","type":"satellite","name":"Terra","domain":"science","entryPath":"/satellites/terra","description":"NASA's flagship Earth Observing System morning satellite, carrying instruments including MODIS and ASTER to study land, ocean, and atmosphere.","aliases":["EOS 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resolution.","aliases":["Surface Water and Ocean Topography"],"sources":["nasa"]},{"id":"satellite:icesat-2","type":"satellite","name":"ICESat-2","domain":"science","entryPath":"/satellites/icesat-2","description":"A NASA laser-altimetry mission measuring the elevation of ice sheets, glaciers, sea ice, and vegetation to track a changing planet.","sources":["nasa"]},{"id":"satellite:jason-3","type":"satellite","name":"Jason-3","domain":"science","entryPath":"/satellites/jason-3","description":"A radar-altimetry mission continuing the decades-long record of global sea-surface height for oceanography and climate monitoring.","sources":["noaa"]},{"id":"satellite:worldview-3","type":"satellite","name":"WorldView-3","domain":"science","entryPath":"/satellites/worldview-3","description":"A Maxar very-high-resolution commercial Earth-imaging satellite used for mapping, defence, and 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ESA's Hera will survey the aftermath.","catalogNumbers":["(65803) Didymos I Dimorphos"],"sources":["nasa","jpl"]},{"id":"asteroid:toutatis","type":"asteroid","name":"4179 Toutatis","domain":"science","entryPath":"/asteroids/toutatis","description":"An elongated near-Earth asteroid in a chaotic, tumbling rotation, flown past by China's Chang'e 2 in 2012; it crosses both Earth's and Mars's orbits.","catalogNumbers":["(4179) Toutatis"],"sources":["nasa","jpl"]},{"id":"asteroid:geographos","type":"asteroid","name":"1620 Geographos","domain":"science","entryPath":"/asteroids/geographos","description":"One of the most elongated known asteroids, a near-Earth Apollo object well characterised by radar.","catalogNumbers":["(1620) Geographos"],"sources":["nasa","jpl"]},{"id":"asteroid:golevka","type":"asteroid","name":"6489 Golevka","domain":"science","entryPath":"/asteroids/golevka","description":"A small near-Earth Apollo asteroid on which the Yarkovsky effect — the tiny orbital push from 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traditionally named after Trojan heroes — including the binary 617 Patroclus.","sources":["nasa","jpl"]},{"id":"trojan_group:neptune-trojans","type":"trojan_group","name":"Neptune Trojans","domain":"science","entryPath":"/asteroids/trojans/neptune-trojans","description":"Minor planets sharing Neptune's orbit in a 1:1 resonance at its L4 and L5 points — a population thought to rival the Jupiter Trojans in number.","sources":["nasa","jpl"]},{"id":"orbital_resonance:jupiter-3-2","type":"orbital_resonance","name":"3:2 resonance with Jupiter","domain":"science","entryPath":"/asteroids/resonance/jupiter-3-2","description":"A mean-motion resonance in which a body completes three orbits for every two of Jupiter's, stabilising the Hilda group in the outer main belt.","sources":["nasa","jpl"]},{"id":"orbital_resonance:jupiter-1-1","type":"orbital_resonance","name":"1:1 resonance with Jupiter","domain":"science","entryPath":"/asteroids/resonance/jupiter-1-1","description":"The co-orbital 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33-year returns produce the periodic Leonid storms.","catalogNumbers":["55P/Tempel–Tuttle"],"sources":["nasa","jpl"]},{"id":"comet:giacobini-zinner","type":"comet","name":"Giacobini–Zinner","domain":"science","entryPath":"/comets/giacobini-zinner","description":"A Jupiter-family comet, parent of the Draconid meteor shower, and the first comet ever visited by a spacecraft — NASA's ICE probe flew through its tail in 1985.","catalogNumbers":["21P/Giacobini–Zinner"],"sources":["nasa","jpl"]},{"id":"comet:grigg-skjellerup","type":"comet","name":"Grigg–Skjellerup","domain":"science","entryPath":"/comets/grigg-skjellerup","description":"A Jupiter-family comet visited by ESA's Giotto in 1992 during its extended mission, after Giotto's earlier encounter with Halley.","catalogNumbers":["26P/Grigg–Skjellerup"],"sources":["esa","jpl"]},{"id":"comet:schwassmann-wachmann-3","type":"comet","name":"Schwassmann–Wachmann 3","domain":"science","entryPath":"/comets/schwassmann-wachmann-3","description":"A Jupiter-family comet that began fragmenting in 1995 and has since broken into dozens of pieces — a rare chance to watch a comet disintegrate over successive returns.","catalogNumbers":["73P/Schwassmann–Wachmann 3"],"sources":["nasa","jpl"]},{"id":"comet:hartley-2","type":"comet","name":"Hartley 2","domain":"science","entryPath":"/comets/hartley-2","description":"A small, hyperactive Jupiter-family comet flown past by NASA's EPOXI mission (the repurposed Deep Impact spacecraft) in 2010.","catalogNumbers":["103P/Hartley 2"],"sources":["nasa","jpl"]},{"id":"comet:mcnaught","type":"comet","name":"McNaught","domain":"science","entryPath":"/comets/mcnaught","description":"The 'Great Comet of 2007', the brightest comet in decades, whose vast fanned dust tail was a spectacular sight from the Southern Hemisphere.","catalogNumbers":["C/2006 P1 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rovers.","catalogNumbers":["C/2013 A1 (Siding Spring)"],"sources":["nasa","jpl"]},{"id":"comet:thatcher","type":"comet","name":"Thatcher","domain":"science","entryPath":"/comets/thatcher","description":"A long-period comet on a roughly 415-year orbit, the parent body of the Lyrid meteor shower seen each April.","catalogNumbers":["C/1861 G1 (Thatcher)"],"sources":["nasa","jpl"]},{"id":"comet_class:jupiter-family","type":"comet_class","name":"Jupiter-Family Comets","domain":"science","entryPath":"/comets/class/jupiter-family","description":"The most numerous class of periodic comets, whose orbits are shepherded by Jupiter and which originate in the scattered disc beyond Neptune.","aliases":["JFC"],"sources":["nasa","jpl"]},{"id":"comet_class:halley-type","type":"comet_class","name":"Halley-Type Comets","domain":"science","entryPath":"/comets/class/halley-type","description":"Periodic comets with orbits of decades to a couple of centuries, named for their prototype, Halley's 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Many belong to the Kreutz family and are discovered by solar observatories.","sources":["nasa","jpl"]},{"id":"comet_class:main-belt-comet","type":"comet_class","name":"Main-Belt Comets","domain":"science","entryPath":"/comets/class/main-belt-comet","description":"Objects that orbit within the asteroid belt yet develop tails or comae — a blurring of the traditional line between asteroids and comets, and a possible reservoir of water.","aliases":["MBC"],"sources":["nasa","jpl"]},{"id":"comet_family:kreutz-sungrazers","type":"comet_family","name":"Kreutz Sungrazers","domain":"science","entryPath":"/comets/family/kreutz-sungrazers","description":"A family of sungrazing comets on very similar orbits, thought to be the fragments of a single giant comet that broke apart many centuries ago. They include some of the brightest comets in history and are discovered in large numbers by solar spacecraft.","sources":["nasa"]},{"id":"small_body_reservoir:oort-cloud","type":"small_body_reservoir","name":"Oort Cloud","domain":"science","entryPath":"/comets/reservoir/oort-cloud","description":"A hypothesised spherical cloud of trillions of icy bodies at the outermost edge of the Sun's gravitational influence — the reservoir from which long-period and Halley-type comets are nudged inward.","sources":["nasa"]},{"id":"small_body_reservoir:inner-oort-cloud","type":"small_body_reservoir","name":"Inner Oort Cloud","domain":"science","entryPath":"/comets/reservoir/inner-oort-cloud","description":"The dense inner region of the Oort cloud, whose existence is inferred from detached objects like Sedna whose orbits are too distant to be shaped by Neptune.","sources":["nasa"]},{"id":"active_asteroid:phaethon","type":"active_asteroid","name":"3200 Phaethon","domain":"science","entryPath":"/comets/active/phaethon","description":"A near-Earth asteroid that brightens and sheds dust as it passes very close to the Sun — a 'rock comet' — and the parent body of the Geminid meteor shower, unusual for a shower whose source is an asteroid rather than a comet.","catalogNumbers":["(3200) Phaethon"],"sources":["nasa","jpl"]},{"id":"active_asteroid:elst-pizarro","type":"active_asteroid","name":"7968 Elst–Pizarro","domain":"science","entryPath":"/comets/active/elst-pizarro","description":"The prototype main-belt comet — an object on an ordinary asteroid-belt orbit that repeatedly develops a comet-like tail, carrying both an asteroid number and a comet designation.","aliases":["133P/Elst–Pizarro"],"catalogNumbers":["(7968) Elst–Pizarro"],"sources":["nasa","jpl"]},{"id":"dormant_comet:don-quixote","type":"dormant_comet","name":"3552 Don Quixote","domain":"science","entryPath":"/comets/dormant/don-quixote","description":"A large near-Earth object on a comet-like orbit long suspected to be a dormant comet; faint carbon-dioxide activity was detected in 2013, suggesting it is not fully extinct.","catalogNumbers":["(3552) Don Quixote"],"sources":["nasa","jpl"]},{"id":"dormant_comet:2003-eh1","type":"dormant_comet","name":"(196256) 2003 EH1","domain":"science","entryPath":"/comets/dormant/2003-eh1","description":"An asteroid on a short-period, comet-like orbit believed to be a dormant or extinct comet nucleus — the parent body of the sharp, brief Quadrantid meteor shower.","catalogNumbers":["(196256) 2003 EH1"],"sources":["nasa","jpl"]},{"id":"space_mission:giotto","type":"space_mission","name":"Giotto","domain":"science","description":"ESA's mission to Halley's Comet, which flew through the comet's coma in 1986 and returned the first close-up images of a cometary nucleus, later re-targeted to comet Grigg–Skjellerup.","sources":["esa"]},{"id":"space_mission:deep-impact","type":"space_mission","name":"Deep Impact","domain":"science","description":"NASA's mission that fired a 370-kg impactor into comet Tempel 1 in 2005 to excavate and study the material beneath a comet's surface.","sources":["nasa"]},{"id":"space_mission:stardust","type":"space_mission","name":"Stardust","domain":"science","description":"NASA's sample-return mission that captured dust from the coma of comet Wild 2 and returned it to Earth in 2006, and later flew past Tempel 1 as Stardust-NExT.","sources":["nasa"]},{"id":"space_mission:deep-space-1","type":"space_mission","name":"Deep Space 1","domain":"science","description":"NASA's ion-propulsion technology demonstrator that flew past comet Borrelly in 2001, returning detailed images of its nucleus.","aliases":["DS1"],"sources":["nasa"]},{"id":"space_mission:epoxi","type":"space_mission","name":"EPOXI","domain":"science","description":"The extended mission of the Deep Impact spacecraft, which flew past the small, hyperactive comet Hartley 2 in 2010.","sources":["nasa"]},{"id":"meteorite:allende","type":"meteorite","name":"Allende","domain":"science","entryPath":"/meteorites/allende","description":"The largest carbonaceous chondrite found on Earth, which fell in 1969 and became the most-studied meteorite in history — its calcium–aluminium inclusions are among the oldest solid material in the Solar System.","catalogNumbers":["CV3 carbonaceous chondrite"],"sources":["nasa"]},{"id":"meteorite:murchison","type":"meteorite","name":"Murchison","domain":"science","entryPath":"/meteorites/murchison","description":"A carbonaceous chondrite that fell in 1969 and was found to contain a rich suite of amino acids and other organic compounds — key evidence that the building blocks of life exist in space.","catalogNumbers":["CM2 carbonaceous chondrite"],"sources":["nasa"]},{"id":"meteorite:orgueil","type":"meteorite","name":"Orgueil","domain":"science","entryPath":"/meteorites/orgueil","description":"A rare, extremely primitive CI carbonaceous chondrite whose composition closely matches that of the Sun — a benchmark for the bulk composition of the Solar System.","catalogNumbers":["CI1 carbonaceous chondrite"],"sources":["nasa"]},{"id":"meteorite:tagish-lake","type":"meteorite","name":"Tagish Lake","domain":"science","entryPath":"/meteorites/tagish-lake","description":"An exceptionally pristine carbonaceous meteorite recovered frozen from a lake in 2000, preserving organic material with minimal terrestrial contamination.","catalogNumbers":["C2 (ungrouped) carbonaceous chondrite"],"sources":["nasa"]},{"id":"meteorite:aguas-zarcas","type":"meteorite","name":"Aguas Zarcas","domain":"science","entryPath":"/meteorites/aguas-zarcas","description":"A CM2 carbonaceous chondrite that fell in 2019, rapidly recovered and rich in organic compounds — sometimes called a 'second Murchison'.","catalogNumbers":["CM2 carbonaceous chondrite"],"sources":["nasa"]},{"id":"meteorite:winchcombe","type":"meteorite","name":"Winchcombe","domain":"science","entryPath":"/meteorites/winchcombe","description":"A carbonaceous chondrite whose 2021 fall was captured by camera networks, allowing its orbit to be traced and the sample to be recovered within days — one of the most pristine falls ever studied.","catalogNumbers":["CM2 carbonaceous chondrite"],"sources":["nasa"]},{"id":"meteorite:chelyabinsk","type":"meteorite","name":"Chelyabinsk","domain":"science","entryPath":"/meteorites/chelyabinsk","description":"The recovered stones from the 2013 Chelyabinsk airburst, an ordinary chondrite whose spectacular entry — filmed by countless dashcams — was the most damaging meteor event in modern history.","catalogNumbers":["LL5 ordinary chondrite"],"sources":["nasa"]},{"id":"meteorite:peekskill","type":"meteorite","name":"Peekskill","domain":"science","entryPath":"/meteorites/peekskill","description":"An ordinary chondrite whose 1992 fall was videotaped as a brilliant fireball across the eastern United States before it struck and damaged a parked car in Peekskill, New York.","catalogNumbers":["H6 ordinary chondrite"],"sources":["nasa"]},{"id":"meteorite:abee","type":"meteorite","name":"Abee","domain":"science","entryPath":"/meteorites/abee","description":"A large enstatite chondrite that fell in 1952 — a rare, highly reduced meteorite type thought to have formed in the innermost, oxygen-poor part of the solar nebula.","catalogNumbers":["EH4 enstatite chondrite"],"sources":["nasa"]},{"id":"meteorite:hoba","type":"meteorite","name":"Hoba","domain":"science","entryPath":"/meteorites/hoba","description":"The largest known intact meteorite and the largest naturally-occurring piece of iron near the Earth's surface, an ~60-tonne slab still lying where it was found in Namibia.","catalogNumbers":["IVB iron"],"sources":["nasa"]},{"id":"meteorite:sikhote-alin","type":"meteorite","name":"Sikhote-Alin","domain":"science","entryPath":"/meteorites/sikhote-alin","description":"One of the largest observed iron meteorite falls, which broke apart over the Sikhote-Alin mountains in 1947 and scattered thousands of fragments, many with dramatic regmaglypt thumbprint textures, across a strewn field.","catalogNumbers":["IIAB iron"],"sources":["nasa"]},{"id":"meteorite:campo-del-cielo","type":"meteorite","name":"Campo del Cielo","domain":"science","entryPath":"/meteorites/campo-del-cielo","description":"An ancient field of large iron meteorites in Argentina, known to indigenous peoples for millennia, whose fragments include some of the heaviest single meteorite masses ever recovered.","catalogNumbers":["IAB iron"],"sources":["nasa"]},{"id":"meteorite:willamette","type":"meteorite","name":"Willamette","domain":"science","entryPath":"/meteorites/willamette","description":"The largest meteorite ever found in the United States, an ~15-tonne iron sacred to the Clackamas people of the Willamette Valley.","catalogNumbers":["IIIAB iron"],"sources":["nasa"]},{"id":"meteorite:canyon-diablo","type":"meteorite","name":"Canyon Diablo","domain":"science","entryPath":"/meteorites/canyon-diablo","description":"The iron meteorite responsible for Barringer Crater (Meteor Crater) in Arizona; fragments are scattered around the rim of the crater it formed some 50,000 years ago.","catalogNumbers":["IAB iron"],"sources":["nasa"]},{"id":"meteorite:brenham","type":"meteorite","name":"Brenham","domain":"science","entryPath":"/meteorites/brenham","description":"A pallasite strewn field in Kansas — pallasites are among the most beautiful meteorites, with olive-green olivine crystals suspended in a matrix of nickel-iron.","catalogNumbers":["Pallasite"],"sources":["nasa"]},{"id":"meteorite:estherville","type":"meteorite","name":"Estherville","domain":"science","entryPath":"/meteorites/estherville","description":"A large mesosiderite that fell in 1879 — a stony-iron meteorite mixing metal with silicate fragments, thought to record a violent collision between differentiated asteroids.","catalogNumbers":["Mesosiderite"],"sources":["nasa"]},{"id":"meteorite:millbillillie","type":"meteorite","name":"Millbillillie","domain":"science","entryPath":"/meteorites/millbillillie","description":"A eucrite whose fall was witnessed in October 1960 (the stones recovered in the following years) — one of the HED meteorites, basaltic rocks blasted from the surface of the asteroid Vesta, whose spectra they match.","catalogNumbers":["Eucrite (HED)"],"sources":["nasa"]},{"id":"meteorite:nwa-7034","type":"meteorite","name":"NWA 7034","domain":"science","entryPath":"/meteorites/nwa-7034","description":"Nicknamed 'Black Beauty', a Martian breccia containing the most water of any Mars meteorite and some of the oldest Martian crust yet sampled.","aliases":["Black Beauty"],"catalogNumbers":["Martian (polymict breccia)"],"sources":["nasa"]},{"id":"meteorite:alh-84001","type":"meteorite","name":"ALH 84001","domain":"science","entryPath":"/meteorites/alh-84001","description":"A Martian meteorite recovered from Antarctica in 1984 and made famous in 1996 by a disputed claim that microscopic structures within it might be evidence of ancient Martian microbial life.","catalogNumbers":["Martian (orthopyroxenite)"],"sources":["nasa"]},{"id":"meteorite:alha-81005","type":"meteorite","name":"ALHA 81005","domain":"science","entryPath":"/meteorites/alha-81005","description":"The first meteorite recognised as a piece of the Moon, recovered from Antarctica in 1982 — its match to Apollo samples proved that lunar rocks can be delivered to Earth as meteorites.","catalogNumbers":["Lunar (anorthositic breccia)"],"sources":["nasa"]},{"id":"meteorite_class:chondrite","type":"meteorite_class","name":"Chondrites","domain":"science","entryPath":"/meteorites/class/chondrite","description":"The most common meteorites: primitive, undifferentiated stony rocks that preserve material from the birth of the Solar System, subdivided into carbonaceous, ordinary, and enstatite groups.","sources":["nasa"]},{"id":"meteorite_class:achondrite","type":"meteorite_class","name":"Achondrites","domain":"science","entryPath":"/meteorites/class/achondrite","description":"Stony meteorites from bodies that melted and differentiated — including basalts from the asteroid Vesta and rocks blasted off Mars and the Moon.","sources":["nasa"]},{"id":"meteorite_class:iron","type":"meteorite_class","name":"Iron Meteorites","domain":"science","entryPath":"/meteorites/class/iron","description":"Dense meteorites of nickel-iron alloy, thought to be fragments of the metallic cores of asteroids that were shattered by collisions — the source of the largest meteorites found on Earth.","sources":["nasa"]},{"id":"meteorite_class:stony-iron","type":"meteorite_class","name":"Stony-Iron Meteorites","domain":"science","entryPath":"/meteorites/class/stony-iron","description":"Rare meteorites blending rock and metal in roughly equal measure — the pallasites (olivine in metal) and mesosiderites (breccias of metal and silicate).","sources":["nasa"]},{"id":"meteorite_group:carbonaceous-chondrite","type":"meteorite_group","name":"Carbonaceous Chondrites","domain":"science","entryPath":"/meteorites/group/carbonaceous-chondrite","description":"Dark, primitive chondrites carrying carbon, water-bearing minerals, and complex organics — the closest samples we have to the raw ingredients of the Solar System, and to what asteroids like Bennu and Ryugu are made of.","sources":["nasa"]},{"id":"meteorite_group:ordinary-chondrite","type":"meteorite_group","name":"Ordinary Chondrites","domain":"science","entryPath":"/meteorites/group/ordinary-chondrite","description":"By far the most common meteorites to fall, these stony chondrites come from ordinary silicate asteroids in the inner belt.","sources":["nasa"]},{"id":"meteorite_group:enstatite-chondrite","type":"meteorite_group","name":"Enstatite Chondrites","domain":"science","entryPath":"/meteorites/group/enstatite-chondrite","description":"Rare, chemically reduced chondrites that formed in the innermost, oxygen-starved region of the solar nebula — a possible source of much of Earth's own building material.","sources":["nasa"]},{"id":"meteorite_group:hed","type":"meteorite_group","name":"HED Meteorites","domain":"science","entryPath":"/meteorites/group/hed","description":"The howardite–eucrite–diogenite clan of basaltic achondrites, whose spectra match the asteroid Vesta so closely that they are considered pieces of its crust, delivered to Earth after impacts.","sources":["nasa"]},{"id":"meteorite_group:martian","type":"meteorite_group","name":"Martian Meteorites","domain":"science","entryPath":"/meteorites/group/martian","description":"Rocks ejected from Mars by large impacts and later swept up by Earth — identified by trapped gases matching the composition measured in the Martian atmosphere by landers.","sources":["nasa"]},{"id":"meteorite_group:lunar","type":"meteorite_group","name":"Lunar Meteorites","domain":"science","entryPath":"/meteorites/group/lunar","description":"Pieces of the Moon flung to Earth by impacts, whose mineralogy matches the samples returned by the Apollo and Luna missions — a free supply of lunar rock from unsampled regions.","sources":["nasa"]},{"id":"meteorite_group:pallasite","type":"meteorite_group","name":"Pallasites","domain":"science","entryPath":"/meteorites/group/pallasite","description":"The most striking meteorites, in which gem-quality green olivine crystals are suspended in a lattice of nickel-iron — probably formed at the core–mantle boundary of a shattered asteroid.","sources":["nasa"]},{"id":"meteorite_group:mesosiderite","type":"meteorite_group","name":"Mesosiderites","domain":"science","entryPath":"/meteorites/group/mesosiderite","description":"Chaotic stony-iron breccias mixing crustal silicates with metallic core material — thought to record the catastrophic disruption and re-assembly of a differentiated asteroid.","sources":["nasa"]},{"id":"fireball:peekskill-fireball","type":"fireball","name":"Peekskill Fireball","domain":"science","entryPath":"/meteorites/fireball/peekskill-fireball","description":"A brilliant green fireball that crossed the eastern United States in October 1992, filmed by at least 16 people, before a fragment struck a parked car in Peekskill, New York — one of the best-documented fireball-to-meteorite events.","sources":["nasa"]},{"id":"fireball:bering-sea-fireball","type":"fireball","name":"Bering Sea Fireball","domain":"science","entryPath":"/meteorites/fireball/bering-sea-fireball","description":"A powerful bolide that exploded over the Bering Sea in December 2018 with roughly ten times the energy of the Hiroshima bomb — the largest airburst since Chelyabinsk, unnoticed at the time because it occurred over the remote ocean.","sources":["nasa"]},{"id":"impact_structure:barringer-crater","type":"impact_structure","name":"Barringer Crater (Meteor Crater)","domain":"science","entryPath":"/meteorites/impact-structure/barringer-crater","description":"The best-preserved impact crater on Earth, gouged out ~50,000 years ago by the Canyon Diablo iron meteorite — the site where the impact origin of craters was first firmly established.","aliases":["Meteor Crater"],"sources":["nasa"]},{"id":"impact_structure:vredefort","type":"impact_structure","name":"Vredefort Structure","domain":"science","entryPath":"/meteorites/impact-structure/vredefort","description":"The largest confirmed impact structure on Earth, the deeply eroded remnant of a crater formed roughly two billion years ago by one of the largest impacts in the planet's history.","sources":["nasa"]},{"id":"impact_structure:sudbury","type":"impact_structure","name":"Sudbury Basin","domain":"science","entryPath":"/meteorites/impact-structure/sudbury","description":"One of the oldest and largest known impact structures, whose ancient impact melt hosts some of the world's richest nickel and copper ore deposits.","sources":["nasa"]},{"id":"impact_structure:ries","type":"impact_structure","name":"Nördlinger Ries","domain":"science","entryPath":"/meteorites/impact-structure/ries","description":"A well-studied mid-sized impact crater in Germany whose shocked minerals and impact glass were used by Apollo astronauts as a training ground for recognising impact features on the Moon.","aliases":["Ries Crater"],"sources":["nasa"]},{"id":"recovery_site:sikhote-alin-field","type":"recovery_site","name":"Sikhote-Alin Strewn Field","domain":"science","entryPath":"/meteorites/site/sikhote-alin-field","description":"The strewn field left by the 1947 Sikhote-Alin iron meteorite fall, where thousands of fragments and impact pits were scattered across the taiga of the Russian Far East.","sources":["nasa"]},{"id":"recovery_site:campo-del-cielo-field","type":"recovery_site","name":"Campo del Cielo Field","domain":"science","entryPath":"/meteorites/site/campo-del-cielo-field","description":"A field of craters and large iron masses in northern Argentina, formed by an ancient fall and known to local peoples for thousands of years — the source of some of the heaviest meteorite masses on Earth.","sources":["nasa"]},{"id":"interstellar_object:oumuamua","type":"interstellar_object","name":"1I/ʻOumuamua","domain":"science","entryPath":"/interstellar-objects/oumuamua","description":"The first confirmed interstellar object, detected in October 2017 on its way out of the Solar System. Its strongly hyperbolic orbit (eccentricity about 1.2) showed it was never bound to the Sun. It displayed no visible coma, is highly elongated, and showed a slight non-gravitational acceleration — features that drew wide attention, though the scientific consensus is that it is a natural body.","aliases":["ʻOumuamua","1I/2017 U1","A/2017 U1"],"catalogNumbers":["1I/ʻOumuamua"],"sources":["mpc","jpl","nasa","ads"]},{"id":"interstellar_object:borisov","type":"interstellar_object","name":"2I/Borisov","domain":"science","entryPath":"/interstellar-objects/borisov","description":"The second confirmed interstellar object and the first that was unmistakably a comet, discovered in August 2019 by amateur astronomer Gennadiy Borisov. Its eccentricity of about 3.4 made its interstellar origin certain. Unlike 1I/ʻOumuamua it showed an active dust coma and tail, letting astronomers study the chemistry of a comet formed around another star; it proved unusually rich in carbon monoxide.","aliases":["2I/Borisov","C/2019 Q4 (Borisov)"],"catalogNumbers":["2I/Borisov"],"sources":["mpc","jpl","nasa","esa","eso"]},{"id":"interstellar_object:atlas-3i","type":"interstellar_object","name":"3I/ATLAS","domain":"science","entryPath":"/interstellar-objects/atlas-3i","description":"The third confirmed interstellar object, discovered on 1 July 2025 by the ATLAS survey in Chile. Its orbit is the most strongly hyperbolic of the three found so far, with an eccentricity of roughly 6, and it showed cometary activity as it passed through the inner Solar System in late 2025. Some physical parameters remain preliminary, but its interstellar origin is established by the trajectory.","aliases":["3I/ATLAS","C/2025 N1 (ATLAS)"],"catalogNumbers":["3I/ATLAS"],"sources":["mpc","jpl","nasa"]},{"id":"interstellar_candidate:cneos-2014-01-08","type":"interstellar_candidate","name":"CNEOS 2014-01-08","domain":"science","entryPath":"/interstellar-objects/cneos-2014-01-08","description":"A bright meteor (bolide) that entered Earth's atmosphere near Papua New Guinea on 8 January 2014, recorded in NASA CNEOS's fireball database. From the reported high velocity it was proposed in 2019 to have originated outside the Solar System, which would make it a candidate interstellar meteor. The claim is disputed: the underlying velocity data come from US Government sensors whose uncertainties are not public, and the interstellar interpretation is not accepted by the wider community. It is not a confirmed interstellar object.","aliases":["2014-01-08 bolide","IM1 (proposed name)"],"sources":["nasa","jpl","ads"]},{"id":"hyperbolic_comet:bowell","type":"hyperbolic_comet","name":"C/1980 E1 (Bowell)","domain":"science","entryPath":"/interstellar-objects/bowell","description":"A long-period comet that a close encounter with Jupiter in 1980 flung onto a clearly hyperbolic orbit (eccentricity about 1.06). It is now leaving the Solar System, but — unlike a true interstellar object — it formed here; the hyperbolic orbit is the result of a planetary slingshot, not an origin around another star.","aliases":["C/1980 E1","Comet Bowell"],"catalogNumbers":["C/1980 E1 (Bowell)"],"sources":["mpc","jpl","nasa"]},{"id":"hyperbolic_comet:linear-1999-s4","type":"hyperbolic_comet","name":"C/1999 S4 (LINEAR)","domain":"science","entryPath":"/interstellar-objects/linear-1999-s4","description":"A near-parabolic long-period comet from the Oort cloud, famous for disintegrating completely near perihelion in July 2000 — one of the best-observed comet break-ups. Its orbit was close to the parabolic boundary (eccentricity near 1), the hallmark of a first-time visitor from the distant Solar System, not from interstellar space.","aliases":["C/1999 S4","Comet LINEAR"],"catalogNumbers":["C/1999 S4 (LINEAR)"],"sources":["mpc","jpl","nasa"]},{"id":"hyperbolic_comet:boattini","type":"hyperbolic_comet","name":"C/2007 W1 (Boattini)","domain":"science","entryPath":"/interstellar-objects/boattini","description":"A long-period comet discovered by Andrea Boattini through the Mount Lemmon Survey, on a near-parabolic orbit with an eccentricity extremely close to 1. Like the other long-period comets here it is a distant Solar-System visitor, not an interstellar object: its original orbit is bound and it is not being ejected from the Solar System — the tiny excess over a parabola is an epoch-dependent, perturbed value.","aliases":["C/2007 W1","Comet Boattini"],"catalogNumbers":["C/2007 W1 (Boattini)"],"sources":["mpc","jpl","nasa"]},{"id":"hyperbolic_comet:panstarrs-k2","type":"hyperbolic_comet","name":"C/2017 K2 (PANSTARRS)","domain":"science","entryPath":"/interstellar-objects/panstarrs-k2","description":"A dynamically new, near-parabolic long-period comet discovered by Pan-STARRS in 2017 and notable for showing activity at a record distance — a coma was detected beyond Saturn's orbit, on the comet's first passage in from the Oort cloud. Its near-parabolic orbit marks it as a distant Solar-System visitor, not an interstellar object.","aliases":["C/2017 K2","Comet PANSTARRS K2"],"catalogNumbers":["C/2017 K2 (PANSTARRS)"],"sources":["mpc","jpl","nasa"]},{"id":"interstellar_detection_method:excess-hyperbolic-velocity","type":"interstellar_detection_method","name":"Excess Hyperbolic Velocity","domain":"science","entryPath":"/interstellar-objects/detection/excess-hyperbolic-velocity","description":"The primary signature of an interstellar object: its speed relative to the Sun exceeds the local escape velocity by enough that the orbit is strongly hyperbolic (eccentricity well above 1). A large hyperbolic excess velocity (v∞) cannot be produced by planetary perturbations, so it points to an origin outside the Solar System. A small excess, by contrast, can come from a planetary slingshot and does not by itself prove an interstellar origin.","aliases":["Excess velocity (v∞)","Hyperbolic excess speed"],"sources":["jpl","nasa","ads"]},{"id":"interstellar_detection_method:incoming-trajectory-analysis","type":"interstellar_detection_method","name":"Incoming-Trajectory Analysis","domain":"science","entryPath":"/interstellar-objects/detection/incoming-trajectory-analysis","description":"Determining an object's orbit from astrometry and tracing its path backward. An unbound, strongly hyperbolic incoming trajectory — arriving from interstellar space rather than from the planetary region — establishes that the object was not on a closed Solar orbit. The direction it came from (its radiant) can also be identified, though no specific parent star has been pinned down for any interstellar object.","aliases":["Orbit determination","Backward trajectory tracing"],"sources":["mpc","jpl","nasa"]},{"id":"interstellar_detection_method:spectroscopic-composition","type":"interstellar_detection_method","name":"Spectroscopic Composition Analysis","domain":"science","entryPath":"/interstellar-objects/detection/spectroscopic-composition","description":"Taking spectra and colours of a visitor to characterise its surface or coma chemistry and compare it with Solar-System comets and asteroids. Spectroscopy does not by itself prove an interstellar origin — the orbit does that — but it reveals what a body from another planetary system is made of, as with the carbon-monoxide-rich coma of 2I/Borisov.","aliases":["Spectroscopy","Compositional characterisation"],"sources":["eso","nasa","ads"]},{"id":"trajectory_class:bound-orbit","type":"trajectory_class","name":"Bound (Elliptical) Orbit","domain":"science","entryPath":"/interstellar-objects/trajectory/bound-orbit","description":"An orbit with eccentricity below 1: the object is gravitationally bound to the Sun and returns. Planets, asteroids, and periodic comets all follow bound elliptical orbits. A bound orbit is the baseline against which unbound, hyperbolic trajectories are recognised.","aliases":["Elliptical orbit","Closed orbit"],"sources":["jpl","nasa"]},{"id":"trajectory_class:near-parabolic","type":"trajectory_class","name":"Near-Parabolic Orbit","domain":"science","entryPath":"/interstellar-objects/trajectory/near-parabolic","description":"An orbit with eccentricity very close to 1 — the boundary between bound and unbound. Long-period comets falling in from the Oort cloud on their first passage follow near-parabolic orbits. A near-parabolic orbit signals a distant Solar-System origin, not an interstellar one.","aliases":["Parabolic orbit"],"sources":["jpl","nasa"]},{"id":"trajectory_class:hyperbolic-ejection","type":"trajectory_class","name":"Hyperbolic Orbit (Solar-System Origin)","domain":"science","entryPath":"/interstellar-objects/trajectory/hyperbolic-ejection","description":"An orbit with eccentricity just above 1, produced when a Solar-System comet is perturbed by a planet (usually Jupiter) onto an escape trajectory. The object is leaving the Solar System, but it formed here — the small excess over e = 1 is a slingshot effect, not evidence of an interstellar origin.","aliases":["Weakly hyperbolic orbit"],"sources":["jpl","nasa"]},{"id":"trajectory_class:interstellar-hyperbolic","type":"trajectory_class","name":"Interstellar Hyperbolic Trajectory","domain":"science","entryPath":"/interstellar-objects/trajectory/interstellar-hyperbolic","description":"A strongly hyperbolic trajectory — eccentricity well above 1 with a large excess velocity relative to the Sun — that cannot be produced by planetary perturbations. This is the signature of an interstellar object: a body that entered the Solar System already unbound, from another star system, and will leave on the same path. 1I/ʻOumuamua, 2I/Borisov, and 3I/ATLAS all follow such trajectories.","aliases":["Strongly hyperbolic trajectory"],"sources":["jpl","nasa","ads"]},{"id":"sky_survey:atlas","type":"sky_survey","name":"ATLAS","domain":"science","description":"The Asteroid Terrestrial-impact Last Alert System — a NASA-funded network of small survey telescopes, operated by the University of Hawaiʻi, that scans the whole visible sky nightly for moving objects and impact hazards. Its Chilean telescope discovered the third interstellar object, 3I/ATLAS, in 2025.","aliases":["Asteroid Terrestrial-impact Last Alert System"],"sources":["nasa","jpl"]},{"id":"sky_survey:catalina-sky-survey","type":"sky_survey","name":"Catalina Sky Survey","domain":"science","description":"A NASA-funded near-Earth-object survey based at the University of Arizona, using telescopes on Mount Lemmon and Mount Bigelow. It is a prolific discoverer of comets and near-Earth asteroids, including the hyperbolic long-period comet C/2007 W1 (Boattini).","aliases":["CSS","Mount Lemmon Survey"],"sources":["nasa","jpl"]},{"id":"organization:minor-planet-center","type":"organization","name":"Minor Planet Center","domain":"science","description":"The International Astronomical Union's clearinghouse for the astrometry, orbits, and designations of small Solar-System bodies — and of interstellar objects, to which it assigns the special \"I\" (interstellar) designations such as 1I, 2I, and 3I. It is operated under the auspices of the IAU.","aliases":["MPC","IAU Minor Planet Center"],"sources":["iau","mpc"]},{"id":"organization:cneos","type":"organization","name":"CNEOS","domain":"science","description":"NASA's Center for Near-Earth Object Studies, at the Jet Propulsion Laboratory, which computes near-Earth-object orbits and impact risk and maintains the public fireball database. Its reported velocity for the 2014-01-08 bolide is the basis of a debated — and unconfirmed — claim of an interstellar meteor.","aliases":["Center for Near-Earth Object Studies"],"sources":["nasa","jpl"]},{"id":"space_mission:mmx","type":"space_mission","name":"MMX (Martian Moons eXploration)","domain":"science","entryPath":"/small-body-missions/mmx","description":"JAXA's planned mission to the moons of Mars — it will study Phobos and Deimos and return a sample of Phobos to Earth, testing whether the Martian moons are captured asteroids or debris from a giant impact.","aliases":["Martian Moons eXploration"],"sources":["jaxa"]},{"id":"space_mission:comet-interceptor","type":"space_mission","name":"Comet Interceptor","domain":"science","entryPath":"/small-body-missions/comet-interceptor","description":"An ESA (with JAXA) fast-class mission that will wait at the Sun–Earth L2 point for a suitable target, then fly by a pristine, dynamically-new comet — ideally one entering the inner Solar System for the first time, or even an interstellar object.","sources":["esa"]},{"id":"space_mission:destiny-plus","type":"space_mission","name":"DESTINY+","domain":"science","entryPath":"/small-body-missions/destiny-plus","description":"A JAXA technology-demonstration and flyby mission that will test advanced ion propulsion en route to a flyby of 3200 Phaethon — the rock-comet source of the Geminid meteor shower — studying its dust.","sources":["jaxa"]},{"id":"space_mission:caesar","type":"space_mission","name":"CAESAR (concept)","domain":"science","entryPath":"/small-body-missions/caesar","description":"A NASA New Frontiers proposal to return a sample from comet 67P/Churyumov–Gerasimenko — the comet Rosetta explored. It was a finalist in the New Frontiers 4 competition but was not selected (Dragonfly was chosen instead).","aliases":["Comet Astrobiology Exploration Sample Return"],"sources":["nasa"]},{"id":"space_mission:don-quijote","type":"space_mission","name":"Don Quijote (concept)","domain":"science","entryPath":"/small-body-missions/don-quijote","description":"An early-2000s ESA planetary-defense concept — a two-spacecraft study in which an impactor (Hidalgo) would strike an asteroid while an orbiter (Sancho) measured the deflection. It was never built, but it prefigured the AIDA/DART–Hera approach.","sources":["esa"]},{"id":"space_mission:janus","type":"space_mission","name":"Janus (cancelled)","domain":"science","entryPath":"/small-body-missions/janus","description":"A NASA SIMPLEx pair of small spacecraft designed to fly by binary asteroids. Built to share Psyche's launch, the twins were left without a viable trajectory when Psyche slipped by a year, and the mission was cancelled with the spacecraft put into storage.","sources":["nasa"]},{"id":"space_mission:aim","type":"space_mission","name":"AIM (concept)","domain":"science","entryPath":"/small-body-missions/aim","description":"ESA's Asteroid Impact Mission — the original European orbiter half of the AIDA collaboration, meant to observe the DART impact in real time. It was not funded in 2016, but its science was largely revived and reshaped as the Hera mission.","aliases":["Asteroid Impact Mission"],"sources":["esa"]},{"id":"mission_class:flyby","type":"mission_class","name":"Flyby Mission","domain":"science","entryPath":"/small-body-missions/type/flyby","description":"A spacecraft that passes a small body once at high speed, gathering images and data during a brief encounter. Flybys are the cheapest way to reach a new target — Giotto at Halley, Deep Space 1 at Borrelly, Lucy at the Trojans.","sources":["nasa","esa"]},{"id":"mission_class:rendezvous","type":"mission_class","name":"Rendezvous Mission","domain":"science","entryPath":"/small-body-missions/type/rendezvous","description":"A spacecraft that matches a small body's orbit and stays with it for an extended study, rather than flying past. Rendezvous enables detailed mapping and, often, orbiting or landing.","sources":["nasa","esa"]},{"id":"mission_class:orbiter","type":"mission_class","name":"Orbiter Mission","domain":"science","entryPath":"/small-body-missions/type/orbiter","description":"A spacecraft that enters orbit around a small body to map it globally over time — NEAR at Eros, Dawn at Vesta and Ceres, Rosetta at comet 67P.","sources":["nasa","esa"]},{"id":"mission_class:lander","type":"mission_class","name":"Lander Mission","domain":"science","entryPath":"/small-body-missions/type/lander","description":"A spacecraft (or a deployed element) that touches down on a small body's surface — Philae on comet 67P, NEAR on Eros, and the touchdown sampling of Hayabusa and Hayabusa2.","sources":["nasa","esa","jaxa"]},{"id":"mission_class:impactor","type":"mission_class","name":"Impactor Mission","domain":"science","entryPath":"/small-body-missions/type/impactor","description":"A spacecraft (or a released projectile) that deliberately strikes a small body — to excavate subsurface material (Deep Impact) or to deflect it (DART).","sources":["nasa"]},{"id":"mission_class:sample-return","type":"mission_class","name":"Sample-Return Mission","domain":"science","entryPath":"/small-body-missions/type/sample-return","description":"A mission that collects material from a small body and brings it back to Earth for laboratory study — Hayabusa (Itokawa), Hayabusa2 (Ryugu), OSIRIS-REx (Bennu), and Stardust (comet Wild 2).","sources":["nasa","jaxa"]},{"id":"returned_sample:itokawa-sample","type":"returned_sample","name":"Itokawa Sample (Hayabusa)","domain":"science","entryPath":"/small-body-missions/sample/itokawa-sample","description":"More than 1,500 microscopic grains from the S-type asteroid 25143 Itokawa, returned by Hayabusa in 2010 — the first sample ever returned from an asteroid. The grains tied ordinary (LL) chondrite meteorites to S-type asteroids and showed signs of space weathering.","sources":["jaxa","nasa"]},{"id":"returned_sample:ryugu-sample","type":"returned_sample","name":"Ryugu Sample (Hayabusa2)","domain":"science","entryPath":"/small-body-missions/sample/ryugu-sample","description":"5.4 grams of surface and subsurface material from the carbonaceous asteroid 162173 Ryugu, returned by Hayabusa2 in 2020. The pristine, water- and organic-bearing grains contain amino acids and predate the Solar System's planets.","sources":["jaxa","nasa"]},{"id":"returned_sample:bennu-sample","type":"returned_sample","name":"Bennu Sample (OSIRIS-REx)","domain":"science","entryPath":"/small-body-missions/sample/bennu-sample","description":"121.6 grams of dust and rock from the carbonaceous near-Earth asteroid 101955 Bennu, returned by OSIRIS-REx in 2023 — the largest asteroid sample yet returned. Early analysis shows abundant carbon and water-bearing clay minerals.","sources":["nasa","jpl"]},{"id":"returned_sample:wild-2-sample","type":"returned_sample","name":"Wild 2 Sample (Stardust)","domain":"science","entryPath":"/small-body-missions/sample/wild-2-sample","description":"Thousands of cometary dust particles captured in aerogel as Stardust flew through the coma of comet 81P/Wild 2, returned in 2006 — the first cometary material and the first sample from beyond the Moon. The grains revealed high-temperature minerals and the amino acid glycine.","sources":["nasa","jpl"]},{"id":"sample_return_capsule:hayabusa-src","type":"sample_return_capsule","name":"Hayabusa Sample-Return Capsule","domain":"science","description":"The small heat-shielded capsule that carried Hayabusa's Itokawa grains back through the atmosphere, separating from the spacecraft (which burned up) and landing by parachute in the Australian outback.","sources":["jaxa"]},{"id":"sample_return_capsule:hayabusa2-src","type":"sample_return_capsule","name":"Hayabusa2 Sample-Return Capsule","domain":"science","description":"The reentry capsule that returned Hayabusa2's 5.4 g of Ryugu material, recovered in the Australian desert while the spacecraft continued on to an extended mission.","sources":["jaxa"]},{"id":"sample_return_capsule:osiris-rex-src","type":"sample_return_capsule","name":"OSIRIS-REx Sample-Return Capsule","domain":"science","description":"The capsule that delivered 121.6 g of asteroid Bennu to Earth, released by OSIRIS-REx on a flyby before the spacecraft diverted toward Apophis.","sources":["nasa"]},{"id":"sample_return_capsule:stardust-src","type":"sample_return_capsule","name":"Stardust Sample-Return Capsule","domain":"science","description":"The capsule that returned Stardust's aerogel trays of comet Wild 2 dust — the first sample-return capsule to bring material back from beyond the Moon.","sources":["nasa","jpl"]},{"id":"mission_phase:launch-and-cruise","type":"mission_phase","name":"Launch & Cruise","domain":"science","description":"The launch and the long interplanetary cruise to the target, often using gravity assists or ion propulsion to reach a distant small body.","sources":["nasa","esa"]},{"id":"mission_phase:approach-and-characterization","type":"mission_phase","name":"Approach & Characterization","domain":"science","description":"The final approach, when the target grows from a point of light into a resolved world and the spacecraft measures its shape, spin, and gravity to plan operations.","sources":["nasa","esa"]},{"id":"mission_phase:proximity-operations","type":"mission_phase","name":"Proximity Operations","domain":"science","description":"Extended operations close to the body — global mapping, orbiting, and selecting sites for a landing, sampling, or impact.","sources":["nasa","jaxa"]},{"id":"mission_phase:surface-operations","type":"mission_phase","name":"Surface Operations & Sampling","domain":"science","description":"The critical interaction with the surface — a touchdown, a landing, a sample-collection manoeuvre, or a deliberate impact.","sources":["nasa","jaxa"]},{"id":"mission_phase:return-and-reentry","type":"mission_phase","name":"Return & Reentry","domain":"science","description":"For sample-return missions, the journey home and the high-speed atmospheric reentry of the capsule to a recovery site — the phase that delivers the science to Earth.","sources":["nasa","jaxa"]},{"id":"science_campaign:aida","type":"science_campaign","name":"AIDA","domain":"science","description":"The Asteroid Impact and Deflection Assessment — an international collaboration to test and characterise asteroid deflection at the Didymos–Dimorphos binary. NASA's DART performed the kinetic impact in 2022; ESA's Hera will survey the result in detail, together turning a one-off experiment into a repeatable, well-understood technique.","aliases":["Asteroid Impact and Deflection Assessment"],"sources":["nasa","esa"]},{"id":"tracking_network:chinese-deep-space-network","type":"tracking_network","name":"Chinese Deep Space Network","domain":"science","entryPath":"/deep-space-network/network/chinese-deep-space-network","description":"China's deep-space tracking network, operated for CNSA, with large antennas at Jiamusi (66 m) and Kashgar (35 m) in China and a station in Argentina. It supports China's lunar (Chang'e) and planetary (Tianwen) missions.","aliases":["CDSN"],"sources":["nasa"]},{"id":"tracking_network:russian-deep-space-network","type":"tracking_network","name":"Russian Deep Space Network","domain":"science","entryPath":"/deep-space-network/network/russian-deep-space-network","description":"Russia's deep-space communication facilities, operated by Roscosmos, with large antennas at Ussuriysk in the Far East and historically at Bear Lakes and Yevpatoria (Crimea). It descends from the Soviet deep-space network that supported the Luna, Venera, and Mars probes.","aliases":["RDSN"],"sources":["nasa"]},{"id":"tracking_network:indian-deep-space-network","type":"tracking_network","name":"Indian Deep Space Network","domain":"science","entryPath":"/deep-space-network/network/indian-deep-space-network","description":"ISRO's deep-space network, centred on the 32 m and 18 m antennas at Byalalu near Bengaluru. It provided tracking and communication for the Chandrayaan lunar missions and the Mars Orbiter Mission (Mangalyaan).","aliases":["IDSN"],"sources":["nasa"]},{"id":"tracking_network:jaxa-deep-space-network","type":"tracking_network","name":"JAXA Deep Space Network","domain":"science","entryPath":"/deep-space-network/network/jaxa-deep-space-network","description":"Japan's deep-space tracking network, run by JAXA/ISAS, centred on the Usuda Deep Space Center in Nagano (a 64 m antenna) and the newer 54 m Misasa antenna. It supported the Hayabusa asteroid missions and Japan's other deep-space probes.","aliases":["Usuda Deep Space Center"],"sources":["jaxa"]},{"id":"tracking_network:commercial-deep-space","type":"tracking_network","name":"Commercial Deep-Space Services","domain":"science","entryPath":"/deep-space-network/network/commercial-deep-space","description":"A growing set of commercial providers — such as KSAT, SSC, and Goonhilly — that offer deep-space and near-Earth ground-station support on a service basis, augmenting the government networks as mission traffic grows. NASA's Near Space Network increasingly buys commercial services alongside its own antennas.","aliases":["Commercial ground-station networks"],"sources":["nasa"]},{"id":"tracking_station:goldstone","type":"tracking_station","name":"Goldstone Deep Space Communications Complex","domain":"science","entryPath":"/deep-space-network/station/goldstone","description":"The US complex of NASA's Deep Space Network, in California's Mojave Desert. Its 70 m antenna (DSS-14, the 'Mars' dish) and a cluster of 34 m beam-waveguide antennas track spacecraft across the Solar System.","sources":["nasa","jpl"]},{"id":"tracking_station:madrid","type":"tracking_station","name":"Madrid Deep Space Communications Complex","domain":"science","entryPath":"/deep-space-network/station/madrid","description":"The European complex of NASA's Deep Space Network, outside Madrid. With Goldstone and Canberra it forms the three-station ring that keeps deep-space missions continuously in view.","sources":["nasa","jpl"]},{"id":"tracking_station:canberra","type":"tracking_station","name":"Canberra Deep Space Communication Complex","domain":"science","entryPath":"/deep-space-network/station/canberra","description":"The southern-hemisphere complex of NASA's Deep Space Network, in Australia. Its 70 m antenna (DSS-43) is the only one able to command Voyager 2 on its southward interstellar trajectory.","sources":["nasa","jpl"]},{"id":"tracking_station:new-norcia","type":"tracking_station","name":"New Norcia Station","domain":"science","entryPath":"/deep-space-network/station/new-norcia","description":"ESA's first deep-space antenna (DSA 1), a 35 m dish in Western Australia, supporting Estrack's interplanetary missions.","aliases":["DSA 1"],"sources":["esa"]},{"id":"tracking_station:cebreros","type":"tracking_station","name":"Cebreros Station","domain":"science","entryPath":"/deep-space-network/station/cebreros","description":"ESA's second deep-space antenna (DSA 2), a 35 m dish in central Spain.","aliases":["DSA 2"],"sources":["esa"]},{"id":"tracking_station:malargue","type":"tracking_station","name":"Malargüe Station","domain":"science","entryPath":"/deep-space-network/station/malargue","description":"ESA's third deep-space antenna (DSA 3), a 35 m dish in Argentina — the southern-hemisphere member of Estrack's deep-space trio.","aliases":["DSA 3"],"sources":["esa"]},{"id":"tracking_station:maspalomas","type":"tracking_station","name":"Maspalomas Station","domain":"science","entryPath":"/deep-space-network/station/maspalomas","description":"An Estrack ground station in the Canary Islands, used for launch and early-orbit support and near-Earth tracking.","sources":["esa"]},{"id":"tracking_station:jiamusi","type":"tracking_station","name":"Jiamusi Station","domain":"science","entryPath":"/deep-space-network/station/jiamusi","description":"China's 66 m deep-space antenna in the northeast, a principal station of the Chinese Deep Space Network for lunar and planetary missions.","sources":["nasa"]},{"id":"tracking_station:kashgar","type":"tracking_station","name":"Kashgar Station","domain":"science","entryPath":"/deep-space-network/station/kashgar","description":"China's western deep-space station, with a cluster of 35 m antennas, part of the Chinese Deep Space Network.","sources":["nasa"]},{"id":"tracking_station:ussuriysk","type":"tracking_station","name":"Ussuriysk Station","domain":"science","entryPath":"/deep-space-network/station/ussuriysk","description":"A Russian deep-space tracking station in the Far East, part of the network that descends from the Soviet-era deep-space facilities.","sources":["nasa"]},{"id":"tracking_station:byalalu","type":"tracking_station","name":"Byalalu Station (IDSN)","domain":"science","entryPath":"/deep-space-network/station/byalalu","description":"ISRO's Indian Deep Space Network station near Bengaluru, whose 32 m antenna supported the Chandrayaan and Mars Orbiter missions.","aliases":["Indian Deep Space Network station"],"sources":["nasa"]},{"id":"tracking_station:usuda","type":"tracking_station","name":"Usuda Deep Space Center","domain":"science","entryPath":"/deep-space-network/station/usuda","description":"JAXA's 64 m deep-space antenna in Nagano, which supported the Hayabusa asteroid missions and Japan's other deep-space probes.","sources":["jaxa"]},{"id":"ground_station:white-sands","type":"ground_station","name":"White Sands Complex","domain":"science","entryPath":"/deep-space-network/station/white-sands","description":"NASA's primary ground terminal for the TDRS relay satellites, in New Mexico. Nearly all Space Network traffic — including from the ISS and Hubble — passes through White Sands.","sources":["nasa"]},{"id":"ground_station:svalbard","type":"ground_station","name":"Svalbard Satellite Station","domain":"science","entryPath":"/deep-space-network/station/svalbard","description":"A high-latitude ground station at 78°N able to see every pass of a polar-orbiting satellite. Operated commercially by KSAT and used by NASA's Near Space Network.","aliases":["SvalSat"],"sources":["nasa"]},{"id":"ground_station:alaska-satellite-facility","type":"ground_station","name":"Alaska Satellite Facility","domain":"science","entryPath":"/deep-space-network/station/alaska-satellite-facility","description":"A high-latitude ground station in Fairbanks, part of NASA's Near Space Network, heavily used for polar-orbiting Earth-observation satellites.","sources":["nasa"]},{"id":"ground_station:wallops-ground-station","type":"ground_station","name":"Wallops Ground Station","domain":"science","entryPath":"/deep-space-network/station/wallops-ground-station","description":"A NASA Near Space Network ground station on the US east coast, providing tracking and data services for near-Earth missions (distinct from the co-located Wallops launch range).","sources":["nasa"]},{"id":"antenna:seventy-metre","type":"antenna","name":"70-metre Antenna","domain":"science","entryPath":"/deep-space-network/antenna/seventy-metre","description":"The largest and most sensitive dishes of the Deep Space Network — one at each complex (Goldstone, Madrid, Canberra). Their huge collecting area is reserved for the most distant or weakest spacecraft, such as the Voyagers, and for radar astronomy.","sources":["nasa","jpl"]},{"id":"antenna:thirty-four-metre-beam-waveguide","type":"antenna","name":"34-metre Beam-Waveguide Antenna","domain":"science","entryPath":"/deep-space-network/antenna/thirty-four-metre-beam-waveguide","description":"The modern workhorse antennas of the Deep Space Network. A beam-waveguide design routes the signal through mirrors to equipment in a shielded room below, allowing several to be arrayed and supporting X- and Ka-band.","aliases":["34 m BWG"],"sources":["nasa","jpl"]},{"id":"antenna:thirty-four-metre-high-efficiency","type":"antenna","name":"34-metre High-Efficiency Antenna","domain":"science","entryPath":"/deep-space-network/antenna/thirty-four-metre-high-efficiency","description":"An earlier generation of 34 m Deep Space Network antenna with the feed at the dish, being gradually retired in favour of the beam-waveguide design.","aliases":["34 m HEF"],"sources":["nasa","jpl"]},{"id":"antenna:phased-array","type":"antenna","name":"Phased-Array Antenna","domain":"science","entryPath":"/deep-space-network/antenna/phased-array","description":"Instead of one large dish, many smaller antennas whose signals are combined electronically to act as a single larger aperture. Arraying is a future direction for the Deep Space Network, offering flexible, scalable collecting area.","sources":["nasa","jpl"]},{"id":"antenna:spacecraft-high-gain","type":"antenna","name":"High-Gain Antenna (Spacecraft)","domain":"science","entryPath":"/deep-space-network/antenna/spacecraft-high-gain","description":"The main dish on a spacecraft, which focuses its signal into a narrow, high-gain beam that must be pointed accurately at Earth. It carries the high-rate science downlink — for example Voyager's 3.7 m dish.","aliases":["HGA"],"sources":["nasa","jpl"]},{"id":"antenna:spacecraft-medium-gain","type":"antenna","name":"Medium-Gain Antenna (Spacecraft)","domain":"science","entryPath":"/deep-space-network/antenna/spacecraft-medium-gain","description":"A spacecraft antenna with a broader beam than the high-gain dish, trading data rate for easier pointing — useful during manoeuvres or as a backup.","aliases":["MGA"],"sources":["nasa","jpl"]},{"id":"antenna:spacecraft-low-gain","type":"antenna","name":"Low-Gain Antenna (Spacecraft)","domain":"science","entryPath":"/deep-space-network/antenna/spacecraft-low-gain","description":"A near-omnidirectional spacecraft antenna that needs no accurate pointing, used for command and low-rate telemetry — the safety-net link that works even when a spacecraft has lost attitude control.","aliases":["LGA"],"sources":["nasa","jpl"]},{"id":"antenna:laser-communication-terminal","type":"antenna","name":"Laser Communication Terminal","domain":"science","entryPath":"/deep-space-network/antenna/laser-communication-terminal","description":"An optical (laser) communication terminal that transmits data on an infrared beam rather than radio. NASA's Deep Space Optical Communications terminal flew on the Psyche spacecraft and set deep-space data-rate records.","sources":["nasa","jpl"]},{"id":"signal_band:s-band","type":"signal_band","name":"S-band","domain":"science","entryPath":"/deep-space-network/band/s-band","description":"A lower-frequency microwave band long used for spacecraft command and low-rate telemetry, and for near-Earth links. Robust and less affected by weather than higher bands, but limited in data rate.","sources":["nasa","jpl"]},{"id":"signal_band:x-band","type":"signal_band","name":"X-band","domain":"science","entryPath":"/deep-space-network/band/x-band","description":"The workhorse band of deep-space communication and radiometric navigation. Most interplanetary missions send their science data and are tracked on X-band, which balances data rate against antenna size and weather losses.","sources":["nasa","jpl"]},{"id":"signal_band:ka-band","type":"signal_band","name":"Ka-band","domain":"science","entryPath":"/deep-space-network/band/ka-band","description":"A higher-frequency band that carries much more data than X-band for the same antenna, at the cost of greater sensitivity to rain and pointing. Increasingly used for high-rate science downlink from deep space.","sources":["nasa","jpl"]},{"id":"signal_band:uhf","type":"signal_band","name":"UHF","domain":"science","entryPath":"/deep-space-network/band/uhf","description":"An ultra-high-frequency band used for short-range proximity links — for example between a Mars rover and an orbiter that relays the data to Earth — rather than for direct deep-space communication.","sources":["nasa","jpl"]},{"id":"signal_band:optical","type":"signal_band","name":"Optical (Laser)","domain":"science","entryPath":"/deep-space-network/band/optical","description":"Laser communication encodes data on an infrared beam instead of radio waves. Its far shorter wavelength packs data into a tighter beam, promising data rates 10–100× higher than radio — the frontier of deep-space communication, demonstrated by DSOC on the Psyche spacecraft.","sources":["nasa","jpl"]},{"id":"navigation_system:radiometric-navigation","type":"navigation_system","name":"Radiometric Navigation","domain":"science","entryPath":"/deep-space-network/navigation/radiometric-navigation","description":"Measuring a spacecraft's distance and velocity from its radio signal — range from the round-trip signal time, and line-of-sight velocity from the Doppler shift. Combined over time from the ground stations, these fix a spacecraft's trajectory across the Solar System.","sources":["nasa","jpl"]},{"id":"navigation_system:delta-dor","type":"navigation_system","name":"Delta-DOR","domain":"science","entryPath":"/deep-space-network/navigation/delta-dor","description":"A precise angular-position technique: two widely separated stations record the spacecraft's signal and that of a distant quasar, and the tiny difference in arrival times pins down the spacecraft's position on the sky to a few nanoradians — vital for accurate planetary arrivals.","aliases":["Delta Differential One-way Ranging"],"sources":["nasa","jpl","esa"]},{"id":"navigation_system:optical-navigation","type":"navigation_system","name":"Optical Navigation","domain":"science","entryPath":"/deep-space-network/navigation/optical-navigation","description":"Using a spacecraft's own camera images of a target body against the background stars to determine its position relative to that body — essential in the final approach to an asteroid, comet, or moon, where ground tracking alone is not precise enough.","sources":["nasa","jpl"]},{"id":"navigation_system:autonomous-navigation","type":"navigation_system","name":"Autonomous Navigation","domain":"science","entryPath":"/deep-space-network/navigation/autonomous-navigation","description":"Onboard software that processes optical-navigation images in real time and steers the spacecraft itself, without waiting for commands from Earth. It was pioneered by Deep Space 1 and used for terminal guidance in fast flybys and the DART impact.","aliases":["AutoNav"],"sources":["nasa","jpl"]},{"id":"navigation_system:star-tracker","type":"navigation_system","name":"Star Tracker","domain":"science","entryPath":"/deep-space-network/navigation/star-tracker","description":"A small camera that identifies star patterns to determine which way a spacecraft is pointed, to a fraction of an arcsecond. Star trackers give the precise attitude a spacecraft needs to aim its high-gain antenna at Earth and its instruments at a target.","sources":["nasa","jpl"]},{"id":"navigation_system:inertial-navigation","type":"navigation_system","name":"Inertial Navigation","domain":"science","entryPath":"/deep-space-network/navigation/inertial-navigation","description":"Gyroscopes and accelerometers in an inertial measurement unit that sense a spacecraft's rotation and acceleration, propagating its orientation between star-tracker updates and through manoeuvres when other references are unavailable.","aliases":["IMU"],"sources":["nasa","jpl"]},{"id":"navigation_system:deep-space-atomic-clock","type":"navigation_system","name":"Deep Space Atomic Clock","domain":"science","entryPath":"/deep-space-network/navigation/deep-space-atomic-clock","description":"A miniaturised, ultra-stable atomic clock small enough to fly on a spacecraft. By putting precise timekeeping onboard, it enables one-way radiometric navigation — the spacecraft can determine its own position without the round-trip to a ground clock — a technology demonstrated in Earth orbit.","aliases":["DSAC"],"sources":["nasa","jpl"]},{"id":"time_standard:tai","type":"time_standard","name":"International Atomic Time (TAI)","domain":"science","description":"A continuous atomic timescale kept by hundreds of atomic clocks worldwide — the stable foundation from which civil time is derived. TAI never inserts leap seconds, making it ideal for measuring precise intervals.","aliases":["TAI"],"sources":["nasa"]},{"id":"time_standard:utc","type":"time_standard","name":"Coordinated Universal Time (UTC)","domain":"science","description":"The civil time standard, derived from International Atomic Time but kept within a second of the Earth's rotation by occasional leap seconds. Deep-space tracking tags its measurements in UTC.","aliases":["UTC"],"sources":["nasa"]},{"id":"time_standard:gps-time","type":"time_standard","name":"GPS Time","domain":"science","description":"The continuous timescale of the Global Positioning System, offset from TAI by a fixed number of seconds and widely used to synchronise ground equipment.","sources":["nasa"]},{"id":"time_standard:spacecraft-clock","type":"time_standard","name":"Spacecraft Clock (SCLK)","domain":"science","description":"The onboard counter that timestamps a spacecraft's data. Because it drifts relative to ground time, mission teams maintain a correlation (SCLK-to-ground time) using the tracking network so that events can be placed on a common timescale.","aliases":["SCLK"],"sources":["nasa","jpl"]},{"id":"communication_system:dsoc","type":"communication_system","name":"Deep Space Optical Communications (DSOC)","domain":"science","description":"NASA's technology demonstration of laser communication from deep space, flying as a rider on the Psyche spacecraft. It transmitted data over tens of millions of kilometres at rates far beyond radio, proving optical links for future missions.","aliases":["DSOC"],"sources":["nasa","jpl"]},{"id":"communication_system:lcrd","type":"communication_system","name":"Laser Communications Relay Demonstration (LCRD)","domain":"science","description":"A NASA optical-communication relay in geostationary orbit that demonstrates two-way laser links between ground stations and spacecraft, a stepping stone toward operational optical relays in the Near Space Network.","aliases":["LCRD"],"sources":["nasa"]},{"id":"communication_system:tdrs","type":"communication_system","name":"Tracking and Data Relay Satellite System (TDRS)","domain":"science","description":"A fleet of geostationary relay satellites that give near-Earth spacecraft — including the ISS and Hubble — near-continuous contact with the ground, instead of only during the few minutes of a ground-station pass. TDRS is the space-based half of NASA's Near Space Network.","aliases":["TDRS","Space Network"],"sources":["nasa"]},{"id":"communication_system:telemetry-tracking-command","type":"communication_system","name":"Telemetry, Tracking & Command (TT&C)","domain":"science","description":"The end-to-end function every mission depends on: downlinking telemetry (spacecraft health and science), measuring the signal for tracking and navigation, and uplinking commands. The deep-space and near-Earth networks exist to provide TT&C.","aliases":["TT&C"],"sources":["nasa","jpl"]},{"id":"space_weather_phenomenon:solar-wind","type":"space_weather_phenomenon","name":"Solar Wind","domain":"science","entryPath":"/space-environment/solar-wind","description":"The continuous stream of charged particles — mostly protons and electrons — that flows outward from the Sun's corona at hundreds of kilometres per second, filling the Solar System and shaping planetary magnetospheres.","sources":["nasa","noaa"]},{"id":"space_weather_phenomenon:solar-flare","type":"space_weather_phenomenon","name":"Solar Flare","domain":"science","entryPath":"/space-environment/solar-flare","description":"A sudden, intense burst of radiation from the Sun's surface, released when magnetic energy in the corona is explosively reconfigured. The X-rays arrive in minutes and can ionise Earth's upper atmosphere, causing radio blackouts.","sources":["nasa","noaa"]},{"id":"space_weather_phenomenon:coronal-mass-ejection","type":"space_weather_phenomenon","name":"Coronal Mass Ejection (CME)","domain":"science","entryPath":"/space-environment/coronal-mass-ejection","description":"An enormous eruption of magnetised plasma from the Sun's corona, launching billions of tonnes of material into space. When aimed at Earth, a CME can drive the largest geomagnetic storms one to three days later.","aliases":["CME"],"sources":["nasa","noaa"]},{"id":"space_weather_phenomenon:geomagnetic-storm","type":"space_weather_phenomenon","name":"Geomagnetic Storm","domain":"science","entryPath":"/space-environment/geomagnetic-storm","description":"A temporary disturbance of Earth's magnetosphere, driven by the arrival of a fast solar wind or a coronal mass ejection. Strong storms can disrupt satellites, power grids, and navigation, and drive bright auroras.","sources":["noaa","nasa"]},{"id":"space_weather_phenomenon:aurora","type":"space_weather_phenomenon","name":"Aurora","domain":"science","entryPath":"/space-environment/aurora","description":"The glow produced when energetic particles from the magnetosphere spiral down Earth's magnetic-field lines and excite gases in the upper atmosphere — the visible signature of space weather over the polar regions.","aliases":["Northern & Southern Lights"],"sources":["nasa","noaa"]},{"id":"space_weather_phenomenon:magnetosphere","type":"space_weather_phenomenon","name":"Magnetosphere","domain":"science","entryPath":"/space-environment/magnetosphere","description":"The region around a planet dominated by its magnetic field, which deflects the solar wind and traps charged particles. Earth's magnetosphere shields the surface from most space radiation.","sources":["nasa"]},{"id":"space_weather_phenomenon:heliosphere","type":"space_weather_phenomenon","name":"Heliosphere","domain":"science","entryPath":"/space-environment/heliosphere","description":"The vast bubble of solar wind and magnetic field that surrounds the entire Solar System, carving out a cavity in the surrounding interstellar medium and shielding the planets from a fraction of the galactic cosmic rays.","sources":["nasa"]},{"id":"space_weather_phenomenon:heliopause","type":"space_weather_phenomenon","name":"Heliopause","domain":"science","entryPath":"/space-environment/heliopause","description":"The outer boundary of the heliosphere, where the outward pressure of the solar wind balances the pressure of the interstellar medium — the edge of the Sun's domain, crossed by the two Voyager spacecraft.","sources":["nasa"]},{"id":"radiation_environment:cosmic-rays","type":"radiation_environment","name":"Cosmic Rays","domain":"science","entryPath":"/space-environment/cosmic-rays","description":"High-energy charged particles that stream through space near the speed of light. They come from the Sun (solar energetic particles) and from beyond the Solar System (galactic cosmic rays), and are a primary radiation hazard for astronauts.","sources":["nasa"]},{"id":"radiation_environment:galactic-cosmic-rays","type":"radiation_environment","name":"Galactic Cosmic Rays (GCR)","domain":"science","entryPath":"/space-environment/galactic-cosmic-rays","description":"Extremely energetic charged particles from outside the Solar System — the remnants of supernovae and other violent events. They pervade deep space, are hard to shield against, and pose the dominant long-term radiation risk on missions to Mars.","aliases":["GCR"],"sources":["nasa"]},{"id":"radiation_environment:solar-energetic-particles","type":"radiation_environment","name":"Solar Energetic Particles (SEP)","domain":"science","entryPath":"/space-environment/solar-energetic-particles","description":"Bursts of high-energy particles accelerated by solar flares and coronal mass ejections. Unlike the steady galactic cosmic rays, SEP events are sudden and can deliver a dangerous radiation dose to astronauts within hours.","aliases":["SEP"],"sources":["nasa","noaa"]},{"id":"radiation_environment:van-allen-belts","type":"radiation_environment","name":"Van Allen Radiation Belts","domain":"science","entryPath":"/space-environment/van-allen-belts","description":"Two (sometimes more) doughnut-shaped zones of energetic charged particles trapped by Earth's magnetic field. Spacecraft crossing the belts — and those in orbits within them — must be hardened against the intense radiation.","aliases":["Radiation belts"],"sources":["nasa"]},{"id":"space_hazard:orbital-debris","type":"space_hazard","name":"Orbital Debris","domain":"science","entryPath":"/space-environment/orbital-debris","description":"Defunct satellites, spent rocket stages, and fragments left in Earth orbit. Travelling at kilometres per second, even a small piece can destroy a working spacecraft, and collisions create more debris — a growing hazard in low Earth orbit.","aliases":["Space junk"],"sources":["nasa","esa"]},{"id":"space_hazard:micrometeoroids","type":"space_hazard","name":"Micrometeoroids","domain":"science","entryPath":"/space-environment/micrometeoroids","description":"Tiny natural particles — grains of comet and asteroid dust — moving at tens of kilometres per second. They erode surfaces and can puncture spacecraft; together with orbital debris they define the impact hazard for spacecraft.","sources":["nasa"]},{"id":"space_hazard:spacecraft-charging","type":"space_hazard","name":"Spacecraft Charging","domain":"science","entryPath":"/space-environment/spacecraft-charging","description":"The build-up of electric charge on a spacecraft as it moves through the space plasma, especially during geomagnetic storms. A sudden discharge can damage electronics — a leading cause of space-weather-related spacecraft anomalies.","sources":["nasa"]},{"id":"space_hazard:atomic-oxygen","type":"space_hazard","name":"Atomic Oxygen","domain":"science","entryPath":"/space-environment/atomic-oxygen","description":"Single oxygen atoms that dominate the thin atmosphere of low Earth orbit. Highly reactive, atomic oxygen slowly erodes exposed spacecraft materials, a design concern for anything operating for long periods in LEO.","sources":["nasa"]},{"id":"space_hazard:plasma-environment","type":"space_hazard","name":"Plasma Environment","domain":"science","entryPath":"/space-environment/plasma-environment","description":"The ionised gas that pervades near-Earth space, from the ionosphere out through the magnetosphere. Its density and energy govern spacecraft charging, radio propagation, and the behaviour of the radiation belts.","sources":["nasa"]},{"id":"geomagnetic_index:kp-index","type":"geomagnetic_index","name":"Kp Index","domain":"science","entryPath":"/space-environment/kp-index","description":"A global index of geomagnetic activity, derived from magnetometer readings and reported every three hours on a scale of 0 (quiet) to 9 (extreme storm). Kp is the standard measure used to forecast auroras and satellite disturbances.","sources":["noaa"]},{"id":"geomagnetic_index:dst-index","type":"geomagnetic_index","name":"Dst Index","domain":"science","entryPath":"/space-environment/dst-index","description":"The Disturbance storm-time index, which tracks the strength of the equatorial ring current and so measures the intensity of a geomagnetic storm — the more negative the Dst, the stronger the storm.","sources":["noaa"]},{"id":"geomagnetic_index:noaa-g-scale","type":"geomagnetic_index","name":"NOAA G-Scale (Geomagnetic Storms)","domain":"science","entryPath":"/space-environment/noaa-g-scale","description":"NOAA's five-level scale for the severity of geomagnetic storms, from G1 (minor) to G5 (extreme), describing the expected effects on power grids, satellites, and navigation.","sources":["noaa"]},{"id":"geomagnetic_index:noaa-s-scale","type":"geomagnetic_index","name":"NOAA S-Scale (Solar Radiation Storms)","domain":"science","entryPath":"/space-environment/noaa-s-scale","description":"NOAA's five-level scale for solar radiation (energetic-particle) storms, from S1 to S5, describing the radiation hazard to astronauts, high-altitude flights, and spacecraft.","sources":["noaa"]},{"id":"geomagnetic_index:noaa-r-scale","type":"geomagnetic_index","name":"NOAA R-Scale (Radio Blackouts)","domain":"science","entryPath":"/space-environment/noaa-r-scale","description":"NOAA's five-level scale for radio blackouts caused by solar-flare X-rays ionising the dayside upper atmosphere, from R1 (minor) to R5 (extreme).","sources":["noaa"]},{"id":"space_mission:soho","type":"space_mission","name":"SOHO (Solar and Heliospheric Observatory)","domain":"science","description":"A joint ESA/NASA solar observatory at the Sun–Earth L1 point, operating since 1995. Its coronagraphs image coronal mass ejections and it is a workhorse of space-weather monitoring (and a prolific comet discoverer).","aliases":["Solar and Heliospheric Observatory"],"sources":["esa","nasa"]},{"id":"space_mission:sdo","type":"space_mission","name":"SDO (Solar Dynamics Observatory)","domain":"science","description":"A NASA mission that images the Sun in many ultraviolet wavelengths at high cadence, studying solar activity, flares, and the magnetic field that drives space weather.","aliases":["Solar Dynamics Observatory"],"sources":["nasa"]},{"id":"space_mission:ace","type":"space_mission","name":"ACE (Advanced Composition Explorer)","domain":"science","description":"A NASA mission at the Sun–Earth L1 point that measures the solar wind and energetic particles upstream of Earth, giving roughly an hour of warning before disturbances reach the planet.","aliases":["Advanced Composition Explorer"],"sources":["nasa"]},{"id":"space_mission:dscovr","type":"space_mission","name":"DSCOVR (Deep Space Climate Observatory)","domain":"science","description":"A NOAA/NASA mission at the Sun–Earth L1 point that provides real-time solar-wind measurements for operational space-weather forecasting, along with full-disc images of Earth.","aliases":["Deep Space Climate Observatory"],"sources":["noaa","nasa"]},{"id":"organization:swpc","type":"organization","name":"Space Weather Prediction Center (SWPC)","domain":"science","description":"NOAA's official source of space-weather forecasts, watches, and warnings — the operational centre that issues the Kp, G-, S-, and R-scale alerts used to protect power grids, satellites, and aviation.","aliases":["NOAA SWPC"],"sources":["noaa"]},{"id":"mission_operations_center:jpl-sfof","type":"mission_operations_center","name":"JPL Space Flight Operations Facility (SFOF)","domain":"science","entryPath":"/mission-operations/jpl-sfof","description":"NASA's nerve centre for deep-space missions, at the Jet Propulsion Laboratory in Pasadena. From the SFOF, controllers command and monitor spacecraft across the Solar System through the Deep Space Network.","aliases":["SFOF","The Center of the Universe"],"sources":["nasa","jpl"]},{"id":"mission_operations_center:goddard-moc","type":"mission_operations_center","name":"Goddard Mission Operations","domain":"science","entryPath":"/mission-operations/goddard-moc","description":"NASA's Goddard Space Flight Center in Maryland operates many Earth-orbiting and astrophysics missions and hosts the Near Space Network's control functions.","aliases":["GSFC operations"],"sources":["nasa"]},{"id":"mission_operations_center:johnson-mcc","type":"mission_operations_center","name":"Johnson Mission Control Center (MCC-H)","domain":"science","entryPath":"/mission-operations/johnson-mcc","description":"NASA's iconic human-spaceflight control room at the Johnson Space Center in Houston, which has directed crewed missions from Gemini and Apollo to the International Space Station.","aliases":["Mission Control Houston","MCC-H"],"sources":["nasa"]},{"id":"mission_operations_center:esoc","type":"mission_operations_center","name":"European Space Operations Centre (ESOC)","domain":"science","entryPath":"/mission-operations/esoc","description":"ESA's mission-control centre in Darmstadt, Germany, from which the agency operates its scientific and interplanetary spacecraft through the Estrack network.","aliases":["ESOC"],"sources":["esa"]},{"id":"mission_operations_center:jaxa-operations","type":"mission_operations_center","name":"JAXA Mission Operations","domain":"science","entryPath":"/mission-operations/jaxa-operations","description":"JAXA operates its science and deep-space missions from centres including the Sagamihara campus (ISAS) and the Tsukuba Space Center, working with the Usuda deep-space antenna.","aliases":["Sagamihara / Tsukuba 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(BACC)","domain":"science","entryPath":"/mission-operations/bacc","description":"China's principal mission-control centre in Beijing, which directs the country's human-spaceflight, lunar (Chang'e), and planetary (Tianwen) missions.","aliases":["BACC"],"sources":["nasa"]},{"id":"operations_function:mission-control","type":"operations_function","name":"Mission Control","domain":"science","entryPath":"/mission-operations/mission-control","description":"The team and facility that command and monitor a spacecraft in real time — the heart of mission operations, staffed by controllers each responsible for a subsystem.","sources":["nasa"]},{"id":"operations_function:flight-dynamics","type":"operations_function","name":"Flight Dynamics","domain":"science","entryPath":"/mission-operations/flight-dynamics","description":"The discipline of determining and predicting a spacecraft's orbit and attitude, and computing the manoeuvres needed to keep it on its planned trajectory.","sources":["nasa","esa"]},{"id":"operations_function:orbit-determination","type":"operations_function","name":"Orbit Determination","domain":"science","entryPath":"/mission-operations/orbit-determination","description":"Estimating a spacecraft's precise position and velocity from tracking data (ranging, Doppler, and angles) — the input to every manoeuvre and every science observation.","sources":["nasa","jpl"]},{"id":"operations_function:navigation-operations","type":"operations_function","name":"Navigation Operations","domain":"science","entryPath":"/mission-operations/navigation-operations","description":"The operational process of guiding a spacecraft to its target — combining orbit determination with manoeuvre design, using the deep-space network's radiometric tracking.","sources":["nasa","jpl"]},{"id":"operations_function:telemetry-processing","type":"operations_function","name":"Telemetry 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when, and within its power, data, and pointing limits.","sources":["nasa","esa"]},{"id":"operations_function:flight-rules","type":"operations_function","name":"Flight Rules","domain":"science","entryPath":"/mission-operations/flight-rules","description":"The pre-agreed decision rules that tell a control team how to respond to situations, so that time-critical calls are made consistently and safely rather than improvised.","sources":["nasa"]},{"id":"operations_function:spacecraft-health-monitoring","type":"operations_function","name":"Spacecraft Health Monitoring","domain":"science","entryPath":"/mission-operations/spacecraft-health-monitoring","description":"Continuously watching a spacecraft's telemetry against expected limits to catch anomalies early — the routine vigilance that keeps a mission alive.","sources":["nasa"]},{"id":"operations_function:fault-protection","type":"operations_function","name":"Fault Protection","domain":"science","entryPath":"/mission-operations/fault-protection","description":"The onboard and ground logic that detects failures and responds automatically to keep a spacecraft safe when the ground cannot react in time — vital across the long light-time to deep space.","sources":["nasa","jpl"]},{"id":"operations_function:safe-mode","type":"operations_function","name":"Safe Mode","domain":"science","entryPath":"/mission-operations/safe-mode","description":"A protective state a spacecraft autonomously enters when it detects a serious problem — pointing its solar arrays at the Sun and its antenna toward Earth, and waiting for instructions.","sources":["nasa"]},{"id":"operations_function:automation","type":"operations_function","name":"Operations Automation","domain":"science","entryPath":"/mission-operations/automation","description":"Software that automates routine operations — from pass scheduling and telemetry screening to onboard sequence execution — reducing workload and enabling operations at deep-space distances.","sources":["nasa","esa"]},{"id":"operations_function:launch-operations","type":"operations_function","name":"Launch Operations","domain":"science","entryPath":"/mission-operations/launch-operations","description":"The operations phase spanning launch and the critical early days — acquiring the spacecraft, checking it out, and getting it onto its planned trajectory (Launch and Early Orbit Phase, LEOP).","sources":["nasa","esa"]},{"id":"operations_function:cruise-operations","type":"operations_function","name":"Cruise Operations","domain":"science","entryPath":"/mission-operations/cruise-operations","description":"The long interplanetary-cruise phase — keeping the spacecraft healthy, performing trajectory-correction manoeuvres, and preparing for arrival.","sources":["nasa"]},{"id":"operations_function:science-operations","type":"operations_function","name":"Science 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violence of launch, plus the mechanisms that deploy solar arrays, antennas, and instruments once in space.","sources":["nasa","esa"]},{"id":"spacecraft_subsystem:thermal-control","type":"spacecraft_subsystem","name":"Thermal Control","domain":"science","entryPath":"/spacecraft-systems/thermal-control","description":"The subsystem that keeps every part of a spacecraft within its allowable temperature range, radiating away waste heat and insulating against the extreme cold of space and the heat of the Sun.","sources":["nasa","esa"]},{"id":"spacecraft_subsystem:electrical-power","type":"spacecraft_subsystem","name":"Electrical Power","domain":"science","entryPath":"/spacecraft-systems/electrical-power","description":"The subsystem that generates, stores, and distributes electricity — from solar arrays or radioisotope generators, through batteries, to every instrument and heater on board.","sources":["nasa","esa"]},{"id":"spacecraft_subsystem:propulsion","type":"spacecraft_subsystem","name":"Propulsion","domain":"science","entryPath":"/spacecraft-systems/propulsion","description":"The subsystem that changes a spacecraft's velocity — for orbit insertion, trajectory corrections, and station-keeping — using chemical, electric, or cold-gas thrusters.","sources":["nasa","esa"]},{"id":"spacecraft_subsystem:attitude-control","type":"spacecraft_subsystem","name":"Attitude Determination & Control (ADCS)","domain":"science","entryPath":"/spacecraft-systems/attitude-control","description":"The subsystem that determines and controls which way a spacecraft points — sensing its orientation with star trackers and gyroscopes, and turning it with reaction wheels or thrusters.","aliases":["ADCS","GNC"],"sources":["nasa","esa"]},{"id":"spacecraft_subsystem:command-and-data-handling","type":"spacecraft_subsystem","name":"Command & Data Handling (Avionics)","domain":"science","entryPath":"/spacecraft-systems/command-and-data-handling","description":"The spacecraft's onboard computing — the flight computer, software, and memory that execute commands, run the spacecraft autonomously, and manage faults across the long light-time to deep space.","aliases":["C&DH","Avionics"],"sources":["nasa","jpl"]},{"id":"spacecraft_subsystem:telecommunications","type":"spacecraft_subsystem","name":"Telecommunications","domain":"science","entryPath":"/spacecraft-systems/telecommunications","description":"The subsystem that carries commands up and telemetry and science data down — the spacecraft's radios and antennas, working with the ground network.","sources":["nasa","jpl"]},{"id":"spacecraft_subsystem:entry-descent-and-landing","type":"spacecraft_subsystem","name":"Entry, Descent & Landing (EDL)","domain":"science","entryPath":"/spacecraft-systems/entry-descent-and-landing","description":"The subsystem — and the few dramatic minutes — that gets a spacecraft from the top of an atmosphere to a safe landing: a heat shield to survive entry, a parachute or thrusters to slow down, and legs or airbags to touch down.","aliases":["EDL"],"sources":["nasa","jpl"]},{"id":"spacecraft_subsystem:robotics","type":"spacecraft_subsystem","name":"Robotics","domain":"science","entryPath":"/spacecraft-systems/robotics","description":"The robotic arms and manipulators that let spacecraft build, service, sample, and move cargo — from the Space Shuttle and station arms to the sampling arms of planetary landers.","sources":["nasa","esa"]},{"id":"spacecraft_subsystem:crew-systems","type":"spacecraft_subsystem","name":"Crew & Life-Support Systems","domain":"science","entryPath":"/spacecraft-systems/crew-systems","description":"For crewed spacecraft, the systems that keep people alive and let vehicles join up — environmental control and life support (ECLSS) and the docking mechanisms that connect spacecraft.","sources":["nasa","esa"]},{"id":"spacecraft_component:solar-array","type":"spacecraft_component","name":"Solar Array","domain":"science","entryPath":"/spacecraft-systems/solar-array","description":"Panels of photovoltaic cells that convert sunlight into electricity — the primary power source for most spacecraft in the inner Solar System. Beyond Jupiter, sunlight becomes too weak and other sources are needed.","sources":["nasa"]},{"id":"spacecraft_component:battery","type":"spacecraft_component","name":"Battery","domain":"science","entryPath":"/spacecraft-systems/battery","description":"Rechargeable batteries store energy from the solar arrays to power a spacecraft through eclipse, at night, or during peak demand. Lithium-ion has largely replaced older nickel chemistries.","sources":["nasa"]},{"id":"spacecraft_component:rtg","type":"spacecraft_component","name":"Radioisotope Thermoelectric Generator (RTG)","domain":"science","entryPath":"/spacecraft-systems/rtg","description":"A nuclear power source that converts the heat of decaying plutonium-238 directly into electricity. RTGs let missions operate far from the Sun or through the lunar night — powering Voyager, Cassini, and the nuclear Mars rovers Curiosity and Perseverance (the earlier rovers were solar-powered).","aliases":["RTG"],"sources":["nasa","jpl"]},{"id":"spacecraft_component:fuel-cell","type":"spacecraft_component","name":"Fuel Cell","domain":"science","entryPath":"/spacecraft-systems/fuel-cell","description":"A device that generates electricity by combining hydrogen and oxygen, producing water as a by-product. Fuel cells powered the Apollo and Space Shuttle missions, useful for short crewed flights needing high power.","sources":["nasa"]},{"id":"spacecraft_component:chemical-propulsion","type":"spacecraft_component","name":"Chemical Propulsion","domain":"science","entryPath":"/spacecraft-systems/chemical-propulsion","description":"Thrusters and engines that burn propellants for high thrust — the standard means of orbit insertion and large manoeuvres, using monopropellants (hydrazine) or bipropellants.","sources":["nasa"]},{"id":"spacecraft_component:ion-thruster","type":"spacecraft_component","name":"Ion Thruster","domain":"science","entryPath":"/spacecraft-systems/ion-thruster","description":"A gridded electrostatic thruster that ionises a propellant (usually xenon) and accelerates it with electric-field grids to very high exhaust velocity. It delivers tiny thrust but sips fuel, enabling missions like Deep Space 1 and Dawn.","aliases":["Gridded ion thruster"],"sources":["nasa","jpl"]},{"id":"spacecraft_component:hall-effect-thruster","type":"spacecraft_component","name":"Hall-Effect Thruster","domain":"science","entryPath":"/spacecraft-systems/hall-effect-thruster","description":"A type of electric propulsion that traps electrons in a magnetic field to ionise and accelerate propellant. Widely used for satellite station-keeping and, increasingly, for deep-space missions — NASA's Psyche is the first to fly Hall-effect thrusters beyond lunar orbit.","sources":["nasa","esa"]},{"id":"spacecraft_component:cold-gas-thruster","type":"spacecraft_component","name":"Cold-Gas Thruster","domain":"science","entryPath":"/spacecraft-systems/cold-gas-thruster","description":"The simplest thruster — it just releases a stored, pressurised gas through a nozzle. Low-performance but reliable, used for fine attitude control and on small spacecraft.","sources":["nasa"]},{"id":"spacecraft_component:nuclear-thermal-propulsion","type":"spacecraft_component","name":"Nuclear Thermal Propulsion","domain":"science","entryPath":"/spacecraft-systems/nuclear-thermal-propulsion","description":"A propulsion concept that heats a propellant with a nuclear reactor for high thrust and efficiency. Long studied and tested on the ground, it is a candidate for future fast crewed trips to Mars.","sources":["nasa"]},{"id":"spacecraft_component:reaction-control-system","type":"spacecraft_component","name":"Reaction Control System (RCS)","domain":"science","entryPath":"/spacecraft-systems/reaction-control-system","description":"A set of small thrusters arranged around a spacecraft for precise control of orientation and small translations — used for pointing, docking, and stabilisation.","aliases":["RCS"],"sources":["nasa"]},{"id":"spacecraft_component:reaction-wheel","type":"spacecraft_component","name":"Reaction Wheel","domain":"science","entryPath":"/spacecraft-systems/reaction-wheel","description":"A spinning flywheel that a spacecraft speeds up or slows down to rotate itself, by conservation of angular momentum, without using any propellant — the workhorse of precise pointing.","sources":["nasa","esa"]},{"id":"spacecraft_component:control-moment-gyro","type":"spacecraft_component","name":"Control Moment Gyroscope (CMG)","domain":"science","entryPath":"/spacecraft-systems/control-moment-gyro","description":"A spinning gyroscope whose axis is tilted to produce large control torques efficiently — used on big, agile spacecraft such as the International Space Station and Earth-imaging satellites.","aliases":["CMG"],"sources":["nasa"]},{"id":"spacecraft_component:flight-computer","type":"spacecraft_component","name":"Flight Computer","domain":"science","entryPath":"/spacecraft-systems/flight-computer","description":"The central processor that runs a spacecraft — executing command sequences, controlling subsystems, and reacting to faults. Deep-space computers are radiation-hardened and modest by consumer standards, prizing reliability over speed.","sources":["nasa","jpl"]},{"id":"spacecraft_component:onboard-software","type":"spacecraft_component","name":"Onboard Flight Software","domain":"science","entryPath":"/spacecraft-systems/onboard-software","description":"The programs that fly the spacecraft — running the control loops, sequences, and autonomy. Flight software is exhaustively tested, because a bug billions of kilometres away cannot be fixed by hand.","sources":["nasa","jpl"]},{"id":"spacecraft_component:radiation-hardened-memory","type":"spacecraft_component","name":"Radiation-Hardened Memory","domain":"science","entryPath":"/spacecraft-systems/radiation-hardened-memory","description":"Memory and electronics designed to withstand the charged particles of space, which can flip bits or damage circuits. Error-correcting codes and hardened parts keep the computer trustworthy.","sources":["nasa"]},{"id":"spacecraft_component:fault-management","type":"spacecraft_component","name":"Fault Management","domain":"science","entryPath":"/spacecraft-systems/fault-management","description":"The onboard logic that detects, isolates, and recovers from failures autonomously — putting the spacecraft into a safe state and calling home when it cannot resolve a problem itself.","sources":["nasa","jpl"]},{"id":"spacecraft_component:radiator","type":"spacecraft_component","name":"Radiator","domain":"science","entryPath":"/spacecraft-systems/radiator","description":"A surface that sheds a spacecraft's waste heat into space by infrared radiation — the only way to cool in a vacuum, where there is no air to carry heat away.","sources":["nasa"]},{"id":"spacecraft_component:multi-layer-insulation","type":"spacecraft_component","name":"Multi-Layer Insulation (MLI)","domain":"science","entryPath":"/spacecraft-systems/multi-layer-insulation","description":"The shiny, quilted blankets that wrap most spacecraft — many thin reflective layers that block radiative heat transfer, insulating against both the Sun's heat and the cold of space.","aliases":["MLI"],"sources":["nasa"]},{"id":"spacecraft_component:heater","type":"spacecraft_component","name":"Heater & Heat Pipe","domain":"science","entryPath":"/spacecraft-systems/heater","description":"Electric heaters and passive heat pipes that keep components — propellant lines, batteries, instruments — above their minimum temperatures, moving heat from where it is made to where it is needed or shed.","sources":["nasa"]},{"id":"spacecraft_component:primary-structure","type":"spacecraft_component","name":"Primary Structure","domain":"science","entryPath":"/spacecraft-systems/primary-structure","description":"The main load-bearing frame of the spacecraft, which carries the launch loads and provides the rigid backbone to which everything else is mounted.","sources":["nasa","esa"]},{"id":"spacecraft_component:deployable-mechanisms","type":"spacecraft_component","name":"Deployable Mechanisms","domain":"science","entryPath":"/spacecraft-systems/deployable-mechanisms","description":"The hinges, booms, and release devices that unfold solar arrays, antennas, and instrument booms after launch — single-use mechanisms that must work the first time.","sources":["nasa","esa"]},{"id":"spacecraft_component:heat-shield","type":"spacecraft_component","name":"Heat Shield","domain":"science","entryPath":"/spacecraft-systems/heat-shield","description":"The ablative or reusable shield that protects a spacecraft from the searing heat of atmospheric entry, where air violently compressed ahead of the vehicle's bow shock can reach thousands of degrees (the heating is dominated by shock compression, not friction). Ablative shields char and carry heat away as they erode.","sources":["nasa","jpl"]},{"id":"spacecraft_component:parachute","type":"spacecraft_component","name":"Parachute","domain":"science","entryPath":"/spacecraft-systems/parachute","description":"The decelerator that slows a spacecraft in an atmosphere after the heat shield has done its work — from the supersonic parachutes of Mars landers to the splashdown chutes of crew capsules.","sources":["nasa"]},{"id":"spacecraft_component:retropropulsion","type":"spacecraft_component","name":"Retropropulsion & Landing Systems","domain":"science","entryPath":"/spacecraft-systems/retropropulsion","description":"The thrusters, legs, or airbags that manage the final touchdown — from the sky-crane of the Mars rovers to the propulsive landings of crew and booster vehicles.","sources":["nasa","jpl"]},{"id":"spacecraft_component:robotic-arm","type":"spacecraft_component","name":"Robotic Arm","domain":"science","entryPath":"/spacecraft-systems/robotic-arm","description":"A jointed manipulator used to move cargo, service hardware, capture spacecraft, or collect samples. The Shuttle's Canadarm helped assemble the Space Station and the permanently-installed Canadarm2 services it; planetary landers carry smaller sampling arms.","aliases":["Canadarm","Manipulator arm"],"sources":["nasa","esa"]},{"id":"instrument_class:optical-camera","type":"instrument_class","name":"Optical Camera","domain":"science","entryPath":"/instruments/optical-camera","description":"An imaging instrument that records visible (and often near-infrared or ultraviolet) light — the eyes of a spacecraft, from wide-angle context cameras to high-resolution narrow-angle telescopes.","sources":["nasa","esa"]},{"id":"instrument_class:imaging-spectrometer","type":"instrument_class","name":"Imaging Spectrometer","domain":"science","entryPath":"/instruments/imaging-spectrometer","description":"An instrument that captures both an image and a spectrum for every pixel, mapping the composition of a surface or atmosphere by the wavelengths of light it reflects or emits.","sources":["nasa","esa"]},{"id":"instrument_class:spectrometer","type":"instrument_class","name":"Spectrometer","domain":"science","entryPath":"/instruments/spectrometer","description":"An instrument that splits light into its component wavelengths to reveal composition, temperature, and motion — the workhorse of remote sensing, spanning ultraviolet, visible, infrared, X-ray, and gamma-ray bands.","sources":["nasa","esa"]},{"id":"instrument_class:mass-spectrometer","type":"instrument_class","name":"Mass Spectrometer","domain":"science","entryPath":"/instruments/mass-spectrometer","description":"An instrument that sorts atoms and molecules by mass, identifying the chemical and isotopic makeup of a sample of gas or dust — essential for atmospheres, plumes, and returned samples.","sources":["nasa"]},{"id":"instrument_class:magnetometer","type":"instrument_class","name":"Magnetometer","domain":"science","entryPath":"/instruments/magnetometer","description":"An instrument that measures magnetic fields, revealing a planet's internal dynamo, a moon's hidden ocean, or the structure of the solar wind and magnetospheres.","sources":["nasa","esa"]},{"id":"instrument_class:charged-particle-detector","type":"instrument_class","name":"Charged-Particle Detector","domain":"science","entryPath":"/instruments/charged-particle-detector","description":"An instrument that counts and characterises the electrons, ions, and cosmic rays of space plasmas — mapping radiation belts, the solar wind, and energetic-particle events.","sources":["nasa"]},{"id":"instrument_class:dust-detector","type":"instrument_class","name":"Dust Detector","domain":"science","entryPath":"/instruments/dust-detector","description":"An instrument that detects the tiny dust grains of space — from cometary and interplanetary dust to the particles of planetary rings — measuring their speed, mass, and sometimes composition.","sources":["nasa","esa"]},{"id":"instrument_class:radar","type":"instrument_class","name":"Radar","domain":"science","entryPath":"/instruments/radar","description":"An active instrument that transmits radio waves and analyses the echoes to map surfaces through cloud and darkness, or to probe beneath the surface. Synthetic-aperture radar (SAR) achieves high resolution from orbit.","aliases":["SAR"],"sources":["nasa","esa"]},{"id":"instrument_class:laser-altimeter","type":"instrument_class","name":"Laser Altimeter (Lidar)","domain":"science","entryPath":"/instruments/laser-altimeter","description":"An active instrument that fires laser pulses and times their return to measure distance precisely — mapping the topography of a planet, moon, or asteroid with height accuracy of metres.","aliases":["Lidar"],"sources":["nasa"]},{"id":"instrument_class:seismometer","type":"instrument_class","name":"Seismometer","domain":"science","entryPath":"/instruments/seismometer","description":"An instrument that senses the tiny ground motions of quakes and impacts, probing the interior structure of a world by how seismic waves travel through it — as InSight did for Mars.","sources":["nasa"]},{"id":"instrument_class:gamma-ray-neutron-spectrometer","type":"instrument_class","name":"Gamma-Ray & Neutron 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detailed images of Pluto and the Kuiper Belt object Arrokoth.","aliases":["LORRI"],"sources":["nasa"]},{"id":"scientific_instrument:alice-nh","type":"scientific_instrument","name":"Alice (New Horizons UV Spectrometer)","domain":"science","entryPath":"/instruments/alice-nh","description":"New Horizons's ultraviolet imaging spectrometer, which probed the composition and structure of Pluto's atmosphere as the spacecraft flew through its shadow.","aliases":["Alice"],"sources":["nasa"]},{"id":"scientific_instrument:junocam","type":"scientific_instrument","name":"JunoCam","domain":"science","entryPath":"/instruments/junocam","description":"Juno's wide-angle visible-light camera, included partly for public engagement, which has returned spectacular images of Jupiter's turbulent poles and cloud bands.","sources":["nasa"]},{"id":"scientific_instrument:cassini-iss","type":"scientific_instrument","name":"Cassini Imaging Science Subsystem 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Earth.","aliases":["Voyager ISS"],"sources":["nasa","jpl"]},{"id":"scientific_instrument:ocams","type":"scientific_instrument","name":"OCAMS (OSIRIS-REx Camera Suite)","domain":"science","entryPath":"/instruments/ocams","description":"OSIRIS-REx's camera suite, which mapped the asteroid Bennu in detail and documented the touch-and-go sample collection.","aliases":["OCAMS"],"sources":["nasa"]},{"id":"scientific_instrument:insight-seis","type":"scientific_instrument","name":"SEIS (Seismic Experiment for Interior Structure)","domain":"science","entryPath":"/instruments/insight-seis","description":"InSight's ultra-sensitive seismometer, which detected hundreds of marsquakes and, for the first time, revealed the internal structure of Mars.","aliases":["SEIS"],"sources":["nasa","jpl"]},{"id":"scientific_instrument:magellan-sar","type":"scientific_instrument","name":"Magellan Synthetic Aperture Radar","domain":"science","entryPath":"/instruments/magellan-sar","description":"Magellan's imaging radar, which pierced Venus's thick clouds to map 98% of the planet's surface at high resolution.","aliases":["Magellan SAR"],"sources":["nasa","jpl"]},{"id":"scientific_instrument:messenger-grns","type":"scientific_instrument","name":"MESSENGER Gamma-Ray & Neutron Spectrometer","domain":"science","entryPath":"/instruments/messenger-grns","description":"MESSENGER's spectrometer, which measured the elemental composition of Mercury's surface and helped confirm water ice in its permanently shadowed polar craters.","aliases":["GRNS"],"sources":["nasa"]},{"id":"scientific_instrument:dawn-framing-camera","type":"scientific_instrument","name":"Dawn Framing Camera","domain":"science","entryPath":"/instruments/dawn-framing-camera","description":"Dawn's camera, which mapped the giant asteroid Vesta and the dwarf planet Ceres, including the bright carbonate deposits of Ceres's Occator crater.","sources":["nasa","jpl"]},{"id":"scientific_instrument:galileo-nims","type":"scientific_instrument","name":"Galileo Near-Infrared Mapping Spectrometer (NIMS)","domain":"science","entryPath":"/instruments/galileo-nims","description":"Galileo's imaging spectrometer, which mapped the composition of Jupiter's moons and found evidence for salts and a subsurface ocean on Europa.","aliases":["NIMS"],"sources":["nasa","jpl"]},{"id":"scientific_instrument:voyager-crs","type":"scientific_instrument","name":"Voyager Cosmic Ray Subsystem (CRS)","domain":"science","entryPath":"/instruments/voyager-crs","description":"The Voyager cosmic-ray detectors, whose measurements of the sudden change in particle counts marked each spacecraft's crossing of the heliopause into interstellar space.","aliases":["CRS"],"sources":["nasa","jpl"]},{"id":"scientific_instrument:cassini-cda","type":"scientific_instrument","name":"Cassini Cosmic Dust Analyzer (CDA)","domain":"science","entryPath":"/instruments/cassini-cda","description":"Cassini's dust detector, which sampled the grains of Saturn's rings and the ice particles of Enceladus's plume, measuring their composition and revealing the moon's subsurface ocean.","aliases":["CDA"],"sources":["nasa","jpl"]},{"id":"scientific_instrument:messenger-mla","type":"scientific_instrument","name":"Mercury Laser Altimeter (MLA)","domain":"science","entryPath":"/instruments/messenger-mla","description":"MESSENGER's laser altimeter, which measured the topography of Mercury's northern hemisphere and helped confirm water ice in its permanently shadowed polar craters.","aliases":["MLA"],"sources":["nasa"]},{"id":"scientific_instrument:cassini-rss","type":"scientific_instrument","name":"Cassini Radio Science Subsystem (RSS)","domain":"science","entryPath":"/instruments/cassini-rss","description":"Cassini's radio-science experiment, which used the spacecraft's radio link — tracking tiny frequency shifts and radio occultations — to weigh Saturn, map its gravity field, and probe the structure of its rings and atmosphere.","aliases":["RSS"],"sources":["nasa","jpl"]},{"id":"geological_feature_type:impact-crater","type":"geological_feature_type","name":"Impact Crater","domain":"science","entryPath":"/planetary-geology/impact-crater","description":"A bowl-shaped depression blasted out when an asteroid or comet strikes a solid surface. Craters are the most common landform in the Solar System, and their density is used to date surfaces — the more craters, the older the terrain.","sources":["nasa"]},{"id":"geological_feature_type:impact-basin","type":"geological_feature_type","name":"Impact Basin","domain":"science","entryPath":"/planetary-geology/impact-basin","description":"An enormous impact structure, hundreds to thousands of kilometres across, formed by a giant early impact — often multi-ringed and later flooded by lava, as with the lunar maria.","sources":["nasa"]},{"id":"geological_feature_type:shield-volcano","type":"geological_feature_type","name":"Shield Volcano","domain":"science","entryPath":"/planetary-geology/shield-volcano","description":"A broad, gently-sloping volcano built by fluid lava flows. On Mars, low gravity and a stationary crust let shield volcanoes grow to enormous size — Olympus Mons is the tallest in the Solar System.","sources":["nasa"]},{"id":"geological_feature_type:cryovolcano","type":"geological_feature_type","name":"Cryovolcano","domain":"science","entryPath":"/planetary-geology/cryovolcano","description":"An 'ice volcano' that erupts water, ammonia, or methane instead of molten rock, resurfacing the frozen worlds of the outer Solar System — from Ceres's Ahuna Mons to the plumes of Enceladus.","sources":["nasa"]},{"id":"geological_feature_type:lava-plain","type":"geological_feature_type","name":"Lava Plain (Mare)","domain":"science","entryPath":"/planetary-geology/lava-plain","description":"A broad, dark plain of solidified lava. The lunar maria — the 'seas' — are vast basalt flows that filled ancient impact basins; similar plains cover much of Venus and Mars.","aliases":["Mare"],"sources":["nasa"]},{"id":"geological_feature_type:highlands","type":"geological_feature_type","name":"Highlands","domain":"science","entryPath":"/planetary-geology/highlands","description":"The ancient, heavily-cratered high terrain of a world, older and more rugged than the smooth plains — like the bright lunar highlands or the tessera terrain of Venus.","sources":["nasa"]},{"id":"geological_feature_type:canyon","type":"geological_feature_type","name":"Canyon","domain":"science","entryPath":"/planetary-geology/canyon","description":"A deep, steep-sided valley cut by tectonics or water. Mars's Valles Marineris is a canyon system so large it would stretch across the entire United States.","sources":["nasa"]},{"id":"geological_feature_type:fault-scarp","type":"geological_feature_type","name":"Fault Scarp","domain":"science","entryPath":"/planetary-geology/fault-scarp","description":"A cliff formed where the crust has broken and one side has risen relative to the other. Mercury is covered in long lobate scarps produced as the planet cooled and shrank.","sources":["nasa"]},{"id":"geological_feature_type:mountain-range","type":"geological_feature_type","name":"Mountain Range (Montes)","domain":"science","entryPath":"/planetary-geology/mountain-range","description":"A chain or massif of mountains, whether uplifted by tectonics, thrown up around an impact basin, or built by volcanism — from Venus's Maxwell Montes to the water-ice mountains of Pluto.","aliases":["Montes"],"sources":["nasa"]},{"id":"geological_feature_type:tessera","type":"geological_feature_type","name":"Tessera","domain":"science","entryPath":"/planetary-geology/tessera","description":"Complex, intensely deformed 'tile' terrain unique to Venus — the planet's oldest and most tectonically tortured surface, ridged and grooved in intersecting directions.","sources":["nasa"]},{"id":"geological_feature_type:corona","type":"geological_feature_type","name":"Corona","domain":"science","entryPath":"/planetary-geology/corona","description":"A large circular volcanic-tectonic feature, ringed by fractures, thought to form where hot material rises and pushes up the crust — a signature landform of Venus.","sources":["nasa"]},{"id":"geological_feature_type:grooved-terrain","type":"geological_feature_type","name":"Grooved Terrain (Sulci)","domain":"science","entryPath":"/planetary-geology/grooved-terrain","description":"Bright bands of parallel ridges and grooves that cut across the dark, ancient surface of Ganymede — young, tectonically-resurfaced ice.","aliases":["Sulci"],"sources":["nasa"]},{"id":"geological_feature_type:dune-field","type":"geological_feature_type","name":"Dune Field","domain":"science","entryPath":"/planetary-geology/dune-field","description":"A field of wind-blown dunes, showing that a world has an atmosphere and mobile sediment — from the basaltic-sand dunes of Mars to the hydrocarbon-sand dunes of Titan.","sources":["nasa"]},{"id":"geological_feature_type:outflow-channel","type":"geological_feature_type","name":"Outflow Channel","domain":"science","entryPath":"/planetary-geology/outflow-channel","description":"A giant channel carved by catastrophic floods of water in the distant past, evidence that liquid water once flowed across the surface of Mars.","sources":["nasa"]},{"id":"geological_feature_type:river-delta","type":"geological_feature_type","name":"River Delta","domain":"science","entryPath":"/planetary-geology/river-delta","description":"A fan of sediment deposited where an ancient river entered a standing body of water — a prime target in the search for past life, as at Jezero crater on Mars.","sources":["nasa"]},{"id":"geological_feature_type:ice-plain","type":"geological_feature_type","name":"Ice Plain & Glacier","domain":"science","entryPath":"/planetary-geology/ice-plain","description":"A broad plain or flowing sheet of ice. On Pluto, the nitrogen-ice glaciers of Sputnik Planitia churn and flow; on Mars and the icy moons, water ice shapes the surface.","sources":["nasa"]},{"id":"geological_feature_type:chaos-terrain","type":"geological_feature_type","name":"Chaos Terrain","domain":"science","entryPath":"/planetary-geology/chaos-terrain","description":"A jumble of broken, tilted blocks of crust, often where a surface has been disrupted from below — as on Europa, where it may mark places the ice shell interacts with the ocean beneath.","sources":["nasa"]},{"id":"geological_feature_type:hydrocarbon-lake","type":"geological_feature_type","name":"Hydrocarbon Lake","domain":"science","entryPath":"/planetary-geology/hydrocarbon-lake","description":"A lake or sea of liquid methane and ethane — found only on Titan, the one other world in the Solar System with stable liquid on its surface.","sources":["nasa"]},{"id":"surface_feature:tharsis-montes","type":"surface_feature","name":"Tharsis Montes","domain":"science","entryPath":"/planetary-geology/tharsis-montes","description":"A chain of three vast shield volcanoes on the Tharsis rise, a bulge so large it may have tilted the whole planet. Tharsis dominates the western hemisphere of Mars.","sources":["nasa","jpl"]},{"id":"surface_feature:hellas-basin","type":"surface_feature","name":"Hellas Planitia","domain":"science","entryPath":"/planetary-geology/hellas-basin","description":"One of the largest visible impact basins in the Solar System and the lowest point on Mars, deep enough that the atmospheric pressure at its floor can allow liquid water briefly.","aliases":["Hellas Basin"],"sources":["nasa","jpl"]},{"id":"surface_feature:gale-crater","type":"surface_feature","name":"Gale Crater","domain":"science","entryPath":"/planetary-geology/gale-crater","description":"A 154 km impact crater with a central mountain (Aeolis Mons / Mount Sharp) of layered sediments. The Curiosity rover has climbed it, reading a history of ancient lakes.","sources":["nasa","jpl"]},{"id":"surface_feature:jezero-crater","type":"surface_feature","name":"Jezero Crater","domain":"science","entryPath":"/planetary-geology/jezero-crater","description":"A crater that once held a lake, with a well-preserved river delta at its rim. The Perseverance rover is caching samples here in the search for signs of ancient life.","sources":["nasa","jpl"]},{"id":"surface_feature:kasei-valles","type":"surface_feature","name":"Kasei Valles","domain":"science","entryPath":"/planetary-geology/kasei-valles","description":"One of the largest outflow channels on Mars, carved by catastrophic floods of water that burst from the Tharsis region billions of years ago.","sources":["nasa"]},{"id":"surface_feature:mare-imbrium","type":"surface_feature","name":"Mare Imbrium","domain":"science","entryPath":"/planetary-geology/mare-imbrium","description":"The vast lava-filled 'Sea of Showers', one of the largest lunar maria, occupying a giant ancient impact basin on the Moon's near side.","sources":["nasa"]},{"id":"surface_feature:copernicus-crater","type":"surface_feature","name":"Copernicus","domain":"science","entryPath":"/planetary-geology/copernicus-crater","description":"A young, prominent lunar impact crater with terraced walls and bright rays of ejecta, a classic example of a complex crater.","sources":["nasa"]},{"id":"surface_feature:caloris-basin","type":"surface_feature","name":"Caloris Planitia","domain":"science","entryPath":"/planetary-geology/caloris-basin","description":"One of the largest impact basins in the Solar System, on Mercury, so violent that its antipode is marked by chaotic 'weird terrain' shaken up by the focused seismic waves.","aliases":["Caloris Basin"],"sources":["nasa"]},{"id":"surface_feature:discovery-rupes","type":"surface_feature","name":"Discovery Rupes","domain":"science","entryPath":"/planetary-geology/discovery-rupes","description":"A great lobate cliff on Mercury, formed as the planet's interior cooled and its crust contracted, thrusting one block of terrain over another.","sources":["nasa"]},{"id":"surface_feature:maxwell-montes","type":"surface_feature","name":"Maxwell Montes","domain":"science","entryPath":"/planetary-geology/maxwell-montes","description":"The highest mountains on Venus, rising about 11 km above the mean surface in the northern highlands of Ishtar Terra — higher than Everest above sea level.","sources":["nasa"]},{"id":"surface_feature:aphrodite-terra","type":"surface_feature","name":"Aphrodite Terra","domain":"science","entryPath":"/planetary-geology/aphrodite-terra","description":"A continent-sized highland region straddling Venus's equator, roughly the size of Africa, cut by deep rifts and dotted with volcanic features.","sources":["nasa"]},{"id":"surface_feature:artemis-corona","type":"surface_feature","name":"Artemis Corona","domain":"science","entryPath":"/planetary-geology/artemis-corona","description":"The largest corona on Venus — a vast circular volcano-tectonic feature ringed by fractures, marking where hot material welled up beneath the crust.","sources":["nasa"]},{"id":"surface_feature:alpha-regio","type":"surface_feature","name":"Alpha Regio","domain":"science","entryPath":"/planetary-geology/alpha-regio","description":"One of the first-recognised tessera regions on Venus — a patch of the planet's oldest, most intensely deformed 'tile' terrain, ridged and grooved by ancient tectonics.","sources":["nasa"]},{"id":"surface_feature:olympia-undae","type":"surface_feature","name":"Olympia Undae","domain":"science","entryPath":"/planetary-geology/olympia-undae","description":"A vast field of dark, wind-blown dunes wrapping around the north polar ice cap of Mars — one of the largest dune fields on the planet.","sources":["nasa"]},{"id":"surface_feature:occator-crater","type":"surface_feature","name":"Occator Crater","domain":"science","entryPath":"/planetary-geology/occator-crater","description":"A crater on the dwarf planet Ceres famous for its bright deposits — salts left behind by briny water that reached the surface, hinting at a subsurface reservoir.","sources":["nasa","jpl"]},{"id":"surface_feature:ahuna-mons","type":"surface_feature","name":"Ahuna Mons","domain":"science","entryPath":"/planetary-geology/ahuna-mons","description":"A steep, isolated mountain on Ceres interpreted as a cryovolcano — a dome built by icy, briny material erupting from within the dwarf planet.","sources":["nasa","jpl"]},{"id":"surface_feature:rheasilvia","type":"surface_feature","name":"Rheasilvia","domain":"science","entryPath":"/planetary-geology/rheasilvia","description":"An enormous impact basin covering much of the south pole of the asteroid Vesta, with a central peak among the tallest in the Solar System. 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NASA's MOXIE experiment on the Perseverance rover demonstrated making oxygen on Mars.","aliases":["Oxygen extraction"],"sources":["nasa"]},{"id":"isru_technique:regolith-processing","type":"isru_technique","name":"Regolith Processing","domain":"science","entryPath":"/space-infrastructure/regolith-processing","description":"Working the loose surface soil of the Moon and Mars — sintering or melting it into building material, extracting metals and oxygen, and using it for radiation shielding — turning the ground itself into a resource.","sources":["nasa"]},{"id":"isru_technique:metal-extraction","type":"isru_technique","name":"Metal Extraction","domain":"science","entryPath":"/space-infrastructure/metal-extraction","description":"Extracting metals — iron, nickel, and precious metals — from asteroids and from lunar and Martian regolith, to build structures in space without lifting the mass from Earth. Metal-rich M-type asteroids such as Psyche are studied as future resources.","aliases":["Asteroid mining"],"sources":["nasa"]},{"id":"isru_technique:propellant-production","type":"isru_technique","name":"Propellant Production","domain":"science","entryPath":"/space-infrastructure/propellant-production","description":"Making rocket propellant in space — splitting water into hydrogen and oxygen, or combining Martian carbon dioxide with hydrogen to make methane and oxygen — so a return vehicle can be fuelled at its destination instead of carrying all its propellant from Earth.","aliases":["In-situ propellant"],"sources":["nasa"]},{"id":"space_manufacturing_process:additive-manufacturing","type":"space_manufacturing_process","name":"Additive Manufacturing","domain":"science","entryPath":"/space-infrastructure/additive-manufacturing","description":"3D-printing parts and tools in orbit, layer by layer. A 3D printer has operated aboard the ISS since 2014, printing tools and spares on demand and pointing toward a future where spacecraft parts are made in space rather than launched.","aliases":["3D printing in space"],"sources":["nasa"]},{"id":"space_manufacturing_process:in-space-assembly","type":"space_manufacturing_process","name":"In-Space Assembly","domain":"science","entryPath":"/space-infrastructure/in-space-assembly","description":"Building large structures in space from parts, rather than folding a finished structure into a rocket fairing. 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Robotic servicing missions have already docked with and relocated satellites.","aliases":["Satellite servicing"],"sources":["nasa"]},{"id":"space_manufacturing_process:autonomous-construction","type":"space_manufacturing_process","name":"Autonomous Construction","domain":"science","entryPath":"/space-infrastructure/autonomous-construction","description":"Using robots to build and maintain infrastructure in space and on other worlds with little or no human presence — laying landing pads, assembling habitats, and constructing solar farms before crews arrive.","aliases":["Construction robotics","Autonomous assembly"],"sources":["nasa"]},{"id":"space_infrastructure:propellant-depot","type":"space_infrastructure","name":"Propellant Depot","domain":"science","entryPath":"/space-infrastructure/propellant-depot","description":"An orbiting fuel station that stores propellant so spacecraft can refuel in space. A depot would let missions launch 'dry' and top up on orbit, breaking the tyranny of carrying all their propellant from the ground.","aliases":["Fuel depot"],"sources":["nasa"]},{"id":"space_infrastructure:cryogenic-fuel-storage","type":"space_infrastructure","name":"Cryogenic Fuel Storage","domain":"science","entryPath":"/space-infrastructure/cryogenic-fuel-storage","description":"Keeping cryogenic propellants — liquid hydrogen and oxygen — cold enough not to boil away over long missions. Cryogenic fluid management is a key enabling technology for depots and for deep-space transfer stages.","aliases":["Zero-boil-off storage"],"sources":["nasa"]},{"id":"space_infrastructure:orbital-habitat","type":"space_infrastructure","name":"Commercial Orbital Habitat","domain":"science","entryPath":"/space-infrastructure/orbital-habitat","description":"Privately-built and operated space stations intended to succeed the ISS as destinations in low Earth orbit — for research, manufacturing, and tourism. Axiom Station is being assembled to begin attached to the ISS before flying free.","aliases":["Commercial space station"],"sources":["nasa"]},{"id":"space_infrastructure:inflatable-habitat","type":"space_infrastructure","name":"Inflatable Habitat","domain":"science","entryPath":"/space-infrastructure/inflatable-habitat","description":"Habitats that launch compact and expand in space, giving far more volume per kilogram than rigid modules. The Genesis demonstrators and the BEAM module on the ISS have proven the concept in orbit.","aliases":["Expandable module"],"sources":["nasa"]},{"id":"space_infrastructure:lunar-surface-base","type":"space_infrastructure","name":"Lunar Surface Base","domain":"science","entryPath":"/space-infrastructure/lunar-surface-base","description":"A sustained human outpost on the Moon — habitats, power, and ISRU plants supporting long stays — the surface counterpart of the Gateway station, and a proving ground for the technologies of a Mars base.","aliases":["Moon base"],"sources":["nasa"]},{"id":"space_infrastructure:space-elevator","type":"space_infrastructure","name":"Space Elevator","domain":"science","entryPath":"/space-infrastructure/space-elevator","description":"A cable anchored to the ground and reaching beyond geostationary orbit, up which vehicles would climb to space without rockets. It remains theoretical: no known material has the strength-to-weight needed to build the tether on Earth.","sources":["nasa"]},{"id":"space_infrastructure:mass-driver","type":"space_infrastructure","name":"Mass Driver","domain":"science","entryPath":"/space-infrastructure/mass-driver","description":"An electromagnetic catapult that accelerates payloads to high speed along a track — proposed especially on the Moon, where the low gravity and airlessness would let a mass driver launch mined material into space without rockets.","aliases":["Electromagnetic launcher"],"sources":["nasa"]},{"id":"space_infrastructure:solar-power-satellite","type":"space_infrastructure","name":"Solar Power Satellite","domain":"science","entryPath":"/space-infrastructure/solar-power-satellite","description":"A large satellite that collects sunlight in orbit — where the Sun always shines — and beams the energy to receivers on the ground as microwaves. Small-scale power-beaming has been demonstrated; a full system remains a concept.","aliases":["Space solar power"],"sources":["nasa"]},{"id":"space_infrastructure:surface-fission-power","type":"space_infrastructure","name":"Surface Fission Power","domain":"science","entryPath":"/space-infrastructure/surface-fission-power","description":"Compact nuclear reactors to power a Moon or Mars base through the long lunar night and the dim Martian winter, when solar power is not enough. NASA's KRUSTY test demonstrated the underlying Kilopower reactor technology on the ground.","aliases":["Fission surface power","Kilopower"],"sources":["nasa"]},{"id":"space_infrastructure:space-tug","type":"space_infrastructure","name":"Space Tug","domain":"science","entryPath":"/space-infrastructure/space-tug","description":"A reusable vehicle that moves other spacecraft between orbits — delivering satellites to their final orbit, boosting or de-orbiting them, and ferrying cargo — a workhorse of an in-space transport network.","aliases":["Orbital transfer vehicle"],"sources":["nasa"]},{"id":"space_infrastructure:orbital-refueling","type":"space_infrastructure","name":"Orbital Refuelling","domain":"science","entryPath":"/space-infrastructure/orbital-refueling","description":"Transferring propellant between spacecraft in orbit, so a vehicle can be refuelled rather than replaced. Refuelling a large in-space stage is central to plans for crewed missions to the Moon and Mars.","aliases":["In-space refuelling"],"sources":["nasa"]},{"id":"space_infrastructure:reusable-logistics-vehicle","type":"space_infrastructure","name":"Reusable Logistics Vehicle","domain":"science","entryPath":"/space-infrastructure/reusable-logistics-vehicle","description":"Cargo spacecraft that resupply stations and return payloads, increasingly designed to be reused. Commercial cargo vehicles routinely deliver supplies to the ISS, and reusable capsules now return and fly again.","aliases":["Reusable cargo vehicle"],"sources":["nasa"]},{"id":"exploration_theme:lunar-exploration","type":"exploration_theme","name":"Lunar Exploration","domain":"science","entryPath":"/future-exploration/lunar-exploration","description":"The return of humans to the Moon and the build-out of a sustained presence — the Artemis crewed missions and the Gateway station in lunar orbit.","sources":["nasa"]},{"id":"exploration_theme:mars-exploration","type":"exploration_theme","name":"Mars Exploration","domain":"science","entryPath":"/future-exploration/mars-exploration","description":"The next steps at Mars — returning the samples now being cached by Perseverance, studying the moons of Mars, and preparing for human missions.","sources":["nasa"]},{"id":"exploration_theme:venus-exploration","type":"exploration_theme","name":"Venus 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us.","sources":["nasa"]},{"id":"exploration_theme:astrophysics-observatories","type":"exploration_theme","name":"Astrophysics Observatories","domain":"science","entryPath":"/future-exploration/astrophysics-observatories","description":"The great observatories of the coming decades — surveying dark energy, imaging habitable worlds, and opening the low-frequency gravitational-wave and X-ray skies.","sources":["nasa","esa"]},{"id":"exploration_theme:outer-solar-system","type":"exploration_theme","name":"Outer Solar System","domain":"science","entryPath":"/future-exploration/outer-solar-system","description":"Reaching the least-explored worlds — an orbiter for an ice giant, and a probe designed to travel deliberately beyond the heliosphere into interstellar space.","sources":["nasa"]},{"id":"mission_concept:artemis-ii","type":"mission_concept","name":"Artemis II","domain":"science","entryPath":"/future-exploration/artemis-ii","description":"The first crewed flight of NASA's Artemis program — a crew of four flying around the Moon and back aboard Orion, the first humans beyond low Earth orbit since 1972.","sources":["nasa"]},{"id":"mission_concept:artemis-iii","type":"mission_concept","name":"Artemis III","domain":"science","entryPath":"/future-exploration/artemis-iii","description":"The mission intended to return humans to the surface of the Moon — the first crewed lunar landing since Apollo 17, targeting the water-ice-bearing south-polar region.","sources":["nasa"]},{"id":"mission_concept:davinci","type":"mission_concept","name":"DAVINCI","domain":"science","entryPath":"/future-exploration/davinci","description":"A NASA Discovery mission to drop a probe through the atmosphere of Venus, measuring its chemistry and origins layer by layer, and imaging the surface as it descends.","aliases":["Deep Atmosphere Venus 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will fly across the dunes and impact craters of Saturn's moon Titan, sampling a world with a thick atmosphere and a rich organic chemistry.","sources":["nasa"]},{"id":"mission_concept:neo-surveyor","type":"mission_concept","name":"NEO Surveyor","domain":"science","entryPath":"/future-exploration/neo-surveyor","description":"A NASA infrared space telescope dedicated to planetary defence — hunting for the near-Earth objects that are hard to spot from the ground, to find hazards decades before any possible impact.","aliases":["Near-Earth Object Surveyor"],"sources":["nasa"]},{"id":"mission_concept:habitable-worlds-observatory","type":"mission_concept","name":"Habitable Worlds Observatory","domain":"science","entryPath":"/future-exploration/habitable-worlds-observatory","description":"NASA's next flagship space telescope, recommended by the astronomy decadal survey — designed to directly image potentially habitable planets around other stars and search their atmospheres for signs of life.","aliases":["HWO"],"sources":["nasa"]},{"id":"mission_concept:athena","type":"mission_concept","name":"Athena","domain":"science","entryPath":"/future-exploration/athena","description":"ESA's next great X-ray observatory — designed to study the hot, energetic universe, from the gas that binds galaxy clusters to the black holes that shaped galaxies, at far higher sensitivity than today's X-ray telescopes.","aliases":["Advanced Telescope for High-Energy Astrophysics","NewAthena"],"sources":["esa"]},{"id":"mission_concept:lisa","type":"mission_concept","name":"LISA","domain":"science","entryPath":"/future-exploration/lisa","description":"A space-based gravitational-wave observatory — three spacecraft forming a giant laser interferometer to hear the low-frequency ripples in spacetime that ground detectors cannot, from the mergers of the largest black holes.","aliases":["Laser Interferometer Space 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The foundation on which distances across the galaxy are built.","sources":["nasa"]},{"id":"method_category:photometry-and-imaging","type":"method_category","name":"Photometry & Imaging","domain":"science","entryPath":"/methods/photometry-and-imaging","description":"Measuring how bright things are and resolving their fine detail — the magnitude system, precision photometry, and the interferometry and adaptive optics that sharpen the view.","sources":["nasa"]},{"id":"method_category:spectroscopy-and-classification","type":"method_category","name":"Spectroscopy & Classification","domain":"science","entryPath":"/methods/spectroscopy-and-classification","description":"Splitting light into its spectrum to read the composition, temperature, motion, and magnetic fields of distant objects — and classifying stars by what their spectra reveal.","sources":["nasa"]},{"id":"method_category:the-cosmic-distance-ladder","type":"method_category","name":"The Cosmic Distance Ladder","domain":"science","entryPath":"/methods/the-cosmic-distance-ladder","description":"How astronomers measure distances across the universe — a ladder from parallax to standard candles to redshift, each rung calibrating the next, reaching from nearby stars to the edge of the observable universe.","sources":["nasa"]},{"id":"method_category:exoplanet-detection","type":"method_category","name":"Exoplanet Detection","domain":"science","entryPath":"/methods/exoplanet-detection","description":"The techniques that find and weigh planets around other stars — from the tiny dimming of a transit to the wobble of radial velocity — most of them modelled already in the exoplanet encyclopedia.","sources":["nasa"]},{"id":"method_category:time-domain-and-seismology","type":"method_category","name":"Time-Domain & Seismology","domain":"science","entryPath":"/methods/time-domain-and-seismology","description":"Watching how things change with time — the oscillations that let us sound the interiors of the Sun and stars, the occultations that reveal sizes, and the study of the variable and transient sky.","sources":["nasa"]},{"id":"method_category:gravitation-and-multi-messenger","type":"method_category","name":"Gravitation & Multi-Messenger","domain":"science","entryPath":"/methods/gravitation-and-multi-messenger","description":"Astronomy beyond light — the bending of light by gravity, the direct detection of gravitational waves and cosmic neutrinos, and the combined multi-messenger view of the most violent events.","sources":["nasa"]},{"id":"method_category:measurement-data-and-statistics","type":"method_category","name":"Measurement, Data & Statistics","domain":"science","entryPath":"/methods/measurement-data-and-statistics","description":"How raw measurements become knowledge — deriving the properties of stars and galaxies, weighing black holes, mapping dark matter through rotation curves, and the calibration, error analysis, and honest uncertainty that make a measurement science.","sources":["nasa"]},{"id":"astronomy_method:parallax","type":"astronomy_method","name":"Parallax","domain":"science","entryPath":"/methods/parallax","description":"The apparent shift of a nearby star against distant background stars as the Earth orbits the Sun. The size of that shift gives the star's distance by simple geometry — the first and most fundamental rung of the distance ladder.","aliases":["Trigonometric parallax"],"sources":["nasa","esa"]},{"id":"astronomy_method:proper-motion","type":"astronomy_method","name":"Proper Motion","domain":"science","entryPath":"/methods/proper-motion","description":"The slow drift of a star across the sky over years, as it and the Sun move through the galaxy. Combined with radial velocity and distance, it yields a star's true motion through space.","sources":["nasa","esa"]},{"id":"astronomy_method:space-astrometry","type":"astronomy_method","name":"Space Astrometry","domain":"science","entryPath":"/methods/space-astrometry","description":"Measuring stellar positions, distances, and motions from space at extraordinary precision. ESA's Hipparcos and then Gaia have charted more than a billion stars, transforming our three-dimensional map of the galaxy.","aliases":["Gaia","Hipparcos"],"sources":["esa","nasa"]},{"id":"astronomy_method:photometry","type":"astronomy_method","name":"Photometry","domain":"science","entryPath":"/methods/photometry","description":"The precise measurement of the brightness of a star or galaxy, in one or more filters. Photometry over time reveals variable stars, transiting planets, and supernovae; photometry in different colours reveals temperature.","sources":["nasa"]},{"id":"astronomy_method:the-magnitude-system","type":"astronomy_method","name":"The Magnitude System","domain":"science","entryPath":"/methods/the-magnitude-system","description":"Astronomy's logarithmic, backwards brightness scale, in which smaller numbers are brighter. Apparent magnitude is how bright an object looks; absolute magnitude is how bright it truly is — and the difference gives its distance.","aliases":["Apparent and absolute magnitude"],"sources":["nasa"]},{"id":"astronomy_method:interferometry","type":"astronomy_method","name":"Interferometry","domain":"science","entryPath":"/methods/interferometry","description":"Combining the light of separate telescopes so they act as one much larger instrument, achieving resolution impossible for a single dish. Radio interferometry links antennas across continents; it produced the first images of black-hole shadows.","sources":["nasa"]},{"id":"astronomy_method:adaptive-optics","type":"astronomy_method","name":"Adaptive Optics","domain":"science","entryPath":"/methods/adaptive-optics","description":"Deformable mirrors that flex hundreds of times a second to cancel the blurring of Earth's turbulent atmosphere, giving ground telescopes near space-quality sharpness.","sources":["nasa"]},{"id":"astronomy_method:spectroscopy","type":"astronomy_method","name":"Spectroscopy","domain":"science","entryPath":"/methods/spectroscopy","description":"Spreading light into its spectrum to read the fingerprints of the elements. Spectral lines reveal what an object is made of, how hot it is, how it moves (through the Doppler shift), and the strength of its magnetic fields — the single most powerful tool in astronomy.","sources":["nasa"]},{"id":"astronomy_method:spectral-classification","type":"astronomy_method","name":"Spectral Classification","domain":"science","entryPath":"/methods/spectral-classification","description":"Sorting stars by the lines in their spectra into the sequence O, B, A, F, G, K, M — a classification that turned out to be an ordering by temperature, and the basis of the Hertzsprung–Russell diagram.","aliases":["The OBAFGKM sequence"],"sources":["nasa"]},{"id":"astronomy_method:polarimetry","type":"astronomy_method","name":"Polarimetry","domain":"science","entryPath":"/methods/polarimetry","description":"Measuring the polarisation of light, which carries information no brightness or spectrum can — magnetic-field geometry, scattering by dust and grains, and the physics of everything from stellar surfaces to the cosmic microwave background.","sources":["nasa"]},{"id":"astronomy_method:standard-candles","type":"astronomy_method","name":"Standard Candles","domain":"science","entryPath":"/methods/standard-candles","description":"Objects whose true brightness is known, so that how faint they appear gives their distance. Cepheid variables and Type Ia supernovae are the great standard candles that carry the distance ladder out into the universe.","sources":["nasa"]},{"id":"astronomy_method:cepheid-distance-scale","type":"astronomy_method","name":"The Cepheid Distance Scale","domain":"science","entryPath":"/methods/cepheid-distance-scale","description":"Cepheid variable stars pulse with a period that depends on their true luminosity — Henrietta Leavitt's discovery. Measure the period, know the luminosity, and the apparent brightness gives the distance. Cepheids calibrated the scale of the galaxy and beyond.","aliases":["Period–luminosity relation"],"sources":["nasa"]},{"id":"astronomy_method:redshift-and-hubble-law","type":"astronomy_method","name":"Redshift & the Hubble–Lemaître Law","domain":"science","entryPath":"/methods/redshift-and-hubble-law","description":"For distant galaxies, the expansion of the universe stretches their light to longer, redder wavelengths in proportion to their distance. Measure the redshift, apply the Hubble–Lemaître law, and you have the distance — the top rung of the ladder.","sources":["nasa"]},{"id":"astronomy_method:cosmic-distance-ladder","type":"astronomy_method","name":"The Cosmic Distance Ladder","domain":"science","entryPath":"/methods/cosmic-distance-ladder","description":"The chain of methods, each calibrating the next, that measures the universe: geometric parallax for nearby stars, standard candles for nearby galaxies, and redshift for the far reaches. The mismatch between its rungs is at the heart of today's Hubble tension.","sources":["nasa"]},{"id":"astronomy_method:helioseismology","type":"astronomy_method","name":"Helioseismology","domain":"science","entryPath":"/methods/helioseismology","description":"Reading the Sun's interior from the oscillations that ripple across its surface, as seismologists read the Earth from earthquakes. Helioseismology has mapped the Sun's internal rotation and the depth of its convection zone.","sources":["nasa"]},{"id":"astronomy_method:asteroseismology","type":"astronomy_method","name":"Asteroseismology","domain":"science","entryPath":"/methods/asteroseismology","description":"Applying the same idea to other stars — measuring their tiny brightness oscillations to determine their internal structure, mass, radius, and age. Space photometry from Kepler and TESS turned it into a precision tool.","sources":["nasa"]},{"id":"astronomy_method:stellar-occultations","type":"astronomy_method","name":"Stellar Occultations","domain":"science","entryPath":"/methods/stellar-occultations","description":"Watching a star wink out as a foreground body passes in front of it. The timing reveals the size and shape of asteroids, the rings of the giant planets, and the atmospheres of distant worlds — even Pluto's.","sources":["nasa"]},{"id":"astronomy_method:gravitational-lensing","type":"astronomy_method","name":"Gravitational Lensing","domain":"science","entryPath":"/methods/gravitational-lensing","description":"Gravity bends light, so massive foreground objects magnify and distort background ones — strongly, into arcs and multiple images, or weakly, subtly shearing distant galaxies. Lensing weighs matter directly, mapping dark matter that emits no light.","aliases":["Weak lensing","Strong lensing"],"sources":["nasa"]},{"id":"astronomy_method:gravitational-wave-detection","type":"astronomy_method","name":"Gravitational-Wave Detection","domain":"science","entryPath":"/methods/gravitational-wave-detection","description":"Detecting the minute stretching and squeezing of space as gravitational waves pass, using kilometre-scale laser interferometers. Since 2015, detectors have heard the mergers of black holes and neutron stars, opening a new sense for astronomy.","sources":["nasa"]},{"id":"astronomy_method:neutrino-astronomy","type":"astronomy_method","name":"Neutrino Astronomy","domain":"science","entryPath":"/methods/neutrino-astronomy","description":"Catching the ghostly neutrinos that stream from the Sun, from supernovae, and from the most energetic events in the universe. Neutrinos pass through matter almost untouched, carrying information from places light cannot escape.","sources":["nasa"]},{"id":"astronomy_method:multi-messenger-astronomy","type":"astronomy_method","name":"Multi-Messenger Astronomy","domain":"science","entryPath":"/methods/multi-messenger-astronomy","description":"Combining light, gravitational waves, neutrinos, and cosmic rays from the same event to learn what no single messenger could tell. The 2017 neutron-star merger, seen in gravitational waves and across the spectrum, was its landmark.","sources":["nasa"]},{"id":"astronomy_method:cmb-measurements","type":"astronomy_method","name":"CMB Measurements","domain":"science","entryPath":"/methods/cmb-measurements","description":"Mapping the faint microwave afterglow of the Big Bang and its minute temperature and polarisation ripples. Their statistics — including the baryon acoustic oscillations frozen into them — pin down the composition, geometry, and age of the universe.","aliases":["Cosmic microwave background measurements"],"sources":["nasa"]},{"id":"astronomy_method:determining-stellar-properties","type":"astronomy_method","name":"Determining Stellar Properties","domain":"science","entryPath":"/methods/determining-stellar-properties","description":"How the measurable — brightness, colour, spectrum, motion — becomes the physical: a star's temperature, luminosity, mass, radius, chemical composition (metallicity), and age, mostly inferred through models rather than measured directly.","aliases":["Temperature, luminosity, mass, metallicity, age"],"sources":["nasa"]},{"id":"astronomy_method:galaxy-rotation-curves","type":"astronomy_method","name":"Galaxy Rotation Curves","domain":"science","entryPath":"/methods/galaxy-rotation-curves","description":"Measuring how fast a galaxy rotates at each radius, usually from the Doppler shift of its gas. The stars orbit far faster than the visible matter can explain — the classic evidence that galaxies are embedded in halos of dark matter.","sources":["nasa"]},{"id":"astronomy_method:black-hole-mass-measurement","type":"astronomy_method","name":"Black-Hole Mass Measurement","domain":"science","entryPath":"/methods/black-hole-mass-measurement","description":"Weighing a black hole by the motion of what orbits it — stars near the galactic centre, gas in a disk, or the gravitational waves of a merger. The masses range from a few Suns to billions.","sources":["nasa"]},{"id":"astronomy_method:error-analysis-and-calibration","type":"astronomy_method","name":"Error Analysis & Calibration","domain":"science","entryPath":"/methods/error-analysis-and-calibration","description":"The discipline that makes a number science: calibrating instruments against known standards, tying measurements to common reference frames, propagating uncertainties, and stating the statistical confidence of a result. In astronomy, a measurement without an error bar is not a measurement.","aliases":["Uncertainty, statistics, reference frames"],"sources":["nasa"]},{"id":"transient_class:type-ia-supernova","type":"transient_class","name":"Type Ia Supernova","domain":"science","entryPath":"/time-domain/type-ia-supernova","description":"The thermonuclear detonation of a white dwarf that has been pushed over a critical mass. Their remarkably uniform peak brightness makes them the standard candles that measured the accelerating expansion of the universe.","aliases":["Thermonuclear supernova"],"sources":["nasa"]},{"id":"transient_class:core-collapse-supernova","type":"transient_class","name":"Core-Collapse Supernova","domain":"science","entryPath":"/time-domain/core-collapse-supernova","description":"The catastrophic collapse of the core of a massive star, which rebounds into an explosion and leaves a neutron star or black hole. Most of the energy escapes as neutrinos — first detected from SN 1987A — making these among the earliest multi-messenger sources.","aliases":["Type II supernova","Type Ib/Ic supernova"],"sources":["nasa"]},{"id":"transient_class:hypernova","type":"transient_class","name":"Hypernova","domain":"science","entryPath":"/time-domain/hypernova","description":"An exceptionally energetic core-collapse explosion of a very massive star, releasing far more kinetic energy than an ordinary supernova. Hypernovae from rapidly-rotating collapsars are thought to power the long gamma-ray bursts.","aliases":["Broad-lined Type Ic supernova","Collapsar"],"sources":["nasa"]},{"id":"transient_class:classical-nova","type":"transient_class","name":"Classical Nova","domain":"science","entryPath":"/time-domain/classical-nova","description":"A thermonuclear runaway on the surface of a white dwarf that is accreting matter from a companion star. Unlike a supernova, the white dwarf survives, and the outburst can recur.","aliases":["Nova"],"sources":["nasa"]},{"id":"transient_class:gamma-ray-burst","type":"transient_class","name":"Gamma-Ray Burst","domain":"science","entryPath":"/time-domain/gamma-ray-burst","description":"The most luminous electromagnetic events in the universe — brief, intense flashes of gamma rays. Long bursts come from the collapse of massive stars; short bursts from the mergers of neutron stars. Each is followed by a fading multi-wavelength afterglow.","aliases":["GRB"],"sources":["nasa"]},{"id":"transient_class:magnetar-flare","type":"transient_class","name":"Magnetar Flare","domain":"science","entryPath":"/time-domain/magnetar-flare","description":"Sudden, intense bursts of gamma and X-rays from magnetars — neutron stars with the strongest magnetic fields known. Their giant flares are so bright they can be detected across the galaxy, and are now linked to some fast radio bursts.","aliases":["Soft gamma repeater","Giant flare"],"sources":["nasa"]},{"id":"transient_class:kilonova","type":"transient_class","name":"Kilonova","domain":"science","entryPath":"/time-domain/kilonova","description":"The optical and infrared glow that follows the merger of two neutron stars, powered by the radioactive decay of the heavy elements forged in the merger. The 2017 event GW170817, seen in gravitational waves and light, was the landmark of multi-messenger astronomy.","sources":["nasa"]},{"id":"transient_class:compact-binary-merger","type":"transient_class","name":"Compact-Binary Merger","domain":"science","entryPath":"/time-domain/compact-binary-merger","description":"The inspiral and merger of two compact objects — black holes or neutron stars — radiating a chirp of gravitational waves. Since 2015 these have been heard routinely; neutron-star mergers also shine as kilonovae.","aliases":["Black-hole / neutron-star merger"],"sources":["nasa"]},{"id":"transient_class:tidal-disruption-event","type":"transient_class","name":"Tidal Disruption Event","domain":"science","entryPath":"/time-domain/tidal-disruption-event","description":"The flare produced when a star wanders too close to a supermassive black hole and is torn apart by tides, some of its debris blazing as it falls in. TDEs light up otherwise-quiet galactic nuclei for months.","aliases":["TDE"],"sources":["nasa"]},{"id":"transient_class:fast-radio-burst","type":"transient_class","name":"Fast Radio Burst","domain":"science","entryPath":"/time-domain/fast-radio-burst","description":"Millisecond flashes of radio waves from far across the universe, immensely energetic for their brevity. At least some come from magnetars; most are one-off, though a few repeat. Their dispersion probes the matter between the galaxies.","aliases":["FRB"],"sources":["nasa"]},{"id":"transient_class:cataclysmic-variable","type":"transient_class","name":"Cataclysmic Variable","domain":"science","entryPath":"/time-domain/cataclysmic-variable","description":"A close binary in which a white dwarf accretes matter from a companion through a disk, producing recurrent outbursts as the disk brightens — the dwarf novae and related variables of the time-domain sky.","aliases":["Dwarf nova"],"sources":["nasa"]},{"id":"transient_class:eruptive-variable-star","type":"transient_class","name":"Eruptive Variable Star","domain":"science","entryPath":"/time-domain/eruptive-variable-star","description":"Stars whose brightness changes irregularly through eruptions and flares — from the giant eruptions of luminous blue variables to the flares of young and magnetically-active stars.","aliases":["Flare star","Luminous blue variable"],"sources":["nasa"]},{"id":"alert_system:gcn","type":"alert_system","name":"General Coordinates Network","domain":"science","entryPath":"/time-domain/gcn","description":"NASA's network for the rapid distribution of alerts about transient events — gamma-ray bursts, gravitational-wave triggers, and neutrino detections — so that telescopes around the world can slew to a fresh event within seconds.","aliases":["GCN","Gamma-ray Coordinates Network"],"sources":["nasa"]},{"id":"alert_system:voevent","type":"alert_system","name":"VOEvent","domain":"science","entryPath":"/time-domain/voevent","description":"The Virtual Observatory's standard machine-readable format for reporting a transient celestial event — what, where, when, and how confident — so that alerts flow automatically between observatories, brokers, and robotic telescopes.","sources":["nasa"]},{"id":"alert_system:transient-name-server","type":"alert_system","name":"Transient Name Server","domain":"science","entryPath":"/time-domain/transient-name-server","description":"The official IAU registry that assigns the discovery names of supernovae and other transients, and collects the reports and classifications that establish who found what, and when.","aliases":["TNS"],"sources":["nasa"]},{"id":"alert_system:astronomers-telegram","type":"alert_system","name":"The Astronomer's Telegram","domain":"science","entryPath":"/time-domain/astronomers-telegram","description":"A short-notice publication service for rapidly announcing and commenting on new astronomical observations, widely used to share follow-up of transients within hours.","aliases":["ATel"],"sources":["nasa"]},{"id":"alert_system:rubin-alert-stream","type":"alert_system","name":"Rubin Alert Stream","domain":"science","entryPath":"/time-domain/rubin-alert-stream","description":"The torrent of alerts the Vera C. Rubin Observatory will issue — millions per night — as it scans the whole southern sky every few nights, feeding community brokers that filter the deluge into the events worth chasing.","aliases":["LSST alert stream"],"sources":["nasa"]},{"id":"observation_stage:discovery","type":"observation_stage","name":"Discovery","domain":"science","entryPath":"/time-domain/discovery","description":"A wide-field survey images the sky repeatedly and flags anything that has changed — a new point of light, or one that has brightened or moved. The candidate is issued as an alert within seconds.","sources":["nasa"]},{"id":"observation_stage:follow-up","type":"observation_stage","name":"Follow-Up","domain":"science","entryPath":"/time-domain/follow-up","description":"Other telescopes turn to the candidate to gather more data — deeper images, colours, and the first spectra — often within minutes to hours, before a fast-fading event disappears.","sources":["nasa"]},{"id":"observation_stage:confirmation","type":"observation_stage","name":"Confirmation","domain":"science","entryPath":"/time-domain/confirmation","description":"The candidate is verified as a real astrophysical transient — not an instrument artefact, asteroid, or known variable — and registered with an official discovery name.","sources":["nasa"]},{"id":"observation_stage:classification","type":"observation_stage","name":"Classification","domain":"science","entryPath":"/time-domain/classification","description":"A spectrum reveals what the transient is — the type of supernova, the redshift of a burst, the nature of the source — placing it in its class and distance.","sources":["nasa"]},{"id":"observation_stage:publication","type":"observation_stage","name":"Publication","domain":"science","entryPath":"/time-domain/publication","description":"The result is shared with the community and the scientific record — as a rapid telegram, a circular, and ultimately a peer-reviewed paper — so that the event contributes to the wider science.","sources":["nasa"]},{"id":"galaxy_morphology:spiral","type":"galaxy_morphology","name":"Spiral Galaxy","domain":"science","entryPath":"/galaxies/spiral","description":"A flattened, rotating disk of stars, gas, and dust wound into spiral arms, with a central bulge. The arms are where new stars form, tracing waves of star formation sweeping through the disk.","sources":["nasa"]},{"id":"galaxy_morphology:barred-spiral","type":"galaxy_morphology","name":"Barred Spiral Galaxy","domain":"science","entryPath":"/galaxies/barred-spiral","description":"A spiral galaxy whose arms wind out from the ends of a straight bar of stars crossing the centre. The bar channels gas inward, feeding star formation and the central black hole. The Milky Way is one.","sources":["nasa"]},{"id":"galaxy_morphology:elliptical","type":"galaxy_morphology","name":"Elliptical Galaxy","domain":"science","entryPath":"/galaxies/elliptical","description":"A smooth, featureless ellipsoid of mostly old stars, with little gas and little ongoing star formation. The largest ellipticals sit at the centres of galaxy clusters and are thought to be built by mergers.","sources":["nasa"]},{"id":"galaxy_morphology:lenticular","type":"galaxy_morphology","name":"Lenticular Galaxy","domain":"science","entryPath":"/galaxies/lenticular","description":"A disk galaxy with a prominent bulge but no spiral arms — a transitional form between spirals and ellipticals, with an old stellar population and little cold gas left to form stars.","sources":["nasa"]},{"id":"galaxy_morphology:irregular","type":"galaxy_morphology","name":"Irregular Galaxy","domain":"science","entryPath":"/galaxies/irregular","description":"A galaxy with no regular spiral or elliptical structure, often small and gas-rich with vigorous star formation. Many are shaped by the gravitational pull of larger neighbours, like the Magellanic Clouds beside the Milky Way.","sources":["nasa"]},{"id":"galaxy_morphology:ring","type":"galaxy_morphology","name":"Ring Galaxy","domain":"science","entryPath":"/galaxies/ring","description":"A galaxy with a bright ring of stars and gas around a comparatively empty centre, usually formed when a smaller galaxy plunges through the disk of a larger one, sending a wave of star formation outward.","sources":["nasa"]},{"id":"galaxy_morphology:dwarf","type":"galaxy_morphology","name":"Dwarf Galaxy","domain":"science","entryPath":"/galaxies/dwarf","description":"A small galaxy with far fewer stars than a giant like the Milky Way. Dwarfs are by far the most numerous galaxies, and many orbit larger ones as satellites; they are dominated by dark matter.","sources":["nasa"]},{"id":"galaxy_morphology:peculiar","type":"galaxy_morphology","name":"Peculiar & Interacting Galaxy","domain":"science","entryPath":"/galaxies/peculiar","description":"A galaxy distorted from any regular form — by a close encounter, an ongoing merger, or an active nucleus. The tidal tails and bridges of interacting pairs, like the Antennae, are the clearest signs of galaxies in collision.","sources":["nasa"]},{"id":"agn_type:seyfert-galaxy","type":"agn_type","name":"Seyfert Galaxy","domain":"science","entryPath":"/galaxies/seyfert-galaxy","description":"A spiral galaxy with a bright, compact active nucleus whose spectrum shows broad or narrow emission lines from gas swirling near the central black hole — a relatively low-luminosity active galactic nucleus in an otherwise normal-looking galaxy.","sources":["nasa"]},{"id":"agn_type:liner","type":"agn_type","name":"LINER","domain":"science","entryPath":"/galaxies/liner","description":"A galactic nucleus whose spectrum is dominated by emission from weakly-ionized gas. LINERs are the most common type of active nucleus, though whether they are all powered by a black hole or partly by hot old stars is still debated.","aliases":["Low-Ionization Nuclear Emission-line Region"],"sources":["nasa"]},{"id":"agn_type:radio-galaxy","type":"agn_type","name":"Radio Galaxy","domain":"science","entryPath":"/galaxies/radio-galaxy","description":"A galaxy — usually a giant elliptical — that pours enormous energy into twin jets and lobes of radio-emitting plasma, launched by its central black hole and reaching far beyond the visible galaxy. Centaurus A is the nearest.","sources":["nasa"]},{"id":"agn_type:bl-lac-object","type":"agn_type","name":"BL Lac Object","domain":"science","entryPath":"/galaxies/bl-lac-object","description":"A blazar seen looking almost straight down its jet, so its light is dominated by the rapidly-variable, featureless glow of the jet itself rather than by emission lines — one of the most extreme, fast-varying kinds of active nucleus.","aliases":["BL Lacertae object"],"sources":["nasa"]},{"id":"agn_model:unified-agn-model","type":"agn_model","name":"The Unified AGN Model","domain":"science","entryPath":"/galaxies/unified-agn-model","description":"The framework that the many types of active galactic nucleus — Seyferts, quasars, radio galaxies, blazars — are largely the same underlying object, a supermassive black hole accreting through a disk and torus, seen from different angles and at different luminosities. A model that explains the types, rather than a type itself.","sources":["nasa"]},{"id":"galactic_process:galaxy-evolution","type":"galactic_process","name":"Galaxy Evolution","domain":"science","entryPath":"/galaxies/galaxy-evolution","description":"How galaxies grow and change over cosmic time — assembling from smaller pieces, forming stars, exhausting or losing their gas, and transforming from blue, star-forming disks into red, quiescent ellipticals.","sources":["nasa"]},{"id":"galactic_process:galaxy-merger","type":"galactic_process","name":"Galaxy Merger","domain":"science","entryPath":"/galaxies/galaxy-merger","description":"The collision and coalescence of two galaxies. Mergers trigger bursts of star formation, funnel gas to the central black hole, and can turn two spirals into a single elliptical — a driving force of galaxy evolution.","sources":["nasa"]},{"id":"galactic_process:galaxy-interaction","type":"galactic_process","name":"Galaxy Interaction","domain":"science","entryPath":"/galaxies/galaxy-interaction","description":"The gravitational give-and-take of galaxies passing close without fully merging — drawing out tidal tails and bridges, triggering star formation, and, in a direct hit, punching out a ring galaxy.","sources":["nasa"]},{"id":"galactic_process:black-hole-feedback","type":"galactic_process","name":"Black-Hole Feedback","domain":"science","entryPath":"/galaxies/black-hole-feedback","description":"The way an active central black hole regulates its galaxy — its winds and jets heating and expelling gas, quenching star formation, and explaining the tight link between a galaxy's black-hole mass and its bulge.","aliases":["AGN feedback"],"sources":["nasa"]},{"id":"galactic_process:starburst","type":"galactic_process","name":"Starburst","domain":"science","entryPath":"/galaxies/starburst","description":"A phase of exceptionally intense star formation, forming stars far faster than a galaxy can sustain — often triggered by a merger or interaction and driving powerful galactic winds. M82 is the archetype.","sources":["nasa"]},{"id":"galactic_process:galaxy-quenching","type":"galactic_process","name":"Galaxy Quenching","domain":"science","entryPath":"/galaxies/galaxy-quenching","description":"The shutdown of star formation in a galaxy, as it loses or is stripped of its cold gas, or has it heated by feedback — leaving a red, passively-evolving elliptical or lenticular of ageing stars.","sources":["nasa"]},{"id":"cosmic_structure:local-group","type":"cosmic_structure","name":"The Local Group","domain":"science","entryPath":"/galaxies/local-group","description":"The gravitationally-bound group of galaxies the Milky Way belongs to — dominated by the Milky Way and Andromeda, with the Triangulum galaxy and dozens of dwarfs. Andromeda and the Milky Way are approaching, and will merge in a few billion years.","sources":["nasa"]},{"id":"cosmic_structure:virgo-cluster","type":"cosmic_structure","name":"The Virgo Cluster","domain":"science","entryPath":"/galaxies/virgo-cluster","description":"The nearest large galaxy cluster, over a thousand galaxies bound together and centred on the giant elliptical M87. Its gravity draws the Local Group toward it, and it anchors our corner of the local supercluster.","sources":["nasa"]},{"id":"cosmic_structure:coma-cluster","type":"cosmic_structure","name":"The Coma Cluster","domain":"science","entryPath":"/galaxies/coma-cluster","description":"A rich, dense cluster of over a thousand galaxies. In 1933 Fritz Zwicky found its galaxies moving far too fast to be held together by their visible mass — the first evidence for dark matter.","sources":["nasa"]},{"id":"cosmic_structure:laniakea-supercluster","type":"cosmic_structure","name":"Laniakea Supercluster","domain":"science","entryPath":"/galaxies/laniakea-supercluster","description":"The vast supercluster the Milky Way belongs to, defined in 2014 by the flows of galaxies toward a common gravitational focus. It contains around a hundred thousand galaxies across half a billion light-years.","aliases":["Laniakea"],"sources":["nasa"]},{"id":"cosmic_structure:sloan-great-wall","type":"cosmic_structure","name":"The Sloan Great Wall","domain":"science","entryPath":"/galaxies/sloan-great-wall","description":"One of the largest known structures in the universe — an immense wall of galaxies stretching over a billion light-years, mapped by the Sloan Digital Sky Survey, part of the filamentary cosmic web.","sources":["nasa"]},{"id":"cosmic_structure:bootes-void","type":"cosmic_structure","name":"The Boötes Void","domain":"science","entryPath":"/galaxies/bootes-void","description":"One of the largest known voids — an enormous, nearly-empty region of space containing very few galaxies, a vast bubble between the filaments and walls of the cosmic web.","aliases":["The Great Void"],"sources":["nasa"]},{"id":"astrobiology_topic:origins-of-life","type":"astrobiology_topic","name":"Origins of Life","domain":"science","entryPath":"/astrobiology/origins-of-life","description":"The study of how life began — the chemistry that turned simple molecules into self-replicating systems on the early Earth, and whether the same steps could happen elsewhere. A question that frames the entire search for life beyond Earth.","sources":["nasa"]},{"id":"astrobiology_topic:planetary-habitability","type":"astrobiology_topic","name":"Planetary Habitability","domain":"science","entryPath":"/astrobiology/planetary-habitability","description":"What makes a world able to host life — liquid water, an energy source, the chemical building blocks, and a stable enough environment for long enough. Habitability is judged by these factors, not by any detection of life.","sources":["nasa"]},{"id":"astrobiology_topic:biosignature-science","type":"astrobiology_topic","name":"Biosignature Science","domain":"science","entryPath":"/astrobiology/biosignature-science","description":"The search for signs of life — atmospheric gases, surface features, and chemical patterns that life could produce — and the rigorous work of telling a true biosignature from a false positive made by non-living processes.","sources":["nasa"]},{"id":"astrobiology_topic:technosignatures-and-seti","type":"astrobiology_topic","name":"Technosignatures & SETI","domain":"science","entryPath":"/astrobiology/technosignatures-and-seti","description":"The search for signs of technology — radio and optical signals, and other technosignatures — carried out by the SETI Institute and programs like Breakthrough Listen. A search for intelligence, distinct from the search for microbial life.","sources":["nasa"]},{"id":"astrobiology_topic:ocean-worlds-astrobiology","type":"astrobiology_topic","name":"Ocean Worlds","domain":"science","entryPath":"/astrobiology/ocean-worlds-astrobiology","description":"The icy moons with liquid-water oceans beneath their shells — Europa, Enceladus, and Titan — now the most promising places to search for life in the Solar System, targets of the Europa Clipper and Dragonfly missions.","sources":["nasa"]},{"id":"astrobiology_topic:planetary-protection","type":"astrobiology_topic","name":"Planetary Protection","domain":"science","entryPath":"/astrobiology/planetary-protection","description":"The discipline of preventing contamination — protecting other worlds from Earth microbes carried by spacecraft (forward contamination), and protecting Earth from any material returned from them (backward contamination), so the search for life is not fooled and no harm is done.","sources":["nasa"]},{"id":"biosignature:atmospheric-biosignature","type":"biosignature","name":"Atmospheric Biosignature","domain":"science","entryPath":"/astrobiology/atmospheric-biosignature","description":"Gases in a planet's atmosphere that life could produce and maintain — especially a chemical disequilibrium, like oxygen and methane together, that non-living chemistry would quickly erase. Detected by the spectroscopy of a planet's light.","sources":["nasa"]},{"id":"biosignature:surface-biosignature","type":"biosignature","name":"Surface Biosignature","domain":"science","entryPath":"/astrobiology/surface-biosignature","description":"Signs of life on a surface — pigments, the 'red edge' reflectance of vegetation, or patterns and textures a biosphere leaves behind — sought both on exoplanets and on the surface of Mars.","sources":["nasa"]},{"id":"biosignature:chemical-biosignature","type":"biosignature","name":"Chemical Biosignature","domain":"science","entryPath":"/astrobiology/chemical-biosignature","description":"Chemical fingerprints of life in rock or ice — the isotopic ratios life prefers, the handedness (chirality) of its molecules, and specific organic byproducts — the kind of evidence the Perseverance rover seeks and caches on Mars.","sources":["nasa"]},{"id":"biosignature:geological-biosignature","type":"biosignature","name":"Geological Biosignature","domain":"science","entryPath":"/astrobiology/geological-biosignature","description":"Structures preserved in rock that life can build — layered stromatolites, biominerals, and microfossils. Perseverance is exploring an ancient Martian river delta where such signs might be preserved.","sources":["nasa"]},{"id":"biosignature:technosignature","type":"biosignature","name":"Technosignature","domain":"science","entryPath":"/astrobiology/technosignature","description":"A sign not of life but of technology — a radio or optical signal, an artificial light, an industrial pollutant, or a megastructure. The search for technosignatures is the search for intelligence, led by SETI and Breakthrough Listen.","sources":["nasa"]},{"id":"biosignature:biosignature-false-positive","type":"biosignature","name":"Biosignature False Positive","domain":"science","entryPath":"/astrobiology/biosignature-false-positive","description":"A signal that mimics life but is made by non-living processes — abiotic oxygen from water splitting, geological methane, or a mis-measured spectral feature. Ruling out false positives is the hardest and most important part of any claim of life; the Venus phosphine debate is a recent lesson.","sources":["nasa"]},{"id":"habitability_factor:liquid-water","type":"habitability_factor","name":"Liquid Water","domain":"science","entryPath":"/astrobiology/liquid-water","description":"The one requirement every known form of life shares — a liquid solvent for its chemistry. The habitable zone is defined by where a planet could hold liquid water on its surface, but subsurface oceans extend the possibilities far beyond it.","sources":["nasa"]},{"id":"habitability_factor:energy-source","type":"habitability_factor","name":"Energy Source","domain":"science","entryPath":"/astrobiology/energy-source","description":"Life needs a source of energy to drive its chemistry — sunlight for photosynthesis, or chemical and thermal energy where the Sun cannot reach. Tidal heating warms the interiors of the icy moons, powering hydrothermal vents like those that may nourish life on Earth.","sources":["nasa"]},{"id":"habitability_factor:chemical-building-blocks","type":"habitability_factor","name":"Chemical Building Blocks","domain":"science","entryPath":"/astrobiology/chemical-building-blocks","description":"The elements and molecules life is built from — carbon, hydrogen, nitrogen, oxygen, phosphorus, sulfur, and complex organic chemistry. Titan has a rich organic chemistry, and Enceladus's plumes carry organic molecules from its ocean.","aliases":["CHNOPS"],"sources":["nasa"]},{"id":"habitability_factor:extremophiles","type":"habitability_factor","name":"Extremophiles","domain":"science","entryPath":"/astrobiology/extremophiles","description":"Earth organisms that thrive in extremes — searing vents, acid, salt, cold, and intense radiation — that once seemed impossible for life. They vastly widen where life might survive, and are the closest analogs for what an ocean-world biosphere might be.","sources":["nasa"]},{"id":"habitability_factor:subsurface-ocean","type":"habitability_factor","name":"Subsurface Ocean","domain":"science","entryPath":"/astrobiology/subsurface-ocean","description":"A layer of liquid water beneath an icy shell, kept warm by tidal heating and in contact with a rocky seafloor. Europa and Enceladus have them; they are the leading places to look for life beyond Earth, and the target of the Europa Clipper mission.","sources":["nasa"]},{"id":"planetary_protection:forward-contamination","type":"planetary_protection","name":"Forward Contamination","domain":"science","entryPath":"/astrobiology/forward-contamination","description":"The risk of carrying Earth microbes to another world on a spacecraft, which could harm any native biosphere or, worse, be mistaken for alien life. Missions to Mars and the ocean worlds are cleaned and sterilised to strict standards to prevent it.","sources":["nasa"]},{"id":"planetary_protection:backward-contamination","type":"planetary_protection","name":"Backward Contamination","domain":"science","entryPath":"/astrobiology/backward-contamination","description":"The risk of bringing potentially hazardous material back to Earth in a returned sample. Sample-return missions are designed to contain their cargo as strictly as the most dangerous pathogens, so nothing escapes before it is shown to be safe.","sources":["nasa"]},{"id":"planetary_protection:sample-handling","type":"planetary_protection","name":"Sample Handling & Curation","domain":"science","entryPath":"/astrobiology/sample-handling","description":"The careful containment, quarantine, and curation of returned samples in specialised facilities — keeping them pristine for science while keeping Earth safe, and preserving them for study by instruments not yet invented.","sources":["nasa"]},{"id":"defense_stage:neo-discovery","type":"defense_stage","name":"NEO Discovery","domain":"science","entryPath":"/planetary-defense/neo-discovery","description":"Dedicated survey telescopes scan the sky night after night for moving points of light — the near-Earth asteroids and comets. Catalina, Pan-STARRS, and ATLAS lead the search from the ground, and the Rubin Observatory will transform it.","sources":["nasa"]},{"id":"defense_stage:orbit-determination","type":"defense_stage","name":"Orbit Determination","domain":"science","entryPath":"/planetary-defense/orbit-determination","description":"A newly-found object's observations are reported to the Minor Planet Center, which links them into a single orbit. The more observations over a longer arc, the more precisely the future path is known.","sources":["nasa"]},{"id":"defense_stage:characterization","type":"defense_stage","name":"Characterization","domain":"science","entryPath":"/planetary-defense/characterization","description":"Determining what an object is — its size, shape, spin, and composition — from light curves, radar, spectra, and, for a few, spacecraft visits. Hera is en route to survey the asteroid DART struck, to learn how a deflection actually worked.","sources":["nasa"]},{"id":"defense_stage:impact-monitoring","type":"defense_stage","name":"Impact Monitoring","domain":"science","entryPath":"/planetary-defense/impact-monitoring","description":"Automatic systems at CNEOS and ESA continuously propagate every known orbit forward for a century or more, flagging any that could approach Earth. Apophis was tracked this way until observations ruled out an impact for the next century.","sources":["nasa"]},{"id":"defense_stage:risk-assessment","type":"defense_stage","name":"Risk Assessment","domain":"science","entryPath":"/planetary-defense/risk-assessment","description":"Judging how serious a possible impact is — its probability, the object's size and energy, and the time until the encounter — and expressing it on the Torino and Palermo scales so the risk can be understood and compared.","sources":["nasa"]},{"id":"defense_stage:risk-communication","type":"defense_stage","name":"Risk Communication","domain":"science","entryPath":"/planetary-defense/risk-communication","description":"Explaining a risk to decision-makers and the public accurately and without alarm — including retracting a warning when better data clears an object, as happened with Apophis. Clear communication is itself part of planetary defence.","sources":["nasa"]},{"id":"defense_stage:decision-and-planning","type":"defense_stage","name":"Decision & Mission Planning","domain":"science","entryPath":"/planetary-defense/decision-and-planning","description":"If an object were found on a collision course with enough warning, agencies and governments would decide on a response — and plan the reconnaissance and deflection mission it would require. NEO Surveyor is being built to give that warning decades ahead.","sources":["nasa"]},{"id":"defense_stage:deflection","type":"defense_stage","name":"Deflection","domain":"science","entryPath":"/planetary-defense/deflection","description":"The last stage — actually changing an asteroid's orbit so it misses the Earth. DART showed a kinetic impactor works; a gravity tractor, ion beam, or, as a last resort, a nuclear device are other options, chosen by how much warning time is available.","sources":["nasa"]},{"id":"risk_scale:torino-scale","type":"risk_scale","name":"The Torino Scale","domain":"science","entryPath":"/planetary-defense/torino-scale","description":"A 0–10 scale, like a hazard traffic light, for communicating the risk of a near-Earth object to the public — combining impact probability and energy into a single colour-coded number. Apophis briefly reached level 4, the highest ever, before further observations returned it to zero.","sources":["nasa"]},{"id":"risk_scale:palermo-scale","type":"risk_scale","name":"The Palermo Scale","domain":"science","entryPath":"/planetary-defense/palermo-scale","description":"A more technical, logarithmic scale used by specialists to rank impact hazards against the background risk of a random impact of the same size over the same time. Values below zero mean a threat less than the everyday background; above zero warrants attention.","sources":["nasa"]},{"id":"deflection_method:kinetic-impactor","type":"deflection_method","name":"Kinetic Impactor","domain":"science","entryPath":"/planetary-defense/kinetic-impactor","description":"Crashing a spacecraft into an asteroid at high speed to nudge its orbit — and getting an extra push from the plume of debris thrown off. NASA's DART did exactly this to the moonlet Dimorphos in 2022, measurably shortening its orbit; ESA's Hera is on its way to study the result up close, arriving in late 2026.","sources":["nasa"]},{"id":"deflection_method:gravity-tractor","type":"deflection_method","name":"Gravity Tractor","domain":"science","entryPath":"/planetary-defense/gravity-tractor","description":"A spacecraft that hovers near an asteroid for years, its own tiny gravity slowly towing the asteroid onto a new path. Very slow, but precise and controllable — best used with decades of warning, and often after a kinetic impact to fine-tune the result.","sources":["nasa"]},{"id":"deflection_method:ion-beam-deflection","type":"deflection_method","name":"Ion-Beam Deflection","domain":"science","entryPath":"/planetary-defense/ion-beam-deflection","description":"A spacecraft that points a stream of ions at an asteroid, the gentle continuous thrust pushing it aside over a long time — a slow, controllable method related to the gravity tractor, still at the concept stage.","aliases":["Ion beam shepherd"],"sources":["nasa"]},{"id":"deflection_method:nuclear-deflection","type":"deflection_method","name":"Nuclear Deflection","domain":"science","entryPath":"/planetary-defense/nuclear-deflection","description":"Detonating a nuclear device near an asteroid — not to blow it apart, but to vaporise a layer of its surface, the escaping material shoving it onto a new course. Studied only as a last resort for the largest objects or the shortest warning times; it has never been tested and remains theoretical.","sources":["nasa"]},{"id":"data_archive:mast","type":"data_archive","name":"MAST","domain":"science","entryPath":"/data-archives/mast","description":"NASA's archive for the data of its optical, ultraviolet, and near-infrared space telescopes — Hubble, JWST, TESS, Kepler, and more — operated by the Space Telescope Science Institute. One of the most-used archives in astronomy.","aliases":["Mikulski Archive for Space Telescopes"],"sources":["nasa"]},{"id":"data_archive:esa-science-archives","type":"data_archive","name":"ESA Science Archives","domain":"science","entryPath":"/data-archives/esa-science-archives","description":"ESA's science-data archives, hosted at the European Space Astronomy Centre, holding the observations of Europe's astronomy and planetary missions — from Gaia and XMM-Newton to Mars Express and Euclid.","sources":["esa"]},{"id":"data_archive:irsa","type":"data_archive","name":"IRSA","domain":"science","entryPath":"/data-archives/irsa","description":"NASA's archive for infrared and submillimetre astronomy — the data of Spitzer, WISE, 2MASS, and Herschel among others — operated by IPAC at Caltech.","aliases":["NASA/IPAC Infrared Science Archive"],"sources":["nasa"]},{"id":"data_archive:heasarc","type":"data_archive","name":"HEASARC","domain":"science","entryPath":"/data-archives/heasarc","description":"NASA's archive for high-energy astrophysics — the X-ray and gamma-ray data of missions like Chandra, Swift, and Fermi — a central resource for the study of the most energetic objects in the universe.","aliases":["High Energy Astrophysics Science Archive Research Center"],"sources":["nasa"]},{"id":"data_archive:ned","type":"data_archive","name":"NED","domain":"science","entryPath":"/data-archives/ned","description":"A database that gathers everything known about objects beyond the Milky Way — positions, redshifts, images, and the literature — cross-linking millions of galaxies and quasars across all the surveys that have observed them.","aliases":["NASA/IPAC Extragalactic Database"],"sources":["nasa"]},{"id":"data_archive:cds","type":"data_archive","name":"CDS","domain":"science","entryPath":"/data-archives/cds","description":"The Strasbourg astronomical Data Centre, a cornerstone of open astronomy that operates the SIMBAD and VizieR services and helped build the Virtual Observatory, tying the world's catalogues and object databases together.","aliases":["Centre de Données astronomiques de Strasbourg"],"sources":["eso"]},{"id":"data_archive:simbad","type":"data_archive","name":"SIMBAD","domain":"science","entryPath":"/data-archives/simbad","description":"A database of astronomical objects beyond the Solar System, collecting the names, identifiers, measurements, and references for millions of stars and galaxies so that any object can be looked up and cross-identified across the literature.","sources":["eso"]},{"id":"data_archive:vizier","type":"data_archive","name":"VizieR","domain":"science","entryPath":"/data-archives/vizier","description":"The most complete library of published astronomical catalogues, letting anyone query tens of thousands of catalogues and data tables in a uniform way — the reference source for catalogue data.","sources":["eso"]},{"id":"data_archive:eso-archive","type":"data_archive","name":"ESO Science Archive","domain":"science","entryPath":"/data-archives/eso-archive","description":"The archive of the European Southern Observatory, holding the data of its ground-based telescopes in Chile — the Very Large Telescope and its partners — for reuse by astronomers worldwide.","sources":["eso"]},{"id":"data_archive:alma-archive","type":"data_archive","name":"ALMA Science Archive","domain":"science","entryPath":"/data-archives/alma-archive","description":"The archive of the Atacama Large Millimeter/submillimeter Array, the great international millimetre-wave observatory, preserving its observations of cold gas, dust, and the discs where planets form.","sources":["eso"]},{"id":"data_standard:fits","type":"data_standard","name":"FITS","domain":"science","entryPath":"/data-archives/fits","description":"The universal file format of astronomy — a self-describing container for images, tables, and spectra with a human-readable header of metadata. In use since the 1980s and still the standard way astronomical data is stored and shared.","aliases":["Flexible Image Transport System"],"sources":["nasa"]},{"id":"data_standard:votable","type":"data_standard","name":"VOTable","domain":"science","entryPath":"/data-archives/votable","description":"The Virtual Observatory's XML standard for exchanging tabular data — catalogues and query results — between archives, tools, and services, so tables flow between systems without custom parsing.","sources":["nasa"]},{"id":"data_standard:asdf","type":"data_standard","name":"ASDF","domain":"science","entryPath":"/data-archives/asdf","description":"A modern, human-readable data format developed by the astronomy community as a successor to FITS for complex data — used by the James Webb Space Telescope for its calibration and world-coordinate metadata and adopted as the primary data format of the Roman mission.","aliases":["Advanced Scientific Data Format"],"sources":["nasa"]},{"id":"vo_framework:the-virtual-observatory","type":"vo_framework","name":"The Virtual Observatory","domain":"science","entryPath":"/data-archives/the-virtual-observatory","description":"The framework of standards, coordinated by the International Virtual Observatory Alliance, that lets the world's archives be searched and combined as if they were one — so an astronomer can query every telescope's data at once. TAP, Cone Search, VOEvent, and VOTable are among its standards.","aliases":["VO"],"sources":["nasa"]},{"id":"vo_protocol:table-access-protocol","type":"vo_protocol","name":"Table Access Protocol","domain":"science","entryPath":"/data-archives/table-access-protocol","description":"A Virtual Observatory protocol for running database queries against an archive's catalogues over the web, returning the results as VOTables — the standard way to ask an archive a precise question about its tables.","aliases":["TAP"],"sources":["nasa"]},{"id":"vo_protocol:cone-search","type":"vo_protocol","name":"Cone Search","domain":"science","entryPath":"/data-archives/cone-search","description":"The simplest Virtual Observatory query — 'give me every object within this radius of this position' — a standard that any catalogue service can answer, used constantly to find what is known around a point on the sky.","sources":["nasa"]},{"id":"vo_protocol:simple-image-access","type":"vo_protocol","name":"Simple Image Access","domain":"science","entryPath":"/data-archives/simple-image-access","description":"A Virtual Observatory protocol for finding and retrieving images of a region of sky from an archive, regardless of which telescope took them — the image counterpart of the cone search.","aliases":["SIA"],"sources":["nasa"]},{"id":"vo_protocol:simple-spectral-access","type":"vo_protocol","name":"Simple Spectral Access","domain":"science","entryPath":"/data-archives/simple-spectral-access","description":"A Virtual Observatory protocol for finding and retrieving spectra of a target from an archive, bringing the spectroscopy of many instruments into a single uniform search.","aliases":["SSA"],"sources":["nasa"]},{"id":"open_science_practice:data-pipelines-and-calibration","type":"open_science_practice","name":"Data Pipelines & Calibration","domain":"science","entryPath":"/data-archives/data-pipelines-and-calibration","description":"The automated processing that turns raw telescope readouts into calibrated, science-ready data — removing instrument signatures, correcting for the atmosphere or detector, and attaching the metadata and error estimates that make the data usable by anyone.","sources":["nasa"]},{"id":"open_science_practice:cross-matching","type":"open_science_practice","name":"Cross-Matching","domain":"science","entryPath":"/data-archives/cross-matching","description":"Identifying the same object across different catalogues and wavelengths — matching a source in an infrared survey to its optical and X-ray counterparts — so that all that is known about an object can be brought together despite different names and positions.","sources":["nasa"]},{"id":"open_science_practice:the-ads-literature-service","type":"open_science_practice","name":"The ADS Literature Service","domain":"science","entryPath":"/data-archives/the-ads-literature-service","description":"NASA's Astrophysics Data System, the digital library of astronomy — indexing essentially the entire research literature and linking every paper to the data, catalogues, and objects it uses, so the literature and the data are one connected web.","aliases":["Astrophysics Data System","ADS"],"sources":["nasa"]},{"id":"open_science_practice:persistent-identifiers","type":"open_science_practice","name":"Persistent Identifiers","domain":"science","entryPath":"/data-archives/persistent-identifiers","description":"The stable, unique names that make science findable and creditable — DOIs for datasets and papers, ORCID iDs for researchers, and bibcodes for the literature — so a result can be cited, retrieved, and attributed unambiguously years later.","aliases":["DOI","ORCID","bibcodes"],"sources":["nasa"]},{"id":"open_science_practice:reproducibility-and-fair","type":"open_science_practice","name":"Reproducibility & FAIR Data","domain":"science","entryPath":"/data-archives/reproducibility-and-fair","description":"The principles that make science trustworthy and reusable — data that is Findable, Accessible, Interoperable, and Reusable (FAIR), open archives, documented pipelines, and citable datasets — so that a result can be checked and built upon by anyone.","sources":["nasa"]},{"id":"telescope:giant-magellan-telescope","type":"telescope","name":"Giant Magellan Telescope","domain":"science","entryPath":"/observatory-frontier/giant-magellan-telescope","description":"A next-generation optical and near-infrared telescope under construction at Las Campanas Observatory in Chile, using seven 8.4-metre mirror segments to form a single light-collecting surface with a resolving power far beyond today's largest telescopes. One of the extremely large telescopes of the coming decade, alongside the ELT and TMT.","aliases":["GMT"],"sources":["noirlab"]},{"id":"telescope:next-generation-very-large-array","type":"telescope","name":"Next Generation Very Large Array","domain":"science","entryPath":"/observatory-frontier/next-generation-very-large-array","description":"A proposed radio interferometer, designed as the successor to the Very Large Array and a complement to ALMA, that would observe the centimetre-to-millimetre sky with far greater sensitivity and resolution — imaging planet-forming discs, molecular gas, and the distant universe. Led by the U.S. National Radio Astronomy Observatory.","aliases":["ngVLA"],"sources":["noirlab"]},{"id":"observatory:cherenkov-telescope-array","type":"observatory","name":"Cherenkov Telescope Array","domain":"science","entryPath":"/observatory-frontier/cherenkov-telescope-array","description":"The next-generation ground-based observatory for very-high-energy gamma rays, an array of imaging atmospheric Cherenkov telescopes being built across two sites — one in the northern hemisphere on La Palma and one in the southern hemisphere in Chile — to catch the faint blue flashes that gamma rays make in the atmosphere. The largest such observatory ever built.","aliases":["CTA","CTAO"],"sources":["eso"]},{"id":"instrument_technique:laser-guide-star","type":"instrument_technique","name":"Laser Guide Star","domain":"science","entryPath":"/observatory-frontier/laser-guide-star","description":"An artificial star created by shining a laser into the upper atmosphere, exciting sodium atoms ~90 km up to glow. It gives adaptive optics a bright reference point anywhere on the sky — not just near a real bright star — so the shape of the atmosphere's blur can be measured and corrected.","sources":["eso"]},{"id":"instrument_technique:wavefront-sensor","type":"instrument_technique","name":"Wavefront Sensor","domain":"science","entryPath":"/observatory-frontier/wavefront-sensor","description":"The eye of an adaptive-optics system — it measures, hundreds or thousands of times a second, exactly how the atmosphere has distorted the incoming light, so a correction can be computed and applied. Common designs are the Shack–Hartmann and pyramid sensors.","sources":["eso"]},{"id":"instrument_technique:deformable-mirror","type":"instrument_technique","name":"Deformable Mirror","domain":"science","entryPath":"/observatory-frontier/deformable-mirror","description":"A thin mirror whose surface is reshaped hundreds or thousands of times a second by an array of actuators, cancelling the distortion the atmosphere imposes on starlight in real time. The active heart of adaptive optics — the ELT's M4 is one of the largest ever built.","sources":["eso"]},{"id":"instrument_technique:echelle-spectrograph","type":"instrument_technique","name":"Echelle Spectrograph","domain":"science","entryPath":"/observatory-frontier/echelle-spectrograph","description":"A high-resolution spectrograph that uses a coarse, steeply-ruled grating (an échelle) to spread light into many overlapping orders, then a second disperser to separate them — packing very high spectral resolution onto a single detector. The workhorse of precision radial-velocity and stellar-abundance work; HIRES is a classic example.","sources":["eso"]},{"id":"instrument_technique:integral-field-spectrograph","type":"instrument_technique","name":"Integral-Field Spectrograph","domain":"science","entryPath":"/observatory-frontier/integral-field-spectrograph","description":"A spectrograph that records a full spectrum at every point in a two-dimensional field of view at once, producing a 'data cube' of the sky — an image where every pixel is a spectrum. It maps how motion and composition vary across a galaxy or nebula in a single exposure; MUSE on the VLT is a leading example.","aliases":["IFS","IFU"],"sources":["eso"]},{"id":"instrument_technique:coronagraph","type":"instrument_technique","name":"Coronagraph","domain":"science","entryPath":"/observatory-frontier/coronagraph","description":"An instrument that blocks the overwhelming light of a star so the far fainter objects beside it — a planet, a disc, the solar corona — can be seen. First built by Bernard Lyot to study the Sun, it is now central to directly imaging exoplanets; SPHERE on the VLT is a modern example.","sources":["eso"]},{"id":"instrument_technique:starshade","type":"instrument_technique","name":"Starshade","domain":"science","entryPath":"/observatory-frontier/starshade","description":"A concept for blocking a star's light not inside the instrument but far in front of the telescope — a large, precisely-shaped screen flown tens of thousands of kilometres away, casting a deep shadow so an orbiting planet stands clear. A proposed external alternative to the coronagraph for future exoplanet-imaging missions.","sources":["nasa"]},{"id":"detector_technology:ccd","type":"detector_technology","name":"CCD","domain":"science","entryPath":"/observatory-frontier/ccd","description":"The charge-coupled device, the detector that transformed optical astronomy — a silicon chip that converts light into electric charge with high efficiency and low noise, read out pixel by pixel. It replaced photographic plates and remains the standard optical detector; Rubin's camera is built from a mosaic of them.","aliases":["Charge-Coupled Device"],"sources":["noirlab"]},{"id":"detector_technology:cmos","type":"detector_technology","name":"CMOS Sensor","domain":"science","entryPath":"/observatory-frontier/cmos","description":"A detector in which each pixel has its own amplifier, allowing very fast, low-power readout. Increasingly used in astronomy for high-speed imaging and for techniques that need many frames per second, and ubiquitous in consumer cameras.","aliases":["Complementary Metal-Oxide-Semiconductor"],"sources":["noirlab"]},{"id":"detector_technology:mkid","type":"detector_technology","name":"MKID","domain":"science","entryPath":"/observatory-frontier/mkid","description":"A superconducting detector that records not just the arrival of a photon but its energy and precise time, with no read noise. Operating at temperatures near absolute zero, MKIDs are a frontier technology for the millimetre, submillimetre, and optical sky, and scale to large arrays.","aliases":["Microwave Kinetic Inductance Detector"],"sources":["noirlab"]},{"id":"detector_technology:bolometer","type":"detector_technology","name":"Bolometer","domain":"science","entryPath":"/observatory-frontier/bolometer","description":"A detector that measures light by the tiny rise in temperature it causes in an absorbing element — the standard way to detect the faint millimetre and submillimetre sky, including the cosmic microwave background. Cooled to a fraction of a degree above absolute zero; the South Pole Telescope's cameras use large bolometer arrays.","sources":["noirlab"]},{"id":"detector_technology:cryogenic-detector","type":"detector_technology","name":"Cryogenic Detector","domain":"science","entryPath":"/observatory-frontier/cryogenic-detector","description":"The broad family of detectors that must be cooled to cryogenic temperatures — sometimes thousandths of a degree above absolute zero — so that thermal noise does not swamp the faint astronomical signal. Bolometers and MKIDs are cryogenic detectors; the technique is essential across the infrared, millimetre, and X-ray.","sources":["noirlab"]},{"id":"interferometry_technique:radio-interferometry","type":"interferometry_technique","name":"Radio Interferometry","domain":"science","entryPath":"/observatory-frontier/radio-interferometry","description":"Linking many radio dishes so that they act together as one telescope as large as their separation, giving radio astronomy its sharpest images. Arrays like the VLA and ALMA correlate the signals from every pair of antennas to reconstruct the sky.","sources":["eso"]},{"id":"interferometry_technique:aperture-synthesis","type":"interferometry_technique","name":"Aperture Synthesis","domain":"science","entryPath":"/observatory-frontier/aperture-synthesis","description":"The technique, developed by Martin Ryle, of building up an image from an interferometer by combining measurements taken as the Earth's rotation carries the antennas to different orientations — synthesising the resolution of a single huge aperture from many small ones. The basis of modern radio imaging.","sources":["eso"]},{"id":"interferometry_technique:very-long-baseline-interferometry","type":"interferometry_technique","name":"Very Long Baseline Interferometry","domain":"science","entryPath":"/observatory-frontier/very-long-baseline-interferometry","description":"Radio interferometry stretched across continents — antennas thousands of kilometres apart record the sky independently with precise atomic clocks, and the data are combined later. It achieves the finest angular resolution in all of astronomy; a global VLBI network imaged the shadow of a black hole.","aliases":["VLBI"],"sources":["eso"]},{"id":"interferometry_technique:optical-interferometry","type":"interferometry_technique","name":"Optical Interferometry","domain":"science","entryPath":"/observatory-frontier/optical-interferometry","description":"Combining the light of separate optical or infrared telescopes to reach angular resolutions no single telescope could — far harder than in the radio because the light waves must be kept in step to a fraction of their wavelength. The VLT's four unit telescopes can be combined this way.","sources":["eso"]},{"id":"observing_technique:lucky-imaging","type":"observing_technique","name":"Lucky Imaging","domain":"science","entryPath":"/observatory-frontier/lucky-imaging","description":"Taking a rapid burst of very short exposures and keeping only the few sharpest — the lucky moments when the atmosphere happens to be still — then combining them. A simple way to reach near-diffraction-limited resolution on modest telescopes without full adaptive optics.","sources":["noirlab"]},{"id":"observing_technique:speckle-imaging","type":"observing_technique","name":"Speckle Imaging","domain":"science","entryPath":"/observatory-frontier/speckle-imaging","description":"Recovering fine detail from the fleeting speckle pattern that the atmosphere breaks a star's image into, by taking many very short exposures and reconstructing the true image statistically. It resolves close double stars and fine structure below the atmospheric blur.","sources":["noirlab"]},{"id":"observing_technique:image-stacking","type":"observing_technique","name":"Image Stacking","domain":"science","entryPath":"/observatory-frontier/image-stacking","description":"Combining many exposures of the same field to build up signal and average down noise, reaching far fainter objects than any single frame — the foundation of deep imaging, from amateur astrophotography to the deepest survey fields.","sources":["noirlab"]},{"id":"observing_technique:fringe-tracking","type":"observing_technique","name":"Fringe Tracking","domain":"science","entryPath":"/observatory-frontier/fringe-tracking","description":"The real-time control that keeps the interference fringes of an optical interferometer stable against the atmosphere's constantly-changing path lengths, so faint targets can be observed for longer. Without it, the fringes wash out in a fraction of a second.","sources":["eso"]},{"id":"distance_indicator:rr-lyrae","type":"distance_indicator","name":"RR Lyrae Stars","domain":"science","entryPath":"/distance-ladder/rr-lyrae","description":"Old, pulsating horizontal-branch stars with a well-defined luminosity, especially tight when measured in the infrared. Abundant in globular clusters and the haloes of galaxies, they are a standard candle for old stellar populations and, like the Cepheids, are calibrated directly by parallax.","sources":["nasa"]},{"id":"distance_indicator:tip-of-the-red-giant-branch","type":"distance_indicator","name":"Tip of the Red Giant Branch","domain":"science","entryPath":"/distance-ladder/tip-of-the-red-giant-branch","description":"The sharp, near-constant peak brightness that red giant stars reach just before the helium flash — a robust standard candle that can be measured in a galaxy's halo, away from crowding and dust. It provides an independent route to calibrating Type Ia supernovae, and its Hubble-constant value sits between the Cepheid and CMB results.","aliases":["TRGB"],"sources":["nasa"]},{"id":"distance_indicator:surface-brightness-fluctuations","type":"distance_indicator","name":"Surface Brightness Fluctuations","domain":"science","entryPath":"/distance-ladder/surface-brightness-fluctuations","description":"A distance method that uses the graininess of a galaxy's light: because a nearer galaxy resolves into fewer, brighter patches of unresolved stars per pixel, the amount of pixel-to-pixel fluctuation measures distance. Best suited to smooth elliptical galaxies and the bulges of spirals.","aliases":["SBF"],"sources":["nasa"]},{"id":"distance_indicator:tully-fisher-relation","type":"distance_indicator","name":"Tully–Fisher Relation","domain":"science","entryPath":"/distance-ladder/tully-fisher-relation","description":"An empirical relation for spiral galaxies between how fast they rotate and how luminous they are — the faster the rotation, the brighter the galaxy. Measuring the rotation (from the width of the 21-cm line) then gives the luminosity, and comparing with the apparent brightness gives the distance.","sources":["nasa"]},{"id":"distance_indicator:faber-jackson-relation","type":"distance_indicator","name":"Faber–Jackson Relation","domain":"science","entryPath":"/distance-ladder/faber-jackson-relation","description":"The elliptical-galaxy counterpart of the Tully–Fisher relation: a link between a galaxy's luminosity and the velocity dispersion of its stars. It is one projection of the tighter Fundamental Plane of elliptical galaxies, which is used as a distance indicator.","sources":["nasa"]},{"id":"distance_indicator:water-megamaser-distances","type":"distance_indicator","name":"Water Megamaser Distances","domain":"science","entryPath":"/distance-ladder/water-megamaser-distances","description":"A direct, geometric distance measured from water masers orbiting in the accretion disc around a galaxy's central black hole. By tracking their motion and acceleration, the physical size of the disc is found and compared with its angular size — a one-step distance that anchors the ladder without relying on standard candles.","sources":["nasa"]},{"id":"distance_indicator:standard-sirens","type":"distance_indicator","name":"Standard Sirens","domain":"science","entryPath":"/distance-ladder/standard-sirens","description":"Gravitational-wave sources whose distance can be read directly from the shape of the waveform, with no calibration ladder at all — the gravitational analogue of a standard candle. A merging neutron-star pair with an electromagnetic counterpart yielded the first standard-siren measurement of the Hubble constant.","sources":["ligo"]},{"id":"cosmological_parameter:matter-density","type":"cosmological_parameter","name":"Matter Density (Ωm)","domain":"science","entryPath":"/distance-ladder/matter-density","description":"The fraction of the universe's total energy density that is in matter — dark matter plus ordinary baryonic matter — today. Together with the dark-energy density it sets the geometry and the fate of the universe; it is measured most precisely from the cosmic microwave background.","aliases":["Omega matter"],"sources":["planck"]},{"id":"cosmological_parameter:dark-energy-density","type":"cosmological_parameter","name":"Dark Energy Density (ΩΛ)","domain":"science","entryPath":"/distance-ladder/dark-energy-density","description":"The fraction of the universe's total energy density carried by dark energy — the component driving the accelerating expansion. In the standard model it is the cosmological constant Λ, and it makes up the majority of the present-day energy budget.","aliases":["Omega Lambda"],"sources":["planck"]},{"id":"cosmological_parameter:sigma-8","type":"cosmological_parameter","name":"Amplitude of Fluctuations (σ8)","domain":"science","entryPath":"/distance-ladder/sigma-8","description":"A measure of how clumpy the universe is — the amplitude of matter-density fluctuations averaged over spheres of 8 megaparsecs. It links the smooth early universe to today's web of galaxies, and a mild disagreement between its early-universe and weak-lensing determinations — usually quantified through the related combination S8 — is known as the S8 tension.","aliases":["sigma eight"],"sources":["planck"]},{"id":"cosmological_parameter:scalar-spectral-index","type":"cosmological_parameter","name":"Scalar Spectral Index (ns)","domain":"science","entryPath":"/distance-ladder/scalar-spectral-index","description":"The 'tilt' of the spectrum of primordial density fluctuations laid down by inflation — whether fluctuations have slightly more or less power on large scales than on small. A value just below one is a key prediction of, and constraint on, inflationary models, and is measured from the CMB.","aliases":["spectral tilt"],"sources":["planck"]},{"id":"observational_program:sh0es","type":"observational_program","name":"SH0ES","domain":"science","entryPath":"/distance-ladder/sh0es","description":"The programme that measures the Hubble constant from the local distance ladder — anchoring Cepheids with parallax, using them to calibrate Type Ia supernovae, and reading the expansion rate from supernovae in the smooth Hubble flow. Its value comes out consistently higher than the one inferred from the early universe, and that gap is the Hubble tension.","aliases":["Supernovae, H0, for the Equation of State"],"sources":["stsci"]},{"id":"cosmology_concept:early-dark-energy","type":"cosmology_concept","name":"Early Dark Energy","domain":"science","entryPath":"/distance-ladder/early-dark-energy","description":"A proposed but unconfirmed resolution of the Hubble tension in which a small, transient dark-energy-like component acts in the early universe around the time of recombination, shrinking the sound horizon and so raising the Hubble constant inferred from the CMB toward the local value. It is one of several competing ideas — alongside extra relativistic species and modified gravity — and none is yet established.","aliases":["EDE"],"sources":["nasa"]},{"id":"space_weather_phenomenon:solar-cycle","type":"space_weather_phenomenon","name":"The Solar Cycle","domain":"science","entryPath":"/heliophysics/solar-cycle","description":"The roughly eleven-year rise and fall of the Sun's activity, traced by the number of sunspots from solar minimum to solar maximum and back. Its underlying magnetic cycle takes about twenty-two years, as the Sun's polarity flips and returns. Activity — flares, CMEs, and storms — peaks near solar maximum.","sources":["swpc"]},{"id":"space_weather_phenomenon:sunspot","type":"space_weather_phenomenon","name":"Sunspots","domain":"science","entryPath":"/heliophysics/sunspot","description":"Dark, cooler patches on the Sun's visible surface where intense magnetic fields suppress the flow of heat from below. Their number rises and falls with the solar cycle, and they mark the magnetically active regions from which flares and CMEs erupt.","sources":["swpc"]},{"id":"space_weather_phenomenon:active-region","type":"space_weather_phenomenon","name":"Active Regions","domain":"science","entryPath":"/heliophysics/active-region","description":"Areas of strong, complex magnetic field on the Sun, usually marked by sunspots, where magnetic energy builds up and is released. Active regions are the launch sites of the largest solar flares and coronal mass ejections, and are watched closely for space-weather forecasting.","sources":["swpc"]},{"id":"space_weather_phenomenon:coronal-hole","type":"space_weather_phenomenon","name":"Coronal Holes","domain":"science","entryPath":"/heliophysics/coronal-hole","description":"Regions of the Sun's corona where the magnetic field opens out into space rather than looping back, appearing dark in X-ray and ultraviolet images. They are the source of the fast solar wind, and the high-speed streams they send out drive recurring geomagnetic activity.","sources":["swpc"]},{"id":"space_weather_phenomenon:ionosphere","type":"space_weather_phenomenon","name":"The Ionosphere","domain":"science","entryPath":"/heliophysics/ionosphere","description":"The ionised layer of Earth's upper atmosphere, created by solar ultraviolet and X-ray radiation. It reflects and refracts radio waves — enabling long-distance HF communication — but solar flares and geomagnetic storms disturb it, causing radio blackouts and errors in satellite navigation.","sources":["swpc"]},{"id":"space_weather_impact:satellites","type":"space_weather_impact","name":"Satellites","domain":"science","entryPath":"/heliophysics/satellites","description":"Spacecraft are exposed to the full force of space weather: energetic particles charge their surfaces and interiors and flip bits in their electronics, while geomagnetic storms heat and expand the upper atmosphere, increasing drag and pulling low-orbit satellites down faster.","sources":["swpc"]},{"id":"space_weather_impact:gps-and-navigation","type":"space_weather_impact","name":"GPS & Navigation","domain":"science","entryPath":"/heliophysics/gps-and-navigation","description":"Satellite navigation signals pass through the ionosphere, and when solar flares and geomagnetic storms disturb it the signals are delayed and scattered, degrading positioning accuracy — a serious concern for aviation, surveying, and precision agriculture.","aliases":["GNSS"],"sources":["swpc"]},{"id":"space_weather_impact:aviation","type":"space_weather_impact","name":"Aviation","domain":"science","entryPath":"/heliophysics/aviation","description":"Aircraft on polar routes can lose high-frequency radio contact during solar radio blackouts and are exposed to raised radiation levels during solar particle events, sometimes forcing flights to divert to lower latitudes.","sources":["swpc"]},{"id":"space_weather_impact:human-spaceflight","type":"space_weather_impact","name":"Human Spaceflight","domain":"science","entryPath":"/heliophysics/human-spaceflight","description":"Radiation is one of the central hazards of human spaceflight. A large solar particle event can deliver a dangerous dose to astronauts, especially beyond the protection of Earth's magnetic field, and crews may need to shelter in more shielded parts of a spacecraft.","sources":["swpc"]},{"id":"space_weather_impact:power-grids","type":"space_weather_impact","name":"Power Grids","domain":"science","entryPath":"/heliophysics/power-grids","description":"Geomagnetic storms drive currents in the ground that flow into long transmission lines — geomagnetically induced currents — which can saturate and damage transformers and, in severe cases, cause regional blackouts. The 1989 Québec blackout is the classic example.","sources":["swpc"]},{"id":"space_weather_impact:radio-communications","type":"space_weather_impact","name":"Radio Communications","domain":"science","entryPath":"/heliophysics/radio-communications","description":"The X-rays from a solar flare suddenly increase the ionisation of the day-side ionosphere, absorbing high-frequency radio waves and causing radio blackouts across the sunlit Earth — the effect measured by NOAA's R-scale.","sources":["swpc"]},{"id":"organization:esa-space-weather-service-network","type":"organization","name":"ESA Space Weather Service Network","domain":"science","entryPath":"/heliophysics/esa-space-weather-service-network","description":"The operational space-weather arm of the European Space Agency's Space Safety programme, delivering forecasts, warnings, and data products — on solar activity, the near-Earth environment, and the ionosphere — to European operators of satellites, power grids, aviation, and navigation. The European counterpart to NOAA's Space Weather Prediction Center.","aliases":["ESA SSA Space Weather"],"sources":["esa"]},{"id":"ml_method:classification","type":"ml_method","name":"Classification","domain":"science","entryPath":"/astro-ml/classification","description":"Assigning objects to discrete categories from their measured features — star or galaxy, supernova type, real detection or artefact. It is the workhorse of survey astronomy, sorting the millions of objects a modern survey finds into kinds a human never could review one by one.","sources":["nasa"]},{"id":"ml_method:regression","type":"ml_method","name":"Regression","domain":"science","entryPath":"/astro-ml/regression","description":"Predicting a continuous quantity from an object's features — a galaxy's redshift, a star's temperature or age — rather than a discrete label. 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Good representations make every downstream task, from classification to search, easier and more accurate.","sources":["nasa"]},{"id":"ml_method:self-supervised-learning","type":"ml_method","name":"Self-Supervised Learning","domain":"science","entryPath":"/astro-ml/self-supervised-learning","description":"Training a model on unlabelled data by inventing a task it can grade itself on — predicting a hidden part of an image, or telling two views of the same object apart. It is powerful in astronomy, where raw data is abundant but expert labels are scarce.","sources":["nasa"]},{"id":"ml_method:foundation-models","type":"ml_method","name":"Foundation Models","domain":"science","entryPath":"/astro-ml/foundation-models","description":"Large models pre-trained on broad data that can then be adapted to many specific tasks with little extra training. 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One of the earliest large-scale meetings of astronomy and machine learning, building on the labels gathered by citizen-science projects like Galaxy Zoo to train automatic classifiers for surveys too large to inspect by eye.","sources":["nasa"]},{"id":"ml_application:supernova-classification","type":"ml_application","name":"Supernova Classification","domain":"science","entryPath":"/astro-ml/supernova-classification","description":"Deciding what kind of exploding star a transient is — often from its light curve alone, before or without a spectrum. Fast, automatic classification is essential when a survey finds thousands of supernovae a night and only a few can be followed up in detail.","sources":["nasa"]},{"id":"ml_application:photometric-redshifts","type":"ml_application","name":"Photometric Redshifts","domain":"science","entryPath":"/astro-ml/photometric-redshifts","description":"Estimating how far away a galaxy is from its brightness in a few broad colour bands, without taking a full spectrum. 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Machine learning now helps sift the enormous light-curve archives of transit surveys for the faintest candidates.","sources":["nasa"]},{"id":"ml_application:strong-lens-finding","type":"ml_application","name":"Strong Lens Finding","domain":"science","entryPath":"/astro-ml/strong-lens-finding","description":"Searching survey images for the rare, distinctive arcs and rings of strong gravitational lensing — where a foreground mass bends the light of a background galaxy. The lenses are rare enough, and the images numerous enough, that automated finders are the only way to build large samples.","sources":["nasa"]},{"id":"ml_application:source-extraction","type":"ml_application","name":"Source Extraction","domain":"science","entryPath":"/astro-ml/source-extraction","description":"Finding and measuring the individual stars and galaxies in an astronomical image, and separating real sources from noise and artefacts — the first step of nearly every imaging pipeline. Machine-learning methods increasingly complement the classical algorithms, especially in crowded or blended fields.","sources":["nasa"]},{"id":"ml_application:real-time-alert-classification","type":"ml_application","name":"Real-Time Alert Classification","domain":"science","entryPath":"/astro-ml/real-time-alert-classification","description":"Classifying the flood of alerts that a survey like Rubin issues — millions each night when something on the sky changes — quickly enough to catch the fleeting events worth following up. It is the problem the community alert brokers exist to solve.","sources":["nasa"]},{"id":"ml_workflow:training-datasets","type":"ml_workflow","name":"Training Datasets","domain":"science","entryPath":"/astro-ml/training-datasets","description":"The labelled examples a model learns from. 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Well-chosen features can make a simple model succeed; increasingly, representation learning discovers them automatically.","sources":["nasa"]},{"id":"ml_workflow:model-evaluation","type":"ml_workflow","name":"Model Evaluation","domain":"science","entryPath":"/astro-ml/model-evaluation","description":"Measuring honestly how well a model performs — its accuracy, completeness, and purity, whether its confidences are calibrated, and how it behaves on data unlike its training set. Careful evaluation is what separates a genuinely useful model from one that has merely memorised its examples.","sources":["nasa"]},{"id":"alert_system:alerce","type":"alert_system","name":"ALeRCE","domain":"science","entryPath":"/astro-ml/alerce","description":"A community alert broker, led from Chile, that ingests a survey's alert stream and classifies its transients and variable objects in real time with machine learning — first for the Zwicky Transient Facility and, in the era ahead, for Rubin.","aliases":["Automatic Learning for the Rapid Classification of Events"],"sources":["noirlab"]},{"id":"alert_system:antares-broker","type":"alert_system","name":"ANTARES","domain":"science","entryPath":"/astro-ml/antares-broker","description":"NOIRLab's alert broker for time-domain astronomy, which filters and annotates survey alert streams to surface the events most worth following up. One of the community brokers selected to process the full Rubin alert stream.","aliases":["Arizona-NOIRLab Temporal Analysis and Response to Events System"],"sources":["noirlab"]},{"id":"alert_system:fink","type":"alert_system","name":"Fink","domain":"science","entryPath":"/astro-ml/fink","description":"A community alert broker built to process the alert streams of ZTF and Rubin, adding machine-learning classifications and value-added information so that astronomers can select the transients and variables they care about from millions of nightly alerts.","sources":["noirlab"]},{"id":"alert_system:lasair","type":"alert_system","name":"Lasair","domain":"science","entryPath":"/astro-ml/lasair","description":"A UK-led community alert broker for the ZTF and Rubin alert streams, letting astronomers query, filter, and cross-match the live stream of changing objects on the sky.","sources":["noirlab"]},{"id":"citizen_science_project:zooniverse","type":"citizen_science_project","name":"Zooniverse","domain":"science","entryPath":"/citizen-astronomy/zooniverse","description":"The largest platform for people-powered research, where hundreds of thousands of volunteers help classify and analyse data across astronomy and many other sciences. It grew out of Galaxy Zoo and now hosts dozens of projects that turn human pattern-recognition into published results.","sources":["nasa"]},{"id":"citizen_science_project:galaxy-zoo","type":"citizen_science_project","name":"Galaxy Zoo","domain":"science","entryPath":"/citizen-astronomy/galaxy-zoo","description":"The project that asked the public to sort galaxies by shape from survey images — and found volunteers could do it as well as experts, at enormous scale. Its classifications became a landmark dataset and the training labels for the machine-learning classifiers that followed.","sources":["nasa"]},{"id":"citizen_science_project:planet-hunters","type":"citizen_science_project","name":"Planet Hunters","domain":"science","entryPath":"/citizen-astronomy/planet-hunters","description":"A project inviting the public to search stellar light curves for the tiny dips of a transiting planet — finding candidates, including unusual ones, that automated pipelines had missed. A demonstration that human eyes still catch things algorithms overlook.","sources":["nasa"]},{"id":"citizen_science_project:globe-at-night","type":"citizen_science_project","name":"Globe at Night","domain":"science","entryPath":"/citizen-astronomy/globe-at-night","description":"A worldwide campaign to measure light pollution by having people compare the faintest stars they can see — often in Orion — against a set of star charts, and report what they see. The result is a global, year-on-year map of the brightening night sky.","sources":["nasa"]},{"id":"citizen_science_project:aurorasaurus","type":"citizen_science_project","name":"Aurorasaurus","domain":"science","entryPath":"/citizen-astronomy/aurorasaurus","description":"A project that crowdsources real-time reports and photographs of the aurora from the public, improving where and when auroral displays are forecast — turning sky-watchers into a distributed sensor network for space weather.","sources":["nasa"]},{"id":"citizen_science_project:stardust-at-home","type":"citizen_science_project","name":"Stardust@home","domain":"science","entryPath":"/citizen-astronomy/stardust-at-home","description":"A project in which volunteers scanned microscope images of the aerogel flown on NASA's Stardust mission, hunting for the microscopic tracks of interstellar dust grains — a needle-in-a-haystack search that distributed human attention could solve.","sources":["nasa"]},{"id":"amateur_activity:backyard-observing","type":"amateur_activity","name":"Backyard Observing","domain":"science","entryPath":"/citizen-astronomy/backyard-observing","description":"Watching the night sky from home with the naked eye, binoculars, or a small telescope — learning the constellations, following the Moon and planets, and hunting bright deep-sky objects. The foundation of the hobby, and where almost every astronomer begins.","sources":["nasa"]},{"id":"amateur_activity:variable-star-observing","type":"amateur_activity","name":"Variable-Star Observing","domain":"science","entryPath":"/citizen-astronomy/variable-star-observing","description":"Monitoring stars that change in brightness and reporting careful estimates over months and years. Coordinated by organisations like the AAVSO, amateur variable-star observers build long-term light curves that professionals rely on — one of the clearest cases of amateurs doing lasting science.","sources":["nasa"]},{"id":"amateur_activity:asteroid-observing","type":"amateur_activity","name":"Asteroid Observing","domain":"science","entryPath":"/citizen-astronomy/asteroid-observing","description":"Measuring the positions and brightness of asteroids, and timing the moments they pass in front of stars. From these occultation timings, amateurs reconstruct asteroid shapes and sizes to a precision that rivals spacecraft flybys.","sources":["nasa"]},{"id":"amateur_activity:comet-observing","type":"amateur_activity","name":"Comet Observing","domain":"science","entryPath":"/citizen-astronomy/comet-observing","description":"Following comets as they brighten, grow tails, and fade — estimating their brightness and sketching or photographing their changing structure. Amateurs have a long tradition of discovering comets, and their brightness estimates track how these unpredictable visitors evolve.","sources":["nasa"]},{"id":"amateur_activity:occultation-timing","type":"amateur_activity","name":"Occultation Timing","domain":"science","entryPath":"/citizen-astronomy/occultation-timing","description":"Precisely recording the instant a star winks out and reappears as the Moon or an asteroid passes in front of it. Combined across many observers, these timings reveal lunar-limb profiles and the shapes and sizes of asteroids — a niche where amateurs produce genuinely professional data.","sources":["nasa"]},{"id":"amateur_activity:meteor-observing","type":"amateur_activity","name":"Meteor Observing","domain":"science","entryPath":"/citizen-astronomy/meteor-observing","description":"Counting and recording meteors during a shower — their number, brightness, and paths — to measure the shower's strength and structure. Coordinated worldwide by the International Meteor Organization, it is a science anyone can do with nothing but their eyes and patience.","sources":["nasa"]},{"id":"observing_equipment:binoculars","type":"observing_equipment","name":"Binoculars","domain":"science","entryPath":"/citizen-astronomy/binoculars","description":"The most-recommended first instrument in astronomy — wide-field, portable, and forgiving. A modest pair shows the craters of the Moon, the moons of Jupiter, star clusters, and the brighter galaxies and nebulae, and teaches the sky better than any telescope rushed into too soon.","sources":["nasa"]},{"id":"observing_equipment:dobsonian-telescope","type":"observing_equipment","name":"Dobsonian Telescope","domain":"science","entryPath":"/citizen-astronomy/dobsonian-telescope","description":"A large reflecting telescope on a simple, stable, inexpensive alt-azimuth mount — the design that put big apertures within reach of ordinary observers. It offers more light-gathering power per unit cost than anything else, and is the classic instrument for deep-sky observing.","sources":["nasa"]},{"id":"observing_equipment:equatorial-mount","type":"observing_equipment","name":"Equatorial Mount","domain":"science","entryPath":"/citizen-astronomy/equatorial-mount","description":"A telescope mount tilted to align with Earth's rotation axis, so that a single, steady motion cancels the turning of the sky. It keeps an object centred as the Earth spins, which is what makes long-exposure astrophotography possible.","sources":["nasa"]},{"id":"observing_equipment:star-tracker","type":"observing_equipment","name":"Star Tracker","domain":"science","entryPath":"/citizen-astronomy/star-tracker","description":"A small, portable motorised mount that slowly turns a camera to follow the stars, so that long exposures capture faint detail without the stars trailing into streaks. It has made wide-field astrophotography of the Milky Way accessible to anyone with a camera.","sources":["nasa"]},{"id":"observing_equipment:camera","type":"observing_equipment","name":"Camera","domain":"science","entryPath":"/citizen-astronomy/camera","description":"From a standard camera to a cooled, dedicated astronomical one, the imaging heart of the hobby. Stacking many long exposures, an amateur camera reveals colour and faint structure in nebulae and galaxies far beyond what the eye can see at the eyepiece.","aliases":["astrophotography camera"],"sources":["nasa"]},{"id":"observing_equipment:astronomical-filter","type":"observing_equipment","name":"Astronomical Filter","domain":"science","entryPath":"/citizen-astronomy/astronomical-filter","description":"A filter that blocks unwanted light — the orange glow of light pollution, or all but a single emission line such as hydrogen-alpha — so that faint nebulae stand out against the background. 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It gives people a chance to look through a real research-grade telescope and meet the people who use them.","sources":["nasa"]},{"id":"outreach_activity:dark-sky-park","type":"outreach_activity","name":"Dark-Sky Park","domain":"science","entryPath":"/citizen-astronomy/dark-sky-park","description":"A place formally protected for the darkness of its night sky, kept free of light pollution and certified by DarkSky International. Dark-sky parks preserve the vanishing experience of a truly dark sky — and protect the wildlife and human health that artificial light disrupts.","sources":["nasa"]},{"id":"outreach_activity:astronomy-education","type":"outreach_activity","name":"Astronomy Education","domain":"science","entryPath":"/citizen-astronomy/astronomy-education","description":"Teaching and public engagement with astronomy — in classrooms, planetariums, science centres, and online — that turns a glance at the stars into understanding. Modern education draws directly on open data archives and survey imagery, letting anyone explore real observations.","sources":["nasa"]},{"id":"organization:aavso","type":"organization","name":"AAVSO","domain":"science","entryPath":"/citizen-astronomy/aavso","description":"The American Association of Variable Star Observers — for more than a century, the organisation that gathers variable-star observations from amateurs worldwide into a single database that professional astronomers draw on. 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Smaller than LIGO or Virgo, it works as a technology testbed — pioneering the squeezed-light and other techniques the larger detectors adopt — and observes as part of the international network.","sources":["ligo"]},{"id":"observatory:einstein-telescope","type":"observatory","name":"Einstein Telescope","domain":"science","entryPath":"/multi-messenger/einstein-telescope","description":"A proposed European third-generation gravitational-wave observatory, to be built underground in a triangle of ten-kilometre arms. Its far greater sensitivity would detect compact-binary mergers across most of the observable universe.","aliases":["ET"],"sources":["ligo"]},{"id":"observatory:cosmic-explorer","type":"observatory","name":"Cosmic Explorer","domain":"science","entryPath":"/multi-messenger/cosmic-explorer","description":"A proposed United States third-generation gravitational-wave observatory with arms up to forty kilometres long — a scaled-up successor to LIGO that, with the Einstein Telescope, would open the distant gravitational-wave universe.","sources":["ligo"]},{"id":"mission_concept:decigo","type":"mission_concept","name":"DECIGO","domain":"science","entryPath":"/multi-messenger/decigo","description":"A proposed Japanese space-based gravitational-wave observatory designed for the decihertz band, between the low frequencies LISA will observe and the high frequencies of the ground detectors — a range no other instrument covers.","aliases":["DECi-hertz Interferometer Gravitational wave Observatory"],"sources":["nasa"]},{"id":"mission_concept:taiji","type":"mission_concept","name":"Taiji","domain":"science","entryPath":"/multi-messenger/taiji","description":"A proposed Chinese space-based gravitational-wave mission, similar in concept to LISA, that would fly a triangle of spacecraft to detect low-frequency gravitational waves from massive black-hole binaries.","sources":["nasa"]},{"id":"mission_concept:tianqin","type":"mission_concept","name":"TianQin","domain":"science","entryPath":"/multi-messenger/tianqin","description":"A proposed Chinese space-based gravitational-wave detector of three spacecraft in high geocentric orbit, targeting low-frequency sources such as compact binaries in the Milky Way and merging massive black holes.","sources":["nasa"]},{"id":"gw_detection_method:laser-interferometry","type":"gw_detection_method","name":"Laser Interferometry","domain":"science","entryPath":"/multi-messenger/laser-interferometry","description":"The technique behind the ground-based detectors: a laser beam is split down two perpendicular kilometre-scale arms and recombined, and a passing gravitational wave stretches one arm and squeezes the other by a fraction of a proton's width, shifting the interference pattern. LIGO, Virgo, and KAGRA all work this way.","sources":["ligo"]},{"id":"gw_detection_method:space-interferometry","type":"gw_detection_method","name":"Space Interferometry","domain":"science","entryPath":"/multi-messenger/space-interferometry","description":"Laser interferometry carried out between spacecraft millions of kilometres apart, free of the ground noise that limits Earth-based detectors. It opens the low-frequency gravitational-wave band — the mergers of massive black holes and the whir of compact binaries — that the ground detectors cannot reach. LISA is the leading example.","sources":["nasa"]},{"id":"gw_detection_method:pulsar-timing-array","type":"gw_detection_method","name":"Pulsar Timing Array","domain":"science","entryPath":"/multi-messenger/pulsar-timing-array","description":"Using an array of millisecond pulsars — nature's most precise clocks — as a galaxy-sized gravitational-wave detector. A passing nanohertz gravitational wave subtly shifts the arrival times of the pulsars' pulses in a correlated way; timing arrays have found evidence for a background of such waves from supermassive black-hole binaries.","aliases":["PTA"],"sources":["nasa"]},{"id":"transient_class:binary-black-hole-merger","type":"transient_class","name":"Binary Black Hole Merger","domain":"science","entryPath":"/multi-messenger/binary-black-hole-merger","description":"The merger of two black holes spiralling together — the most common gravitational-wave source detected, and usually a purely gravitational event with no light. The first ever direct detection, in 2015, was of such a merger over a billion light-years away.","aliases":["BBH"],"sources":["ligo"]},{"id":"transient_class:binary-neutron-star-merger","type":"transient_class","name":"Binary Neutron Star Merger","domain":"science","entryPath":"/multi-messenger/binary-neutron-star-merger","description":"The merger of two neutron stars — a gravitational-wave source that also lights up across the electromagnetic spectrum, producing a short gamma-ray burst and a kilonova. The 2017 event GW170817 was seen in both gravitational waves and light, founding multi-messenger astronomy with gravitational waves.","aliases":["BNS"],"sources":["ligo"]},{"id":"transient_class:black-hole-neutron-star-merger","type":"transient_class","name":"Black Hole–Neutron Star Merger","domain":"science","entryPath":"/multi-messenger/black-hole-neutron-star-merger","description":"The merger of a black hole with a neutron star — the third class of compact-binary merger, first confidently detected in gravitational waves in early 2020. Whether it produces light depends on whether the black hole tears the neutron star apart before swallowing it.","aliases":["NSBH"],"sources":["ligo"]},{"id":"alert_system:lvk-alert-network","type":"alert_system","name":"LVK Public Alerts","domain":"science","entryPath":"/multi-messenger/lvk-alert-network","description":"The public alert system of the LIGO–Virgo–KAGRA collaboration, which issues automated notices — within seconds to minutes — whenever the detectors flag a candidate gravitational-wave event, so that telescopes around the world can begin the hunt for a counterpart. The alerts are distributed through GCN.","aliases":["LIGO-Virgo-KAGRA alerts"],"sources":["ligo"]},{"id":"alert_system:scimma","type":"alert_system","name":"SCiMMA","domain":"science","entryPath":"/multi-messenger/scimma","description":"An open cyberinfrastructure project building the tools and networks — including the Hopskotch streaming system — to carry the flood of multi-messenger alerts between gravitational-wave, neutrino, and electromagnetic observatories quickly and reliably.","aliases":["Scalable Cyberinfrastructure for Multi-Messenger Astrophysics"],"sources":["ligo"]},{"id":"mm_channel:gravitational-waves-and-light","type":"mm_channel","name":"Gravitational Waves + Light","domain":"science","entryPath":"/multi-messenger/gravitational-waves-and-light","description":"Observing a source in both gravitational waves and electromagnetic light — the channel that transformed astronomy when GW170817 was caught in both, pinning down where a kilonova came from and confirming that neutron-star mergers forge heavy elements.","aliases":["GW + EM"],"sources":["ligo"]},{"id":"mm_channel:gravitational-waves-and-neutrinos","type":"mm_channel","name":"Gravitational Waves + Neutrinos","domain":"science","entryPath":"/multi-messenger/gravitational-waves-and-neutrinos","description":"Searching for neutrinos in coincidence with a gravitational-wave event. Both messengers escape from deep inside cataclysms that light cannot penetrate, so a joint detection would probe the engines of mergers and collapses directly.","aliases":["GW + neutrinos"],"sources":["ligo"]},{"id":"mm_channel:gravitational-waves-and-gamma-rays","type":"mm_channel","name":"Gravitational Waves + Gamma Rays","domain":"science","entryPath":"/multi-messenger/gravitational-waves-and-gamma-rays","description":"The pairing of a gravitational-wave chirp with a short gamma-ray burst. Their near-simultaneous arrival from GW170817 confirmed that neutron-star mergers cause short gamma-ray bursts, and that gravitational waves travel at the speed of light.","aliases":["GW + gamma"],"sources":["ligo"]},{"id":"mm_channel:gravitational-waves-and-radio","type":"mm_channel","name":"Gravitational Waves + Radio","domain":"science","entryPath":"/multi-messenger/gravitational-waves-and-radio","description":"Following a gravitational-wave source into the radio, where the slow afterglow of a merger's jet ploughing into surrounding gas unfolds over weeks to months, revealing the geometry and energetics of the outflow.","aliases":["GW + radio"],"sources":["ligo"]},{"id":"mm_channel:gravitational-waves-and-optical","type":"mm_channel","name":"Gravitational Waves + Optical","domain":"science","entryPath":"/multi-messenger/gravitational-waves-and-optical","description":"The optical hunt for a gravitational-wave counterpart — the wide-field survey campaign that finds and follows the fading glow of a kilonova, measuring how a merger's freshly-made heavy elements light up and cool.","aliases":["GW + optical"],"sources":["ligo"]},{"id":"gw_followup_stage:localization","type":"gw_followup_stage","name":"Localization","domain":"science","entryPath":"/multi-messenger/localization","description":"Working out where on the sky a gravitational-wave source lies, from the tiny differences in when and how strongly each detector in the network registers the wave. With only two or three detectors the region can be huge — hundreds of square degrees — which is what makes the counterpart search so hard.","sources":["ligo"]},{"id":"gw_followup_stage:counterpart-search","type":"gw_followup_stage","name":"Counterpart Search","domain":"science","entryPath":"/multi-messenger/counterpart-search","description":"The race to find the electromagnetic counterpart of a gravitational-wave event — wide-field telescopes tiling the large localization region, imaging it repeatedly to catch the one new point of light that is the merger's afterglow among millions of unrelated sources.","sources":["ligo"]},{"id":"gw_followup_stage:rapid-response","type":"gw_followup_stage","name":"Rapid Response","domain":"science","entryPath":"/multi-messenger/rapid-response","description":"The time-critical mobilisation of telescopes within minutes to hours of a gravitational-wave alert. A kilonova fades in days and the earliest light carries the most information, so automated systems and rapid human decisions decide whether the counterpart is caught at all.","sources":["ligo"]},{"id":"gw_data_product:sky-localization-map","type":"gw_data_product","name":"Sky Localization Map","domain":"science","entryPath":"/multi-messenger/sky-localization-map","description":"The probability map of where a gravitational-wave source lies on the sky, released with each alert. Rather than a single point it is a spread of probability — often a long banana-shaped arc — that observers use to plan which patches of sky to search first.","aliases":["skymap"],"sources":["ligo"]},{"id":"gw_data_product:gravitational-waveform","type":"gw_data_product","name":"Gravitational Waveform","domain":"science","entryPath":"/multi-messenger/gravitational-waveform","description":"The signal itself — the rising chirp of a compact binary as it spirals in, merges, and rings down. Matching the observed waveform against banks of theoretical templates is how a real signal is dug out of the detector noise and how its source is identified.","sources":["ligo"]},{"id":"gw_data_product:parameter-estimation","type":"gw_data_product","name":"Parameter Estimation","domain":"science","entryPath":"/multi-messenger/parameter-estimation","description":"Inferring the properties of a gravitational-wave source — the masses and spins of the merging objects, the distance, the orientation — by comparing the waveform against models. It is how a chirp becomes a measurement, including the standard-siren distance that probes the expansion of the universe.","sources":["ligo"]},{"id":"gw_data_product:gravitational-wave-transient-catalog","type":"gw_data_product","name":"Gravitational-Wave Transient Catalog","domain":"science","entryPath":"/multi-messenger/gravitational-wave-transient-catalog","description":"The cumulative catalogue of confident gravitational-wave detections from the LIGO–Virgo–KAGRA observing runs — the growing census of compact-binary mergers, released as open data, from which the population of black holes and neutron stars across cosmic time is reconstructed.","aliases":["GWTC"],"sources":["ligo"]},{"id":"planetary_interior:core","type":"planetary_interior","name":"Core","domain":"science","entryPath":"/comparative-planetology/core","description":"The dense central region of a planet or moon, typically the heaviest material that sank inward as the body formed. In the terrestrial planets it is largely iron; where it is partly molten and convecting, as in Earth, it can generate a global magnetic field.","sources":["nasa"]},{"id":"planetary_interior:mantle","type":"planetary_interior","name":"Mantle","domain":"science","entryPath":"/comparative-planetology/mantle","description":"The thick layer between core and crust, made of hot rock that, though solid, flows over geological time. Its slow convection carries heat outward and drives the tectonics and volcanism that resurface a planet.","sources":["nasa"]},{"id":"planetary_interior:crust","type":"planetary_interior","name":"Crust","domain":"science","entryPath":"/comparative-planetology/crust","description":"The thin, rigid outermost solid layer of a rocky planet or moon — the product of differentiation and volcanism, and the surface on which its geological history is written.","sources":["nasa"]},{"id":"planetary_process:planetary-differentiation","type":"planetary_process","name":"Planetary Differentiation","domain":"science","entryPath":"/comparative-planetology/planetary-differentiation","description":"The separation of a young, molten planet into layers by density — the heaviest metal sinking to form a core, the lightest material rising to form a crust. It sets the deep structure every other process then acts on.","sources":["nasa"]},{"id":"planetary_process:plate-tectonics","type":"planetary_process","name":"Plate Tectonics","domain":"science","entryPath":"/comparative-planetology/plate-tectonics","description":"The slow motion of a planet's rigid surface plates over its convecting mantle, continually creating and recycling crust. Earth is the only body where plate tectonics is known to operate today, and it is deeply tied to Earth's long-term climate and habitability.","sources":["nasa"]},{"id":"planetary_process:volcanism","type":"planetary_process","name":"Volcanism","domain":"science","entryPath":"/comparative-planetology/volcanism","description":"The eruption of molten rock from a planet's interior onto its surface — from Earth's volcanoes to the relentless silicate volcanism of Jupiter's moon Io, the most volcanically active body in the Solar System, whose surface and plumes are painted with sulphur and sulphur-dioxide frosts.","sources":["nasa"]},{"id":"planetary_process:cryovolcanism","type":"planetary_process","name":"Cryovolcanism","domain":"science","entryPath":"/comparative-planetology/cryovolcanism","description":"'Ice volcanism' — the eruption not of molten rock but of water, ammonia, or methane from the interior of a cold, icy world. Enceladus jets plumes of water ice into space, and Triton has erupting geysers; the erupted material is these worlds' equivalent of lava.","sources":["nasa"]},{"id":"planetary_process:atmospheric-escape","type":"planetary_process","name":"Atmospheric Escape","domain":"science","entryPath":"/comparative-planetology/atmospheric-escape","description":"The gradual loss of a planet's atmosphere to space — light gases escaping thermally, the solar wind stripping the air from an unmagnetised planet, or impacts blasting it away. It is why Mars, which lost its magnetic field, also lost most of its once-thick atmosphere.","sources":["nasa"]},{"id":"planetary_process:climate-evolution","type":"planetary_process","name":"Climate Evolution","domain":"science","entryPath":"/comparative-planetology/climate-evolution","description":"How a planet's climate changes over billions of years — the runaway greenhouse that turned Venus into a furnace, the slow drying and cooling of Mars, and the feedbacks that have kept Earth habitable. Comparing the three is the key to understanding what makes a climate stable.","sources":["nasa"]},{"id":"planetary_process:the-greenhouse-effect","type":"planetary_process","name":"The Greenhouse Effect","domain":"science","entryPath":"/comparative-planetology/the-greenhouse-effect","description":"The warming of a planet's surface by an atmosphere that lets sunlight in but traps the outgoing heat. Modest and life-enabling on Earth, it is extreme on Venus, whose thick carbon-dioxide atmosphere makes it the hottest planet in the Solar System.","sources":["nasa"]},{"id":"planetary_process:atmospheric-circulation","type":"planetary_process","name":"Atmospheric Circulation","domain":"science","entryPath":"/comparative-planetology/atmospheric-circulation","description":"The global movement of a planet's atmosphere, driven by uneven heating and the planet's rotation — the banded jets and great storms of the gas giants, the super-rotating winds of Venus that lap the planet in days, and the planet-wide dust storms of Mars.","sources":["nasa"]},{"id":"planetary_process:magnetospheric-shielding","type":"planetary_process","name":"Magnetospheric Shielding","domain":"science","entryPath":"/comparative-planetology/magnetospheric-shielding","description":"The protection a planet's magnetic field gives its atmosphere by deflecting the solar wind around it. Earth's magnetosphere shields its air; Mars, having lost its global field billions of years ago, was left exposed to the stripping that thinned its atmosphere.","sources":["nasa"]},{"id":"planetary_process:impact-cratering-history","type":"planetary_process","name":"Impact Cratering History","domain":"science","entryPath":"/comparative-planetology/impact-cratering-history","description":"The record of impacts written across a planet's surface, and the way it is read: because craters accumulate over time, a more heavily cratered surface is older. Counting craters is the main way the ages of surfaces across the Solar System are estimated.","sources":["nasa"]},{"id":"planetary_class:ocean-world","type":"planetary_class","name":"Ocean World","domain":"science","entryPath":"/comparative-planetology/ocean-world","description":"A world with a large body of liquid water — most securely the global oceans hidden beneath the ice of moons like Europa and Enceladus, and possibly some water-rich exoplanets. Ocean worlds are among the most promising places to search for life beyond Earth.","sources":["nasa"]},{"id":"planetary_class:lava-world","type":"planetary_class","name":"Lava World","domain":"science","entryPath":"/comparative-planetology/lava-world","description":"A rocky exoplanet orbiting so close to its star that its day side is hot enough to melt rock, covering it in a global magma ocean. Several known super-Earths, such as 55 Cancri e, are thought to be lava worlds, offering a natural laboratory for molten-rock chemistry.","sources":["nasa"]},{"id":"planetary_class:hycean-planet","type":"planetary_class","name":"Hycean Planet","domain":"science","entryPath":"/comparative-planetology/hycean-planet","description":"A proposed class of exoplanet — a hot world with a hydrogen-rich atmosphere over a planet-wide ocean. If they exist, hycean planets would offer a much wider habitable zone than rocky worlds and be easier to study, but the class is hypothetical and its habitability unconfirmed.","sources":["nasa"]},{"id":"interstellar_environment:diffuse-interstellar-medium","type":"interstellar_environment","name":"The Diffuse Interstellar Medium","domain":"science","entryPath":"/astrochemistry/diffuse-interstellar-medium","description":"The thin, warm, mostly atomic gas that fills the space between the stars, laced with dust that reddens the light passing through it. Even here, exposed to starlight, the first simple molecules form — the beginning of cosmic chemistry.","aliases":["diffuse clouds"],"sources":["nasa"]},{"id":"interstellar_environment:molecular-cloud","type":"interstellar_environment","name":"Molecular Clouds","domain":"science","entryPath":"/astrochemistry/molecular-cloud","description":"Cold, dense clouds of molecular hydrogen and dust, dark and shielded from starlight, where nearly all the interstellar molecules reside and where stars are born. They are the richest chemical factories in the galaxy, mapped in the millimetre and submillimetre.","aliases":["dense clouds"],"sources":["eso"]},{"id":"interstellar_environment:star-forming-region","type":"interstellar_environment","name":"Star-Forming Regions","domain":"science","entryPath":"/astrochemistry/star-forming-region","description":"The dense cores of molecular clouds where gravity pulls gas together into new stars, and where the heat and radiation of those young stars drive a burst of chemistry. The Orion Nebula is the nearest region of massive star formation and the most-studied example.","sources":["nasa"]},{"id":"interstellar_environment:protoplanetary-disk","type":"interstellar_environment","name":"Protoplanetary Disks","domain":"science","entryPath":"/astrochemistry/protoplanetary-disk","description":"The disks of gas and dust that surround young stars, out of which planets, moons, and comets form. Their chemistry — imaged in exquisite detail by ALMA — sets the raw ingredients that new planets and their atmospheres are built from.","sources":["eso"]},{"id":"interstellar_environment:interstellar-dust","type":"interstellar_environment","name":"Interstellar Dust","domain":"science","entryPath":"/astrochemistry/interstellar-dust","description":"The tiny grains of silicate and carbon — often coated in mantles of ice — that pervade the interstellar medium. They redden and dim starlight, radiate in the infrared, and, crucially, provide the surfaces on which many molecules are built.","aliases":["cosmic dust","silicate and ice grains"],"sources":["nasa"]},{"id":"interstellar_molecule:water","type":"interstellar_molecule","name":"Water","domain":"science","entryPath":"/astrochemistry/water","description":"One of the most abundant molecules in the universe, present as gas, as ice frozen onto dust grains, and in the disks where planets form. Tracing where water is inherited from the interstellar medium versus made in disks is central to understanding how worlds get their oceans.","sources":["nasa"]},{"id":"interstellar_molecule:carbon-monoxide","type":"interstellar_molecule","name":"Carbon Monoxide","domain":"science","entryPath":"/astrochemistry/carbon-monoxide","description":"After molecular hydrogen, the most abundant molecule in space — and, because hydrogen is hard to see directly in cold gas, the workhorse tracer astronomers use to map molecular clouds and measure how much gas is available to form stars.","sources":["eso"]},{"id":"interstellar_molecule:carbon-dioxide","type":"interstellar_molecule","name":"Carbon Dioxide","domain":"science","entryPath":"/astrochemistry/carbon-dioxide","description":"A common component of the icy mantles that coat interstellar dust grains, detected by the infrared absorption its ice produces against background starlight. Its abundance in ices records the chemistry and radiation history of a cloud.","sources":["nasa"]},{"id":"interstellar_molecule:ammonia","type":"interstellar_molecule","name":"Ammonia","domain":"science","entryPath":"/astrochemistry/ammonia","description":"One of the first polyatomic molecules found in space, and a sensitive thermometer of dense cloud cores: the relative strengths of its radio lines reveal the temperature of the cold gas about to collapse into stars.","sources":["nasa"]},{"id":"interstellar_molecule:hydrogen-cyanide","type":"interstellar_molecule","name":"Hydrogen Cyanide","domain":"science","entryPath":"/astrochemistry/hydrogen-cyanide","description":"A simple nitrogen-bearing molecule widespread in space and central to prebiotic chemistry — many proposed routes to the building blocks of life pass through hydrogen cyanide and its relatives.","sources":["nasa"]},{"id":"interstellar_molecule:methanol","type":"interstellar_molecule","name":"Methanol","domain":"science","entryPath":"/astrochemistry/methanol","description":"A key complex organic molecule that forms not in the gas but on the icy surfaces of dust grains, by the step-by-step addition of hydrogen to frozen carbon monoxide. It is a stepping stone toward the larger organic molecules found around young stars.","sources":["nasa"]},{"id":"interstellar_molecule:polycyclic-aromatic-hydrocarbons","type":"interstellar_molecule","name":"Polycyclic Aromatic Hydrocarbons","domain":"science","entryPath":"/astrochemistry/polycyclic-aromatic-hydrocarbons","description":"Large, flat molecules of linked carbon rings that pervade the galaxy, glowing in a distinctive set of infrared bands and locking up a large share of interstellar carbon. The James Webb Space Telescope maps their emission across galaxies.","aliases":["PAHs"],"sources":["nasa"]},{"id":"interstellar_molecule:amino-acid-precursors","type":"interstellar_molecule","name":"Amino-Acid Precursors","domain":"science","entryPath":"/astrochemistry/amino-acid-precursors","description":"The molecular building blocks from which amino acids can form — some detected in space and in the ices of comets, and amino acids themselves found in meteorites such as Murchison. They link the chemistry of the interstellar medium to the origin of life.","sources":["nasa"]},{"id":"astrochemical_process:gas-phase-chemistry","type":"astrochemical_process","name":"Gas-Phase Chemistry","domain":"science","entryPath":"/astrochemistry/gas-phase-chemistry","description":"Chemistry that happens in the gas between grains, driven especially by fast ion–molecule reactions that proceed even at the frigid temperatures of interstellar clouds. It builds many of the simple molecules seen in space.","sources":["nasa"]},{"id":"astrochemical_process:grain-surface-chemistry","type":"astrochemical_process","name":"Grain-Surface Chemistry","domain":"science","entryPath":"/astrochemistry/grain-surface-chemistry","description":"Chemistry that happens on the icy mantles of dust grains, where atoms and molecules land, wander, and meet. It makes molecules the gas phase cannot — water and methanol among them — and is the source of much of space's complex organic chemistry.","sources":["nasa"]},{"id":"astrochemical_process:photochemistry","type":"astrochemical_process","name":"Photochemistry","domain":"science","entryPath":"/astrochemistry/photochemistry","description":"Chemistry driven by ultraviolet starlight, which breaks molecules apart and ionises atoms at the illuminated edges of clouds and the surfaces of disks — both destroying molecules and opening new reaction pathways.","sources":["nasa"]},{"id":"astrochemical_process:shock-chemistry","type":"astrochemical_process","name":"Shock Chemistry","domain":"science","entryPath":"/astrochemistry/shock-chemistry","description":"Chemistry triggered when gas is suddenly heated and compressed — by the outflows of newborn stars or the blast waves of supernovae. Shocks sputter material off dust grains and power reactions that need high temperatures, changing a cloud's chemistry.","sources":["nasa"]},{"id":"astrochemical_process:prebiotic-chemistry","type":"astrochemical_process","name":"Prebiotic Chemistry","domain":"science","entryPath":"/astrochemistry/prebiotic-chemistry","description":"The astrochemistry of molecules relevant to the origin of life — how the building blocks of biology can be assembled in interstellar clouds, on icy grains, and in the young Solar System, and delivered to a planet's surface.","sources":["nasa"]},{"id":"astrochemical_process:planet-formation-chemistry","type":"astrochemical_process","name":"Planet-Formation Chemistry","domain":"science","entryPath":"/astrochemistry/planet-formation-chemistry","description":"The chemistry of protoplanetary disks that decides what new planets are made of — where ices freeze out, which molecules end up in comets and which in planetary atmospheres, and how much water and organic material a world inherits.","sources":["eso"]},{"id":"astrochemical_process:cometary-and-meteoritic-chemistry","type":"astrochemical_process","name":"Cometary & Meteoritic Chemistry","domain":"science","entryPath":"/astrochemistry/cometary-and-meteoritic-chemistry","description":"The record of the early Solar System's chemistry preserved in comets and meteorites — the amino acids in the Murchison meteorite, the ancient inclusions of Allende, and the ices of comets — a frozen archive of the material that built the planets.","sources":["nasa"]},{"id":"space_treaty:outer-space-treaty","type":"space_treaty","name":"The Outer Space Treaty","domain":"science","entryPath":"/space-policy/outer-space-treaty","description":"The founding treaty of international space law, opened for signature in 1967. It declares space free for exploration and use by all nations, forbids any state from claiming sovereignty over the Moon or other bodies, bans weapons of mass destruction in orbit, and makes states responsible for their national space activities — governmental or private.","aliases":["OST"],"sources":["nasa"]},{"id":"space_treaty:liability-convention","type":"space_treaty","name":"The Liability Convention","domain":"science","entryPath":"/space-policy/liability-convention","description":"A 1972 convention that elaborates the Outer Space Treaty's liability principle: a launching state is absolutely liable for damage its space objects cause on the Earth's surface or to aircraft, and liable for fault for damage caused in space.","sources":["nasa"]},{"id":"space_treaty:registration-convention","type":"space_treaty","name":"The Registration Convention","domain":"science","entryPath":"/space-policy/registration-convention","description":"A 1975 convention, in force from 1976, requiring states to register the objects they launch into space with the United Nations, so that space objects can be identified — the basis of the UN register of space objects that UNOOSA maintains.","sources":["nasa"]},{"id":"space_treaty:moon-agreement","type":"space_treaty","name":"The Moon Agreement","domain":"science","entryPath":"/space-policy/moon-agreement","description":"A 1979 agreement declaring the Moon and its natural resources the common heritage of mankind and calling for an international regime to govern their exploitation. It has been ratified by only a handful of states, none of them major spacefaring powers, which limits its force.","sources":["nasa"]},{"id":"space_treaty:artemis-accords","type":"space_treaty","name":"The Artemis Accords","domain":"science","entryPath":"/space-policy/artemis-accords","description":"A set of principles for cooperative, peaceful, and transparent exploration of the Moon and beyond, established in 2020 and led by NASA, and signed by a growing number of nations. They interpret the Outer Space Treaty for a new era of lunar activity, including the use of space resources.","sources":["nasa"]},{"id":"space_policy_topic:orbital-debris","type":"space_policy_topic","name":"Orbital Debris","domain":"science","entryPath":"/space-policy/orbital-debris","description":"The growing population of defunct satellites, spent rocket stages, and fragments of past collisions and explosions that circle the Earth. Travelling at kilometres per second, even a small piece can destroy an operational spacecraft, and there are millions of untracked fragments.","aliases":["space junk"],"sources":["nasa"]},{"id":"space_policy_topic:kessler-syndrome","type":"space_policy_topic","name":"The Kessler Syndrome","domain":"science","entryPath":"/space-policy/kessler-syndrome","description":"The scenario, named for Donald Kessler, in which the density of objects in orbit becomes high enough that collisions cascade — each impact creating more debris that causes further impacts — potentially making some orbits unusable for generations.","sources":["nasa"]},{"id":"space_policy_topic:space-situational-awareness","type":"space_policy_topic","name":"Space Situational Awareness","domain":"science","entryPath":"/space-policy/space-situational-awareness","description":"The tracking and cataloguing of the tens of thousands of objects in orbit, and the prediction of close approaches, so that operators can be warned and collisions avoided. It is the sensing foundation on which any traffic management must rest.","aliases":["SSA"],"sources":["nasa"]},{"id":"space_policy_topic:space-traffic-management","type":"space_policy_topic","name":"Space Traffic Management","domain":"science","entryPath":"/space-policy/space-traffic-management","description":"The coordination of spacecraft operations — who moves, when, and how — to prevent collisions as orbits grow crowded. Unlike air or sea traffic, space has no established global authority to direct it, making it an urgent and unsolved governance problem.","aliases":["STM"],"sources":["nasa"]},{"id":"space_policy_topic:debris-mitigation","type":"space_policy_topic","name":"Debris Mitigation","domain":"science","entryPath":"/space-policy/debris-mitigation","description":"The guidelines and practices meant to limit the creation of new debris — deorbiting satellites at end of life, venting spent rocket stages so they cannot explode, and clearing valuable orbits within a set number of years after a mission ends.","sources":["nasa"]},{"id":"space_policy_topic:mega-constellations","type":"space_policy_topic","name":"Mega-Constellations","domain":"science","entryPath":"/space-policy/mega-constellations","description":"The deployment of constellations of thousands of satellites in low Earth orbit to provide global broadband. They transform the economics of space but sharply raise concerns over orbital traffic, collision risk, radio-frequency use, and the brightness of the night sky for astronomy.","sources":["nasa"]},{"id":"space_policy_topic:launch-licensing","type":"space_policy_topic","name":"Launch Licensing","domain":"science","entryPath":"/space-policy/launch-licensing","description":"The regulatory approval a national authority requires before a launch, covering public safety, liability insurance, and environmental review. It is the gate through which every launch must pass, and a major point of national space governance.","sources":["nasa"]},{"id":"space_policy_topic:spectrum-allocation","type":"space_policy_topic","name":"Spectrum & Orbital-Slot Allocation","domain":"science","entryPath":"/space-policy/spectrum-allocation","description":"The international coordination of the radio-frequency spectrum satellites use and the orbital slots they occupy — especially the crowded geostationary arc — managed through the International Telecommunication Union to prevent interference.","sources":["nasa"]},{"id":"space_policy_topic:export-control-and-dual-use","type":"space_policy_topic","name":"Export Control & Dual-Use Technology","domain":"science","entryPath":"/space-policy/export-control-and-dual-use","description":"The regulation of space technologies that have both civilian and military uses — rockets, sensors, and satellites — controlling their transfer across borders. It shapes who can build and buy space hardware, and is a persistent tension in the global space industry.","sources":["nasa"]},{"id":"space_policy_topic:space-resource-policy","type":"space_policy_topic","name":"Space Resource Policy","domain":"science","entryPath":"/space-policy/space-resource-policy","description":"The unsettled question of who may extract and own resources from the Moon and asteroids, and under what rules. The Outer Space Treaty forbids claiming territory, but says little about mining, and nations are now enacting their own laws — a live and contested frontier of space law.","sources":["nasa"]},{"id":"space_policy_topic:planetary-protection-policy","type":"space_policy_topic","name":"Planetary Protection Policy","domain":"science","entryPath":"/space-policy/planetary-protection-policy","description":"The international policy framework — coordinated by COSPAR — that keeps missions from contaminating other worlds with terrestrial microbes, and Earth from any hazard in returned samples. It turns the science of planetary protection into binding mission requirements.","sources":["nasa"]},{"id":"space_economy_topic:commercial-launch","type":"space_economy_topic","name":"Commercial Launch","domain":"science","entryPath":"/space-policy/commercial-launch","description":"The private launch industry that has driven the cost of reaching orbit down by an order of magnitude — through reusable rockets and competition — and opened space to companies, universities, and nations that could never before afford it.","sources":["nasa"]},{"id":"space_economy_topic:the-satellite-economy","type":"space_economy_topic","name":"The Satellite Economy","domain":"science","entryPath":"/space-policy/the-satellite-economy","description":"The largest part of the space economy — the industry built on satellites for communications, navigation, and Earth observation, whose services underpin the modern economy on the ground, from banking timestamps to weather forecasts to global positioning.","sources":["nasa"]},{"id":"space_economy_topic:space-insurance","type":"space_economy_topic","name":"Space Insurance","domain":"science","entryPath":"/space-policy/space-insurance","description":"The specialised insurance market that underwrites the risk of launching and operating satellites — covering the moments when a rocket can fail and the years a satellite must survive the hazards of space. It is a small but essential enabler of commercial space.","sources":["nasa"]},{"id":"space_economy_topic:the-space-economy","type":"space_economy_topic","name":"The Space Economy","domain":"science","entryPath":"/space-policy/the-space-economy","description":"The whole economic system of space activity — launch, satellites, ground systems, services, and the emerging markets in resources and on-orbit servicing — and the far larger value it creates on Earth. Increasingly it is driven by private capital as much as by governments.","sources":["nasa"]},{"id":"organization:unoosa","type":"organization","name":"UNOOSA","domain":"science","entryPath":"/space-policy/unoosa","description":"The United Nations Office for Outer Space Affairs, which promotes international cooperation in the peaceful use of space, supports the development of space law, and maintains the United Nations register of objects launched into space.","aliases":["UN Office for Outer Space Affairs"],"sources":["nasa"]},{"id":"organization:cospar","type":"organization","name":"COSPAR","domain":"science","entryPath":"/space-policy/cospar","description":"The Committee on Space Research, an international scientific body that coordinates space research across nations and maintains the planetary-protection policy that keeps missions from contaminating other worlds and Earth from returned samples.","aliases":["Committee on Space Research"],"sources":["nasa"]},{"id":"organization:international-telecommunication-union","type":"organization","name":"International Telecommunication Union","domain":"science","entryPath":"/space-policy/international-telecommunication-union","description":"The United Nations agency that allocates the global radio-frequency spectrum and the geostationary and other orbital slots that satellites use, coordinating between nations and operators to prevent harmful interference.","aliases":["ITU"],"sources":["nasa"]},{"id":"organization:international-astronautical-federation","type":"organization","name":"International Astronautical Federation","domain":"science","entryPath":"/space-policy/international-astronautical-federation","description":"A global space-advocacy organisation that connects space agencies, companies, and societies worldwide and runs the annual International Astronautical Congress, the largest gathering of the space community.","aliases":["IAF"],"sources":["nasa"]},{"id":"discovery_methodology:the-scientific-method","type":"discovery_methodology","name":"The Scientific Method","domain":"science","entryPath":"/discovery-history/the-scientific-method","description":"The cycle of observation, hypothesis, prediction, and test that turned the study of the heavens from stargazing and myth into a science — and the reason astronomy's claims can be checked, challenged, and improved rather than merely believed.","sources":["nasa"]},{"id":"discovery_methodology:paradigm-shifts","type":"discovery_methodology","name":"Paradigm Shifts","domain":"science","entryPath":"/discovery-history/paradigm-shifts","description":"The deep changes in how a field sees the world, as described by the philosopher Thomas Kuhn — moments when one framework of assumptions gives way to another, as when the Earth-centred cosmos was replaced by a Sun-centred one.","sources":["nasa"]},{"id":"discovery_methodology:scientific-revolutions","type":"discovery_methodology","name":"Scientific Revolutions","domain":"science","entryPath":"/discovery-history/scientific-revolutions","description":"The episodes in which accumulated anomalies — observations that will not fit the old picture — build until the framework breaks and a new one takes its place. Astronomy has driven several of the largest revolutions in all of science.","sources":["nasa"]},{"id":"discovery_methodology:instrumentation-driven-discovery","type":"discovery_methodology","name":"Instrumentation-Driven Discovery","domain":"science","entryPath":"/discovery-history/instrumentation-driven-discovery","description":"The recurring pattern by which a new instrument opens a new window on the universe and a wave of discovery follows — the telescope, the spectroscope, the photographic plate, the radio dish, the gravitational-wave detector each launching a new astronomy.","sources":["nasa"]},{"id":"discovery_methodology:observational-bias","type":"discovery_methodology","name":"Observational Bias","domain":"science","entryPath":"/discovery-history/observational-bias","description":"The systematic ways instruments and selection effects skew what astronomers find — brighter objects being easier to see, for instance, biasing a sample. Recognising and correcting these biases is as much a part of a result as the measurement itself.","sources":["nasa"]},{"id":"discovery_methodology:theory-and-observation","type":"discovery_methodology","name":"Theory & Observation","domain":"science","entryPath":"/discovery-history/theory-and-observation","description":"The interplay between prediction and measurement that drives astronomy forward — sometimes theory leads and observation confirms (the prediction of Neptune, of gravitational waves), and sometimes observation surprises and theory must catch up (the accelerating universe).","sources":["nasa"]},{"id":"discovery_methodology:big-science","type":"discovery_methodology","name":"Big Science","domain":"science","entryPath":"/discovery-history/big-science","description":"The modern era of vast, collaborative, and expensive instruments — the great space observatories, the kilometre-scale gravitational-wave detectors, the all-sky surveys — that no single scientist could build or fund, run instead by international collaborations of thousands.","sources":["nasa"]},{"id":"discovery_methodology:the-data-and-ai-revolution","type":"discovery_methodology","name":"The Data & AI Revolution","domain":"science","entryPath":"/discovery-history/the-data-and-ai-revolution","description":"The transformation of astronomy into a data science, in which surveys now produce far more data than any team could inspect by hand, and machine learning is used to classify, discover, and even find what no one thought to look for.","sources":["nasa"]},{"id":"philosophy_of_science:scientific-realism","type":"philosophy_of_science","name":"Scientific Realism","domain":"science","entryPath":"/discovery-history/scientific-realism","description":"The view that our best scientific theories describe a real world — that atoms, black holes, and dark matter are not merely convenient fictions but things that actually exist, even when they cannot be seen directly. It is the working assumption of most astronomers, and a live question in philosophy.","sources":["nasa"]},{"id":"philosophy_of_science:falsifiability","type":"philosophy_of_science","name":"Falsifiability","domain":"science","entryPath":"/discovery-history/falsifiability","description":"The criterion, associated with the philosopher Karl Popper, that a scientific claim must be testable and capable in principle of being proven wrong. It is one influential attempt to mark the boundary between science and non-science.","sources":["nasa"]},{"id":"philosophy_of_science:the-nature-of-evidence","type":"philosophy_of_science","name":"The Nature of Evidence","domain":"science","entryPath":"/discovery-history/the-nature-of-evidence","description":"What counts as evidence in a science where controlled experiments are rarely possible and the universe cannot be put in a laboratory. Astronomy must infer from what it is shown — the light and particles that happen to arrive — which makes the careful weighing of evidence central.","sources":["nasa"]},{"id":"philosophy_of_science:measurement-uncertainty","type":"philosophy_of_science","name":"Measurement Uncertainty","domain":"science","entryPath":"/discovery-history/measurement-uncertainty","description":"Every astronomical measurement carries an uncertainty — statistical scatter and systematic error — and understanding it is inseparable from the result. A number without its error bar is not yet a measurement, and disputes in astronomy are often disputes about uncertainty.","sources":["nasa"]},{"id":"philosophy_of_science:replication-and-reproducibility","type":"philosophy_of_science","name":"Replication & Reproducibility","domain":"science","entryPath":"/discovery-history/replication-and-reproducibility","description":"The demand that a result stand up when others repeat the analysis on the same or new data — a cornerstone of scientific trust, and a growing concern as analyses become more complex and depend on large software pipelines.","sources":["nasa"]},{"id":"philosophy_of_science:open-science","type":"philosophy_of_science","name":"Open Science","domain":"science","entryPath":"/discovery-history/open-science","description":"The movement to make the data, code, and methods behind a result openly available, so that science can be checked, reused, and built upon by anyone. In astronomy, with its open archives and shared surveys, it is both a philosophy and a well-developed practice.","sources":["nasa"]},{"id":"history_theme:the-copernican-revolution","type":"history_theme","name":"The Copernican Revolution","domain":"science","entryPath":"/discovery-history/the-copernican-revolution","description":"The shift from an Earth-centred to a Sun-centred cosmos — from Copernicus's heliocentric proposal, through Galileo's telescopic evidence and Kepler's laws of planetary motion, to Newton's gravity that explained them all. The founding revolution of modern astronomy, and the archetype of a scientific revolution.","sources":["nasa"]},{"id":"history_theme:the-history-of-the-telescope","type":"history_theme","name":"The History of the Telescope","domain":"science","entryPath":"/discovery-history/the-history-of-the-telescope","description":"From Galileo first turning a spyglass on the sky in 1609 — finding craters on the Moon and moons around Jupiter — through William Herschel's reflecting telescopes, one of which discovered Uranus, to the segmented giants and space telescopes of today. Each leap in aperture opened new depths of the universe.","sources":["nasa"]},{"id":"history_theme:the-history-of-spectroscopy","type":"history_theme","name":"The History of Spectroscopy","domain":"science","entryPath":"/discovery-history/the-history-of-spectroscopy","description":"How splitting starlight into its colours revealed what the stars are made of — the dark lines in the spectrum betraying the elements present. It was the birth of astrophysics, the moment astronomy became not just where and when but what and how.","sources":["nasa"]},{"id":"history_theme:the-history-of-radio-astronomy","type":"history_theme","name":"The History of Radio Astronomy","domain":"science","entryPath":"/discovery-history/the-history-of-radio-astronomy","description":"How Karl Jansky's chance detection of radio waves from the Milky Way in the 1930s opened an entirely new window on the universe — leading in time to pulsars, quasars, the cosmic microwave background, and the imaging of a black hole.","sources":["nasa"]},{"id":"history_theme:the-history-of-cosmology","type":"history_theme","name":"The History of Cosmology","domain":"science","entryPath":"/discovery-history/the-history-of-cosmology","description":"From Hubble's discovery that the universe is expanding, through the Big Bang and the detection of its afterglow, to the surprise of the accelerating cosmos and the tensions in today's precision measurements. A century in which cosmology became a science.","sources":["nasa"]},{"id":"history_theme:the-history-of-exoplanets","type":"history_theme","name":"The History of Exoplanets","domain":"science","entryPath":"/discovery-history/the-history-of-exoplanets","description":"From the first confirmed planet around another Sun-like star in 1995 — found by the radial-velocity wobble it induced — to the thousands now known, many by the transit method, a field that went in a generation from speculation to a central pursuit of astronomy, driven by ever more sensitive detection methods.","sources":["nasa"]},{"id":"history_theme:the-history-of-gravitational-waves","type":"history_theme","name":"The History of Gravitational Waves","domain":"science","entryPath":"/discovery-history/the-history-of-gravitational-waves","description":"From Einstein's 1916 prediction that mass in motion should ripple spacetime, through a century of doubt about whether they could ever be detected, to the first direct detection of a black-hole merger in 2015 — and a new way of observing the universe.","sources":["nasa"]},{"id":"history_theme:the-history-of-black-holes","type":"history_theme","name":"The History of Black Holes","domain":"science","entryPath":"/discovery-history/the-history-of-black-holes","description":"From a strange mathematical solution that many thought unphysical, through the theoretical work that made them respectable and the observations that made them real, to the imaging of a black hole's shadow and the star orbits that prove one lurks at the Milky Way's heart.","sources":["nasa"]},{"id":"orbital_mechanics_concept:restricted-three-body-problem","type":"orbital_mechanics_concept","name":"The Restricted Three-Body Problem","domain":"science","entryPath":"/celestial-mechanics/restricted-three-body-problem","description":"The motion of a small body under the gravity of two larger ones orbiting each other. It has no general closed-form solution, yet its study yields the Lagrange points, the concept of orbital stability, and much of modern spacecraft trajectory design.","sources":["jpl"]},{"id":"orbital_mechanics_concept:n-body-dynamics","type":"orbital_mechanics_concept","name":"N-Body Dynamics","domain":"science","entryPath":"/celestial-mechanics/n-body-dynamics","description":"The gravitational motion of many bodies at once. Beyond two bodies there is no general closed-form solution, so the positions of the planets and moons are found by integrating the equations of motion numerically — the basis of modern ephemerides.","sources":["jpl"]},{"id":"orbital_mechanics_concept:lagrange-points","type":"orbital_mechanics_concept","name":"Lagrange Points","domain":"science","entryPath":"/celestial-mechanics/lagrange-points","description":"The five points in a two-body system where a small third body can remain fixed relative to the two, its motion balanced by their combined gravity. The James Webb Space Telescope orbits the Sun–Earth L2 point, and the Trojan asteroids sit at Jupiter's L4 and L5.","aliases":["L1–L5"],"sources":["jpl"]},{"id":"orbital_mechanics_concept:hill-sphere","type":"orbital_mechanics_concept","name":"The Hill Sphere","domain":"science","entryPath":"/celestial-mechanics/hill-sphere","description":"The region around a body within which its own gravity dominates over that of the more massive body it orbits. It sets how far out moons and rings can stably orbit a planet — anything beyond a planet's Hill sphere is pulled away by the Sun.","sources":["jpl"]},{"id":"orbital_mechanics_concept:roche-limit","type":"orbital_mechanics_concept","name":"The Roche Limit","domain":"science","entryPath":"/celestial-mechanics/roche-limit","description":"The distance within which a body held together only by its own gravity is pulled apart by the tidal forces of the body it orbits. It is why planetary rings lie close in — where a moon could not survive — and why comets passing too close to a planet break into fragments.","sources":["jpl"]},{"id":"orbital_mechanics_concept:orbital-perturbations","type":"orbital_mechanics_concept","name":"Orbital Perturbations","domain":"science","entryPath":"/celestial-mechanics/orbital-perturbations","description":"The small departures of a real orbit from a perfect two-body ellipse — caused by the pull of other bodies, a planet's equatorial bulge, atmospheric drag, and radiation. They accumulate over time, which is why orbits must be tracked and recomputed continually.","sources":["jpl"]},{"id":"orbital_mechanics_concept:mean-motion-resonance","type":"orbital_mechanics_concept","name":"Mean-Motion Resonance","domain":"science","entryPath":"/celestial-mechanics/mean-motion-resonance","description":"When the orbital periods of two bodies form a simple whole-number ratio, their repeated close alignments deliver gravitational kicks that add up. Such resonances carve the Kirkwood gaps in the asteroid belt and lock Jupiter's inner moons into a precise chain.","sources":["jpl"]},{"id":"orbital_mechanics_concept:secular-resonance","type":"orbital_mechanics_concept","name":"Secular Resonance","domain":"science","entryPath":"/celestial-mechanics/secular-resonance","description":"A slow resonance not between orbital periods but between the rates at which orbits themselves precess. Acting over millions of years, secular resonances reshape the eccentricities and inclinations of orbits and help clear certain regions of the Solar System.","sources":["jpl"]},{"id":"orbital_mechanics_concept:tidal-evolution","type":"orbital_mechanics_concept","name":"Tidal Evolution","domain":"science","entryPath":"/celestial-mechanics/tidal-evolution","description":"The slow change of orbits and rotations caused by tidal friction. It is why the Moon is receding from the Earth and the day is lengthening, and why close-in moons and planets end up rotating in step with their orbits.","sources":["jpl"]},{"id":"orbital_mechanics_concept:spin-orbit-coupling","type":"orbital_mechanics_concept","name":"Spin–Orbit Coupling","domain":"science","entryPath":"/celestial-mechanics/spin-orbit-coupling","description":"The locking of a body's rotation to its orbit by tides. The Moon keeps one face toward the Earth in a 1:1 lock, while Mercury rotates three times for every two orbits of the Sun — a 3:2 spin–orbit resonance.","sources":["jpl"]},{"id":"orbital_mechanics_concept:orbital-elements","type":"orbital_mechanics_concept","name":"Orbital Elements","domain":"science","entryPath":"/celestial-mechanics/orbital-elements","description":"The set of numbers — typically six — that fully specify an orbit and a body's position along it: its size and shape, its orientation in space, and where the body is at a given time. They are the compact language in which every ephemeris and mission trajectory is expressed.","sources":["jpl"]},{"id":"reference_frame:icrs","type":"reference_frame","name":"The International Celestial Reference System","domain":"science","entryPath":"/celestial-mechanics/icrs","description":"The modern, fixed reference frame for the sky, defined by the positions of hundreds of distant quasars whose motion is undetectable. It replaced frames tied to the slowly-shifting equinox with one anchored to some of the most distant objects known — the standard to which all precise astronomical positions are now referred.","aliases":["ICRS"],"sources":["iau"]},{"id":"reference_frame:bcrs","type":"reference_frame","name":"The Barycentric Celestial Reference System","domain":"science","entryPath":"/celestial-mechanics/bcrs","description":"The reference system centred on the barycentre — the balance point — of the Solar System, used to describe the motion of the planets and the propagation of light across the Solar System. It is the frame in which planetary ephemerides are computed.","aliases":["BCRS"],"sources":["iau"]},{"id":"reference_frame:gcrs","type":"reference_frame","name":"The Geocentric Celestial Reference System","domain":"science","entryPath":"/celestial-mechanics/gcrs","description":"The reference system centred on the Earth, aligned with the barycentric frame but following the Earth in its orbit. It is the natural frame for the motion of satellites and for observations made from the ground.","aliases":["GCRS"],"sources":["iau"]},{"id":"reference_frame:the-ecliptic","type":"reference_frame","name":"The Ecliptic & Equinox","domain":"science","entryPath":"/celestial-mechanics/the-ecliptic","description":"The plane of the Earth's orbit around the Sun, and the equinox where it crosses the celestial equator. For millennia the equinox was the origin of celestial coordinates — but because it slowly precesses, modern frames are fixed to the stars instead.","sources":["iau"]},{"id":"reference_frame:j2000","type":"reference_frame","name":"The J2000 Epoch","domain":"science","entryPath":"/celestial-mechanics/j2000","description":"The standard reference epoch of modern astronomy — noon on 1 January 2000, in Terrestrial Time. Because the sky's apparent frame drifts with precession, coordinates and orbital elements are stated for a fixed epoch, and J2000.0 is the one in near-universal use.","aliases":["J2000.0"],"sources":["iau"]},{"id":"reference_frame:b1950","type":"reference_frame","name":"The B1950 Epoch","domain":"science","entryPath":"/celestial-mechanics/b1950","description":"The older standard epoch, defined by the beginning of the Besselian year 1950, to which many historical star catalogues and coordinates are referred. Converting between B1950 and J2000 positions is a routine but necessary step when using older data.","aliases":["B1950.0"],"sources":["iau"]},{"id":"ephemeris_system:jpl-development-ephemeris","type":"ephemeris_system","name":"JPL Development Ephemeris","domain":"science","entryPath":"/celestial-mechanics/jpl-development-ephemeris","description":"The series of numerically-integrated ephemerides, produced by NASA's Jet Propulsion Laboratory, that give the positions and velocities of the planets, the Moon, and the Sun to high precision over long spans. The DE ephemerides are the standard reference for precise Solar System calculations.","aliases":["JPL DE"],"sources":["jpl"]},{"id":"ephemeris_system:spice-toolkit","type":"ephemeris_system","name":"The SPICE Toolkit","domain":"science","entryPath":"/celestial-mechanics/spice-toolkit","description":"NASA's information system and software toolkit for computing the geometry of spacecraft and Solar System bodies — where a spacecraft is, where it is pointing, and what it can see. Its shared data files (kernels) are a de facto standard across planetary missions.","aliases":["SPICE"],"sources":["jpl"]},{"id":"ephemeris_system:jpl-horizons","type":"ephemeris_system","name":"JPL Horizons","domain":"science","entryPath":"/celestial-mechanics/jpl-horizons","description":"JPL's online ephemeris service, which generates highly accurate positions, distances, and other quantities for Solar System bodies and spacecraft, for any observer and time. It is the go-to tool for planning observations and checking where a body will be.","aliases":["Horizons"],"sources":["jpl"]},{"id":"time_standard:terrestrial-time","type":"time_standard","name":"Terrestrial Time","domain":"science","entryPath":"/celestial-mechanics/terrestrial-time","description":"The idealised time on the Earth's surface used as the time axis for astronomical events and geocentric ephemerides. It runs at the same rate as International Atomic Time but is offset ahead of it by a fixed 32.184 seconds, for continuity with the older ephemeris time.","aliases":["TT"],"sources":["usno"]},{"id":"time_standard:barycentric-dynamical-time","type":"time_standard","name":"Barycentric Dynamical Time","domain":"science","entryPath":"/celestial-mechanics/barycentric-dynamical-time","description":"The time coordinate of the Solar System barycentre, used as the independent variable of the planetary ephemerides. It differs from Terrestrial Time only by small periodic terms arising from the Earth's motion around the Sun, never drifting by more than a couple of milliseconds.","aliases":["TDB"],"sources":["usno"]},{"id":"time_standard:ut1","type":"time_standard","name":"Universal Time (UT1)","domain":"science","entryPath":"/celestial-mechanics/ut1","description":"The form of Universal Time tied to the actual rotation of the Earth, measured from the positions of distant sources. Because the Earth's spin is slightly irregular and slowly slowing, UT1 drifts against the steady beat of atomic time.","aliases":["UT1"],"sources":["usno"]},{"id":"time_standard:leap-second","type":"time_standard","name":"The Leap Second","domain":"science","entryPath":"/celestial-mechanics/leap-second","description":"The extra second occasionally inserted into Coordinated Universal Time to keep it within 0.9 seconds of UT1, so that civil clocks stay in step with the turning of the Earth. As atomic time and Earth rotation drift apart, leap seconds bridge the gap — a practice now being reconsidered.","sources":["usno"]},{"id":"time_standard:sidereal-time","type":"time_standard","name":"Sidereal Time","domain":"science","entryPath":"/celestial-mechanics/sidereal-time","description":"Time kept by the stars rather than the Sun — it measures the Earth's rotation relative to the fixed sky. A sidereal day is about four minutes shorter than a solar day, because the Earth must turn a little further each day to face the Sun again as it moves along its orbit.","sources":["usno"]},{"id":"time_standard:apparent-solar-time","type":"time_standard","name":"Apparent Solar Time","domain":"science","entryPath":"/celestial-mechanics/apparent-solar-time","description":"Time kept by the real Sun, as a sundial shows it — noon is the moment the Sun crosses the meridian. Because the Earth's orbit is elliptical and tilted, the Sun runs fast or slow through the year, so clocks keep mean solar time instead, differing by up to about a quarter of an hour.","sources":["usno"]},{"id":"stellar_process:star-formation","type":"stellar_process","name":"Star Formation","domain":"science","entryPath":"/stellar-astrophysics/star-formation","description":"Stars are born when the densest cores of a giant molecular cloud become unable to support themselves against their own gravity and collapse. As a core falls inward it heats, spins up into a disc, and grows a central protostar — a process that can be triggered by the shock of a nearby supernova or the squeeze of a spiral arm.","sources":["nasa"]},{"id":"stellar_process:pre-main-sequence-evolution","type":"stellar_process","name":"Pre-Main-Sequence Evolution","domain":"science","entryPath":"/stellar-astrophysics/pre-main-sequence-evolution","description":"The stage between a protostar and a fully-fledged star. Still contracting and drawing energy from gravity rather than fusion, the young star — a T Tauri star at low mass, a Herbig Ae/Be star at higher mass — is wrapped in an accretion disc and drives energetic jets, until its core grows hot enough to ignite hydrogen.","aliases":["Protostellar evolution"],"sources":["nasa"]},{"id":"stellar_process:main-sequence-evolution","type":"stellar_process","name":"Main-Sequence Evolution","domain":"science","entryPath":"/stellar-astrophysics/main-sequence-evolution","description":"The long, stable middle age of a star, during which it fuses hydrogen into helium in its core. This is where stars spend most of their lives — the Sun for roughly ten billion years — and a star's mass fixes where it sits along the main sequence, how brightly it burns, and how long it lasts.","sources":["nasa"]},{"id":"stellar_process:red-giant-branch","type":"stellar_process","name":"The Red-Giant Branch","domain":"science","entryPath":"/stellar-astrophysics/red-giant-branch","description":"When a star exhausts the hydrogen in its core, fusion moves to a shell around an inert helium core. The envelope swells enormously and cools to a red glow, and the star climbs the red-giant branch — brightening as it ascends until helium ignites at its tip.","aliases":["RGB"],"sources":["nasa"]},{"id":"stellar_process:helium-flash","type":"stellar_process","name":"The Helium Flash","domain":"science","entryPath":"/stellar-astrophysics/helium-flash","description":"In stars below about two solar masses, the helium core becomes so dense that it is held up by electron degeneracy pressure. When helium finally ignites, the degenerate gas cannot expand to regulate itself, so fusion runs away in a brief, violent flash — over in minutes, and hidden deep inside the star.","sources":["nasa"]},{"id":"stellar_process:horizontal-branch","type":"stellar_process","name":"The Horizontal Branch","domain":"science","entryPath":"/stellar-astrophysics/horizontal-branch","description":"After helium ignites, a low-mass star settles into a stable phase of quiet core helium burning, sitting on the horizontal branch of the colour–magnitude diagram at roughly constant luminosity. Stars crossing the instability strip here pulsate as RR Lyrae variables.","sources":["nasa"]},{"id":"stellar_process:asymptotic-giant-branch","type":"stellar_process","name":"The Asymptotic Giant Branch","domain":"science","entryPath":"/stellar-astrophysics/asymptotic-giant-branch","description":"Late in a low- or intermediate-mass star's life, both a hydrogen shell and a helium shell burn around a carbon–oxygen core. Recurring thermal pulses dredge freshly-made elements to the surface and drive heavy mass loss, as the star climbs the asymptotic giant branch toward the ejection of its envelope.","aliases":["AGB"],"sources":["nasa"]},{"id":"stellar_process:planetary-nebula-ejection","type":"stellar_process","name":"Planetary-Nebula Ejection","domain":"science","entryPath":"/stellar-astrophysics/planetary-nebula-ejection","description":"At the end of the asymptotic giant branch a dying star sheds its outer layers into space, exposing the hot stellar core beneath. The core's ultraviolet light lights up the expanding shell as a glowing planetary nebula — a name from the eighteenth century that has nothing to do with planets — before it fades to a white dwarf.","sources":["nasa"]},{"id":"stellar_process:stellar-mass-loss","type":"stellar_process","name":"Stellar Mass Loss","domain":"science","entryPath":"/stellar-astrophysics/stellar-mass-loss","description":"Throughout their lives, and especially near the end, stars shed mass in winds — driven by radiation pressure on spectral lines in hot, luminous stars, and on dust grains in cool giants and supergiants. Mass loss reshapes a star's fate, stripping envelopes and returning enriched gas to the interstellar medium.","aliases":["Stellar winds"],"sources":["nasa"]},{"id":"stellar_process:massive-star-core-collapse","type":"stellar_process","name":"Massive-Star Core Collapse","domain":"science","entryPath":"/stellar-astrophysics/massive-star-core-collapse","description":"A star born with more than roughly eight solar masses fuses ever-heavier elements until it builds an inert iron core. Iron cannot release energy by fusing, so once the core exceeds its stability limit it collapses in under a second, rebounds, and blows the star apart as a core-collapse supernova, leaving a neutron star or a black hole.","sources":["nasa"]},{"id":"stellar_process:stellar-rotation","type":"stellar_process","name":"Stellar Rotation","domain":"science","entryPath":"/stellar-astrophysics/stellar-rotation","description":"Stars spin, and how fast they spin shapes their lives. Rotation mixes fresh fuel into the core, flattens the star, powers magnetic dynamos, and drives mass loss; it can be measured from the broadening of spectral lines and, for the internal rotation hidden beneath the surface, from asteroseismology.","sources":["nasa"]},{"id":"stellar_process:stellar-magnetic-activity","type":"stellar_process","name":"Stellar Magnetic Activity","domain":"science","entryPath":"/stellar-astrophysics/stellar-magnetic-activity","description":"A star's rotation and convection together drive a magnetic dynamo, giving rise to starspots, flares, and hot outer atmospheres, often waxing and waning in activity cycles. The Sun is the star whose magnetic activity we can watch in closest detail, but the same physics operates across the cool stars.","sources":["nasa"]},{"id":"nucleosynthesis_process:proton-proton-chain","type":"nucleosynthesis_process","name":"The Proton–Proton Chain","domain":"science","entryPath":"/stellar-astrophysics/proton-proton-chain","description":"The dominant way low-mass stars like the Sun turn hydrogen into helium: through a chain of steps, four protons are fused into a single helium-4 nucleus, releasing energy and neutrinos. It powers the cores of the coolest main-sequence stars, where temperatures are too low for the competing CNO cycle.","aliases":["pp chain"],"sources":["nasa"]},{"id":"nucleosynthesis_process:cno-cycle","type":"nucleosynthesis_process","name":"The CNO Cycle","domain":"science","entryPath":"/stellar-astrophysics/cno-cycle","description":"A second route from hydrogen to helium, in which carbon, nitrogen, and oxygen act as catalysts that are used and regenerated. Because it is extremely temperature-sensitive, the CNO cycle dominates hydrogen burning in stars more massive than roughly 1.3 solar masses, whose cores are hotter than the Sun's.","aliases":["Carbon–nitrogen–oxygen cycle"],"sources":["nasa"]},{"id":"nucleosynthesis_process:triple-alpha-process","type":"nucleosynthesis_process","name":"The Triple-Alpha Process","domain":"science","entryPath":"/stellar-astrophysics/triple-alpha-process","description":"How stars make carbon: three helium-4 nuclei (alpha particles) combine into carbon-12. It requires temperatures around a hundred million kelvin and proceeds through a finely-tuned nuclear resonance, so it only switches on in the helium-burning cores of evolved giant stars.","sources":["nasa"]},{"id":"nucleosynthesis_process:s-process","type":"nucleosynthesis_process","name":"The s-Process","domain":"science","entryPath":"/stellar-astrophysics/s-process","description":"The slow capture of neutrons that builds about half the elements heavier than iron, up to lead and bismuth. Neutrons are added one at a time, slowly enough that unstable nuclei usually decay before catching the next — a process that unfolds over thousands of years in the interiors of asymptotic-giant-branch stars.","aliases":["Slow neutron capture"],"sources":["nasa"]},{"id":"nucleosynthesis_process:r-process","type":"nucleosynthesis_process","name":"The r-Process","domain":"science","entryPath":"/stellar-astrophysics/r-process","description":"The rapid capture of neutrons that forges the heaviest elements — gold, platinum, the lanthanides, and uranium. It demands an intense flood of neutrons in a fraction of a second, conditions found when two neutron stars merge, an origin confirmed by the kilonova that followed the 2017 gravitational-wave event GW170817.","aliases":["Rapid neutron capture"],"sources":["nasa"]},{"id":"nucleosynthesis_process:advanced-burning-stages","type":"nucleosynthesis_process","name":"Advanced Burning Stages","domain":"science","entryPath":"/stellar-astrophysics/advanced-burning-stages","description":"In the final phase of a massive star, the core burns successively heavier fuels — carbon, neon, oxygen, and silicon — each stage faster than the last, building an onion-like structure of shells. Silicon burning yields iron, which cannot release energy by fusing, ending the sequence and setting the stage for core collapse.","aliases":["Carbon-to-silicon burning"],"sources":["nasa"]},{"id":"stellar_physics_concept:hertzsprung-russell-diagram","type":"stellar_physics_concept","name":"The Hertzsprung–Russell Diagram","domain":"science","entryPath":"/stellar-astrophysics/hertzsprung-russell-diagram","description":"The single most important diagram in stellar astrophysics: a plot of stars' luminosities against their surface temperatures. Stars are not scattered at random but fall into distinct regions — the diagonal main sequence, the giant and supergiant branches, and the faint white-dwarf sequence — that trace the arc of stellar evolution.","aliases":["HR diagram","Colour–magnitude diagram"],"sources":["eso"]},{"id":"stellar_physics_concept:stellar-structure","type":"stellar_physics_concept","name":"Stellar Structure","domain":"science","entryPath":"/stellar-astrophysics/stellar-structure","description":"A star is a self-regulating sphere of plasma in which the inward pull of gravity is balanced at every depth by the outward push of pressure — hydrostatic equilibrium. Energy generated by fusion in the core is carried outward by radiation and by convection, and a handful of coupled equations capture the whole structure.","sources":["eso"]},{"id":"stellar_physics_concept:electron-degeneracy-pressure","type":"stellar_physics_concept","name":"Electron Degeneracy Pressure","domain":"science","entryPath":"/stellar-astrophysics/electron-degeneracy-pressure","description":"A quantum-mechanical pressure that arises because electrons, by the Pauli exclusion principle, resist being packed too closely — independent of temperature. It supports white dwarfs against gravity, but only up to the Chandrasekhar limit of about 1.4 solar masses, beyond which even degeneracy fails and the star collapses further.","sources":["eso"]},{"id":"stellar_physics_concept:initial-mass-function","type":"stellar_physics_concept","name":"The Initial Mass Function","domain":"science","entryPath":"/stellar-astrophysics/initial-mass-function","description":"The distribution of masses with which stars are born. Nature makes far more low-mass stars than high-mass ones — a steep decline first quantified by Salpeter — so faint red dwarfs vastly outnumber brilliant massive stars. The initial mass function shapes how galaxies light up, enrich, and evolve.","aliases":["IMF"],"sources":["eso"]},{"id":"stellar_physics_concept:stellar-metallicity","type":"stellar_physics_concept","name":"Stellar Metallicity","domain":"science","entryPath":"/stellar-astrophysics/stellar-metallicity","description":"To an astronomer, every element heavier than helium is a \"metal.\" A star's metallicity records the enrichment of the gas from which it formed, since the Big Bang made essentially only hydrogen and helium and successive generations of stars forged the rest. It is usually expressed as [Fe/H], the iron-to-hydrogen ratio relative to the Sun.","sources":["eso"]},{"id":"stellar_physics_concept:stellar-populations-and-clusters","type":"stellar_physics_concept","name":"Stellar Populations & Clusters","domain":"science","entryPath":"/stellar-astrophysics/stellar-populations-and-clusters","description":"Stars fall into broad populations: metal-rich Population I stars in the disc, like the Sun; old, metal-poor Population II stars in the halo and globular clusters; and a hypothesised first generation of metal-free Population III stars, not yet directly observed. Star clusters — young open clusters and ancient globulars — are coeval populations that serve as the great testing grounds of stellar-evolution theory.","sources":["eso"]},{"id":"stellar_physics_concept:luminosity-classification","type":"stellar_physics_concept","name":"Luminosity Classification","domain":"science","entryPath":"/stellar-astrophysics/luminosity-classification","description":"A star's spectrum reveals not only its temperature but its size. The Yerkes system adds a luminosity class — from I for supergiants down through III for giants, V for main-sequence dwarfs, to VII for white dwarfs — to the Harvard spectral type. Together they place a star precisely: the Sun, for instance, is a G2V dwarf.","aliases":["Yerkes classes","MK luminosity class"],"sources":["eso"]},{"id":"stellar_physics_concept:binary-star-systems","type":"stellar_physics_concept","name":"Binary Star Systems","domain":"science","entryPath":"/stellar-astrophysics/binary-star-systems","description":"Most stars are not alone. Pairs bound by gravity — seen as visual, spectroscopic, or eclipsing binaries — let astronomers weigh stars directly from their orbits. When the stars are close enough, one can spill matter across its Roche lobe onto the other, driving novae, X-ray binaries, and the Type Ia supernovae that light up the distant universe.","sources":["eso"]},{"id":"galactic_structure:galactic-thin-disk","type":"galactic_structure","name":"The Thin Disk","domain":"science","entryPath":"/galactic-astronomy/galactic-thin-disk","description":"The flattened, rotating layer that holds most of the Milky Way's stars, gas, and dust, and where stars are still being born today. Only a few hundred parsecs thick but tens of thousands across, it contains the spiral arms and the young, metal-rich stars of the Galactic disc — the Sun among them.","sources":["nasa"]},{"id":"galactic_structure:galactic-thick-disk","type":"galactic_structure","name":"The Thick Disk","domain":"science","entryPath":"/galactic-astronomy/galactic-thick-disk","description":"A more extended, puffed-up disc of older, more metal-poor stars that envelops the thin disk. Its stars move on hotter orbits and formed early in the Galaxy's history, making the thick disk a fossil record of a more turbulent youth — perhaps heated by an ancient merger.","sources":["nasa"]},{"id":"galactic_structure:galactic-bulge","type":"galactic_structure","name":"The Galactic Bulge","domain":"science","entryPath":"/galactic-astronomy/galactic-bulge","description":"The dense, roughly spheroidal concentration of mostly old stars at the heart of the Milky Way. Boxy and peanut-shaped when seen edge-on, the bulge is intimately tied to the central bar and holds clues to how the inner Galaxy assembled.","sources":["nasa"]},{"id":"galactic_structure:galactic-bar","type":"galactic_structure","name":"The Galactic Bar","domain":"science","entryPath":"/galactic-astronomy/galactic-bar","description":"An elongated bar of stars spanning the central few kiloparsecs, which makes the Milky Way a barred spiral galaxy. The bar funnels gas inward, drives the boxy bulge, and sets up resonances that shape the orbits of disc stars far from the centre.","sources":["nasa"]},{"id":"galactic_structure:stellar-halo","type":"galactic_structure","name":"The Stellar Halo","domain":"science","entryPath":"/galactic-astronomy/stellar-halo","description":"A vast, sparse, roughly spherical cloud of the Galaxy's oldest and most metal-poor stars, together with its globular clusters, reaching far beyond the disc. Built largely from the shredded remains of smaller galaxies, the stellar halo is the Milky Way's deep archaeological archive.","sources":["nasa"]},{"id":"galactic_structure:spiral-arms","type":"galactic_structure","name":"The Spiral Arms","domain":"science","entryPath":"/galactic-astronomy/spiral-arms","description":"The bright lanes that wind through the disc, marked out by gas, dust, and freshly-formed luminous stars. The arms are thought to be density waves — regions where orbits crowd together and trigger star formation — rather than fixed structures, so stars drift in and out of them over time.","sources":["nasa"]},{"id":"galactic_structure:galactic-warp","type":"galactic_structure","name":"The Galactic Warp","domain":"science","entryPath":"/galactic-astronomy/galactic-warp","description":"The outer disc of the Milky Way is not flat but bent, curving up on one side and down on the other like a vinyl record left in the sun. This warp, traced by gas and by young stars, is likely stirred by the gravitational tug of the Magellanic Clouds and the dark-matter halo.","sources":["nasa"]},{"id":"galactic_structure:galactic-center","type":"galactic_structure","name":"The Galactic Centre","domain":"science","entryPath":"/galactic-astronomy/galactic-center","description":"The crowded, dust-shrouded core of the Milky Way, about 26,000 light-years away, home to a dense star cluster and the four-million-solar-mass black hole Sagittarius A*. Hidden at optical wavelengths, it is studied in radio, infrared, and X-rays, and its stars' orbits weigh the central black hole directly.","sources":["nasa"]},{"id":"galactic_structure:central-molecular-zone","type":"galactic_structure","name":"The Central Molecular Zone","domain":"science","entryPath":"/galactic-astronomy/central-molecular-zone","description":"The reservoir of dense molecular gas within a few hundred parsecs of the Galactic Centre — a fraction of the Galaxy's volume that holds a large share of its molecular material. Turbulent, magnetised, and forming stars under extreme conditions, it is a nearby laboratory for the hearts of other galaxies.","sources":["nasa"]},{"id":"galactic_structure:galactic-corona","type":"galactic_structure","name":"The Galactic Corona","domain":"science","entryPath":"/galactic-astronomy/galactic-corona","description":"An enormous halo of tenuous, million-degree gas that surrounds the Milky Way, detectable in X-rays and in absorption against distant sources. This hot corona is a reservoir of baryons and the medium through which fresh gas accretes onto the Galaxy and enriched gas is expelled.","aliases":["Hot gaseous halo","Circumgalactic medium"],"sources":["nasa"]},{"id":"galactic_structure:the-solar-neighbourhood","type":"galactic_structure","name":"The Solar Neighbourhood","domain":"science","entryPath":"/galactic-astronomy/the-solar-neighbourhood","description":"The Sun's local patch of the Galaxy — the stars, gas, and structure within a few hundred light-years. It includes the Local Bubble, a cavity of hot, thin gas blown by ancient supernovae, and it is the vantage point from which we map the entire Milky Way, orbiting the Galactic Centre once every roughly 230 million years.","sources":["nasa"]},{"id":"galactic_dynamics:galactic-rotation","type":"galactic_dynamics","name":"Galactic Rotation","domain":"science","entryPath":"/galactic-astronomy/galactic-rotation","description":"The Milky Way's disc does not turn as a solid body: inner and outer stars complete their orbits at different rates. Yet the orbital speed stays surprisingly flat far from the centre instead of falling off, one of the clearest signs that the visible Galaxy is embedded in a massive halo of unseen dark matter.","aliases":["The rotation curve"],"sources":["eso"]},{"id":"galactic_dynamics:stellar-streams","type":"galactic_dynamics","name":"Stellar Streams","domain":"science","entryPath":"/galactic-astronomy/stellar-streams","description":"Ribbons of stars strung out across the halo, torn from dwarf galaxies and globular clusters as the Milky Way's tides pull them apart. The great Sagittarius stream wraps entirely around the Galaxy; mapped in their dozens by Gaia, these streams trace the shape of the dark-matter halo and record the Galaxy's past meals.","aliases":["Tidal streams"],"sources":["eso"]},{"id":"galactic_dynamics:galactic-archaeology","type":"galactic_dynamics","name":"Galactic Archaeology","domain":"science","entryPath":"/galactic-astronomy/galactic-archaeology","description":"The reconstruction of how the Milky Way formed by reading the ages, chemistry, and motions of its stars, which preserve the imprint of their birth. Gaia's precise positions and velocities for over a billion stars have turned this into a precision science, revealing ancient mergers frozen into the halo.","sources":["eso"]},{"id":"galactic_dynamics:stellar-migration","type":"galactic_dynamics","name":"Radial Migration","domain":"science","entryPath":"/galactic-astronomy/stellar-migration","description":"Stars do not stay at the galactocentric radius where they were born. Resonances with the spiral arms and the bar can shuffle a star inward or outward across the disc without heating its orbit, mixing the disc's chemistry over billions of years and complicating any attempt to read history from composition alone.","sources":["eso"]},{"id":"galactic_dynamics:galactic-magnetic-field","type":"galactic_dynamics","name":"The Galactic Magnetic Field","domain":"science","entryPath":"/galactic-astronomy/galactic-magnetic-field","description":"A large-scale magnetic field of a few microgauss threads the Milky Way, ordered along the spiral arms and tangled on smaller scales. Weak though it is, it guides cosmic rays, shapes the interstellar medium, and helps regulate star formation; it is traced through synchrotron radiation, Faraday rotation, and polarised starlight and dust.","sources":["eso"]},{"id":"galactic_dynamics:the-galactic-habitable-zone","type":"galactic_dynamics","name":"The Galactic Habitable Zone","domain":"science","entryPath":"/galactic-astronomy/the-galactic-habitable-zone","description":"A proposed — and much-debated — region of the Galaxy thought to be most favourable to complex life: far enough from the crowded, radiation-soaked centre yet metal-rich enough to build planets. Whether such a zone is truly well-defined remains an open question, and it is offered as a hypothesis rather than an established boundary.","sources":["eso"]},{"id":"galactic_dynamics:satellite-galaxies-and-accretion","type":"galactic_dynamics","name":"Satellite Galaxies & Accretion","domain":"science","entryPath":"/galactic-astronomy/satellite-galaxies-and-accretion","description":"The Milky Way is orbited by dozens of smaller galaxies, the brightest being the Large and Small Magellanic Clouds. In the hierarchical picture of galaxy formation, big galaxies grow by swallowing small ones, and the Milky Way is still feeding — its halo and streams are the debris of satellites consumed long ago.","sources":["eso"]},{"id":"galactic_dynamics:the-milky-way-andromeda-collision","type":"galactic_dynamics","name":"The Milky Way–Andromeda Collision","domain":"science","entryPath":"/galactic-astronomy/the-milky-way-andromeda-collision","description":"The Milky Way and the Andromeda Galaxy are approaching each other and are predicted to merge into a single elliptical galaxy in roughly four to five billion years, though the exact timing and geometry remain uncertain. Stars will almost never collide, but both discs will be transformed as the two giants of the Local Group become one.","aliases":["Milkomeda"],"sources":["eso"]},{"id":"galactic_dynamics:galactic-fountain","type":"galactic_dynamics","name":"The Galactic Fountain","domain":"science","entryPath":"/galactic-astronomy/galactic-fountain","description":"Star formation and supernovae blow hot gas out of the disc, which cools, condenses, and rains back down as clouds — a continual circulation between the disc and the halo. This galactic fountain recycles and mixes gas, and helps deliver the fresh material that keeps the Milky Way forming stars.","sources":["eso"]},{"id":"research_software:scientific-python-ecosystem","type":"research_software","name":"The Scientific Python Ecosystem","domain":"science","entryPath":"/astroinformatics/scientific-python-ecosystem","description":"The open-source foundation of modern astronomical computing: the Python language together with NumPy for array mathematics, SciPy for scientific algorithms, and pandas for tabular data. Free and community-built, it has become the common language in which most astronomical analysis is now written.","aliases":["NumPy","SciPy"],"sources":["stsci"]},{"id":"research_software:astropy","type":"research_software","name":"Astropy","domain":"science","entryPath":"/astroinformatics/astropy","description":"The community-developed core package for astronomy in Python, providing the shared building blocks the field relies on: physical units and constants, celestial coordinate transformations, time scales, cosmological calculations, and reading and writing of FITS and other data formats. A large ecosystem of affiliated packages builds on its foundation.","sources":["stsci"]},{"id":"research_software:sunpy","type":"research_software","name":"SunPy","domain":"science","entryPath":"/astroinformatics/sunpy","description":"The community package for solar physics in Python, the solar counterpart to Astropy. It provides the data structures, coordinate frames, and access to solar observatory archives that let researchers analyse images and time series of the Sun within the same open scientific-Python ecosystem.","sources":["stsci"]},{"id":"research_software:jupyter-notebooks","type":"research_software","name":"Jupyter Notebooks","domain":"science","entryPath":"/astroinformatics/jupyter-notebooks","description":"Interactive documents that weave together live code, results, plots, and narrative text in one place. Notebooks have become the default medium for exploratory analysis, teaching, and sharing reproducible research in astronomy, and they sit at the heart of the cloud-based science platforms now serving the largest surveys.","aliases":["Jupyter"],"sources":["stsci"]},{"id":"research_software:astroquery","type":"research_software","name":"Astroquery","domain":"science","entryPath":"/astroinformatics/astroquery","description":"An Astropy-affiliated package that lets researchers query the major astronomical archives and databases directly from code. Instead of clicking through web forms, a scientist can pull catalogues and images from MAST, VizieR, SIMBAD, and dozens of other services programmatically, making analyses scriptable and repeatable.","sources":["stsci"]},{"id":"research_software:scientific-visualization","type":"research_software","name":"Scientific Visualization","domain":"science","entryPath":"/astroinformatics/scientific-visualization","description":"The tools and craft of turning data into images that reveal structure — from the ubiquitous Matplotlib plots to interactive and three-dimensional renderings of simulations and surveys. Visualisation is both how astronomers explore their data and how they communicate discoveries.","aliases":["Matplotlib"],"sources":["stsci"]},{"id":"research_computing:high-performance-computing","type":"research_computing","name":"High-Performance Computing","domain":"science","entryPath":"/astroinformatics/high-performance-computing","description":"The supercomputers on which astronomers run the largest cosmological simulations and process survey data at scale. By dividing a problem across thousands of tightly-coupled processors, high-performance computing makes it possible to model the growth of cosmic structure or the collision of neutron stars from first principles.","aliases":["HPC","Supercomputing"],"sources":["nasa"]},{"id":"research_computing:gpu-computing","type":"research_computing","name":"GPU Computing","domain":"science","entryPath":"/astroinformatics/gpu-computing","description":"Graphics processing units, originally built for rendering, excel at the massively parallel arithmetic that powers modern simulation and machine learning. Astronomy uses them to accelerate everything from N-body dynamics and radiative transfer to the training of the large neural networks now applied to survey data.","aliases":["Accelerated computing"],"sources":["nasa"]},{"id":"research_computing:cloud-computing","type":"research_computing","name":"Cloud Computing","domain":"science","entryPath":"/astroinformatics/cloud-computing","description":"Elastic, on-demand computing rented from remote data centres. Rather than moving petabytes of survey data to a researcher's own machine, cloud computing lets the analysis run next to the data, a shift that underpins the science platforms being built for the next generation of surveys.","sources":["nasa"]},{"id":"research_computing:distributed-computing","type":"research_computing","name":"Distributed Computing","domain":"science","entryPath":"/astroinformatics/distributed-computing","description":"Spreading a computation across many loosely-coupled machines so that datasets far too large for one computer can be processed in parallel. Frameworks for distributed data processing let astronomers cross-match billion-row catalogues and reduce survey images across clusters of ordinary servers.","aliases":["Parallel data processing"],"sources":["nasa"]},{"id":"research_computing:science-platforms","type":"research_computing","name":"Science Platforms","domain":"science","entryPath":"/astroinformatics/science-platforms","description":"Integrated, cloud-based environments that bring the analysis tools to the data. Platforms such as the Rubin Science Platform give researchers notebooks, catalogue databases, and image access alongside a survey's archive, so that discovery no longer requires downloading the data at all.","aliases":["Rubin Science Platform"],"sources":["nasa"]},{"id":"research_computing:containerisation","type":"research_computing","name":"Containerisation & Reproducible Environments","domain":"science","entryPath":"/astroinformatics/containerisation","description":"Packaging software together with its exact dependencies into a portable container, so that an analysis runs identically on a laptop, a supercomputer, or the cloud. Containers have become a cornerstone of reproducible research, freezing the computational environment in which a result was produced.","aliases":["Docker","Singularity"],"sources":["nasa"]},{"id":"astroinformatics_concept:scientific-workflows","type":"astroinformatics_concept","name":"Scientific Workflows","domain":"science","entryPath":"/astroinformatics/scientific-workflows","description":"The orchestration of a multi-step analysis — each stage's inputs, outputs, and dependencies made explicit — so that a whole computation can be re-run automatically and at scale. Workflow systems turn a tangle of scripts into a repeatable pipeline, the backbone of processing survey data through many stages.","aliases":["Workflow management"],"sources":["noirlab"]},{"id":"astroinformatics_concept:data-provenance","type":"astroinformatics_concept","name":"Data Provenance","domain":"science","entryPath":"/astroinformatics/data-provenance","description":"The recorded lineage of a data product: which raw observations, software versions, and processing steps produced it. Provenance lets a result be traced back to its origins and trusted or reproduced — distinct from a persistent identifier, which names the product, provenance describes how it came to be.","sources":["noirlab"]},{"id":"astroinformatics_concept:astronomical-query-languages","type":"astroinformatics_concept","name":"Astronomical Query Languages","domain":"science","entryPath":"/astroinformatics/astronomical-query-languages","description":"The Astronomical Data Query Language, a dialect of SQL extended with the geometry of the sky, lets astronomers ask precise questions of enormous catalogues — every source within a region, or every object matching a set of criteria. It is the language that the Virtual Observatory's Table Access Protocol serves.","aliases":["ADQL"],"sources":["noirlab"]},{"id":"astroinformatics_concept:big-data-astronomy","type":"astroinformatics_concept","name":"Big-Data Astronomy","domain":"science","entryPath":"/astroinformatics/big-data-astronomy","description":"Modern surveys have turned astronomy into a data-intensive science. Gaia charts over a billion stars, the Rubin Observatory's LSST will image the whole southern sky every few nights, and the Square Kilometre Array will generate data faster than any prior instrument — forcing new ways to store, move, and analyse information at petabyte scale.","aliases":["The data deluge"],"sources":["noirlab"]},{"id":"astroinformatics_concept:the-virtual-research-environment","type":"astroinformatics_concept","name":"The Virtual Research Environment","domain":"science","entryPath":"/astroinformatics/the-virtual-research-environment","description":"The vision of an integrated, online ecosystem where data, software, and computing come together — the Virtual Observatory's interoperable archives joined to cloud science platforms and shared notebooks. In such an environment a researcher can find, access, and analyse data from many facilities without ever leaving the browser.","aliases":["VRE"],"sources":["noirlab"]},{"id":"astroinformatics_concept:research-software-engineering","type":"astroinformatics_concept","name":"Research Software Engineering","domain":"science","entryPath":"/astroinformatics/research-software-engineering","description":"The recognition that scientific software deserves the same care as any other research output: version control, testing, documentation, code review, and open licensing. As astronomy has grown more computational, sustaining and citing the software behind results has become a discipline in its own right.","sources":["stsci"]},{"id":"exploration_architecture:moon-to-mars-architecture","type":"exploration_architecture","name":"The Moon-to-Mars Architecture","domain":"science","entryPath":"/deep-space-exploration/moon-to-mars-architecture","description":"The strategy of returning to the Moon first, and using it as a proving ground for the systems and skills needed to send crews to Mars. Under this integrated approach the Artemis missions and the Lunar Gateway are steps toward a longer campaign, testing habitats, life support, and surface operations close to home before the far harder journey to Mars.","sources":["nasa"]},{"id":"exploration_architecture:the-mars-surface-base","type":"exploration_architecture","name":"The Mars Surface Base","domain":"science","entryPath":"/deep-space-exploration/the-mars-surface-base","description":"A crewed outpost on Mars, the long-term goal of human deep-space exploration. Separated from Earth by months of travel and up to twenty minutes of communication delay, a Mars base must make its own propellant, water, and oxygen from local resources and sustain its crew with little hope of rescue.","sources":["nasa"]},{"id":"exploration_architecture:the-deep-space-transit-habitat","type":"exploration_architecture","name":"The Deep-Space Transit Habitat","domain":"science","entryPath":"/deep-space-exploration/the-deep-space-transit-habitat","description":"The spacecraft in which a crew lives during the months-long cruise between worlds. Cut off from resupply and beyond the protection of Earth's magnetic field, a transit habitat must recycle nearly all its air and water, shield its crew from radiation, and keep them healthy and sane across interplanetary distances.","sources":["nasa"]},{"id":"exploration_architecture:surface-power-systems","type":"exploration_architecture","name":"Surface Power Systems","domain":"science","entryPath":"/deep-space-exploration/surface-power-systems","description":"The electricity that keeps a surface base alive — running life support, recharging rovers, and driving the machines that extract local resources. Solar arrays serve where the Sun shines, but through the long lunar night and the dust of a Martian winter a compact fission reactor offers steady power independent of sunlight.","sources":["nasa"]},{"id":"exploration_architecture:planetary-surface-mobility","type":"exploration_architecture","name":"Planetary Surface Mobility","domain":"science","entryPath":"/deep-space-exploration/planetary-surface-mobility","description":"How crews range across a world beyond the walking distance of their habitat — from unpressurised buggies for short trips to pressurised rovers that serve as mobile homes for days-long expeditions. Mobility multiplies the science a surface mission can do, turning a single landing site into a region to explore.","aliases":["Pressurised rovers"],"sources":["nasa"]},{"id":"exploration_architecture:space-construction-for-habitats","type":"exploration_architecture","name":"Space Construction for Habitats","domain":"science","entryPath":"/deep-space-exploration/space-construction-for-habitats","description":"Building shelter on another world rather than carrying it there. Concepts range from covering habitats with bagged regolith for radiation shielding to three-dimensional printing of structures from local soil, so that the mass launched from Earth shrinks and the base can grow using what is already on the ground.","sources":["nasa"]},{"id":"exploration_architecture:crewed-deep-space-propulsion","type":"exploration_architecture","name":"Crewed Deep-Space Propulsion","domain":"science","entryPath":"/deep-space-exploration/crewed-deep-space-propulsion","description":"Getting a crew to Mars quickly enough to limit their exposure to weightlessness and radiation. Chemical rockets are proven but heavy on propellant; nuclear-thermal and nuclear-electric propulsion promise shorter transits, while solar-electric tugs can pre-position cargo ahead of the crew.","sources":["nasa"]},{"id":"exploration_architecture:mars-entry-descent-and-landing","type":"exploration_architecture","name":"Mars Entry, Descent & Landing","domain":"science","entryPath":"/deep-space-exploration/mars-entry-descent-and-landing","description":"The problem of setting a heavy crewed vehicle down safely on Mars. The atmosphere is thick enough to fiercely heat an incoming craft yet too thin to slow a massive lander by parachute alone, so landing humans will demand a combination of heat shields, retropropulsion, and technologies well beyond those that delivered the robotic rovers.","aliases":["Mars EDL"],"sources":["nasa"]},{"id":"deep_space_challenge:the-deep-space-radiation-challenge","type":"deep_space_challenge","name":"The Deep-Space Radiation Challenge","domain":"science","entryPath":"/deep-space-exploration/the-deep-space-radiation-challenge","description":"Beyond the shelter of Earth's magnetic field, crews are exposed to a steady sleet of galactic cosmic rays and the sudden violence of solar particle events. This radiation raises long-term cancer risk and can damage the nervous system, and shielding against the most energetic particles is one of the hardest unsolved problems of sending humans to Mars.","sources":["nasa"]},{"id":"deep_space_challenge:the-communication-time-delay","type":"deep_space_challenge","name":"The Communication Time Delay","domain":"science","entryPath":"/deep-space-exploration/the-communication-time-delay","description":"Radio signals travel at the speed of light, but the distances are vast: a message to a crew at Mars can take as much as about twenty minutes each way, so a real-time conversation with Earth is impossible. The delay forces crews to handle emergencies themselves and reshapes how missions far from home are commanded and supported.","sources":["nasa"]},{"id":"deep_space_challenge:earth-independence-and-crew-autonomy","type":"deep_space_challenge","name":"Earth Independence & Crew Autonomy","domain":"science","entryPath":"/deep-space-exploration/earth-independence-and-crew-autonomy","description":"Close to Earth, mission control and a waiting ambulance are never far away; at Mars, a crew is largely on its own. Deep-space missions must be able to diagnose and treat illness, repair their own systems, and make decisions without waiting for Earth — a shift from ground-controlled operations toward genuine self-sufficiency.","sources":["nasa"]},{"id":"deep_space_challenge:long-duration-life-support","type":"deep_space_challenge","name":"Long-Duration Life Support","domain":"science","entryPath":"/deep-space-exploration/long-duration-life-support","description":"On the Space Station, water and air can be topped up from Earth; on a multi-year voyage to Mars there is no resupply. Life support must therefore recycle almost everything — reclaiming water from every source and regenerating oxygen — and may ultimately grow food, closing the loop far more tightly than any system flown so far.","sources":["nasa"]},{"id":"deep_space_challenge:behavioral-health-and-crew-cohesion","type":"deep_space_challenge","name":"Behavioural Health & Crew Cohesion","domain":"science","entryPath":"/deep-space-exploration/behavioral-health-and-crew-cohesion","description":"A small crew confined together for years, far from family and the ordinary world, faces real psychological strain — isolation, monotony, and the friction of close quarters. Keeping a team healthy, motivated, and working well together is as vital to a Mars mission as any piece of hardware, and far less forgiving of failure.","sources":["nasa"]},{"id":"deep_space_challenge:planetary-protection-for-crewed-missions","type":"deep_space_challenge","name":"Planetary Protection for Crewed Missions","domain":"science","entryPath":"/deep-space-exploration/planetary-protection-for-crewed-missions","description":"A human crew cannot be sterilised the way a robotic lander can, so people inevitably carry microbes with them. Protecting Mars from Earthly contamination — which could confuse the search for native life — while also guarding the crew against any possible Martian biology is a difficult balance unique to sending humans to another world.","sources":["nasa"]},{"id":"deep_space_challenge:the-planetary-dust-challenge","type":"deep_space_challenge","name":"The Planetary Dust Challenge","domain":"science","entryPath":"/deep-space-exploration/the-planetary-dust-challenge","description":"The dust of the Moon and Mars is not the smooth sand of Earth but sharp, clinging, and chemically reactive. Lunar dust abraded the Apollo astronauts' suits and equipment and irritated their lungs, and Martian soil holds toxic perchlorates — so managing dust is essential to keeping crews, seals, and machinery working on any planetary surface.","sources":["nasa"]},{"id":"atlas_view:all-sky-star-atlas","type":"atlas_view","name":"All-Sky Star Atlas","domain":"science","entryPath":"/sky-atlas/all-sky-star-atlas","description":"A whole-sky chart plotting every catalogued star at its real right ascension and declination, sized by apparent magnitude. Rendered as scalable vector graphics directly from the star catalogue's measured coordinates — nothing is invented; a star appears only where the data places it.","sources":["hyg"]},{"id":"atlas_view:constellation-atlas","type":"atlas_view","name":"Constellation Atlas","domain":"science","entryPath":"/sky-atlas/constellation-atlas","description":"The eighty-eight official constellations, each mapped by the real positions of its brightest stars. A gateway from the familiar patterns of the night sky into the stars, myths, and deep-sky objects each region holds.","sources":["iau"]},{"id":"atlas_view:messier-atlas","type":"atlas_view","name":"Messier Atlas","domain":"science","entryPath":"/sky-atlas/messier-atlas","description":"A chart of the Messier objects — the nebulae, clusters, and galaxies of Charles Messier's eighteenth-century catalogue — each placed at its real celestial coordinates and sized by its apparent extent. The classic target list for a first tour of the deep sky.","sources":["openngc"]},{"id":"atlas_view:deep-sky-atlas","type":"atlas_view","name":"Deep-Sky Atlas","domain":"science","entryPath":"/sky-atlas/deep-sky-atlas","description":"A map of the catalogued deep-sky objects — galaxies, nebulae, and star clusters — drawn from their measured right ascension and declination, with symbols scaled by angular size. The wider sky beyond the naked-eye stars.","sources":["openngc"]},{"id":"atlas_view:bright-star-map","type":"atlas_view","name":"Bright Star Map","domain":"science","entryPath":"/sky-atlas/bright-star-map","description":"A naked-eye view of the sky showing only the brightest stars, ranked by apparent magnitude. The stars that anchor the constellations and guide the eye across the night.","sources":["hyg"]},{"id":"atlas_view:solar-system-explorer","type":"atlas_view","name":"Solar System Explorer","domain":"science","entryPath":"/sky-atlas/solar-system-explorer","description":"An explorer of the Sun's family — the planets, their moons, and the small bodies between them. The data model carries each body's real orbital and physical parameters and is prepared for a future interactive three-dimensional scene; today it presents the ordered, to-scale structure of the system.","sources":["nasa"]},{"id":"atlas_view:milky-way-explorer","type":"atlas_view","name":"Milky Way Explorer","domain":"science","entryPath":"/sky-atlas/milky-way-explorer","description":"An explorer of the structure of our own Galaxy — its discs, bulge, bar, spiral arms, and halo, and the Sun's place within them. Prepared for a three-dimensional rendering of galactic structure; today it maps the anatomy of the Milky Way onto its components.","sources":["nasa"]},{"id":"atlas_view:local-group-explorer","type":"atlas_view","name":"Local Group Explorer","domain":"science","entryPath":"/sky-atlas/local-group-explorer","description":"An explorer of our galactic neighbourhood — the Milky Way, Andromeda, Triangulum, the Magellanic Clouds, and the dozens of dwarf galaxies bound with them into the Local Group. Prepared for a three-dimensional map of the nearby universe.","sources":["nasa"]},{"id":"atlas_view:galaxy-atlas","type":"atlas_view","name":"Galaxy Atlas","domain":"science","entryPath":"/sky-atlas/galaxy-atlas","description":"A browsable index of catalogued galaxies — spirals, ellipticals, and irregulars — organised by morphology and distance. The building blocks of cosmic structure, each linked to its place in the knowledge graph.","sources":["nasa"]},{"id":"atlas_view:planet-explorer","type":"atlas_view","name":"Planet Explorer","domain":"science","entryPath":"/sky-atlas/planet-explorer","description":"An explorer of the planets — their sizes, orbits, atmospheres, and moons, drawn from measured planetary data. From Mercury's scorched rock to the ice giants of the outer system.","sources":["nasa"]},{"id":"atlas_view:moon-explorer","type":"atlas_view","name":"Moon Explorer","domain":"science","entryPath":"/sky-atlas/moon-explorer","description":"An explorer of the moons of the Solar System — from Earth's Moon to the ocean worlds of Jupiter and Saturn — organised by their host planet and physical character.","sources":["nasa"]},{"id":"atlas_view:exoplanet-explorer","type":"atlas_view","name":"Exoplanet Explorer","domain":"science","entryPath":"/sky-atlas/exoplanet-explorer","description":"An explorer of the confirmed planets beyond the Solar System, drawn from the measured exoplanet catalogue — organised by host star, detection method, size, and orbit. The worlds of other suns.","sources":["nasa"]},{"id":"atlas_view:ngc-explorer","type":"atlas_view","name":"NGC Explorer","domain":"science","entryPath":"/sky-atlas/ngc-explorer","description":"An explorer of the New General Catalogue and its deep-sky objects, organised by type, constellation, and catalogue. The deep sky beyond the Messier list.","sources":["openngc"]},{"id":"atlas_view:distance-scale-explorer","type":"atlas_view","name":"Distance & Scale Explorer","domain":"science","entryPath":"/sky-atlas/distance-scale-explorer","description":"An explorer of cosmic distance and scale — from the nearest stars to the edge of the observable universe — built on the rungs of the cosmic distance ladder. Prepared to visualise the vast, logarithmic reach of the cosmos honestly, with distances drawn only from measured indicators.","sources":["nasa"]},{"id":"atlas_overlay:constellation-lines-overlay","type":"atlas_overlay","name":"Constellation Lines Overlay","domain":"science","entryPath":"/sky-atlas/constellation-lines-overlay","description":"The familiar stick-figure lines that join a constellation's stars, drawn between the real stellar positions to make the ancient patterns legible on the star map.","sources":["iau"]},{"id":"atlas_overlay:observation-conditions-overlay","type":"atlas_overlay","name":"Observation Conditions Overlay","domain":"science","entryPath":"/sky-atlas/observation-conditions-overlay","description":"A layer showing which part of the sky is above the horizon for an observer at a given place and time. Computed from the observer's location and the clock — no observing conditions are assumed or invented, and location stays on the device.","sources":["nasa"]},{"id":"atlas_overlay:jwst-target-overlay","type":"atlas_overlay","name":"JWST Target Overlay","domain":"science","entryPath":"/sky-atlas/jwst-target-overlay","description":"A layer marking the positions of objects observed by the James Webb Space Telescope, linking each region of the deep-sky map to the science it has enabled.","sources":["nasa"]},{"id":"atlas_overlay:hubble-target-overlay","type":"atlas_overlay","name":"Hubble Target Overlay","domain":"science","entryPath":"/sky-atlas/hubble-target-overlay","description":"A layer marking the positions of famous Hubble Space Telescope targets across the deep-sky map, from the Deep Fields to the great nebulae.","sources":["nasa"]},{"id":"atlas_overlay:gaia-survey-overlay","type":"atlas_overlay","name":"Gaia Survey Overlay","domain":"science","entryPath":"/sky-atlas/gaia-survey-overlay","description":"A layer representing the all-sky astrometric coverage of the Gaia mission, whose measured positions and parallaxes underpin the modern star catalogue that the atlas draws.","sources":["gaia"]},{"id":"atlas_overlay:telescope-fov-overlay","type":"atlas_overlay","name":"Telescope Field-of-View Overlay","domain":"science","entryPath":"/sky-atlas/telescope-fov-overlay","description":"A layer showing the angular field of view of a chosen telescope or instrument against the sky, so a target's real angular size can be compared with what an instrument can frame in a single pointing.","sources":["nasa"]},{"id":"scientific_calculator:escape-velocity","type":"scientific_calculator","name":"Escape Velocity","domain":"science","entryPath":"/calculators/escape-velocity","description":"The minimum speed an object needs to break free of a body's gravity, ignoring drag. Set by the body's mass and radius alone.","sources":["nasa"]},{"id":"scientific_calculator:orbital-velocity","type":"scientific_calculator","name":"Circular Orbital Velocity","domain":"science","entryPath":"/calculators/orbital-velocity","description":"The speed of a body on a circular orbit at a given distance from a central mass. The Earth circles the Sun at about 29.8 km/s.","sources":["nasa"]},{"id":"scientific_calculator:orbital-period","type":"scientific_calculator","name":"Orbital Period (Kepler's Third Law)","domain":"science","entryPath":"/calculators/orbital-period","description":"Kepler's third law: the time to complete one orbit, from the semi-major axis and the central mass. A planet at 1 AU around the Sun takes one year.","sources":["nasa"]},{"id":"scientific_calculator:surface-gravity","type":"scientific_calculator","name":"Surface Gravity","domain":"science","entryPath":"/calculators/surface-gravity","description":"The gravitational acceleration at a body's surface, from its mass and radius. Earth's is about 9.8 m/s².","sources":["nasa"]},{"id":"scientific_calculator:schwarzschild-radius","type":"scientific_calculator","name":"Schwarzschild Radius","domain":"science","entryPath":"/calculators/schwarzschild-radius","description":"The radius of the event horizon of a non-rotating black hole of a given mass — the size to which that mass must be compressed to become one. The Sun's is just under three kilometres.","sources":["nasa"]},{"id":"scientific_calculator:body-density","type":"scientific_calculator","name":"Mean Density","domain":"science","entryPath":"/calculators/body-density","description":"The average density of a body from its mass and radius — a clue to its composition. Earth's ~5510 kg/m³ points to a rock-and-iron world; the giant planets are far less dense.","sources":["nasa"]},{"id":"scientific_calculator:hill-sphere","type":"scientific_calculator","name":"Hill Sphere Radius","domain":"science","entryPath":"/calculators/hill-sphere","description":"The radius within which a body's gravity dominates over the larger body it orbits — the region where its moons can hold. Earth's Hill sphere reaches about 1.5 million kilometres.","sources":["nasa"]},{"id":"scientific_calculator:roche-limit","type":"scientific_calculator","name":"Roche Limit (fluid)","domain":"science","entryPath":"/calculators/roche-limit","description":"The distance within which a fluid satellite held together only by gravity is pulled apart by tides. Inside the Earth–Moon fluid Roche limit — about 18,000 km — a Moon-like body could not survive.","sources":["nasa"]},{"id":"scientific_calculator:synodic-period","type":"scientific_calculator","name":"Synodic Period","domain":"science","entryPath":"/calculators/synodic-period","description":"How often two orbiting bodies return to the same relative alignment — the interval between successive oppositions, say. Earth and Mars line up about every 2.14 years.","sources":["nasa"]},{"id":"scientific_calculator:stellar-luminosity","type":"scientific_calculator","name":"Stellar Luminosity (Stefan–Boltzmann)","domain":"science","entryPath":"/calculators/stellar-luminosity","description":"A star's total power output, from its radius and surface temperature by the Stefan–Boltzmann law. Doubling the temperature raises luminosity sixteenfold.","sources":["nasa"]},{"id":"scientific_calculator:blackbody-flux","type":"scientific_calculator","name":"Blackbody Surface Flux","domain":"science","entryPath":"/calculators/blackbody-flux","description":"The power radiated per square metre by a blackbody at a given temperature. The Sun's photosphere emits about 63 megawatts per square metre.","sources":["nasa"]},{"id":"scientific_calculator:wien-peak-wavelength","type":"scientific_calculator","name":"Wien Peak Wavelength","domain":"science","entryPath":"/calculators/wien-peak-wavelength","description":"The wavelength at which a blackbody radiates most intensely, by Wien's displacement law. The Sun peaks in green light at about 502 nm; hotter stars peak bluer, cooler stars redder.","sources":["nasa"]},{"id":"scientific_calculator:mass-luminosity","type":"scientific_calculator","name":"Mass–Luminosity Relation","domain":"science","entryPath":"/calculators/mass-luminosity","description":"The steep relation between a main-sequence star's mass and its luminosity: a star twice the Sun's mass shines roughly eleven times as bright. An approximation (exponent ~3.5) valid across the middle main sequence.","sources":["nasa"]},{"id":"scientific_calculator:main-sequence-lifetime","type":"scientific_calculator","name":"Main-Sequence Lifetime","domain":"science","entryPath":"/calculators/main-sequence-lifetime","description":"Roughly how long a star burns hydrogen in its core, scaled from the Sun's ~10 billion years. Massive stars are prodigal — a two-solar-mass star lasts under two billion years — while red dwarfs last far longer than the present age of the universe.","sources":["nasa"]},{"id":"scientific_calculator:absolute-magnitude","type":"scientific_calculator","name":"Absolute Magnitude","domain":"science","entryPath":"/calculators/absolute-magnitude","description":"A star's intrinsic brightness — the apparent magnitude it would have at a standard distance of 10 parsecs. Removes distance so stars can be compared on equal footing.","sources":["nasa"]},{"id":"scientific_calculator:distance-modulus","type":"scientific_calculator","name":"Distance Modulus","domain":"science","entryPath":"/calculators/distance-modulus","description":"The difference between apparent and absolute magnitude, which encodes distance. A modulus of five corresponds to 100 parsecs; each five magnitudes multiply the distance tenfold.","sources":["nasa"]},{"id":"scientific_calculator:parallax-distance","type":"scientific_calculator","name":"Parallax Distance","domain":"science","entryPath":"/calculators/parallax-distance","description":"The most direct distance measurement: a star's distance in parsecs is the reciprocal of its annual parallax in arcseconds. A parallax of one arcsecond defines one parsec — but no star is that close.","sources":["nasa"]},{"id":"scientific_calculator:angular-diameter","type":"scientific_calculator","name":"Angular Diameter","domain":"science","entryPath":"/calculators/angular-diameter","description":"How large an object of known size appears at a given distance. The Moon and the Sun span almost exactly the same half-degree from Earth — the coincidence that makes total solar eclipses possible.","sources":["nasa"]},{"id":"scientific_calculator:angular-separation","type":"scientific_calculator","name":"Angular Separation","domain":"science","entryPath":"/calculators/angular-separation","description":"The angle on the sky between two positions given by their right ascension and declination — the great-circle distance between two points on the celestial sphere.","sources":["nasa"]},{"id":"scientific_calculator:equilibrium-temperature","type":"scientific_calculator","name":"Planet Equilibrium Temperature","domain":"science","entryPath":"/calculators/equilibrium-temperature","description":"The temperature a planet settles at from the balance of starlight absorbed and heat radiated, before any greenhouse warming. Earth's is about 255 K (−18 °C); its atmosphere lifts the surface to habitable warmth.","sources":["nasa"]},{"id":"scientific_calculator:equal-insolation-distance","type":"scientific_calculator","name":"Equal-Insolation Distance","domain":"science","entryPath":"/calculators/equal-insolation-distance","description":"The orbital distance at which a planet receives the same starlight per square metre as Earth does from the Sun — a first anchor for the habitable zone. It scales with the square root of the star's luminosity.","sources":["nasa"]},{"id":"scientific_calculator:transit-probability","type":"scientific_calculator","name":"Transit Probability","domain":"science","entryPath":"/calculators/transit-probability","description":"The geometric chance that a planet's orbit is aligned edge-on enough for it to transit its star as seen from Earth. Only about one in 215 for an Earth-like orbit — which is why transit surveys must watch so many stars at once.","sources":["nasa"]},{"id":"scientific_calculator:redshift-velocity","type":"scientific_calculator","name":"Redshift Recession Velocity","domain":"science","entryPath":"/calculators/redshift-velocity","description":"The recession velocity implied by a small cosmological redshift, v ≈ cz. This linear form holds only for low redshift; at large z the full relativistic and cosmological treatment is required and this approximation overstates the speed.","sources":["nasa"]},{"id":"scientific_calculator:hubble-distance","type":"scientific_calculator","name":"Hubble Distance","domain":"science","entryPath":"/calculators/hubble-distance","description":"The distance to a galaxy from its recession velocity and the Hubble constant, by Hubble's law. Because the measured value of H₀ is itself contested — the Hubble tension — it is left as an input rather than fixed.","sources":["nasa"]},{"id":"scientific_calculator:angular-resolution","type":"scientific_calculator","name":"Angular Resolution (Rayleigh)","domain":"science","entryPath":"/calculators/angular-resolution","description":"The finest detail a telescope can resolve, set by diffraction at its aperture — the Rayleigh criterion. Bigger apertures see finer detail; a 100 mm telescope resolves about 1.4 arcseconds in green light.","aliases":["Diffraction limit"],"sources":["nasa"]},{"id":"scientific_calculator:magnification","type":"scientific_calculator","name":"Telescope Magnification","domain":"science","entryPath":"/calculators/magnification","description":"The magnification of a telescope–eyepiece pair — the ratio of their focal lengths. Useful magnification is capped by the aperture and the atmosphere, not by the eyepiece alone.","sources":["nasa"]},{"id":"scientific_calculator:image-scale","type":"scientific_calculator","name":"Image Scale","domain":"science","entryPath":"/calculators/image-scale","description":"How much sky each camera pixel covers, from the pixel size and focal length. Matching the image scale to the seeing (roughly 1–2″ per pixel) is the key to sharp astrophotography.","sources":["nasa"]},{"id":"scientific_calculator:field-of-view","type":"scientific_calculator","name":"Field of View","domain":"science","entryPath":"/calculators/field-of-view","description":"The angular extent of sky a camera frames, from the sensor size and focal length. A shorter focal length or a larger sensor takes in more sky.","sources":["nasa"]},{"id":"scientific_calculator:limiting-magnitude","type":"scientific_calculator","name":"Limiting Magnitude","domain":"science","entryPath":"/calculators/limiting-magnitude","description":"A rule-of-thumb estimate of the faintest star an aperture can show under dark skies. Approximate — real limits depend on sky brightness, magnification, and the observer — so it is offered as a guide, not a guarantee.","sources":["nasa"]},{"id":"scientific_calculator:shot-noise-snr","type":"scientific_calculator","name":"Photon Shot-Noise SNR","domain":"science","entryPath":"/calculators/shot-noise-snr","description":"The best signal-to-noise achievable when the only noise is the Poisson statistics of the photons themselves — the shot-noise limit. To double the signal-to-noise you must collect four times as many photons.","sources":["nasa"]},{"id":"observing_planner:tonight-planner","type":"observing_planner","name":"Tonight Planner","domain":"science","entryPath":"/observing/tonight-planner","description":"What is worth observing tonight from a given place, drawn together from the platform's computed twilight, Moon, and planet positions. The plan updates with the observer's clock and location, which stay on the device.","sources":["nasa"]},{"id":"observing_planner:visibility-planner","type":"observing_planner","name":"Visibility Planner","domain":"science","entryPath":"/observing/visibility-planner","description":"When and whether a target clears the horizon and the twilight for a given night, from its coordinates and the observer's latitude. Built on the computed rise, set, and twilight times.","sources":["nasa"]},{"id":"observing_planner:target-planner","type":"observing_planner","name":"Target Planner","domain":"science","entryPath":"/observing/target-planner","description":"Builds an observing list from the graph's real objects — stars, deep-sky objects, planets — and checks each against the night's visibility. A bridge from the catalogue to the eyepiece.","sources":["nasa"]},{"id":"observing_planner:moon-planner","type":"observing_planner","name":"Moon Planner","domain":"science","entryPath":"/observing/moon-planner","description":"The Moon's phase, illumination, and rise and set for a chosen night — the single biggest factor in deep-sky observing. Computed, not assumed.","sources":["nasa"]},{"id":"observing_planner:planet-planner","type":"observing_planner","name":"Planet Planner","domain":"science","entryPath":"/observing/planet-planner","description":"Which planets are visible tonight and where, from the platform's computed planetary positions and their altitudes through the night. Jupiter and Saturn to Mercury's fleeting apparitions.","sources":["nasa"]},{"id":"observing_planner:deep-sky-planner","type":"observing_planner","name":"Deep-Sky Planner","domain":"science","entryPath":"/observing/deep-sky-planner","description":"Plans a tour of galaxies, nebulae, and clusters by season, constellation, and difficulty, matched against the night's darkness and the target's altitude. The deep sky, night by night.","sources":["nasa"]},{"id":"observing_planner:season-planner","type":"observing_planner","name":"Season Planner","domain":"science","entryPath":"/observing/season-planner","description":"What each season brings — the constellations overhead, the meteor showers, and the signature deep-sky objects — so a year of observing can be planned in advance.","sources":["nasa"]},{"id":"observing_planner:twilight-planner","type":"observing_planner","name":"Twilight Planner","domain":"science","entryPath":"/observing/twilight-planner","description":"The civil, nautical, and astronomical twilight times for a given place and date — when true darkness begins and ends. Computed from the Sun's position.","sources":["nasa"]},{"id":"observing_planner:darkness-planner","type":"observing_planner","name":"Darkness Planner","domain":"science","entryPath":"/observing/darkness-planner","description":"The window of real darkness on a given night — after astronomical twilight ends and while the Moon is down. The hours that matter most for faint targets.","sources":["nasa"]},{"id":"observing_planner:altitude-chart-planner","type":"observing_planner","name":"Altitude Chart Planner","domain":"science","entryPath":"/observing/altitude-chart-planner","description":"How high a target rides through the night — its altitude against time — so an observer can catch it near the meridian, above the murk of the horizon.","sources":["nasa"]},{"id":"observing_planner:meridian-transit-planner","type":"observing_planner","name":"Meridian Transit Planner","domain":"science","entryPath":"/observing/meridian-transit-planner","description":"When a target crosses the meridian — its highest, sharpest point in the sky — the ideal moment to observe or image it. Computed from its right ascension and the local sidereal time.","sources":["nasa"]},{"id":"observing_planner:equipment-planner","type":"observing_planner","name":"Equipment Planner","domain":"science","entryPath":"/observing/equipment-planner","description":"Matches targets to gear — which objects suit binoculars, a small refractor, or a large Dobsonian — using the platform's real equipment catalogue and the target's brightness and size.","sources":["nasa"]},{"id":"observing_planner:astrophotography-planner","type":"observing_planner","name":"Astrophotography Planner","domain":"science","entryPath":"/observing/astrophotography-planner","description":"Plans an imaging session — the target's framing against the sensor, the Moon and darkness windows, and the capture technique — reusing the real camera, mount, and image-stacking entities.","sources":["nasa"]},{"id":"observing_planner:session-planner","type":"observing_planner","name":"Session Planner","domain":"science","entryPath":"/observing/session-planner","description":"Assembles a full observing session — an ordered list of targets timed to their best moments through a single night — from the visibility, altitude, and darkness plans. Exportable as a calendar or a printable plan.","sources":["nasa"]},{"id":"observing_integration:weather-integration","type":"observing_integration","name":"Weather Integration","domain":"science","entryPath":"/observing/weather-integration","description":"An architecture-ready interface for local weather forecasts — the first thing that decides whether a session happens. The interface is defined and wired into the session planner, but no forecast is shown until a weather provider is connected; nothing is assumed.","sources":["nasa"]},{"id":"observing_integration:seeing-integration","type":"observing_integration","name":"Seeing Integration","domain":"science","entryPath":"/observing/seeing-integration","description":"An architecture-ready interface for atmospheric seeing — the steadiness of the air that sets how fine a detail a night can show. Wired into the astrophotography planner; seeing values appear only from a connected forecast source, never invented.","sources":["nasa"]},{"id":"observing_integration:transparency-integration","type":"observing_integration","name":"Transparency Integration","domain":"science","entryPath":"/observing/transparency-integration","description":"An architecture-ready interface for sky transparency — how much haze and moisture dim faint objects. Wired into the deep-sky planner; transparency is reported only from a connected source.","sources":["nasa"]},{"id":"observing_integration:cloud-cover-integration","type":"observing_integration","name":"Cloud Cover Integration","domain":"science","entryPath":"/observing/cloud-cover-integration","description":"An architecture-ready interface for cloud-cover forecasts and satellite cloud maps. Wired into the tonight planner; cloud data is shown only when a provider is connected.","sources":["nasa"]},{"id":"observing_integration:bortle-integration","type":"observing_integration","name":"Bortle Sky-Brightness Integration","domain":"science","entryPath":"/observing/bortle-integration","description":"An architecture-ready interface for light-pollution and Bortle-class sky-brightness data by location — which sets how faint an object a site can reach. Wired into the deep-sky planner; a site's darkness is reported only from a connected light-pollution source.","sources":["nasa"]},{"id":"graph_view:graph-statistics","type":"graph_view","name":"Graph Statistics","domain":"science","entryPath":"/graph/graph-statistics","description":"The knowledge graph in numbers, counted live from the real data: how many entities and relations it holds, how they split across science, culture, and astrology, which entity types are largest, and which entities are the most connected hubs.","sources":["nasa"]},{"id":"graph_view:knowledge-metrics","type":"graph_view","name":"Knowledge Metrics","domain":"science","entryPath":"/graph/knowledge-metrics","description":"Deeper measures of the graph's structure — the average number of links per entity, the distribution of connectivity, and the hubs that hold the network together. The shape of the knowledge, not just its size.","sources":["nasa"]},{"id":"graph_view:entity-explorer","type":"graph_view","name":"Entity Explorer","domain":"science","entryPath":"/graph/entity-explorer","description":"A browsable index of every entity in the graph, organised by type and domain, each a gateway into its neighbourhood and its place in the wider web of knowledge.","sources":["nasa"]},{"id":"graph_view:relation-explorer","type":"graph_view","name":"Relation Explorer","domain":"science","entryPath":"/graph/relation-explorer","description":"The verbs of the graph — the relation types that connect entities, from 'orbits' and 'discovered by' to 'associated with' — and how often each is used. The grammar of the knowledge.","sources":["nasa"]},{"id":"graph_view:neighborhood-explorer","type":"graph_view","name":"Neighbourhood Explorer","domain":"science","entryPath":"/graph/neighborhood-explorer","description":"The immediate and extended neighbourhood of any entity, expanded breadth-first over the real relations. Start at a star and watch its constellations, catalogues, and physics unfold around it.","sources":["nasa"]},{"id":"graph_view:shortest-path-finder","type":"graph_view","name":"Shortest-Path Finder","domain":"science","entryPath":"/graph/shortest-path-finder","description":"The shortest chain of relations connecting any two entities, found by breadth-first search over the real graph. Every link in the path is a genuine relation — a demonstration of how tightly the knowledge is woven together.","sources":["nasa"]},{"id":"graph_view:taxonomy-explorer","type":"graph_view","name":"Taxonomy Explorer","domain":"science","entryPath":"/graph/taxonomy-explorer","description":"The graph's schema laid bare — the entity types and how they connect to one another, from stars and galaxies to missions and methods. The scaffolding on which every entity hangs.","sources":["nasa"]},{"id":"graph_view:cross-domain-explorer","type":"graph_view","name":"Cross-Domain Explorer","domain":"science","entryPath":"/graph/cross-domain-explorer","description":"The relations that reach across the graph's domains — where the science of the sky meets its cultural and historical meaning, as when a constellation joins its stars to its myths. The threads that make the graph one whole rather than three.","sources":["nasa"]},{"id":"graph_view:force-directed-graph","type":"graph_view","name":"Force-Directed Graph","domain":"science","entryPath":"/graph/force-directed-graph","description":"A node-link visualisation in which entities repel and relations pull, so the graph settles into a shape that reveals its clusters and hubs. A rendering mode over the real neighbourhood data.","sources":["nasa"]},{"id":"graph_view:hierarchical-graph","type":"graph_view","name":"Hierarchical Graph","domain":"science","entryPath":"/graph/hierarchical-graph","description":"A layered layout that arranges entities by level — a taxonomy from the top down, or a dependency chain from cause to effect. A rendering mode for the graph's hierarchical structure.","sources":["nasa"]},{"id":"graph_view:cluster-visualization","type":"graph_view","name":"Cluster Visualisation","domain":"science","entryPath":"/graph/cluster-visualization","description":"A grouping of the graph into its natural communities — the tightly-linked clusters of related entities, such as a mission and its instruments, or a star and its planets. A rendering mode over the real link structure.","sources":["nasa"]},{"id":"graph_view:mission-graph","type":"graph_view","name":"Mission Graph","domain":"science","entryPath":"/graph/mission-graph","description":"The web around a single mission — its instruments, targets, discoveries, and the institutions behind it — drawn from the real relations. A lens that turns a mission from a name into a network.","sources":["nasa"]},{"id":"graph_view:institution-graph","type":"graph_view","name":"Institution Graph","domain":"science","entryPath":"/graph/institution-graph","description":"The reach of a research institution across the graph — the missions it runs, the facilities it operates, and the discoveries it has enabled — traced through the real relations.","sources":["nasa"]},{"id":"graph_view:discovery-graph","type":"graph_view","name":"Discovery Graph","domain":"science","entryPath":"/graph/discovery-graph","description":"A discovery set in its web of context — the people who made it, the instruments that enabled it, the objects it revealed, and the ideas it changed. The story of a discovery as a graph.","sources":["nasa"]},{"id":"graph_view:scientific-lineage","type":"graph_view","name":"Scientific Lineage","domain":"science","entryPath":"/graph/scientific-lineage","description":"The intellectual lineage running through the graph — how an astronomer's work connects to the theories, laws, and later discoveries that built on it. The descent of ideas, traced through the real relations.","sources":["nasa"]},{"id":"graph_view:graph-search","type":"graph_view","name":"Graph Search","domain":"science","entryPath":"/graph/graph-search","description":"A direct search across every entity in the graph by name — the fastest way from a word to a node and its neighbourhood.","sources":["nasa"]},{"id":"graph_view:graph-api","type":"graph_view","name":"Graph API","domain":"science","entryPath":"/graph/graph-api","description":"A live, read-only REST API over the whole knowledge graph — entities, relations, neighbourhoods, and paths — served at /api/v0/entities so other tools can build on the knowledge. Now realised as the Open Platform's public Graph API.","sources":["nasa"]},{"id":"assistant_capability:scientific-search","type":"assistant_capability","name":"Scientific Search","domain":"science","entryPath":"/assistant/scientific-search","description":"Semantic, scientific search across every entity in the knowledge graph — a direct route from a question to the real objects, concepts, missions, and people that answer it. Grounded in the graph; it returns only what is really there.","sources":["nasa"]},{"id":"assistant_capability:object-explanation","type":"assistant_capability","name":"Object Explanation","domain":"science","entryPath":"/assistant/object-explanation","description":"A grounded explanation of any entity — what it is, how it connects to the rest of the graph, and where the knowledge comes from — assembled entirely from the entity's own description, its relations, and its cited sources.","sources":["nasa"]},{"id":"assistant_capability:concept-comparison","type":"assistant_capability","name":"Concept Comparison","domain":"science","entryPath":"/assistant/concept-comparison","description":"Compares two concepts by the real common ground between them — the entities they both connect to in the graph. Mars and Venus, for instance, share atmospheric escape, climate evolution, and their place in the Solar System. A comparison built from relations, not rhetoric.","sources":["nasa"]},{"id":"assistant_capability:relationship-explanation","type":"assistant_capability","name":"Relationship Explanation","domain":"science","entryPath":"/assistant/relationship-explanation","description":"Explains how two entities are related by naming the real relations that link them — 'discovered by', 'orbits', 'is a kind of' — so a connection is never asserted without the graph edge that backs it.","sources":["nasa"]},{"id":"assistant_capability:evidence-chains","type":"assistant_capability","name":"Evidence Chains","domain":"science","entryPath":"/assistant/evidence-chains","description":"Traces the chain of real relations connecting a claim to its supporting entities — for example, from Edwin Hubble through the expansion of the universe to dark energy. Every link in the chain is a genuine edge in the graph, so the reasoning can be followed and checked.","sources":["nasa"]},{"id":"assistant_capability:provenance-aware-answers","type":"assistant_capability","name":"Provenance-Aware Answers","domain":"science","entryPath":"/assistant/provenance-aware-answers","description":"Every grounded answer carries the provenance of the entities it draws on — the sources cited on each, and the review status of the knowledge — so the reader can weigh how far to trust it. No answer without its provenance.","sources":["nasa"]},{"id":"assistant_capability:citation-aware-answers","type":"assistant_capability","name":"Citation-Aware Answers","domain":"science","entryPath":"/assistant/citation-aware-answers","description":"Answers linked back to the literature and catalogues behind them, through the platform's persistent identifiers and the ADS literature service. A grounded assistant that shows its references.","sources":["nasa"]},{"id":"assistant_capability:related-concepts","type":"assistant_capability","name":"Related Concepts","domain":"science","entryPath":"/assistant/related-concepts","description":"Suggests the concepts most closely related to any entity — its real neighbours in the graph. Ask about the main sequence and it surfaces the CNO cycle, the HR diagram, and stellar structure, because those are the entities it actually connects to.","sources":["nasa"]},{"id":"assistant_capability:reading-recommendations","type":"assistant_capability","name":"Reading Recommendations","domain":"science","entryPath":"/assistant/reading-recommendations","description":"Recommends what to read next from the platform's own entries, following the real relations outward from where a reader is — a grounded path deeper into a subject.","sources":["nasa"]},{"id":"assistant_capability:scientific-summaries","type":"assistant_capability","name":"Scientific Summaries","domain":"science","entryPath":"/assistant/scientific-summaries","description":"Concise summaries assembled from the entities' own curated descriptions and their key relations — a faithful digest of what the graph holds, with nothing added.","sources":["nasa"]},{"id":"assistant_capability:learning-path-generation","type":"assistant_capability","name":"Learning-Path Generation","domain":"science","entryPath":"/assistant/learning-path-generation","description":"Assembles a learning path through a subject from the platform's curated paths and the real dependencies between concepts — a grounded curriculum drawn from the graph, ordered from foundations to frontier.","sources":["nasa"]},{"id":"assistant_capability:cross-domain-reasoning","type":"assistant_capability","name":"Cross-Domain Reasoning","domain":"science","entryPath":"/assistant/cross-domain-reasoning","description":"Reasons across the graph's domains — following a constellation from its stars to the myths named for it — using the real relations that bridge science, culture, and history. Connections across domains, never invented.","sources":["nasa"]},{"id":"assistant_capability:no-hallucination-layer","type":"assistant_capability","name":"The No-Hallucination Layer","domain":"science","entryPath":"/assistant/no-hallucination-layer","description":"The design principle beneath the assistant: it surfaces only facts already in the knowledge graph, each with its provenance and a traceable chain of relations. A future language model would phrase these grounded facts, never add to them — so an answer can always be checked against the graph.","sources":["nasa"]},{"id":"assistant_capability:answer-modes","type":"assistant_capability","name":"Answer Modes","domain":"science","entryPath":"/assistant/answer-modes","description":"An architecture-ready interface for tuning the depth of an answer to its audience — an educational mode for newcomers, a research mode for depth, an expert mode for concision. The modes are defined; a language-model layer would realise them over the same grounded facts.","aliases":["Educational, research & expert modes"],"sources":["nasa"]},{"id":"assistant_capability:rag-ready-interfaces","type":"assistant_capability","name":"RAG-Ready Interfaces","domain":"science","entryPath":"/assistant/rag-ready-interfaces","description":"The grounded retrieval — search, neighbourhoods, evidence chains — is exposed as a retrieval-augmented-generation interface, so a future language model can ground every response in the real graph. The retrieval is real today; the generation is future work.","sources":["nasa"]},{"id":"assistant_capability:prompt-orchestration","type":"assistant_capability","name":"Prompt Orchestration","domain":"science","entryPath":"/assistant/prompt-orchestration","description":"An architecture-ready layer for orchestrating a language model over the grounded retrieval — deciding what to fetch, in what order, and how to assemble it. Defined as an interface; no model is wired in yet.","sources":["nasa"]},{"id":"assistant_capability:conversation-memory","type":"assistant_capability","name":"Conversation Memory","domain":"science","entryPath":"/assistant/conversation-memory","description":"An architecture-ready interface for remembering the thread of a conversation — the entities discussed, the questions asked — so follow-ups stay in context. The interface is prepared; memory stays on the device, private-first, and holds only references into the graph.","sources":["nasa"]},{"id":"assistant_capability:llm-integration","type":"assistant_capability","name":"LLM Integration","domain":"science","entryPath":"/assistant/llm-integration","description":"The seam where a language model would join — phrasing the grounded facts the retrieval layer supplies, always constrained to what the graph can back. The interface is defined; the model is future work, and when it comes it will explain, never invent.","sources":["nasa"]},{"id":"live_data_source:noaa-swpc","type":"live_data_source","name":"NOAA Space Weather Prediction Center","domain":"science","entryPath":"/live/noaa-swpc","description":"The United States' official source for space-weather forecasts and alerts — solar wind, the planetary K-index, the geomagnetic storm scale, and radio-blackout and radiation warnings. Modelled here as a real provider with an honest status; no value is shown until it is connected.","aliases":["SWPC"],"sources":["swpc"]},{"id":"live_data_source:nasa-donki","type":"live_data_source","name":"NASA DONKI","domain":"science","entryPath":"/live/nasa-donki","description":"NASA's open database of solar and space-weather events — flares, coronal mass ejections, solar energetic particle events, and interplanetary shocks — served through a public API. Modelled as a real provider with an honest status; no event is shown until it is connected.","aliases":["Space Weather Database Of Notifications, Knowledge, Information"],"sources":["nasa"]},{"id":"live_data_source:minor-planet-center","type":"live_data_source","name":"IAU Minor Planet Center","domain":"science","entryPath":"/live/minor-planet-center","description":"The IAU's clearing house for asteroid and comet observations, designations, and orbits, including near-Earth-object close approaches. Modelled as a real provider with an honest status; no close-approach data is shown until it is connected.","aliases":["MPC"],"sources":["mpc"]},{"id":"live_data_source:jpl-cneos","type":"live_data_source","name":"JPL / CNEOS Close-Approach Data","domain":"science","entryPath":"/live/jpl-cneos","description":"NASA JPL's Center for Near-Earth Object Studies computes close-approach tables and impact-risk (Sentry) summaries for asteroids and comets, served through the Solar System Dynamics APIs. Modelled as a real provider with an honest status; no approach distance or date is shown until it is connected.","aliases":["CNEOS","Center for NEO Studies"],"sources":["jpl"]},{"id":"live_data_source:celestrak-tle","type":"live_data_source","name":"CelesTrak Orbital Elements","domain":"science","entryPath":"/live/celestrak-tle","description":"CelesTrak publishes two-line orbital elements for the ISS and thousands of satellites, from which passes over an observer can be computed by SGP4 propagation. The source and pipeline are modelled here as architecture-ready; neither the live feed nor the propagation is wired, and no pass time is fabricated.","aliases":["CelesTrak","TLE"],"sources":["celestrak"]},{"id":"live_data_source:atmospheric-conditions","type":"live_data_source","name":"Atmospheric Conditions","domain":"science","entryPath":"/live/atmospheric-conditions","description":"The local conditions that decide whether an observing night happens — weather, atmospheric seeing, sky transparency, cloud cover, and Bortle sky brightness. No licence-safe open provider is connected; the interfaces are defined and await one, and no condition is ever fabricated.","aliases":["Weather, seeing, transparency & sky brightness"],"sources":["nasa"]},{"id":"universe_scene:solar-system","type":"universe_scene","name":"The Solar System in 3D","domain":"science","entryPath":"/universe-3d/solar-system","description":"An interactive, to-scale model of the Sun's planetary system. Each orbit ring is drawn at the planet's real semi-major axis, so the true structure of the system — the crowded inner planets and the vast reaches of the outer ones — is genuine. Drag to rotate the system, scroll to zoom.","sources":["nasa"]},{"id":"universe_scene:stars","type":"universe_scene","name":"The Local Stellar Neighbourhood in 3D","domain":"science","entryPath":"/universe-3d/stars","description":"The nearest stars to the Sun, plotted at their true three-dimensional positions from measured parallax distances. This is the view a two-dimensional star chart cannot give: not just where a star lies on the sky, but how far away it truly is. Drag to fly around the neighbourhood; the Sun sits at the centre.","sources":["nasa"]},{"id":"universe_scene:constellations","type":"universe_scene","name":"Constellations on the Celestial Sphere","domain":"science","entryPath":"/universe-3d/constellations","description":"The stars of a constellation shown by their real directions on the celestial sphere — the pattern as it appears from Earth. Turn on the true-distance figures in the table and a striking fact appears: the stars of a constellation lie at wildly different distances and are not physically connected at all. The familiar shape is a line-of-sight illusion.","sources":["nasa"]},{"id":"universe_scene:milky-way","type":"universe_scene","name":"The Milky Way","domain":"science","entryPath":"/universe-3d/milky-way","description":"Our home galaxy and the Sun's place within it. The measured part of this picture — the local stellar neighbourhood — is the real 3D star field; the wider structure of the Galaxy (its disc, bulge, bar, spiral arms, halo, and centre) is presented from the galactic-structure catalogue as described components, because numeric galaxy-scale positions are not part of the data.","sources":["nasa"]},{"id":"universe_scene:local-group","type":"universe_scene","name":"The Local Group","domain":"science","entryPath":"/universe-3d/local-group","description":"Our galactic neighbourhood — the Milky Way, Andromeda, Triangulum, the Magellanic Clouds, and the dozens of dwarf galaxies bound with them. The members and their relationships are drawn from the graph; their separations are given by the catalogue's descriptive scale labels, because numeric inter-galactic distances and positions are not part of the data.","sources":["nasa"]},{"id":"workspace_feature:saved-entities","type":"workspace_feature","name":"Saved Entities","domain":"science","entryPath":"/workspace","description":"Bookmark any entity in the knowledge graph — a planet, star, mission, galaxy, method — to your own workspace with a single click. Saved entities are stored only in your browser and are the raw material of collections, notes, and citations. Nothing is sent to a server.","sources":["nasa"]},{"id":"workspace_feature:collections","type":"workspace_feature","name":"Collections","domain":"science","entryPath":"/workspace/collections","description":"Organise saved entities into named collections — a research theme, a set of targets, a topic to revisit. Collections live in your browser and can be exported or printed. A collection references entities by id; it never copies or alters the underlying data.","sources":["nasa"]},{"id":"workspace_feature:reading-lists","type":"workspace_feature","name":"Reading Lists","domain":"science","entryPath":"/workspace/collections","description":"An ordered reading list — a path through the encyclopedia you intend to follow. A reading list is a collection whose order is meaningful, so you can sequence a study plan. Stored locally; nothing is tracked about what you read.","sources":["nasa"]},{"id":"workspace_feature:observation-projects","type":"workspace_feature","name":"Observation Projects","domain":"science","entryPath":"/workspace/collections","description":"Gather the objects you plan to observe into an observation project — a set of targets you can pair with the observing planners and the live-sky tools. An observation project is a local collection of real targets; it computes nothing and fabricates no ephemeris.","sources":["nasa"]},{"id":"workspace_feature:notes","type":"workspace_feature","name":"Notes","domain":"science","entryPath":"/workspace/notes","description":"Write your own notes and attach them to a saved entity or keep them free-standing — questions, observations, connections you have spotted. Notes are yours alone, held only in your browser, and are included in exports and the printable packet.","sources":["nasa"]},{"id":"workspace_feature:citation-folder","type":"workspace_feature","name":"Citation Folder","domain":"science","entryPath":"/workspace/citations","description":"Collect the citations behind the entities you study into a citation folder, and export them in APA, Chicago, MLA, Harvard, BibTeX, or RIS. It REUSES the platform's citation engine over real, source-backed references — every field comes from a verifiable citation record; none is invented.","sources":["nasa"]},{"id":"workspace_feature:exports","type":"workspace_feature","name":"Exports & Printable Packet","domain":"science","entryPath":"/workspace/exports","description":"Export your whole workspace — saved entities, collections, notes, and citations — to JSON, Markdown, BibTeX, or CSV, or print a clean research packet. Exports are generated in your browser from your local data; nothing is uploaded, and JSON can be re-imported to move your workspace between devices yourself.","sources":["nasa"]},{"id":"workspace_feature:privacy","type":"workspace_feature","name":"Privacy","domain":"science","entryPath":"/workspace/privacy","description":"The workspace is private by construction. It stores everything in your browser's localStorage under a single key, holds no account, sets no cookie, makes no network request, and records no analytics. Your data never leaves your device, and a single control erases all of it. This is a guarantee of the design, not a policy promise.","sources":["nasa"]},{"id":"platform_capability:public-graph-api","type":"platform_capability","name":"Public Graph API","domain":"science","entryPath":"/open-platform/api","description":"A read-only, deterministic REST API over the whole knowledge graph — list and fetch entities, list relationships, search, and traverse neighbourhoods and shortest paths. Every response carries a provenance envelope (version, source, licence, attribution). No auth, no rate limits, no write endpoints.","sources":["nasa"]},{"id":"platform_capability:graph-neighbours-path","type":"platform_capability","name":"Neighbours & Evidence Paths","domain":"science","entryPath":"/open-platform/api","description":"The graph query surface: breadth-first neighbourhood traversal and shortest evidence paths between two entities, cycle-safe and bounded. The same real algorithms behind the graph explorer and the grounded assistant, exposed as an API.","sources":["nasa"]},{"id":"platform_capability:openapi-spec","type":"platform_capability","name":"OpenAPI Specification","domain":"science","entryPath":"/open-platform/api","description":"A machine-readable OpenAPI 3.1 description of every implemented endpoint, generated from the endpoint registry — so a client, a code generator, or an agent can discover the API automatically.","sources":["nasa"]},{"id":"platform_capability:sources-api","type":"platform_capability","name":"Sources API","domain":"science","entryPath":"/open-platform/api","description":"The registry of authoritative sources behind the platform — every source's name, organisation, canonical URL, licence, and scope — served as a public endpoint, so the provenance of any cited fact can be resolved programmatically.","sources":["nasa"]},{"id":"platform_capability:citation-export","type":"platform_capability","name":"Citation Export","domain":"science","entryPath":"/open-platform/api","description":"The real, source-backed citations behind entities, served as an API and exportable in APA, Chicago, MLA, Harvard, BibTeX, and RIS through the platform's citation engine. Every field comes from a verifiable citation record; none is invented.","sources":["nasa"]},{"id":"platform_capability:graph-json","type":"platform_capability","name":"Knowledge Graph Export (JSON)","domain":"science","entryPath":"/open-platform/graph","description":"The complete typed graph — every entity and relation — as a single JSON document, generated from the real graph. The exact bytes served back the download manifest's size and checksum.","sources":["nasa"]},{"id":"platform_capability:graph-jsonld","type":"platform_capability","name":"Knowledge Graph Export (JSON-LD / RDF)","domain":"science","entryPath":"/open-platform/graph","description":"The graph as JSON-LD — an RDF-compatible, SPARQL-ready document with a resolvable @id per node and relations as predicates. The linked-data foundation the SPARQL and federation layers are built to sit on.","sources":["nasa"]},{"id":"platform_capability:dataset-exports","type":"platform_capability","name":"Dataset Exports","domain":"science","entryPath":"/open-platform/datasets","description":"Every curated dataset — from named stars to live-provider status to 3D scenes — exportable as JSON and CSV with real record counts, licences, and provenance. A focused slice of the graph for a specific need.","sources":["nasa"]},{"id":"platform_capability:bulk-downloads","type":"platform_capability","name":"Bulk Downloads","domain":"science","entryPath":"/open-platform/downloads","description":"The full graph exports offered as bulk downloads, each with a REAL byte size and SHA-256 checksum computed from the exact bytes served, plus its licence and release. No download is fabricated — the checksum can be verified against the file.","sources":["nasa"]},{"id":"platform_capability:versioned-releases","type":"platform_capability","name":"Versioned Releases","domain":"science","entryPath":"/open-platform/downloads","description":"The graph and its schema carry versions, surfaced in every API response's provenance envelope, in the OpenAPI description, and on every export — so a consumer can pin a release and know when entities or the schema change.","sources":["nasa"]},{"id":"platform_capability:licensing-matrix","type":"platform_capability","name":"Licensing Matrix","domain":"science","entryPath":"/open-platform/licenses","description":"A clear matrix of the licences that apply — the platform's own CC BY-SA 4.0 for the graph and API, and the individual terms of each upstream source (NASA, ESA, IAU, and the rest) — so reuse obligations are never in doubt.","sources":["nasa"]},{"id":"platform_capability:sparql-endpoint","type":"platform_capability","name":"SPARQL Endpoint","domain":"science","entryPath":"/open-platform/graph","description":"A hosted SPARQL query endpoint over the graph's RDF. The linked-data shape is live in the JSON-LD export; a queryable SPARQL service is the architecture-ready next step and is not yet hosted — no endpoint is advertised as live.","sources":["nasa"]},{"id":"platform_capability:graphql-api","type":"platform_capability","name":"GraphQL API","domain":"science","entryPath":"/open-platform/graph","description":"A GraphQL surface over the same graph, letting a client request exactly the entities, fields, and relations it needs in one query. The schema maps cleanly onto the typed graph; the resolver layer is architecture-ready and not yet served.","sources":["nasa"]},{"id":"platform_capability:doi-releases","type":"platform_capability","name":"DOI-Minted Releases","domain":"science","entryPath":"/open-platform/downloads","description":"Citable, DOI-minted snapshots of the graph, so a specific release can be referenced in the literature. The versioning and checksummed exports that a DOI release needs are live; minting DOIs through a registration agency is architecture-ready.","sources":["nasa"]},{"id":"platform_capability:sdk-python","type":"platform_capability","name":"Python SDK","domain":"science","entryPath":"/open-platform/sdk","description":"A Python client over the public API — typed models for entities and relations, and helpers for search, traversal, and export. The API and its OpenAPI description are live, so a client can be generated today; a curated, published package is architecture-ready.","sources":["nasa"]},{"id":"platform_capability:sdk-js","type":"platform_capability","name":"JavaScript / TypeScript SDK","domain":"science","entryPath":"/open-platform/sdk","description":"A typed JavaScript/TypeScript client over the public API, for the browser or Node. As with the Python SDK, the OpenAPI description makes a client generatable today; a curated, published package is architecture-ready.","sources":["nasa"]},{"id":"platform_capability:federation-metadata","type":"platform_capability","name":"Federation-Ready Metadata","domain":"science","entryPath":"/open-platform/federation","description":"Every entity already carries a resolvable IRI in the JSON-LD export, the foundation for federating the graph with other linked-data sources. A published federation manifest and cross-dataset link set are architecture-ready.","sources":["nasa"]},{"id":"platform_capability:vo-tap-adql","type":"platform_capability","name":"Virtual Observatory (TAP / ADQL)","domain":"science","entryPath":"/open-platform/federation","description":"An interface prepared for the International Virtual Observatory Alliance protocols — a TAP service answering ADQL queries over the tabular catalogues (stars, deep-sky, exoplanets). The catalogues carry the real measured columns; a TAP/ADQL service over them is architecture-ready.","sources":["nasa"]},{"id":"solar_region:solar-core","type":"solar_region","name":"The Solar Core","domain":"science","entryPath":"/solar-physics/solar-core","description":"The innermost region of the Sun, out to about a quarter of its radius, where nuclear fusion powers the star. At roughly 15 million kelvin and immense density, hydrogen fuses to helium mainly through the proton–proton chain, releasing the energy that slowly works its way outward. Almost all of the Sun's luminosity is generated here.","aliases":["Core"],"sources":["nasa"]},{"id":"solar_region:radiative-zone","type":"solar_region","name":"The Radiative Zone","domain":"science","entryPath":"/solar-physics/radiative-zone","description":"The layer surrounding the core, from about a quarter to seven-tenths of the solar radius, where energy travels outward as radiation. Photons are absorbed and re-emitted so many times that a single packet of energy can take on the order of a hundred thousand years to cross it. The plasma here rotates almost as a rigid body.","sources":["nasa"]},{"id":"solar_region:tachocline","type":"solar_region","name":"The Tachocline","domain":"science","entryPath":"/solar-physics/tachocline","description":"The thin shear layer near seven-tenths of the solar radius, where the rigidly rotating radiative interior meets the differentially rotating convection zone. This velocity shear is widely thought to be where the Sun's large-scale magnetic field is generated — the seat of the solar dynamo.","sources":["nasa"]},{"id":"solar_region:convection-zone","type":"solar_region","name":"The Convection Zone","domain":"science","entryPath":"/solar-physics/convection-zone","description":"The outer third of the solar interior, where energy is carried by convection — hot plasma rises, cools, and sinks, like a pot of boiling water. This churning is visible at the surface as granulation and drives the magnetic activity of the Sun. It sits above the tachocline and below the photosphere.","sources":["nasa"]},{"id":"solar_region:photosphere","type":"solar_region","name":"The Photosphere","domain":"science","entryPath":"/solar-physics/photosphere","description":"The visible surface of the Sun — the layer from which sunlight escapes — with an effective temperature near 5,772 kelvin and a thickness of only a few hundred kilometres. Sunspots, granulation, and the limb darkening seen in white-light images all belong to the photosphere. It is the reference surface for the Sun's radius.","aliases":["Solar surface"],"sources":["nasa"]},{"id":"solar_region:chromosphere","type":"solar_region","name":"The Chromosphere","domain":"science","entryPath":"/solar-physics/chromosphere","description":"The reddish layer of the solar atmosphere just above the photosphere, a few thousand kilometres thick, briefly visible as a rosy rim at the start and end of a total eclipse. Its temperature rises with height, and it is threaded by spicules, filaments, and plages. Above it lies the thin transition region.","sources":["nasa"]},{"id":"solar_region:transition-region","type":"solar_region","name":"The Transition Region","domain":"science","entryPath":"/solar-physics/transition-region","description":"The thin, irregular layer between the chromosphere and the corona where the temperature climbs steeply — from around ten thousand to a million kelvin over only a few hundred kilometres. It radiates mostly in the extreme ultraviolet and is central to the still-open question of how the corona is heated.","sources":["nasa"]},{"id":"solar_region:corona","type":"solar_region","name":"The Solar Corona","domain":"science","entryPath":"/solar-physics/corona","description":"The Sun's outermost atmosphere — a tenuous, million-degree plasma extending millions of kilometres into space, visible to the eye only during a total solar eclipse or with a coronagraph. Far hotter than the surface beneath it, it is shaped by magnetic fields into loops, holes, and streamers, and it continually expands outward as the solar wind.","aliases":["Corona"],"sources":["nasa"]},{"id":"solar_feature:granulation","type":"solar_feature","name":"Granulation","domain":"science","entryPath":"/solar-physics/granulation","description":"The mottled, cellular pattern covering the photosphere — the tops of convection cells about a thousand kilometres across, each lasting only minutes. Bright centres are hot plasma rising, dark lanes are cooler plasma sinking. Granulation is the direct visible signature of the convection zone beneath.","sources":["nasa"]},{"id":"solar_feature:supergranulation","type":"solar_feature","name":"Supergranulation","domain":"science","entryPath":"/solar-physics/supergranulation","description":"A larger-scale convective pattern, with cells around thirty thousand kilometres across that persist for roughly a day. Supergranule flows sweep magnetic field to their edges, building the chromospheric network. It was discovered through Doppler measurements of the surface flows.","sources":["nasa"]},{"id":"solar_feature:prominence","type":"solar_feature","name":"Prominence","domain":"science","entryPath":"/solar-physics/prominence","description":"A large, relatively cool and dense structure of plasma suspended above the solar surface by magnetic fields, extending into the hot corona. Seen at the limb against the dark sky it appears as a bright arch; quiescent prominences can last for months, while eruptive ones can launch a coronal mass ejection.","sources":["nasa"]},{"id":"solar_feature:filament","type":"solar_feature","name":"Filament","domain":"science","entryPath":"/solar-physics/filament","description":"The same structure as a prominence, but seen against the bright solar disk rather than at the limb, where it appears as a dark, thread-like channel. A filament is cool plasma along a magnetic boundary; its sudden eruption is a common trigger of a coronal mass ejection.","sources":["nasa"]},{"id":"solar_feature:plage","type":"solar_feature","name":"Plage","domain":"science","entryPath":"/solar-physics/plage","description":"A bright region of the chromosphere associated with an active region, where concentrated magnetic field heats the plasma above a group of sunspots. Plages are conspicuous in the light of hydrogen and calcium and mark magnetically active areas even as the sunspots themselves come and go.","sources":["nasa"]},{"id":"solar_feature:spicule","type":"solar_feature","name":"Spicule","domain":"science","entryPath":"/solar-physics/spicule","description":"A short-lived jet of plasma, a few hundred kilometres across, that shoots up from the chromosphere at tens of kilometres per second and falls back within minutes. Millions cover the Sun at any moment, giving the chromospheric limb a grassy appearance; they may contribute to the mass and energy budget of the corona.","sources":["nasa"]},{"id":"solar_feature:coronal-loop","type":"solar_feature","name":"Coronal Loop","domain":"science","entryPath":"/solar-physics/coronal-loop","description":"An arch of hot, glowing plasma tracing a magnetic field line rooted in the photosphere, the basic building block of the closed corona above active regions. Coronal loops shine brightly in the extreme ultraviolet and X-rays and are central to studies of how the corona is structured and heated.","sources":["nasa"]},{"id":"solar_feature:coronal-streamer","type":"solar_feature","name":"Coronal Streamer","domain":"science","entryPath":"/solar-physics/coronal-streamer","description":"A large, pointed structure in the corona, seen in eclipse and coronagraph images as bright rays extending outward above the streamer belt. Helmet streamers cap closed magnetic regions and are the source of the slow solar wind; their shape changes over the solar cycle.","aliases":["Helmet streamer"],"sources":["nasa"]},{"id":"solar_feature:polar-coronal-plume","type":"solar_feature","name":"Polar Coronal Plume","domain":"science","entryPath":"/solar-physics/polar-coronal-plume","description":"A thin, ray-like structure of denser plasma rooted in the Sun's polar regions and extending into a polar coronal hole. Plumes trace open magnetic field lines from which fast solar wind flows, and appear as delicate streaks in images of the poles.","aliases":["Polar plume"],"sources":["nasa"]},{"id":"stellar_physics_concept:solar-dynamo","type":"stellar_physics_concept","name":"The Solar Dynamo","domain":"science","entryPath":"/solar-physics/solar-dynamo","description":"The mechanism that generates and regenerates the Sun's magnetic field, converting the energy of plasma motions — differential rotation and convection — into magnetic energy. The dynamo drives the roughly eleven-year sunspot cycle and the reversal of the Sun's polarity; the details, especially the role of the tachocline, remain an active research problem.","sources":["nasa"]},{"id":"stellar_physics_concept:magnetic-reconnection","type":"stellar_physics_concept","name":"Magnetic Reconnection","domain":"science","entryPath":"/solar-physics/magnetic-reconnection","description":"The process by which oppositely directed magnetic field lines break and reconnect, converting stored magnetic energy explosively into heat, light, and fast particles. Reconnection powers solar flares and helps launch coronal mass ejections, and is a fundamental plasma process seen throughout the Universe.","sources":["nasa"]},{"id":"stellar_physics_concept:differential-rotation","type":"stellar_physics_concept","name":"Differential Rotation","domain":"science","entryPath":"/solar-physics/differential-rotation","description":"The Sun does not rotate as a solid body: its equator completes a turn in about twenty-five days while the polar regions take around thirty-five. This shearing of the plasma winds up the magnetic field and is a key ingredient of the solar dynamo. It is measured from tracking sunspots and from helioseismology.","sources":["nasa"]},{"id":"stellar_physics_concept:coronal-heating-problem","type":"stellar_physics_concept","name":"The Coronal Heating Problem","domain":"science","entryPath":"/solar-physics/coronal-heating-problem","description":"One of the central open questions in solar physics: why the corona, at a million or more kelvin, is hundreds of times hotter than the photosphere below it. Leading candidate mechanisms include heating by many tiny reconnection events (nanoflares) and by magnetic waves; missions such as Parker Solar Probe and Solar Orbiter are testing them. No single answer is yet established.","sources":["nasa"]},{"id":"stellar_physics_concept:nanoflare-heating","type":"stellar_physics_concept","name":"Nanoflare Heating","domain":"science","entryPath":"/solar-physics/nanoflare-heating","description":"A proposed solution to the coronal heating problem, put forward by Eugene Parker: the corona is heated by a vast number of tiny reconnection events — nanoflares — each far too small to see on its own, but collectively enough to keep the corona hot. It is one of several candidate mechanisms still being tested against observations.","sources":["nasa"]},{"id":"stellar_physics_concept:butterfly-diagram","type":"stellar_physics_concept","name":"The Butterfly Diagram","domain":"science","entryPath":"/solar-physics/butterfly-diagram","description":"A plot of the latitudes at which sunspots appear over time, first drawn by the Maunders. Across each roughly eleven-year cycle, spots emerge first at mid-latitudes and then closer to the equator, so successive cycles trace wing-shaped patterns. It is the clearest visual summary of the solar activity cycle.","sources":["nasa"]},{"id":"stellar_physics_concept:maunder-minimum","type":"stellar_physics_concept","name":"The Maunder Minimum","domain":"science","entryPath":"/solar-physics/maunder-minimum","description":"A roughly seventy-year span in the seventeenth and early eighteenth centuries when sunspots almost vanished from the record. It overlapped part of the cooler period known as the Little Ice Age, though the size of any climate link is debated. It is the archetype of a grand solar minimum.","sources":["nasa"]},{"id":"stellar_physics_concept:dalton-minimum","type":"stellar_physics_concept","name":"The Dalton Minimum","domain":"science","entryPath":"/solar-physics/dalton-minimum","description":"A period of low but not absent solar activity around the turn of the nineteenth century, less deep than the Maunder Minimum. Like other grand minima it is reconstructed from sunspot counts and from cosmogenic isotopes recorded in ice cores and tree rings.","sources":["nasa"]},{"id":"stellar_physics_concept:solar-irradiance-variation","type":"stellar_physics_concept","name":"Solar Irradiance Variation","domain":"science","entryPath":"/solar-physics/solar-irradiance-variation","description":"The total energy the Sun radiates varies slightly over the activity cycle — by about a tenth of a percent between solar maximum and minimum — as dark sunspots and bright faculae come and go. Measured continuously from space since the late 1970s, these variations are a key input to studies of the Sun's influence on climate.","sources":["nasa"]},{"id":"stellar_physics_concept:fast-solar-wind","type":"stellar_physics_concept","name":"The Fast Solar Wind","domain":"science","entryPath":"/solar-physics/fast-solar-wind","description":"The steady, high-speed stream of the solar wind — around seven to eight hundred kilometres per second — that flows out along open magnetic field lines from coronal holes, especially over the poles at solar minimum. It is smoother and less dense than the slow wind.","sources":["nasa"]},{"id":"stellar_physics_concept:slow-solar-wind","type":"stellar_physics_concept","name":"The Slow Solar Wind","domain":"science","entryPath":"/solar-physics/slow-solar-wind","description":"The denser, more variable component of the solar wind — around three to five hundred kilometres per second — associated with the streamer belt near the solar equator. Its exact sources and release mechanisms are still being pinned down by close-in missions.","sources":["nasa"]},{"id":"heliosphere_structure:parker-spiral","type":"heliosphere_structure","name":"The Parker Spiral","domain":"science","entryPath":"/solar-physics/parker-spiral","description":"The spiral shape the Sun's magnetic field takes as it is carried outward by the solar wind while the Sun rotates, like water from a spinning sprinkler. Predicted by Eugene Parker in 1958 and since confirmed by spacecraft, the Parker spiral sets the geometry of the interplanetary magnetic field and how solar storms reach the planets.","aliases":["Interplanetary magnetic field"],"sources":["nasa"]},{"id":"heliosphere_structure:termination-shock","type":"heliosphere_structure","name":"The Termination Shock","domain":"science","entryPath":"/solar-physics/termination-shock","description":"The boundary where the supersonic solar wind abruptly slows as it runs into the pressure of the interstellar medium, roughly ninety astronomical units from the Sun. Voyager 1 crossed it in 2004 and Voyager 2 in 2007 — the first direct measurements of this shock.","sources":["nasa"]},{"id":"heliosphere_structure:heliosheath","type":"heliosphere_structure","name":"The Heliosheath","domain":"science","entryPath":"/solar-physics/heliosheath","description":"The turbulent outer region of the heliosphere, between the termination shock and the heliopause, where the slowed solar wind piles up and is deflected by the interstellar medium. Both Voyager spacecraft spent years traversing it before reaching interstellar space.","sources":["nasa"]},{"id":"heliosphere_structure:heliospheric-bow-wave","type":"heliosphere_structure","name":"The Heliospheric Bow Wave","domain":"science","entryPath":"/solar-physics/heliospheric-bow-wave","description":"The disturbance ahead of the heliosphere as it moves through the surrounding interstellar cloud. Earlier work expected a sharp bow shock, but measurements from IBEX and the Voyagers suggest the Sun moves too slowly through the local medium for a strong shock — a gentler bow wave instead. The exact nature of the boundary is still being studied.","aliases":["Bow wave"],"sources":["nasa"]},{"id":"cosmology_concept:ergosphere","type":"cosmology_concept","name":"The Ergosphere","domain":"science","entryPath":"/compact-objects/ergosphere","description":"The region just outside the event horizon of a rotating (Kerr) black hole where spacetime itself is dragged around so fast that nothing can stay still relative to the distant stars. Energy can, in principle, be extracted from a black hole's rotation here through the Penrose process. A non-rotating black hole has no ergosphere.","sources":["nasa"]},{"id":"cosmology_concept:photon-sphere","type":"cosmology_concept","name":"The Photon Sphere","domain":"science","entryPath":"/compact-objects/photon-sphere","description":"The radius around a non-rotating black hole — one and a half Schwarzschild radii — at which gravity bends light so strongly that photons can orbit in unstable circles. It sets the size of the black hole's 'shadow' and the bright ring seen in the Event Horizon Telescope images of M87* and Sgr A*.","sources":["nasa"]},{"id":"cosmology_concept:innermost-stable-circular-orbit","type":"cosmology_concept","name":"The Innermost Stable Circular Orbit","domain":"science","entryPath":"/compact-objects/innermost-stable-circular-orbit","description":"The closest orbit around a black hole in which matter can circle stably — at three Schwarzschild radii for a non-spinning black hole, and closer for a rapidly spinning one. Inside it, matter spirals inevitably inward. The ISCO sets the inner edge of an accretion disk and thus how much energy accretion can release.","aliases":["ISCO"],"sources":["nasa"]},{"id":"cosmology_concept:no-hair-theorem","type":"cosmology_concept","name":"The No-Hair Theorem","domain":"science","entryPath":"/compact-objects/no-hair-theorem","description":"The result that a black hole in equilibrium is fully described by just three numbers — its mass, its spin, and its electric charge — and retains no other detail of whatever formed it. All the complexity of the collapsing matter is lost to the outside universe, hidden behind the event horizon with the central singularity, giving black holes a remarkable simplicity.","sources":["nasa"]},{"id":"cosmology_concept:frame-dragging","type":"cosmology_concept","name":"Frame-Dragging","domain":"science","entryPath":"/compact-objects/frame-dragging","description":"The twisting of spacetime by a rotating mass, which drags nearby matter and light around with it. Extreme near a spinning black hole, it creates the ergosphere; it is tiny near the Earth, where it was measured by the Gravity Probe B and LAGEOS satellite experiments — a direct confirmation of a subtle prediction of general relativity.","aliases":["Lense–Thirring effect"],"sources":["nasa"]},{"id":"cosmology_concept:gravitational-redshift","type":"cosmology_concept","name":"Gravitational Redshift","domain":"science","entryPath":"/compact-objects/gravitational-redshift","description":"The stretching of light to longer wavelengths as it climbs out of a gravitational well, a prediction of general relativity. It is extreme near a black hole's event horizon, where light is redshifted without limit, and has been measured for the Sun, for white dwarfs, and even for atomic clocks at different heights on Earth.","sources":["nasa"]},{"id":"cosmology_concept:spaghettification","type":"cosmology_concept","name":"Spaghettification","domain":"science","entryPath":"/compact-objects/spaghettification","description":"The stretching of an object into a long, thin shape by the difference in a black hole's gravity between its near and far sides. Around a small stellar black hole the tidal force is lethal well outside the horizon; around a supermassive black hole it is gentle at the horizon, so an infalling object could cross without being torn apart.","aliases":["Tidal stretching"],"sources":["nasa"]},{"id":"cosmology_concept:relativistic-jet","type":"cosmology_concept","name":"Relativistic Jet","domain":"science","entryPath":"/compact-objects/relativistic-jet","description":"A narrow beam of plasma launched at nearly the speed of light from the vicinity of an accreting black hole — from stellar black holes in binaries and from the supermassive black holes powering active galaxies. Jets can span from light-years to millions of light-years and are thought to be powered by the black hole's spin and magnetic fields.","sources":["nasa"]},{"id":"cosmology_concept:blandford-znajek-mechanism","type":"cosmology_concept","name":"The Blandford–Znajek Mechanism","domain":"science","entryPath":"/compact-objects/blandford-znajek-mechanism","description":"The leading explanation for how relativistic jets are powered: magnetic field lines threading a spinning black hole extract its rotational energy and fling plasma outward. Proposed by Roger Blandford and Roman Znajek in 1977, it lets a black hole act as a cosmic engine, converting spin into the enormous power of a jet.","sources":["nasa"]},{"id":"cosmology_concept:quasi-periodic-oscillation","type":"cosmology_concept","name":"Quasi-Periodic Oscillation","domain":"science","entryPath":"/compact-objects/quasi-periodic-oscillation","description":"A near-regular flickering in the X-ray brightness of matter orbiting a black hole or neutron star, revealed in the power spectrum as a broad peak rather than a sharp tone. QPOs probe the innermost accretion flow, close to the innermost stable circular orbit, and are used to study strong gravity — though their exact origin is still debated.","aliases":["QPO"],"sources":["nasa"]},{"id":"cosmology_concept:bondi-accretion","type":"cosmology_concept","name":"Bondi Accretion","domain":"science","entryPath":"/compact-objects/bondi-accretion","description":"The idealised, spherically symmetric capture of surrounding gas by a compact object, worked out by Hermann Bondi in 1952. It sets a benchmark rate at which a black hole or neutron star can swallow the gas around it, and underlies estimates of how quiescent supermassive black holes such as Sgr A* are fed.","sources":["nasa"]},{"id":"stellar_physics_concept:neutron-degeneracy-pressure","type":"stellar_physics_concept","name":"Neutron Degeneracy Pressure","domain":"science","entryPath":"/compact-objects/neutron-degeneracy-pressure","description":"The quantum pressure — arising from the Pauli exclusion principle acting on densely packed neutrons — that holds a neutron star up against its own gravity. It is far stronger than the electron degeneracy pressure that supports a white dwarf, but it too has a limit: above roughly two to three solar masses, no known pressure can prevent collapse into a black hole.","sources":["nasa"]},{"id":"stellar_physics_concept:neutron-star-equation-of-state","type":"stellar_physics_concept","name":"The Neutron-Star Equation of State","domain":"science","entryPath":"/compact-objects/neutron-star-equation-of-state","description":"The still-uncertain relationship between pressure and density inside a neutron star, which decides how compressible its ultra-dense matter is and therefore the star's radius and maximum mass. Pinning it down — from radius measurements by NICER, from massive pulsars, and from the tidal signature in neutron-star mergers — is a central goal of modern astrophysics.","sources":["nasa"]},{"id":"stellar_physics_concept:pulsar-mechanism","type":"stellar_physics_concept","name":"The Pulsar Mechanism","domain":"science","entryPath":"/compact-objects/pulsar-mechanism","description":"How a pulsar pulses: a rapidly rotating, strongly magnetised neutron star beams radiation from its magnetic poles, and if a beam sweeps across the Earth we see a regular pulse once per rotation, like a lighthouse. The precise physics of how the beam is generated in the star's magnetosphere is still not fully understood.","aliases":["Lighthouse effect"],"sources":["nasa"]},{"id":"stellar_physics_concept:pulsar-glitch","type":"stellar_physics_concept","name":"Pulsar Glitch","domain":"science","entryPath":"/compact-objects/pulsar-glitch","description":"A sudden, tiny speed-up in a pulsar's otherwise steadily slowing rotation, followed by a gradual relaxation. Glitches are thought to be caused by the sudden transfer of angular momentum from a superfluid deep inside the neutron star to its solid crust, giving a rare window onto matter at supernuclear density.","sources":["nasa"]},{"id":"stellar_physics_concept:magnetar-magnetic-field","type":"stellar_physics_concept","name":"The Magnetar Magnetic Field","domain":"science","entryPath":"/compact-objects/magnetar-magnetic-field","description":"The most powerful magnetic fields known in the Universe — around a hundred trillion to a quadrillion gauss — carried by magnetars, a class of young neutron star. The decay of this colossal field powers their X-ray and gamma-ray flares, including the giant flares bright enough to be detected across the Galaxy and beyond.","sources":["nasa"]},{"id":"astrophysical_object_class:pulsar","type":"astrophysical_object_class","name":"Pulsar","domain":"science","entryPath":"/compact-objects/pulsar","description":"A rapidly rotating, magnetised neutron star observed as a source of regular pulses of radiation, usually in radio. The first was found in 1967 by Jocelyn Bell Burnell and Antony Hewish; thousands are now known, with periods from milliseconds to seconds. Pulsars are precise cosmic clocks used to test gravity and to search for gravitational waves.","sources":["nasa"]},{"id":"astrophysical_object_class:millisecond-pulsar","type":"astrophysical_object_class","name":"Millisecond Pulsar","domain":"science","entryPath":"/compact-objects/millisecond-pulsar","description":"An old pulsar spun up to hundreds of rotations per second by accreting matter from a companion star — 'recycled' to spin periods of only a few milliseconds. Their extraordinary rotational stability makes them the most precise clocks known and the basis of pulsar-timing arrays searching for low-frequency gravitational waves.","sources":["nasa"]},{"id":"astrophysical_object_class:x-ray-pulsar","type":"astrophysical_object_class","name":"X-ray Pulsar","domain":"science","entryPath":"/compact-objects/x-ray-pulsar","description":"A neutron star in a binary system that pulls gas from its companion; the gas is funnelled by the star's magnetic field onto its poles, where it heats up and shines in pulsed X-rays as the star rotates. X-ray pulsars are how many neutron stars are weighed, and how millisecond pulsars are recycled.","sources":["nasa"]},{"id":"astrophysical_object_class:rotation-powered-pulsar","type":"astrophysical_object_class","name":"Rotation-Powered Pulsar","domain":"science","entryPath":"/compact-objects/rotation-powered-pulsar","description":"A pulsar whose radiation is powered by the gradual loss of its rotational energy as it slowly spins down — the classic young pulsar, of which the Crab is the archetype. This is distinct from an accretion-powered X-ray pulsar, which draws its energy from infalling matter rather than from its own spin.","sources":["nasa"]},{"id":"black_hole:cygnus-x-1","type":"black_hole","name":"Cygnus X-1 (black hole)","domain":"science","entryPath":"/compact-objects/cygnus-x-1","description":"The compact object of Cygnus X-1 — the first widely accepted black hole. A bright X-ray source in Cygnus discovered in 1964, it is a stellar-mass black hole of roughly twenty-one solar masses pulling gas from its blue-supergiant donor star (HD 226868). It was the subject of a famous bet between Stephen Hawking and Kip Thorne, which Hawking conceded in 1990.","aliases":["Cygnus X-1","Cyg X-1"],"sources":["nasa"]},{"id":"black_hole:v404-cygni","type":"black_hole","name":"V404 Cygni","domain":"science","entryPath":"/compact-objects/v404-cygni","description":"A stellar-mass black hole of about nine solar masses in a binary system in Cygnus, and one of the nearest black holes with a precisely measured distance from radio parallax. Normally quiet, it erupted in a dramatic X-ray and radio outburst in June 2015 — a nearby microquasar caught devouring gas from its companion.","sources":["nasa"]},{"id":"neutron_star:crab-pulsar","type":"neutron_star","name":"The Crab Pulsar","domain":"science","entryPath":"/compact-objects/crab-pulsar","description":"The young neutron star at the heart of the Crab Nebula, formed in the supernova recorded by observers in 1054. It spins about thirty times a second and is the archetypal rotation-powered pulsar, its wind lighting up the surrounding nebula across the spectrum, from radio to gamma rays.","aliases":["PSR B0531+21"],"sources":["nasa"]},{"id":"neutron_star:vela-pulsar","type":"neutron_star","name":"The Vela Pulsar","domain":"science","entryPath":"/compact-objects/vela-pulsar","description":"A young, bright pulsar in the Vela supernova remnant, spinning about eleven times a second. It is the classic glitching pulsar — famous for sudden small speed-ups in its rotation that reveal the superfluid interior of a neutron star — and one of the brightest gamma-ray sources in the sky.","aliases":["PSR B0833−45"],"sources":["nasa"]},{"id":"neutron_star:psr-b1919-21","type":"neutron_star","name":"PSR B1919+21","domain":"science","entryPath":"/compact-objects/psr-b1919-21","description":"The first pulsar ever discovered, found by Jocelyn Bell Burnell and Antony Hewish in 1967 as a startlingly regular radio signal once labelled 'LGM-1' for Little Green Men. Its 1.337-second pulses opened the study of neutron stars; the discovery is commemorated on the cover of Joy Division's album Unknown Pleasures.","aliases":["The first pulsar","CP 1919"],"sources":["nasa"]},{"id":"neutron_star:psr-j0740-6620","type":"neutron_star","name":"PSR J0740+6620","domain":"science","entryPath":"/compact-objects/psr-j0740-6620","description":"One of the most massive neutron stars known, at about 2.08 solar masses, weighed through the Shapiro delay of its pulses. Its radius has been measured by NASA's NICER X-ray telescope, and together the mass and radius are among the tightest constraints on the neutron-star equation of state and how dense matter behaves.","sources":["nasa"]},{"id":"physics_concept:wave-function","type":"physics_concept","name":"The Wave Function","domain":"science","entryPath":"/fundamental-physics/wave-function","description":"The mathematical object that captures everything knowable about a quantum system; its squared magnitude gives the probability of finding a particle in a given state. Wave functions underlie the discrete energy levels of atoms — and therefore the spectral lines that let astronomers read the composition, temperature, and motion of distant stars and gas.","sources":["nasa"]},{"id":"physics_concept:quantum-superposition","type":"physics_concept","name":"Quantum Superposition","domain":"science","entryPath":"/fundamental-physics/quantum-superposition","description":"The principle that a quantum system can exist in a combination of states at once until it is measured, when a single outcome is realised. It is the heart of quantum weirdness and of quantum computing, and it is the reason atomic transitions and particle interactions must be described in probabilities rather than certainties.","sources":["nasa"]},{"id":"physics_concept:quantum-entanglement","type":"physics_concept","name":"Quantum Entanglement","domain":"science","entryPath":"/fundamental-physics/quantum-entanglement","description":"A deep correlation between quantum particles such that measuring one instantly fixes the state of the other, however far apart they are — what Einstein called 'spooky action at a distance.' Confirmed in ever-more-stringent experiments, it does not allow faster-than-light signalling and is a foundation of quantum information science.","sources":["nasa"]},{"id":"physics_concept:heisenberg-uncertainty-principle","type":"physics_concept","name":"The Heisenberg Uncertainty Principle","domain":"science","entryPath":"/fundamental-physics/heisenberg-uncertainty-principle","description":"The fundamental limit that a particle's position and momentum cannot both be known with arbitrary precision — a property of quantum nature itself, not of imperfect instruments. Together with the Pauli exclusion principle it sets the scale of the degeneracy pressure — the resistance of fermions such as electrons and neutrons to being crowded together — that holds up white dwarfs and neutron stars against gravity.","aliases":["Uncertainty principle"],"sources":["nasa"]},{"id":"physics_concept:wave-particle-duality","type":"physics_concept","name":"Wave–Particle Duality","domain":"science","entryPath":"/fundamental-physics/wave-particle-duality","description":"The finding that light and matter each behave as both waves and particles depending on how they are observed — light as photons in the photoelectric effect, electrons as interfering waves in a double slit. It reconciled centuries of debate about the nature of light and underlies how detectors count the photons that carry astronomy's information.","sources":["nasa"]},{"id":"physics_concept:quantum-spin","type":"physics_concept","name":"Quantum Spin","domain":"science","entryPath":"/fundamental-physics/quantum-spin","description":"An intrinsic form of angular momentum carried by particles, quantised in units of the reduced Planck constant and unrelated to any literal spinning. Spin divides particles into fermions and bosons and, through the Pauli exclusion principle, into the electron shells of atoms; the spin-flip of hydrogen produces the 21-centimetre radio line that maps neutral gas across the Galaxy.","sources":["nasa"]},{"id":"physics_concept:quantum-tunneling","type":"physics_concept","name":"Quantum Tunneling","domain":"science","entryPath":"/fundamental-physics/quantum-tunneling","description":"The quantum ability of a particle to cross an energy barrier it classically could not surmount. Tunnelling lets protons in the Sun's core fuse despite their electrical repulsion — without it the Sun could not shine — and it is central to the theory of how radiation escapes a black hole.","sources":["nasa"]},{"id":"physics_concept:zero-point-energy","type":"physics_concept","name":"Zero-Point Energy","domain":"science","entryPath":"/fundamental-physics/zero-point-energy","description":"The lowest possible energy of a quantum system, which is never zero — even empty space seethes with quantum fluctuations. This vacuum energy is a real, measured effect (the Casimir force), and its possible connection to the accelerating expansion of the Universe is one of the deepest open problems in physics.","sources":["nasa"]},{"id":"physics_concept:quantum-decoherence","type":"physics_concept","name":"Quantum Decoherence","domain":"science","entryPath":"/fundamental-physics/quantum-decoherence","description":"The process by which a quantum system loses its delicate superposition through unavoidable interaction with its environment, giving rise to the definite, classical world we observe. Decoherence explains why quantum weirdness is hard to see at everyday scales and is a central challenge for building quantum computers.","sources":["nasa"]},{"id":"physics_concept:elementary-particle","type":"physics_concept","name":"Elementary Particles","domain":"science","entryPath":"/fundamental-physics/elementary-particle","description":"The fundamental constituents of matter and force in the Standard Model — the quarks and leptons that make up matter, and the force-carrying bosons. Everything from a star to a galaxy is built from a handful of these particles, and understanding them connects the physics of the very small to the structure of the whole Universe.","sources":["nasa"]},{"id":"physics_concept:fundamental-forces","type":"physics_concept","name":"The Fundamental Forces","domain":"science","entryPath":"/fundamental-physics/fundamental-forces","description":"The four basic interactions of nature — gravity, electromagnetism, and the strong and weak nuclear forces. Together they govern everything from the fusion that powers stars to the collapse of a massive core, and unifying them, especially gravity with the quantum forces, remains a central goal of physics.","aliases":["The four fundamental interactions"],"sources":["nasa"]},{"id":"physics_concept:higgs-boson","type":"physics_concept","name":"The Higgs Boson","domain":"science","entryPath":"/fundamental-physics/higgs-boson","description":"The particle associated with the Higgs field, which gives many elementary particles their mass. Predicted in the 1960s and discovered at CERN's Large Hadron Collider in 2012, it completed the Standard Model; the origin of mass it explains is fundamental to why matter — and therefore stars and galaxies — exists as it does.","sources":["nasa"]},{"id":"physics_concept:neutrino","type":"physics_concept","name":"The Neutrino","domain":"science","entryPath":"/fundamental-physics/neutrino","description":"A tiny, electrically neutral particle that interacts only very weakly and so streams almost unimpeded through matter — trillions pass through you each second. Neutrinos are produced in the Sun's core, in supernovae, and by cosmic rays, and detecting them opens a window onto processes hidden from light, a pillar of multi-messenger astronomy.","sources":["nasa"]},{"id":"physics_concept:neutrino-oscillation","type":"physics_concept","name":"Neutrino Oscillation","domain":"science","entryPath":"/fundamental-physics/neutrino-oscillation","description":"The quantum phenomenon in which a neutrino changes flavour — electron, muon, or tau — as it travels. Its discovery proved that neutrinos have a small mass, resolved the decades-old 'solar neutrino problem' of the Sun apparently producing too few, and was recognised with the 2015 Nobel Prize in Physics.","sources":["nasa"]},{"id":"physics_concept:antimatter","type":"physics_concept","name":"Antimatter","domain":"science","entryPath":"/fundamental-physics/antimatter","description":"Matter's mirror image — particles with the same mass but opposite charge, such as the positron discovered in cosmic rays in 1932. When matter and antimatter meet they annihilate into pure energy. Antiparticles are produced in high-energy astrophysical environments and are detected in cosmic rays reaching the Earth.","sources":["nasa"]},{"id":"physics_concept:matter-antimatter-asymmetry","type":"physics_concept","name":"Matter–Antimatter Asymmetry","domain":"science","entryPath":"/fundamental-physics/matter-antimatter-asymmetry","description":"The unexplained fact that the Universe is made almost entirely of matter, even though the Big Bang should have produced matter and antimatter in equal amounts, which would have annihilated completely. Why a tiny excess of matter survived — the problem of baryogenesis — is one of the great open questions in physics and cosmology.","aliases":["Baryon asymmetry"],"sources":["nasa"]},{"id":"physics_concept:mass-energy-equivalence","type":"physics_concept","name":"Mass–Energy Equivalence","domain":"science","entryPath":"/fundamental-physics/mass-energy-equivalence","description":"Einstein's result that mass and energy are two forms of the same thing, related by the speed of light squared. It is the accounting behind starlight: fusing hydrogen into helium in the Sun's core converts about four million tonnes of mass into energy every second, and it governs the annihilation of matter with antimatter.","sources":["nasa"]},{"id":"physics_concept:time-dilation","type":"physics_concept","name":"Time Dilation","domain":"science","entryPath":"/fundamental-physics/time-dilation","description":"The relativistic effect by which time runs slower for fast-moving observers and deeper in a gravitational field. It is measured every day — GPS satellites must correct for it — and it steepens near neutron stars and black holes, where clocks near the horizon crawl relative to distant ones. Even distant supernovae are seen to fade in slow motion as the Universe expands.","sources":["nasa"]},{"id":"physics_concept:length-contraction","type":"physics_concept","name":"Length Contraction","domain":"science","entryPath":"/fundamental-physics/length-contraction","description":"The relativistic shortening of an object along its direction of motion as seen by an observer it moves past, becoming dramatic near the speed of light. It is the companion of time dilation, and it explains how short-lived muons created high in the atmosphere by cosmic rays still reach the ground.","sources":["nasa"]},{"id":"physics_concept:equivalence-principle","type":"physics_concept","name":"The Equivalence Principle","domain":"science","entryPath":"/fundamental-physics/equivalence-principle","description":"The principle that gravitational and inertial mass are identical, so that being in free fall is locally indistinguishable from floating in empty space. This insight led Einstein from special to general relativity, recasting gravity as the curvature of spacetime; it is tested to extraordinary precision by lunar laser ranging and dedicated satellites.","sources":["nasa"]},{"id":"physics_concept:quantum-fluctuations","type":"physics_concept","name":"Quantum Fluctuations","domain":"science","entryPath":"/fundamental-physics/quantum-fluctuations","description":"Fleeting, unavoidable variations in the energy of a field, permitted by the uncertainty principle. Stretched to astronomical size during cosmic inflation, tiny quantum fluctuations are believed to have seeded the density variations we now see imprinted on the cosmic microwave background and grown into galaxies and clusters.","sources":["nasa"]},{"id":"physics_concept:vacuum-energy","type":"physics_concept","name":"Vacuum Energy","domain":"science","entryPath":"/fundamental-physics/vacuum-energy","description":"The energy that fills empty space even in the absence of matter or radiation, arising from quantum fields in their lowest state. Vacuum energy is a leading candidate for the dark energy driving cosmic acceleration and is closely tied to the cosmological constant in Einstein's equations.","sources":["nasa"]},{"id":"physics_concept:cosmological-constant-problem","type":"physics_concept","name":"The Cosmological Constant Problem","domain":"science","entryPath":"/fundamental-physics/cosmological-constant-problem","description":"The vast mismatch between the tiny dark-energy density measured in the Universe and the enormous vacuum energy that naive quantum theory predicts — a discrepancy of many tens of orders of magnitude. Often called the worst prediction in physics, it remains one of the deepest unsolved problems where quantum theory meets gravity.","sources":["nasa"]},{"id":"physics_concept:cosmic-neutrino-background","type":"physics_concept","name":"The Cosmic Neutrino Background","domain":"science","entryPath":"/fundamental-physics/cosmic-neutrino-background","description":"A sea of relic neutrinos released about one second after the Big Bang, when the young Universe became transparent to them — the neutrino analogue of the cosmic microwave background. Its existence is strongly supported by its imprint on primordial element abundances and the microwave background, though the neutrinos themselves are far too low in energy to have been detected directly.","aliases":["Relic neutrinos","CνB"],"sources":["nasa"]},{"id":"physics_concept:gzk-limit","type":"physics_concept","name":"The GZK Limit","domain":"science","entryPath":"/fundamental-physics/gzk-limit","description":"A theoretical ceiling on the energy of cosmic-ray protons that reach us from far away: above roughly 5×10¹⁹ electronvolts they collide with cosmic-microwave-background photons and lose energy, so the highest-energy cosmic rays must originate relatively nearby. Observatories studying the ultra-high-energy sky test this predicted cutoff.","aliases":["Greisen–Zatsepin–Kuzmin cutoff"],"sources":["nasa"]},{"id":"space_engineering_concept:electric-propulsion","type":"space_engineering_concept","name":"Electric Propulsion","domain":"science","entryPath":"/space-engineering/electric-propulsion","description":"A family of thrusters that accelerate propellant using electrical energy rather than combustion, reaching exhaust velocities several times higher than chemical rockets. The trade is thrust: forces are gentle — millinewtons to newtons — so electric propulsion excels at station-keeping and patient deep-space cruises, as NASA's Dawn demonstrated in reaching both Vesta and Ceres.","sources":["nasa"]},{"id":"space_engineering_concept:nuclear-electric-propulsion","type":"space_engineering_concept","name":"Nuclear Electric Propulsion","domain":"science","entryPath":"/space-engineering/nuclear-electric-propulsion","description":"An architecture that pairs a space nuclear reactor with electric thrusters: the reactor generates electricity, which drives ion or Hall thrusters. Unlike solar-electric propulsion it is independent of distance from the Sun, making it a candidate for crewed missions to Mars and the outer Solar System. No nuclear-electric system has yet flown; it remains a design and technology-development goal.","aliases":["NEP"],"sources":["nasa"]},{"id":"space_engineering_concept:vasimr","type":"space_engineering_concept","name":"VASIMR","domain":"science","entryPath":"/space-engineering/vasimr","description":"An electric-propulsion concept that heats propellant to a plasma with radio waves and confines and exhausts it with magnetic fields, in principle allowing the exhaust velocity to be tuned in flight. It has been tested on the ground but has not flown in space, and operating it at useful power levels would require an electrical source far beyond today's spacecraft.","aliases":["Variable Specific Impulse Magnetoplasma Rocket"],"sources":["nasa"]},{"id":"space_engineering_concept:arcjet","type":"space_engineering_concept","name":"Arcjet Thruster","domain":"science","entryPath":"/space-engineering/arcjet","description":"An electrothermal thruster that passes propellant through an electric arc, heating it far beyond what a chemical reaction alone allows before it expands through a nozzle. Arcjets have flown operationally for satellite station-keeping, offering higher exhaust velocity than cold-gas or simple resistojet systems.","sources":["nasa"]},{"id":"space_engineering_concept:resistojet","type":"space_engineering_concept","name":"Resistojet Thruster","domain":"science","entryPath":"/space-engineering/resistojet","description":"The simplest electric thruster: propellant is warmed by flowing over an electrically heated element and then expelled through a nozzle. Modest but reliable, resistojets have long been used for satellite attitude control and station-keeping, bridging cold-gas systems and higher-performance electric propulsion.","sources":["nasa"]},{"id":"space_engineering_concept:solar-sail","type":"space_engineering_concept","name":"Solar Sail","domain":"science","entryPath":"/space-engineering/solar-sail","description":"Propulsion with no propellant at all: a large, lightweight reflective sail is pushed by the momentum of sunlight itself. The thrust is minute but continuous and free, building up large velocity changes over time. Japan's IKAROS proved the principle in interplanetary space in 2010, and The Planetary Society's LightSail 2 demonstrated sail-raised orbits around Earth.","sources":["nasa"]},{"id":"space_engineering_concept:monopropellant","type":"space_engineering_concept","name":"Monopropellant Propulsion","domain":"science","entryPath":"/space-engineering/monopropellant","description":"A simple chemical system in which a single propellant — classically hydrazine — is decomposed over a catalyst bed to produce hot gas, needing no separate oxidiser or ignition. Monopropellant thrusters are workhorses for spacecraft attitude control and small maneuvers, valued for their simplicity and quick, repeatable pulses.","sources":["nasa"]},{"id":"space_engineering_concept:bipropellant","type":"space_engineering_concept","name":"Bipropellant Propulsion","domain":"science","entryPath":"/space-engineering/bipropellant","description":"A chemical system that burns a separate fuel and oxidiser, releasing far more energy than a monopropellant and delivering higher exhaust velocity. Bipropellant engines — from hypergolic storable combinations to cryogenic hydrogen–oxygen — power launch vehicles, orbit-insertion burns, and deep-space main engines.","sources":["nasa"]},{"id":"space_engineering_concept:staged-combustion-cycle","type":"space_engineering_concept","name":"Staged-Combustion Cycle","domain":"science","entryPath":"/space-engineering/staged-combustion-cycle","description":"A high-efficiency rocket-engine power cycle in which propellant burned in a preburner drives the turbopumps and is then routed into the main chamber, so almost none is wasted. It is harder to build than the simpler gas-generator cycle but yields higher performance; the Space Shuttle's RS-25 used it, and SpaceX's Raptor uses the even more demanding full-flow staged-combustion variant.","sources":["nasa"]},{"id":"space_engineering_concept:tsiolkovsky-rocket-equation","type":"space_engineering_concept","name":"The Tsiolkovsky Rocket Equation","domain":"science","entryPath":"/space-engineering/tsiolkovsky-rocket-equation","description":"The founding relation of astronautics, derived by Konstantin Tsiolkovsky in 1903: the velocity change a rocket can achieve equals its exhaust velocity times the natural logarithm of the ratio of its starting mass to its empty mass. Because the mass ratio enters logarithmically, reaching high Δv demands either very high exhaust velocity or an impractically large fraction of propellant — the 'tyranny' that shapes every mission design.","aliases":["The ideal rocket equation"],"sources":["nasa"]},{"id":"space_engineering_concept:specific-impulse","type":"space_engineering_concept","name":"Specific Impulse","domain":"science","entryPath":"/space-engineering/specific-impulse","description":"The standard measure of a rocket's fuel efficiency: the thrust produced per unit weight-flow of propellant, expressed in seconds. Higher specific impulse means more velocity change from the same propellant. Chemical engines reach roughly 300–450 seconds; electric thrusters, trading thrust for efficiency, reach thousands.","aliases":["Isp"],"sources":["nasa"]},{"id":"space_engineering_concept:thrust-to-weight-ratio","type":"space_engineering_concept","name":"Thrust-to-Weight Ratio","domain":"science","entryPath":"/space-engineering/thrust-to-weight-ratio","description":"The ratio of an engine's or vehicle's thrust to its weight. To lift off, a launch vehicle's thrust must exceed its weight — a thrust-to-weight ratio above one — while efficient upper-stage and in-space engines can operate well below one. It is the counterpoint to specific impulse: high-thrust engines often trade away efficiency, and vice versa.","sources":["nasa"]},{"id":"space_engineering_concept:delta-v-budget","type":"space_engineering_concept","name":"The Delta-v Budget","domain":"science","entryPath":"/space-engineering/delta-v-budget","description":"An accounting of every velocity change a mission requires — launch to orbit, orbital transfers, planetary capture, landing, and margins — summed into a total 'delta-v budget' that the propulsion system must deliver. Comparing the budget against what the rocket equation allows is the central feasibility check of mission design.","aliases":["Δv budget"],"sources":["nasa"]},{"id":"space_engineering_concept:rocket-staging","type":"space_engineering_concept","name":"Rocket Staging","domain":"science","entryPath":"/space-engineering/rocket-staging","description":"The practice of discarding spent tanks and engines during ascent so the rocket no longer has to accelerate empty mass. Staging sidesteps the rocket equation's steep penalty on mass ratio and is how essentially every orbital launch vehicle reaches space — from the Saturn V's three stages to the Falcon 9's two.","aliases":["Multistage rocket"],"sources":["nasa"]},{"id":"space_engineering_concept:thrust-vector-control","type":"space_engineering_concept","name":"Thrust Vector Control","domain":"science","entryPath":"/space-engineering/thrust-vector-control","description":"Steering a rocket by aiming its thrust — most often by gimballing the engines on hydraulic or electric actuators, and sometimes with vanes or differential throttling. Because a climbing rocket is aerodynamically unstable, thrust vector control is what keeps it pointed and on course from liftoff through staging.","aliases":["TVC","Engine gimballing"],"sources":["nasa"]},{"id":"space_engineering_concept:orbital-rendezvous","type":"space_engineering_concept","name":"Orbital Rendezvous","domain":"science","entryPath":"/space-engineering/orbital-rendezvous","description":"The guided approach of two spacecraft to the same orbit and position so they can dock or berth — a delicate dance governed by orbital mechanics, where firing to speed up raises the orbit and paradoxically slows the chase down on a target ahead, while slowing down drops into a lower, faster orbit that catches up. First achieved by Gemini in 1965, rendezvous is the foundation of space-station crew and cargo flights and of in-space assembly.","sources":["nasa"]},{"id":"space_engineering_concept:station-keeping","type":"space_engineering_concept","name":"Station-Keeping","domain":"science","entryPath":"/space-engineering/station-keeping","description":"The small, regular maneuvers that hold a spacecraft in its intended orbit or slot against perturbations — atmospheric drag, the Moon and Sun's pull, and the Earth's uneven gravity. Geostationary satellites, for instance, must be nudged north–south and east–west to stay on station, a task increasingly handed to efficient electric thrusters.","sources":["nasa"]},{"id":"space_engineering_concept:aerobraking","type":"space_engineering_concept","name":"Aerobraking","domain":"science","entryPath":"/space-engineering/aerobraking","description":"Using repeated shallow passes through the upper fringe of a planet's atmosphere to shed orbital energy through drag, gradually shrinking a large capture orbit into the desired one — trading time for a large saving in propellant. NASA's Mars orbiters, including Mars Global Surveyor and Mars Reconnaissance Orbiter, used months of aerobraking to reach their science orbits.","sources":["nasa"]},{"id":"space_engineering_concept:aerocapture","type":"space_engineering_concept","name":"Aerocapture","domain":"science","entryPath":"/space-engineering/aerocapture","description":"A single, deep pass through a planet's atmosphere to slow a spacecraft enough for orbital capture in one stroke, behind a heat shield — far faster than aerobraking but far more demanding, requiring precise guidance and thermal protection. It has been studied and validated in analysis but has not yet been used on a planetary mission.","sources":["nasa"]},{"id":"space_engineering_concept:gravity-turn","type":"space_engineering_concept","name":"Gravity-Turn Ascent","domain":"science","entryPath":"/space-engineering/gravity-turn","description":"The efficient launch trajectory in which a rocket pitches over slightly after liftoff and then lets gravity gradually bend its path toward the horizontal, keeping the vehicle aligned with its velocity to minimise aerodynamic loads and steering losses. Nearly every orbital launch follows a gravity-turn profile from the pad to orbit.","sources":["nasa"]},{"id":"exoplanet_science_concept:transmission-spectroscopy","type":"exoplanet_science_concept","name":"Transmission Spectroscopy","domain":"science","entryPath":"/exoplanet-science/transmission-spectroscopy","description":"The workhorse of exoplanet atmospheres: as a planet transits its star, a sliver of starlight filters through the ring of atmosphere at its edge, and the gases there imprint absorption features that vary with wavelength. Comparing the planet's apparent size across a spectrum reveals which molecules — water, carbon dioxide, methane — are present. JWST has made this a routine, high-precision technique.","sources":["nasa"]},{"id":"exoplanet_science_concept:emission-spectroscopy","type":"exoplanet_science_concept","name":"Emission Spectroscopy","domain":"science","entryPath":"/exoplanet-science/emission-spectroscopy","description":"Measuring the light a planet itself emits — usually its thermal glow — to probe the temperature structure and composition of its dayside. Because the planet's emission is measured against the star, it is easiest for hot planets, and it reveals whether temperature rises or falls with altitude in ways transmission spectra cannot.","sources":["nasa"]},{"id":"exoplanet_science_concept:secondary-eclipse","type":"exoplanet_science_concept","name":"The Secondary Eclipse","domain":"science","entryPath":"/exoplanet-science/secondary-eclipse","description":"The moment a planet passes behind its star. The dip in the system's combined light equals the light the planet was contributing, so subtracting the two isolates the planet's thermal emission and reflected light — the basis of emission spectroscopy and dayside temperature measurements.","aliases":["Occultation"],"sources":["nasa"]},{"id":"exoplanet_science_concept:phase-curve","type":"exoplanet_science_concept","name":"Phase Curves","domain":"science","entryPath":"/exoplanet-science/phase-curve","description":"Tracking a planet's brightness through its whole orbit as its illuminated fraction changes, like the phases of the Moon. The shape of the curve reveals the temperature difference between day and night sides and how efficiently winds carry heat around the planet — a direct window onto atmospheric circulation.","sources":["nasa"]},{"id":"exoplanet_science_concept:atmospheric-retrieval","type":"exoplanet_science_concept","name":"Atmospheric Retrieval","domain":"science","entryPath":"/exoplanet-science/atmospheric-retrieval","description":"The statistical machinery that turns a spectrum into numbers: models of an atmosphere are compared against the data, usually with Bayesian inference, to find the mix of gases, temperatures, and clouds that best explains it — along with honest uncertainties. Retrieval is how a wiggly spectrum becomes a measured abundance.","sources":["nasa"]},{"id":"exoplanet_science_concept:high-resolution-cross-correlation-spectroscopy","type":"exoplanet_science_concept","name":"High-Resolution Cross-Correlation Spectroscopy","domain":"science","entryPath":"/exoplanet-science/high-resolution-cross-correlation-spectroscopy","description":"A ground-based technique that resolves thousands of individual spectral lines and uses the planet's changing Doppler shift along its orbit to separate its light from the star's and the Earth's atmosphere. Cross-correlating against molecular templates detects specific gases and even measures atmospheric winds; it is a headline science case for the coming extremely large telescopes.","aliases":["HRCCS"],"sources":["nasa"]},{"id":"exoplanet_science_concept:rossiter-mclaughlin-effect","type":"exoplanet_science_concept","name":"The Rossiter–McLaughlin Effect","domain":"science","entryPath":"/exoplanet-science/rossiter-mclaughlin-effect","description":"A spectroscopic signature seen during transit: as the planet crosses the face of its rotating star, it blocks first the approaching then the receding limb, distorting the star's measured velocity. The shape of that distortion reveals whether the planet's orbit is aligned with the star's spin — a key clue to how the system formed and migrated.","sources":["nasa"]},{"id":"exoplanet_science_concept:clouds-and-hazes","type":"exoplanet_science_concept","name":"Clouds & Hazes","domain":"science","entryPath":"/exoplanet-science/clouds-and-hazes","description":"Condensate clouds and photochemically produced hazes are common in exoplanet atmospheres, and they matter for observers: high-altitude aerosols mute or flatten the features in a transmission spectrum, masking the gases below. Distinguishing a genuinely cloudy atmosphere from a clear one is a central challenge of characterization.","aliases":["Aerosols"],"sources":["nasa"]},{"id":"exoplanet_science_concept:thermal-inversion","type":"exoplanet_science_concept","name":"Thermal Inversion","domain":"science","entryPath":"/exoplanet-science/thermal-inversion","description":"A layer in which temperature rises with altitude rather than falling, created when high-altitude absorbers soak up starlight — the exoplanet analogue of Earth's ozone stratosphere. On the hottest giant planets, absorbers such as titanium oxide or metals can drive inversions, which flip molecular features in an emission spectrum from absorption to emission.","aliases":["Stratosphere"],"sources":["nasa"]},{"id":"exoplanet_science_concept:equilibrium-temperature","type":"exoplanet_science_concept","name":"Equilibrium Temperature","domain":"science","entryPath":"/exoplanet-science/equilibrium-temperature","description":"The temperature a planet would settle at if it simply balanced the starlight it absorbs against the heat it radiates, set by the star's output, the orbital distance, and the planet's reflectivity. It is a first estimate — real atmospheres shift it through greenhouse warming and heat redistribution — but it frames where a world sits relative to the habitable zone.","sources":["nasa"]},{"id":"exoplanet_science_concept:atmospheric-metallicity","type":"exoplanet_science_concept","name":"Atmospheric Metallicity & C/O Ratio","domain":"science","entryPath":"/exoplanet-science/atmospheric-metallicity","description":"The enrichment of an atmosphere in elements heavier than hydrogen and helium, and the ratio of carbon to oxygen within it. These quantities are more than bookkeeping: because different ices and gases condense at different distances in the disk, a planet's measured metallicity and C/O ratio carry a fingerprint of where and how it formed.","sources":["nasa"]},{"id":"exoplanet_science_concept:core-accretion","type":"exoplanet_science_concept","name":"Core Accretion","domain":"science","entryPath":"/exoplanet-science/core-accretion","description":"The leading model of planet formation: dust in a protoplanetary disk sticks into ever-larger bodies until a solid core grows massive enough — roughly ten Earth masses — to pull in a thick envelope of gas, becoming a giant planet. It naturally explains rocky planets, ice giants, and gas giants as a sequence, though building cores fast enough before the gas disperses is a live problem.","sources":["nasa"]},{"id":"exoplanet_science_concept:disk-instability","type":"exoplanet_science_concept","name":"Disk Instability","domain":"science","entryPath":"/exoplanet-science/disk-instability","description":"An alternative route to giant planets in which a massive, cool region of a protoplanetary disk becomes gravitationally unstable and fragments directly into a bound clump of gas, skipping the slow core-building step. It may account for massive planets on wide orbits that are hard to make by core accretion within the disk's lifetime.","sources":["nasa"]},{"id":"exoplanet_science_concept:planetary-migration","type":"exoplanet_science_concept","name":"Planetary Migration","domain":"science","entryPath":"/exoplanet-science/planetary-migration","description":"Planets do not necessarily stay where they form: gravitational interaction with the gas disk, or later with other bodies, can move them inward or outward over time. Migration is the standard explanation for hot Jupiters — giant planets on scorching close-in orbits where they could not have formed — and shapes the architecture of whole systems.","sources":["nasa"]},{"id":"exoplanet_science_concept:snow-line","type":"exoplanet_science_concept","name":"The Snow Line","domain":"science","entryPath":"/exoplanet-science/snow-line","description":"The distance from a young star beyond which it is cold enough for a volatile such as water to freeze into ice. Past the snow line the supply of solid material jumps, favouring the rapid growth of massive cores — one reason the Solar System's giant planets lie beyond it — and its location leaves an imprint on a planet's later atmospheric composition.","aliases":["Frost line"],"sources":["nasa"]},{"id":"exoplanet_science_concept:pebble-accretion","type":"exoplanet_science_concept","name":"Pebble Accretion","domain":"science","entryPath":"/exoplanet-science/pebble-accretion","description":"A mechanism that helps solve core accretion's timing problem: centimetre-sized 'pebbles' drifting inward through the disk are efficiently swept up by a growing embryo, letting cores reach giant-planet mass far faster than by collisions of larger bodies alone. It has become a central ingredient in modern planet-formation theory.","sources":["nasa"]},{"id":"space_telescope:ariel","type":"space_telescope","name":"Ariel (exoplanet mission)","domain":"science","entryPath":"/exoplanet-science/ariel","description":"The European Space Agency's Ariel is the first mission dedicated to surveying the atmospheres of a large, diverse sample of known exoplanets — around a thousand — chiefly by transmission and emission spectroscopy at infrared wavelengths. Selected as ESA's fourth medium-class mission and planned for launch in 2029, it aims to link atmospheric composition to how and where planets form.","aliases":["ARIEL","Atmospheric Remote-sensing Infrared Exoplanet Large-survey"],"sources":["nasa"]},{"id":"space_telescope:plato","type":"space_telescope","name":"PLATO (exoplanet mission)","domain":"science","entryPath":"/exoplanet-science/plato","description":"PLATO is a European Space Agency mission that will hunt for terrestrial planets in the habitable zones of bright, Sun-like stars using an array of small telescopes to watch for transits, while asteroseismology of the host stars pins down their ages and sizes. Selected as ESA's third medium-class mission, it is planned for launch in 2026.","aliases":["PLATO","PLAnetary Transits and Oscillations of stars"],"sources":["nasa"]},{"id":"catalog:caldwell","type":"catalog","name":"Caldwell Catalogue","domain":"science","entryPath":"/sky-catalogs/caldwell","description":"A list of 109 bright deep-sky objects compiled by the British amateur astronomer Sir Patrick Moore to complement the Messier Catalogue, which it deliberately avoids duplicating. Ordered by declination and spanning both hemispheres, it gathers showpiece galaxies, clusters, and nebulae — such as the Hyades and NGC 869/884 — that Messier omitted. Objects carry a 'C' number.","aliases":["Caldwell"],"sources":["iau"]},{"id":"catalog:barnard","type":"catalog","name":"Barnard Catalogue of Dark Nebulae","domain":"science","entryPath":"/sky-catalogs/barnard","description":"The first systematic catalogue of dark nebulae, compiled by Edward Emerson Barnard from his pioneering photographs of the Milky Way. The 1919 list of 182 objects was later extended to 370; each 'B' object is a cloud of interstellar dust silhouetted against the star fields behind it, such as B33, the Horsehead Nebula.","aliases":["Barnard Catalogue","Barnard's Catalogue of Dark Markings"],"sources":["iau"]},{"id":"catalog:sharpless","type":"catalog","name":"Sharpless Catalogue","domain":"science","entryPath":"/sky-catalogs/sharpless","description":"A catalogue of HII regions — clouds of ionised hydrogen glowing around hot young stars — compiled by Stewart Sharpless. Its second edition (Sh2, 1959) lists 313 emission nebulae across the northern Milky Way, including many of the sky's great star-forming complexes. Objects carry an 'Sh2' number.","aliases":["Sh2","Sharpless HII Region Catalogue"],"sources":["iau"]},{"id":"catalog:abell","type":"catalog","name":"Abell Catalogue","domain":"science","entryPath":"/sky-catalogs/abell","description":"Two catalogues compiled by George Abell. The 1958 catalogue of rich clusters of galaxies — later extended southward — became the standard reference for galaxy clusters, listing thousands of the densest concentrations in the Universe. Separately, Abell catalogued 86 large, faint planetary nebulae. Objects carry an 'Abell' number in both.","aliases":["Abell Cluster Catalogue"],"sources":["iau"]},{"id":"catalog:pgc-catalogue","type":"catalog","name":"Principal Galaxies Catalogue (PGC)","domain":"science","entryPath":"/sky-catalogs/pgc-catalogue","description":"A comprehensive catalogue of galaxies begun by Paturel and collaborators, providing a unique 'PGC' identifier, position, and basic parameters for tens of thousands of galaxies. It forms the backbone of the HyperLEDA database, and its PGC numbers are widely used as a standard cross-reference for galaxies lacking a common name.","aliases":["PGC","LEDA"],"sources":["iau"]},{"id":"catalog:ugc-catalogue","type":"catalog","name":"Uppsala General Catalogue of Galaxies (UGC)","domain":"science","entryPath":"/sky-catalogs/ugc-catalogue","description":"A catalogue of 12,921 galaxies north of declination −02°30′, compiled by Peter Nilson at Uppsala from the Palomar Sky Survey. Selected mainly by apparent size, it was for decades the most complete catalogue of nearby northern galaxies and remains a common cross-reference; objects carry a 'UGC' number.","aliases":["UGC"],"sources":["iau"]},{"id":"catalog:gliese-catalogue","type":"catalog","name":"Gliese Catalogue of Nearby Stars","domain":"science","entryPath":"/sky-catalogs/gliese-catalogue","description":"The standard catalogue of stars in the immediate solar neighbourhood, begun by Wilhelm Gliese and later extended with Hartmut Jahreiß. It lists the stars known to lie within about 25 parsecs of the Sun, with distances and motions; its 'GJ' (or older 'Gl') numbers are the usual designations for nearby red dwarfs and other close stars.","aliases":["Gliese Catalogue","CNS","Gl"],"sources":["iau"]},{"id":"catalog:tycho-catalogue","type":"catalog","name":"Tycho-2 Catalogue","domain":"science","entryPath":"/sky-catalogs/tycho-catalogue","description":"An astrometric and photometric catalogue of about 2.5 million of the brightest stars, derived from the star-mapper data of ESA's Hipparcos satellite. Named in honour of Tycho Brahe, it provides positions, proper motions, and two-colour photometry, and its 'TYC' identifiers are a standard reference for stars fainter than the main Hipparcos catalogue.","aliases":["Tycho-2","Tycho Catalogue"],"sources":["iau"]},{"id":"catalog:sao-catalogue","type":"catalog","name":"SAO Star Catalog","domain":"science","entryPath":"/sky-catalogs/sao-catalogue","description":"A catalogue of 258,997 stars compiled by the Smithsonian Astrophysical Observatory, combining earlier positional catalogues to support satellite tracking. Its dense, uniform coverage and widely printed star atlas made 'SAO' numbers a long-standing standard designation for stars down to about ninth magnitude.","aliases":["Smithsonian Astrophysical Observatory Star Catalog"],"sources":["iau"]},{"id":"catalog:gcvs","type":"catalog","name":"General Catalogue of Variable Stars (GCVS)","domain":"science","entryPath":"/sky-catalogs/gcvs","description":"The authoritative catalogue of variable stars, first published in Moscow in 1948 and maintained since at the Sternberg Astronomical Institute. It assigns official variable-star designations and records variability type, period, and amplitude for tens of thousands of stars, serving as the reference for the naming of newly confirmed variables.","aliases":["GCVS"],"sources":["iau"]},{"id":"catalog:wds","type":"catalog","name":"Washington Double Star Catalog (WDS)","domain":"science","entryPath":"/sky-catalogs/wds","description":"The principal database of double and multiple stars, maintained by the United States Naval Observatory. It gathers positions, separations, position angles, and magnitudes for well over a hundred thousand pairs from centuries of measurements, and its 'WDS' identifiers are the standard reference for binary and multiple systems.","aliases":["WDS"],"sources":["usno"]},{"id":"catalog:lhs-catalogue","type":"catalog","name":"Luyten Half-Second Catalogue (LHS)","domain":"science","entryPath":"/sky-catalogs/lhs-catalogue","description":"A catalogue of stars with large proper motions — at least half an arcsecond per year — compiled by Willem Luyten from decades of photographic plate comparisons. Because high proper motion usually signals a nearby star, the 'LHS' catalogue is a rich hunting ground for the Sun's closest neighbours, including many faint red and white dwarfs.","aliases":["LHS","Luyten Half-Second"],"sources":["iau"]},{"id":"catalog:wolf-catalogue","type":"catalog","name":"Wolf Catalogue of High-Proper-Motion Stars","domain":"science","entryPath":"/sky-catalogs/wolf-catalogue","description":"An early catalogue of high-proper-motion stars assembled by Max Wolf, a pioneer of astrophotography, from his survey of moving stars. Its 'Wolf' numbers survive as designations for several well-known nearby stars — most famously Wolf 359, one of the closest stars to the Sun.","aliases":["Wolf Catalogue"],"sources":["iau"]},{"id":"catalog:bonner-durchmusterung","type":"catalog","name":"Bonner Durchmusterung (BD)","domain":"science","entryPath":"/sky-catalogs/bonner-durchmusterung","description":"The great pre-photographic survey of the northern sky, carried out under Friedrich Argelander at Bonn and published from 1863. It recorded positions and magnitudes for about 325,000 stars to roughly ninth magnitude — the most comprehensive star catalogue of its era — and its 'BD' designations remain in use for naked-eye and telescopic stars today.","aliases":["BD","Bonner Durchmusterung","Argelander Durchmusterung"],"sources":["iau"]},{"id":"catalog_family:deep-sky-visual-catalogs","type":"catalog_family","name":"Deep-Sky Visual Catalogues","domain":"science","entryPath":"/sky-catalogs/deep-sky-visual-catalogs","description":"The catalogues of bright deep-sky showpieces made for the eye and the small telescope — Charles Messier's eighteenth-century list of 'objects to avoid' when comet-hunting, and Patrick Moore's later Caldwell Catalogue that gathers the bright objects Messier passed over.","sources":["iau"]},{"id":"catalog_family:dreyer-general-catalogs","type":"catalog_family","name":"Dreyer's General Catalogues","domain":"science","entryPath":"/sky-catalogs/dreyer-general-catalogs","description":"The New General Catalogue and its two Index Catalogue supplements, compiled by J. L. E. Dreyer from the visual discoveries of the Herschels and their successors. Together the NGC and IC number nearly 13,000 galaxies, clusters, and nebulae and remain the most widely used designations for deep-sky objects.","sources":["iau"]},{"id":"catalog_family:nebula-catalogs","type":"catalog_family","name":"Nebula Catalogues","domain":"science","entryPath":"/sky-catalogs/nebula-catalogs","description":"The specialist catalogues of interstellar clouds — Sharpless's HII regions glowing around young stars, Barnard's dark dust clouds silhouetted against the Milky Way, and Abell's large, faint planetary nebulae. Together they map the gas and dust between the stars.","sources":["iau"]},{"id":"catalog_family:galaxy-catalogs","type":"catalog_family","name":"Galaxy Catalogues","domain":"science","entryPath":"/sky-catalogs/galaxy-catalogs","description":"The great reference catalogues of galaxies — the Uppsala General Catalogue's size-selected northern galaxies and the Principal Galaxies Catalogue that underpins the HyperLEDA database, providing standard identifiers for galaxies far beyond those with common names.","sources":["iau"]},{"id":"catalog_family:astrometric-star-catalogs","type":"catalog_family","name":"Astrometric Star Catalogues","domain":"science","entryPath":"/sky-catalogs/astrometric-star-catalogs","description":"The positional catalogues that pin down where the stars are — from Argelander's pre-photographic Bonner Durchmusterung and the Smithsonian's SAO catalogue to the space-based precision of Hipparcos, Tycho-2, and Gaia.","sources":["iau"]},{"id":"catalog_family:nearby-star-catalogs","type":"catalog_family","name":"Nearby-Star Catalogues","domain":"science","entryPath":"/sky-catalogs/nearby-star-catalogs","description":"The catalogues that map the Sun's immediate neighbourhood — Gliese's census of stars within about 25 parsecs, and the high-proper-motion catalogues of Luyten (LHS) and Max Wolf, whose fast-moving stars are usually the closest ones.","sources":["iau"]},{"id":"catalog_family:variable-and-double-star-catalogs","type":"catalog_family","name":"Variable & Double Star Catalogues","domain":"science","entryPath":"/sky-catalogs/variable-and-double-star-catalogs","description":"The catalogues of stars that change and stars that come in pairs — the General Catalogue of Variable Stars, which names and classifies variables, and the Washington Double Star Catalog, the master reference for binary and multiple systems.","sources":["iau"]},{"id":"designation_system:bayer-designation","type":"designation_system","name":"Bayer Designation","domain":"science","entryPath":"/sky-catalogs/bayer-designation","description":"The system introduced by Johann Bayer in his 1603 atlas Uranometria, labelling the bright stars of each constellation with a Greek letter followed by the Latin genitive of the constellation's name — so α Orionis is Betelgeuse, even though Rigel (β Orionis) is usually the brighter of the two, a reminder that the ordering is only approximate. Roughly in order of brightness, Bayer letters remain the most familiar designations for naked-eye stars.","aliases":["Bayer letters"],"sources":["iau"]},{"id":"designation_system:flamsteed-designation","type":"designation_system","name":"Flamsteed Designation","domain":"science","entryPath":"/sky-catalogs/flamsteed-designation","description":"A numbering scheme drawn from John Flamsteed's star catalogue, published posthumously in 1725, that labels the stars of each constellation with a number in order of increasing right ascension — so 61 Cygni is the sixty-first Flamsteed star of Cygnus. Flamsteed numbers name many stars that have no Bayer letter.","aliases":["Flamsteed numbers"],"sources":["iau"]},{"id":"designation_system:variable-star-designation","type":"designation_system","name":"Variable-Star Designation","domain":"science","entryPath":"/sky-catalogs/variable-star-designation","description":"The scheme for naming variable stars, formalised in the General Catalogue of Variable Stars. Within each constellation the first variables take the letters R through Z, then two-letter combinations RR through ZZ and AA through QZ, and thereafter V335, V336, and so on — a system that grew from a handful of early discoveries into a labelling scheme for tens of thousands of variables.","aliases":["Variable-star naming"],"sources":["iau"]},{"id":"astrophysical_object_class:deep-sky-object","type":"astrophysical_object_class","name":"Deep-Sky Object","domain":"science","entryPath":"/deep-sky-encyclopedia/deep-sky-object","description":"A catch-all term for any object beyond the Solar System that is neither a single star nor a planet — the star clusters, nebulae, and galaxies that fill catalogues from Messier to the NGC. Deep-sky objects are the classic targets of the amateur telescope and the workhorses of stellar and galactic astrophysics.","aliases":["DSO"],"sources":["nasa"]},{"id":"astrophysical_object_class:open-cluster","type":"astrophysical_object_class","name":"Open Cluster","domain":"science","entryPath":"/deep-sky-encyclopedia/open-cluster","description":"A loose, irregular group of a few dozen to a few thousand stars born together from the same molecular cloud, found in the disk of the Galaxy. Their stars share an age and composition, making open clusters key laboratories for stellar evolution; because they are only weakly bound, they gradually disperse over hundreds of millions of years.","aliases":["Galactic cluster"],"sources":["nasa"]},{"id":"astrophysical_object_class:globular-cluster","type":"astrophysical_object_class","name":"Globular Cluster","domain":"science","entryPath":"/deep-sky-encyclopedia/globular-cluster","description":"A dense, roughly spherical swarm of tens of thousands to millions of very old stars, tightly bound by gravity and orbiting in the halo of a galaxy. Globular clusters are among the oldest structures in the Universe, and their tightly packed, coeval stars make them benchmarks for stellar ages and the early history of the Galaxy.","sources":["nasa"]},{"id":"astrophysical_object_class:stellar-association","type":"astrophysical_object_class","name":"Stellar Association","domain":"science","entryPath":"/deep-sky-encyclopedia/stellar-association","description":"A loose grouping of young, massive stars that formed together but are not gravitationally bound, so they drift apart over tens of millions of years. OB associations trace the sites of recent star formation along a galaxy's spiral arms and are often still embedded in the gas of their parent clouds.","aliases":["OB association"],"sources":["nasa"]},{"id":"astrophysical_object_class:emission-nebula","type":"astrophysical_object_class","name":"Emission Nebula","domain":"science","entryPath":"/deep-sky-encyclopedia/emission-nebula","description":"A cloud of interstellar gas that glows with its own light, ionised by the ultraviolet radiation of nearby hot stars so that it re-emits in characteristic lines — most famously the red of hydrogen. Emission nebulae mark regions of active star formation and include the great HII regions of the Galaxy.","sources":["nasa"]},{"id":"astrophysical_object_class:hii-region","type":"astrophysical_object_class","name":"HII Region","domain":"science","entryPath":"/deep-sky-encyclopedia/hii-region","description":"A large cloud of ionised atomic hydrogen (H II) surrounding one or more hot O- and B-type stars, whose ultraviolet light strips the electrons from the surrounding gas. HII regions are the glowing signposts of massive-star formation, and their sizes and spectra are used to trace star formation across galaxies.","aliases":["H II region"],"sources":["nasa"]},{"id":"astrophysical_object_class:reflection-nebula","type":"astrophysical_object_class","name":"Reflection Nebula","domain":"science","entryPath":"/deep-sky-encyclopedia/reflection-nebula","description":"A cloud of interstellar dust that shines not by its own emission but by scattering the light of nearby stars. Because fine dust scatters blue light most efficiently, reflection nebulae typically appear blue — as in the wisps of nebulosity draped around the Pleiades.","sources":["nasa"]},{"id":"astrophysical_object_class:dark-nebula","type":"astrophysical_object_class","name":"Dark Nebula","domain":"science","entryPath":"/deep-sky-encyclopedia/dark-nebula","description":"A dense cloud of interstellar dust so opaque that it blots out the light of the stars and glowing gas behind it, appearing as a dark silhouette. Catalogued systematically by E. E. Barnard, dark nebulae are the cold, dusty reservoirs — often molecular clouds — from which new stars condense.","aliases":["Absorption nebula"],"sources":["nasa"]},{"id":"astrophysical_object_class:bok-globule","type":"astrophysical_object_class","name":"Bok Globule","domain":"science","entryPath":"/deep-sky-encyclopedia/bok-globule","description":"A small, dense, isolated cloud of cold gas and dust — a compact kind of dark nebula, named for Bart Bok — within which one or a few stars are collapsing into being. Bok globules are among the coldest objects in the Universe and are studied as the birthplaces of low-mass stars.","sources":["nasa"]},{"id":"astrophysical_object_class:planetary-nebula","type":"astrophysical_object_class","name":"Planetary Nebula","domain":"science","entryPath":"/deep-sky-encyclopedia/planetary-nebula","description":"The glowing shell of gas cast off by a dying Sun-like star as it becomes a white dwarf, ionised and lit up by the hot stellar core at its centre. Despite the name — coined because their round disks resembled planets in early telescopes — planetary nebulae have nothing to do with planets; they are a brief, beautiful final phase of low- and intermediate-mass stars.","sources":["nasa"]},{"id":"astrophysical_object_class:supernova-remnant","type":"astrophysical_object_class","name":"Supernova Remnant","domain":"science","entryPath":"/deep-sky-encyclopedia/supernova-remnant","description":"The expanding cloud of debris left behind when a star explodes as a supernova, sweeping up and shock-heating the surrounding interstellar medium. Supernova remnants seed the galaxy with heavy elements, accelerate cosmic rays, and — like the Crab — can harbour the neutron star born in the collapse.","aliases":["SNR"],"sources":["nasa"]},{"id":"nebula:horsehead-nebula","type":"nebula","name":"The Horsehead Nebula","domain":"science","entryPath":"/deep-sky-encyclopedia/horsehead-nebula","description":"One of the most recognisable dark nebulae in the sky — a column of cold, dusty gas in the Orion molecular cloud, about 1,500 light-years away, shaped by radiation into the silhouette of a horse's head. Catalogued as Barnard 33, it is seen against the soft red glow of the emission nebula IC 434 behind it, in the constellation Orion just south of the belt star Alnitak.","aliases":["Barnard 33","B33"],"sources":["nasa"]},{"id":"nebula:cone-nebula","type":"nebula","name":"The Cone Nebula","domain":"science","entryPath":"/deep-sky-encyclopedia/cone-nebula","description":"A tall pillar of cold molecular gas and dust, about seven light-years long, sculpted by the radiation and winds of hot young stars in the NGC 2264 star-forming region in Monoceros. The Cone lies at the southern end of the same complex as the Christmas Tree Cluster, roughly 2,700 light-years away, and is a textbook example of a star-forming pillar.","aliases":["part of NGC 2264"],"sources":["nasa"]},{"id":"coordinate_system:celestial-sphere","type":"coordinate_system","name":"The Celestial Sphere","domain":"science","entryPath":"/reference-systems/celestial-sphere","description":"The imaginary sphere of arbitrarily large radius, centred on the observer, onto which all celestial bodies appear projected. It is the geometric stage on which every astronomical coordinate system is drawn — the sky treated as a two-dimensional surface whose points are fixed by pairs of angles.","sources":["iau"]},{"id":"coordinate_system:right-ascension","type":"coordinate_system","name":"Right Ascension","domain":"science","entryPath":"/reference-systems/right-ascension","description":"The celestial equivalent of longitude — the angle measured eastward along the celestial equator from the vernal equinox, conventionally expressed in hours, minutes, and seconds (24 hours around the sky). Together with declination it fixes a star's place in the equatorial system, and it connects directly to sidereal time.","aliases":["RA"],"sources":["iau"]},{"id":"coordinate_system:declination","type":"coordinate_system","name":"Declination","domain":"science","entryPath":"/reference-systems/declination","description":"The celestial equivalent of latitude — the angle of a body north (positive) or south (negative) of the celestial equator, from +90° at the north celestial pole to −90° at the south. With right ascension it pins a star's position in the equatorial coordinate system.","aliases":["Dec"],"sources":["iau"]},{"id":"coordinate_system:equatorial-coordinate-system","type":"coordinate_system","name":"The Equatorial Coordinate System","domain":"science","entryPath":"/reference-systems/equatorial-coordinate-system","description":"The standard astronomical coordinate system, projecting the Earth's equator and poles onto the sky and fixing positions by right ascension and declination. Because it is tied to the slowly precessing equator and equinox, an equatorial position must be qualified by a reference frame and epoch, such as ICRS or J2000.","sources":["iau"]},{"id":"coordinate_system:galactic-coordinate-system","type":"coordinate_system","name":"The Galactic Coordinate System","domain":"science","entryPath":"/reference-systems/galactic-coordinate-system","description":"A coordinate system aligned with the Milky Way, measuring galactic longitude from the direction of the Galactic Centre along the galactic plane and galactic latitude above or below it. It is the natural frame for describing the structure of our Galaxy — spiral arms, the disk, and the distribution of stars and gas.","sources":["iau"]},{"id":"coordinate_system:ecliptic-coordinate-system","type":"coordinate_system","name":"The Ecliptic Coordinate System","domain":"science","entryPath":"/reference-systems/ecliptic-coordinate-system","description":"A coordinate system based on the ecliptic — the plane of the Earth's orbit and the Sun's apparent yearly path — measuring ecliptic longitude eastward from the vernal equinox and ecliptic latitude perpendicular to it. It is the natural frame for the Solar System, where the planets and the Moon stay close to the ecliptic.","sources":["iau"]},{"id":"coordinate_system:horizontal-coordinate-system","type":"coordinate_system","name":"The Horizontal Coordinate System","domain":"science","entryPath":"/reference-systems/horizontal-coordinate-system","description":"The observer-centred system that describes where a body appears in the local sky: altitude above the horizon and azimuth around it. Simple and intuitive for pointing a telescope, horizontal coordinates change continuously as the Earth turns and depend on the observer's location and the moment of observation.","aliases":["Altazimuth coordinates","Alt-azimuth"],"sources":["iau"]},{"id":"coordinate_system:supergalactic-coordinate-system","type":"coordinate_system","name":"The Supergalactic Coordinate System","domain":"science","entryPath":"/reference-systems/supergalactic-coordinate-system","description":"A coordinate system whose equator follows the flattened plane in which the nearby galaxies and clusters are concentrated — the supergalactic plane of the Local Supercluster. It is used to describe the large-scale distribution of galaxies in our cosmic neighbourhood.","sources":["iau"]},{"id":"reference_frame:icrf3","type":"reference_frame","name":"The International Celestial Reference Frame (ICRF3)","domain":"science","entryPath":"/reference-systems/icrf3","description":"The practical realisation of the International Celestial Reference System — a catalogue of precise positions for several thousand extragalactic radio sources, mostly quasars, measured by very-long-baseline interferometry. Its third realisation, ICRF3, was adopted in 2018; because quasars are effectively fixed, it provides the quasi-inertial grid to which optical frames such as Gaia's are aligned.","aliases":["ICRF","ICRF3"],"sources":["iau"]},{"id":"reference_frame:fk5","type":"reference_frame","name":"The Fifth Fundamental Catalogue (FK5)","domain":"science","entryPath":"/reference-systems/fk5","description":"A fundamental reference frame published in 1988, giving precise positions and proper motions for 1,535 bright stars on the equinox and epoch J2000. FK5 was the optical standard of its era, but it rested on a limited number of stars; it was superseded when the ICRS, realised by Hipparcos and later Gaia, replaced star-based frames with an extragalactic one.","aliases":["FK5"],"sources":["iau"]},{"id":"reference_frame:fk4","type":"reference_frame","name":"The Fourth Fundamental Catalogue (FK4)","domain":"science","entryPath":"/reference-systems/fk4","description":"The predecessor of FK5, a fundamental star frame referred to the equinox and epoch B1950. Positions given in the FK4 (B1950) system must be precessed and rotated to be compared with modern J2000/ICRS coordinates — a common source of small errors when working with older catalogues and charts.","aliases":["FK4"],"sources":["iau"]},{"id":"time_standard:julian-date","type":"time_standard","name":"Julian Date","domain":"science","entryPath":"/reference-systems/julian-date","description":"A continuous count of days (and fractions) since noon Universal Time on 1 January 4713 BC in the proleptic Julian calendar, used throughout astronomy to timestamp observations without the awkwardness of calendar months and leap years. The Modified Julian Date (MJD = JD − 2400000.5) shifts the origin to a recent midnight for convenience.","aliases":["JD"],"sources":["iau"]},{"id":"astrometric_effect:precession","type":"astrometric_effect","name":"Precession","domain":"science","entryPath":"/reference-systems/precession","description":"The slow conical wobble of the Earth's rotation axis, driven by the gravitational pull of the Sun and Moon on the equatorial bulge, which carries the celestial poles and the equinoxes around the sky once in about 25,772 years. Precession is why equatorial coordinates drift with time and must be referred to a stated epoch, and why Polaris is only temporarily the pole star.","aliases":["Axial precession"],"sources":["iau"]},{"id":"astrometric_effect:nutation","type":"astrometric_effect","name":"Nutation","domain":"science","entryPath":"/reference-systems/nutation","description":"The small, shorter-period nodding of the Earth's axis superimposed on the steady precessional wobble, caused mainly by the changing orientation of the Moon's orbit, with a dominant period of about 18.6 years. Nutation must be added to precession to compute a body's true position of date to arcsecond precision.","sources":["iau"]},{"id":"astrometric_effect:aberration-of-light","type":"astrometric_effect","name":"The Aberration of Light","domain":"science","entryPath":"/reference-systems/aberration-of-light","description":"The small apparent shift of a star's position in the direction of the observer's motion, because light travels at a finite speed while the observer moves. The Earth's orbital motion makes every star describe a tiny yearly ellipse whose semi-major axis — the maximum displacement from the true position — is about 20.5 arcseconds; discovered by James Bradley in 1728, it was early direct evidence that the Earth orbits the Sun.","aliases":["Stellar aberration"],"sources":["iau"]},{"id":"astrometric_effect:atmospheric-refraction","type":"astrometric_effect","name":"Atmospheric Refraction","domain":"science","entryPath":"/reference-systems/atmospheric-refraction","description":"The bending of a light ray as it passes through the Earth's atmosphere, which lifts the apparent position of a celestial body above its true one — by about half a degree right at the horizon, so the Sun is fully refracted into view when geometrically it has already set. Refraction must be removed to turn an observed altitude into a true one.","sources":["iau"]},{"id":"astrometric_effect:light-time-correction","type":"astrometric_effect","name":"Light-Time Correction","domain":"science","entryPath":"/reference-systems/light-time-correction","description":"The correction that accounts for the time light takes to travel from a moving Solar-System body to the observer: what is seen is where the body was when the light left it, not where it is now. Together with stellar aberration it makes up what is called planetary aberration, and it is essential for computing accurate apparent positions of planets, moons, and spacecraft.","aliases":["Retardation"],"sources":["iau"]},{"id":"astrometric_effect:earth-orientation-parameters","type":"astrometric_effect","name":"Earth Orientation Parameters","domain":"science","entryPath":"/reference-systems/earth-orientation-parameters","description":"The measured quantities that describe how the real, wobbling, irregularly rotating Earth is oriented in space relative to the celestial reference frame — the difference UT1−UTC, the position of the pole (polar motion), and small corrections to the precession-nutation model. Determined and published by the IERS, they are what make it possible to transform between celestial and terrestrial coordinates to full precision.","aliases":["EOP"],"sources":["iau"]},{"id":"organization:iau","type":"organization","name":"International Astronomical Union (IAU)","domain":"science","entryPath":"/reference-systems/iau","description":"The international body, founded in 1919, that is the recognised authority for astronomical nomenclature and standards — it defines constellation boundaries, names celestial bodies and their features, and adopts the reference systems and constants used throughout astronomy, including the International Celestial Reference System.","aliases":["IAU"],"sources":["iau"]},{"id":"organization:iers","type":"organization","name":"International Earth Rotation and Reference Systems Service (IERS)","domain":"science","entryPath":"/reference-systems/iers","description":"The service that maintains the international celestial and terrestrial reference frames and the parameters linking them — the Earth orientation parameters. The IERS monitors the Earth's rotation and axis, publishes UT1−UTC and polar motion, and announces the leap seconds that keep civil time aligned with the turning Earth.","aliases":["IERS"],"sources":["iau"]},{"id":"observing_technique:visual-astronomy","type":"observing_technique","name":"Visual Astronomy","domain":"science","entryPath":"/observation-techniques/visual-astronomy","description":"Observing the sky directly with the eye, whether unaided or through binoculars or a telescope. Visual astronomy trains the observer to see faint detail through averted vision and dark adaptation, and remains the most immediate way to experience the Moon, planets, and brighter deep-sky objects — the foundation on which every imaging technique is built.","aliases":["Visual observing"],"sources":["nasa"]},{"id":"observing_technique:astrophotography","type":"observing_technique","name":"Astrophotography","domain":"science","entryPath":"/observation-techniques/astrophotography","description":"Capturing images of celestial objects with a camera, from wide starfields on a fixed tripod to long, tracked exposures through a telescope. Astrophotography trades the eye's real-time view for the camera's ability to accumulate light over minutes or hours, revealing colour and faint structure the eye can never see. It spans planetary, deep-sky, and narrowband techniques.","sources":["nasa"]},{"id":"observing_technique:planetary-imaging","type":"observing_technique","name":"Planetary Imaging","domain":"science","entryPath":"/observation-techniques/planetary-imaging","description":"High-resolution imaging of the Moon and planets by recording thousands of short-exposure frames and keeping only the sharpest, to beat the blurring of atmospheric turbulence. This 'lucky imaging' approach, usually with a fast CMOS camera, lets modest telescopes resolve cloud belts on Jupiter, the rings of Saturn, and craters on the Moon.","sources":["nasa"]},{"id":"observing_technique:deep-sky-imaging","type":"observing_technique","name":"Deep-Sky Imaging","domain":"science","entryPath":"/observation-techniques/deep-sky-imaging","description":"Long-exposure imaging of faint, extended objects — galaxies, nebulae, and clusters — that requires accurate tracking of the sky's motion, often over many hours of accumulated exposure. Deep-sky imaging leans on an equatorial mount, autoguiding, and careful calibration to draw out signal from targets far too faint to see by eye.","sources":["nasa"]},{"id":"observing_technique:narrowband-imaging","type":"observing_technique","name":"Narrowband Imaging","domain":"science","entryPath":"/observation-techniques/narrowband-imaging","description":"Imaging through filters that pass only the light of specific emission lines — hydrogen-alpha, oxygen-III, sulphur-II — to isolate the glow of ionised gas and cut through light pollution and moonlight. Narrowband imaging reveals the intricate structure of emission nebulae and is the basis of the popular false-colour 'Hubble palette'.","sources":["nasa"]},{"id":"observing_technique:autoguiding","type":"observing_technique","name":"Autoguiding","domain":"science","entryPath":"/observation-techniques/autoguiding","description":"Keeping a telescope locked precisely on target during a long exposure by continuously imaging a guide star and sending tiny correction commands to the mount to cancel tracking errors. Autoguiding is what makes hours-long deep-sky exposures possible without the stars trailing.","sources":["nasa"]},{"id":"observing_technique:calibration-frames","type":"observing_technique","name":"Calibration Frames","domain":"science","entryPath":"/observation-techniques/calibration-frames","description":"The reference exposures that remove a camera's own signature from an image: bias frames capture the sensor's read pedestal, dark frames the thermal signal that builds up during an exposure, and flat frames the uneven illumination and dust shadows of the optics. Subtracting and dividing by these calibration frames turns raw data into a faithful record of the sky.","aliases":["Bias, dark, and flat frames"],"sources":["nasa"]},{"id":"observing_technique:image-processing","type":"observing_technique","name":"Astronomical Image Processing","domain":"science","entryPath":"/observation-techniques/image-processing","description":"The steps that turn calibrated, stacked exposures into a finished image — stretching the very high dynamic range so faint nebulosity and bright cores both show, balancing colour, reducing noise, and sharpening detail. Done honestly it reveals what the data contain; the goal is to represent real signal, not to invent it.","sources":["nasa"]},{"id":"observing_technique:drizzle","type":"observing_technique","name":"Drizzle","domain":"science","entryPath":"/observation-techniques/drizzle","description":"A technique for combining many dithered exposures that recovers resolution lost to undersampling, by mapping each input pixel onto a finer output grid. Developed for the Hubble Space Telescope's deep fields, drizzling is now widely used in both professional and amateur imaging to sharpen stacks of slightly shifted frames.","aliases":["Drizzling","Variable-pixel linear reconstruction"],"sources":["nasa"]},{"id":"observing_technique:plate-solving","type":"observing_technique","name":"Plate Solving","domain":"science","entryPath":"/observation-techniques/plate-solving","description":"Identifying exactly where an image points by matching the pattern of stars it contains against a reference catalogue, and so assigning precise celestial coordinates to every pixel. Plate solving lets software centre a target automatically, sync a mount's pointing, and stamp images with an accurate coordinate solution.","aliases":["Astrometric solving"],"sources":["nasa"]},{"id":"observing_technique:imaging-workflow","type":"observing_technique","name":"The Imaging Workflow","domain":"science","entryPath":"/observation-techniques/imaging-workflow","description":"The end-to-end chain that turns a night at the telescope into a finished picture: mount, optics, and camera acquire tracked, autoguided exposures of the target and matching calibration frames; the frames are calibrated, aligned, and stacked; and the result is stretched and processed. Understanding the whole chain — where signal is gained and where it is lost — is what separates a snapshot from a scientific-grade image.","aliases":["Acquisition-to-image pipeline","Equipment chain"],"sources":["nasa"]},{"id":"astronomy_software:stellarium","type":"astronomy_software","name":"Stellarium","domain":"science","entryPath":"/astronomy-software/stellarium","description":"A free, open-source planetarium that renders a photorealistic sky in real time, showing the stars, planets, constellations, and deep-sky objects as they appear from any location and time. Widely used for planning observing sessions and for teaching, Stellarium can also control telescopes and simulate the view through different eyepieces.","sources":["nasa"]},{"id":"astronomy_software:kstars","type":"astronomy_software","name":"KStars","domain":"science","entryPath":"/astronomy-software/kstars","description":"A free, open-source desktop planetarium and observation planner from the KDE project, showing the sky for any date and location with millions of stars and thousands of deep-sky objects. KStars integrates the Ekos astrophotography suite, making it a complete free platform for both planning and capturing images.","sources":["nasa"]},{"id":"astronomy_software:celestia","type":"astronomy_software","name":"Celestia","domain":"science","entryPath":"/astronomy-software/celestia","description":"A free, open-source real-time 3D space simulator that lets the user fly beyond the Earth's sky to visit the planets, moons, stars, and galaxies, viewing the Solar System and beyond from any vantage point. 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PHD2 is the de-facto standard guider, used on its own or driven by imaging suites like N.I.N.A. and Ekos.","aliases":["PHD2","PHD Guiding"],"sources":["nasa"]},{"id":"astronomy_software:ascom","type":"astronomy_software","name":"ASCOM Platform","domain":"science","entryPath":"/astronomy-software/ascom","description":"A widely adopted standard and driver platform on Windows that lets astronomy software talk to mounts, cameras, focusers, and other devices through a common interface, so any compliant application can control any compliant device. 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Once ubiquitous in professional astronomy, it is no longer actively developed by the observatory but is maintained by the community, and much of its role has passed to the Python ecosystem.","aliases":["Image Reduction and Analysis Facility"],"sources":["nasa"]},{"id":"research_software:casa","type":"research_software","name":"CASA","domain":"science","entryPath":"/astronomy-software/casa","description":"The Common Astronomy Software Applications package, the primary tool for calibrating and imaging data from radio interferometers, developed for ALMA and the Very Large Array. 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TOPCAT is a workhorse for exploring catalogue data from surveys and archives.","aliases":["Tool for OPerations on Catalogues And Tables"],"sources":["nasa"]},{"id":"research_software:ds9","type":"research_software","name":"SAOImage DS9","domain":"science","entryPath":"/astronomy-software/ds9","description":"A widely used astronomical imaging and data-visualisation application for displaying FITS images, with support for multiple frames, colour scales, region analysis, and coordinate overlays. DS9 is a standard viewer for inspecting professional image data.","aliases":["DS9"],"sources":["nasa"]},{"id":"research_software:aladin","type":"research_software","name":"Aladin","domain":"science","entryPath":"/astronomy-software/aladin","description":"An interactive sky-atlas application from the Strasbourg astronomical data centre that lets the user overlay images, surveys, and catalogues on the same patch of sky and query Virtual Observatory services directly. Aladin is a central tool for cross-identifying objects across archives.","aliases":["Aladin Sky Atlas"],"sources":["nasa"]},{"id":"research_software:astroimagej","type":"research_software","name":"AstroImageJ","domain":"science","entryPath":"/astronomy-software/astroimagej","description":"An astronomy-focused build of the ImageJ image-analysis program, adding precise astronomical image display, calibration, and differential photometry. AstroImageJ is especially popular for measuring exoplanet transit light curves from amateur and small-professional telescopes.","aliases":["AIJ"],"sources":["nasa"]},{"id":"research_software:montage","type":"research_software","name":"Montage","domain":"science","entryPath":"/astronomy-software/montage","description":"A toolkit for assembling astronomical images into custom mosaics, reprojecting many overlapping FITS images onto a common grid and matching their backgrounds to make a seamless whole. 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Its active development is now archived, with the work continuing in a successor library, but it remains a well-known tool for orbit computations.","sources":["nasa"]},{"id":"research_software:orekit","type":"research_software","name":"Orekit","domain":"science","entryPath":"/astronomy-software/orekit","description":"A mature, low-level space-flight-dynamics library in Java (with Python bindings) providing high-precision orbit propagation, attitude modelling, time and frame transformations, and maneuver planning. 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galaxy rotation and dark-matter evidence."},{"id":"astronomer:carl-sagan|studies|galaxy:milky-way","from":"astronomer:carl-sagan","to":"galaxy:milky-way","type":"studies","confidence":"likely","domain":"science","note":"Astronomer and science communicator."},{"id":"astronomer:henrietta-leavitt|studies|galaxy:milky-way","from":"astronomer:henrietta-leavitt","to":"galaxy:milky-way","type":"studies","confidence":"likely","domain":"science","note":"Discovered the Cepheid period–luminosity relation."},{"id":"astronomer:annie-jump-cannon|studies|galaxy:milky-way","from":"astronomer:annie-jump-cannon","to":"galaxy:milky-way","type":"studies","confidence":"likely","domain":"science","note":"Developed stellar spectral classification."},{"id":"astronomer:caroline-herschel|studies|galaxy:milky-way","from":"astronomer:caroline-herschel","to":"galaxy:milky-way","type":"studies","confidence":"likely","domain":"science","note":"Comet hunter and astronomer."},{"id":"astronomer:tycho-brahe|studies|galaxy:milky-way","from":"astronomer:tycho-brahe","to":"galaxy:milky-way","type":"studies","confidence":"likely","domain":"science","note":"Made precise pre-telescopic observations."},{"id":"astronomer:ptolemy|studies|galaxy:milky-way","from":"astronomer:ptolemy","to":"galaxy:milky-way","type":"studies","confidence":"likely","domain":"science","note":"Author of the Almagest."},{"id":"astronomer:hipparchus|studies|galaxy:milky-way","from":"astronomer:hipparchus","to":"galaxy:milky-way","type":"studies","confidence":"likely","domain":"science","note":"Compiled an early star catalogue."},{"id":"astronomer:nancy-grace-roman|studies|galaxy:milky-way","from":"astronomer:nancy-grace-roman","to":"galaxy:milky-way","type":"studies","confidence":"likely","domain":"science","note":"Helped establish space-based 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shower's radiant lies in the constellation Taurus."},{"id":"star:canopus|belongs_to|constellation:carina","from":"star:canopus","to":"constellation:carina","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:achernar|belongs_to|constellation:eridanus","from":"star:achernar","to":"constellation:eridanus","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:hadar|belongs_to|constellation:centaurus","from":"star:hadar","to":"constellation:centaurus","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:acrux|belongs_to|constellation:crux","from":"star:acrux","to":"constellation:crux","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:gacrux|belongs_to|constellation:crux","from":"star:gacrux","to":"constellation:crux","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:bellatrix|belongs_to|constellation:orion","from":"star:bellatrix","to":"constellation:orion","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:mintaka|belongs_to|constellation:orion","from":"star:mintaka","to":"constellation:orion","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:alnilam|belongs_to|constellation:orion","from":"star:alnilam","to":"constellation:orion","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:alnitak|belongs_to|constellation:orion","from":"star:alnitak","to":"constellation:orion","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:saiph|belongs_to|constellation:orion","from":"star:saiph","to":"constellation:orion","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:dubhe|belongs_to|constellation:ursa-major","from":"star:dubhe","to":"constellation:ursa-major","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:merak|belongs_to|constellation:ursa-major","from":"star:merak","to":"constellation:ursa-major","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:alkaid|belongs_to|constellation:ursa-major","from":"star:alkaid","to":"constellation:ursa-major","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:mizar|belongs_to|constellation:ursa-major","from":"star:mizar","to":"constellation:ursa-major","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:alioth|belongs_to|constellation:ursa-major","from":"star:alioth","to":"constellation:ursa-major","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:denebola|belongs_to|constellation:leo","from":"star:denebola","to":"constellation:leo","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:algol|belongs_to|constellation:perseus","from":"star:algol","to":"constellation:perseus","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:mirfak|belongs_to|constellation:perseus","from":"star:mirfak","to":"constellation:perseus","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:rasalhague|belongs_to|constellation:ophiuchus","from":"star:rasalhague","to":"constellation:ophiuchus","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:vindemiatrix|belongs_to|constellation:virgo","from":"star:vindemiatrix","to":"constellation:virgo","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:sadr|belongs_to|constellation:cygnus","from":"star:sadr","to":"constellation:cygnus","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:albireo|belongs_to|constellation:cygnus","from":"star:albireo","to":"constellation:cygnus","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:deneb-algedi|belongs_to|constellation:capricornus","from":"star:deneb-algedi","to":"constellation:capricornus","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:hamal|belongs_to|constellation:aries","from":"star:hamal","to":"constellation:aries","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:alpheratz|belongs_to|constellation:andromeda","from":"star:alpheratz","to":"constellation:andromeda","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:mirach|belongs_to|constellation:andromeda","from":"star:mirach","to":"constellation:andromeda","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:schedar|belongs_to|constellation:cassiopeia","from":"star:schedar","to":"constellation:cassiopeia","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:caph|belongs_to|constellation:cassiopeia","from":"star:caph","to":"constellation:cassiopeia","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:trappist-1|belongs_to|constellation:aquarius","from":"star:trappist-1","to":"constellation:aquarius","type":"belongs_to","confidence":"confirmed","domain":"science"},{"id":"star:kepler-22|belongs_to|constellation:cygnus"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known exoplanet to the Solar System."},{"id":"exoplanet:trappist-1-b|child_of|star:trappist-1","from":"exoplanet:trappist-1-b","to":"star:trappist-1","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"exoplanet:trappist-1-c|child_of|star:trappist-1","from":"exoplanet:trappist-1-c","to":"star:trappist-1","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"exoplanet:trappist-1-d|child_of|star:trappist-1","from":"exoplanet:trappist-1-d","to":"star:trappist-1","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"exoplanet:trappist-1-e|child_of|star:trappist-1","from":"exoplanet:trappist-1-e","to":"star:trappist-1","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"exoplanet:trappist-1-f|child_of|star:trappist-1","from":"exoplanet:trappist-1-f","to":"star:trappist-1","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"exoplanet:trappist-1-g|child_of|star:trappist-1","from":"exoplanet:trappist-1-g","to":"star:trappist-1","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"exoplanet:trappist-1-h|child_of|star:trappist-1","from":"exoplanet:trappist-1-h","to":"star:trappist-1","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"exoplanet:51-pegasi-b|child_of|star:helvetios","from":"exoplanet:51-pegasi-b","to":"star:helvetios","type":"child_of","confidence":"confirmed","domain":"science","note":"First exoplanet found around a Sun-like star."},{"id":"exoplanet:kepler-22b|child_of|star:kepler-22","from":"exoplanet:kepler-22b","to":"star:kepler-22","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"exoplanet:kepler-186f|child_of|star:kepler-186","from":"exoplanet:kepler-186f","to":"star:kepler-186","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"exoplanet:hd-209458-b|child_of|star:hd-209458","from":"exoplanet:hd-209458-b","to":"star:hd-209458","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"exoplanet:55-cancri-e|child_of|star:copernicus","from":"exoplanet:55-cancri-e","to":"star:copernicus","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"exoplanet:gliese-581c|child_of|star:gliese-581","from":"exoplanet:gliese-581c","to":"star:gliese-581","type":"child_of","confidence":"confirmed","domain":"science"},{"id":"asteroid:vesta|part_of|location:solar-system","from":"asteroid:vesta","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"asteroid:pallas|part_of|location:solar-system","from":"asteroid:pallas","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"asteroid:hygiea|part_of|location:solar-system","from":"asteroid:hygiea","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"asteroid:bennu|part_of|location:solar-system","from":"asteroid:bennu","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"asteroid:ryugu|part_of|location:solar-system","from":"asteroid:ryugu","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"asteroid:eros|part_of|location:solar-system","from":"asteroid:eros","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"asteroid:itokawa|part_of|location:solar-system","from":"asteroid:itokawa","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"asteroid:psyche|part_of|location:solar-system","from":"asteroid:psyche","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"asteroid:apophis|part_of|location:solar-system","from":"asteroid:apophis","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"comet:hale-bopp|part_of|location:solar-system","from":"comet:hale-bopp","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"comet:hyakutake|part_of|location:solar-system","from":"comet:hyakutake","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"comet:churyumov-gerasimenko|part_of|location:solar-system","from":"comet:churyumov-gerasimenko","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"comet:shoemaker-levy-9|part_of|location:solar-system","from":"comet:shoemaker-levy-9","to":"location:solar-system","type":"part_of","confidence":"confirmed","domain":"science"},{"id":"space_telescope:hubble-space-telescope|studies|galaxy:andromeda-galaxy","from":"space_telescope:hubble-space-telescope","to":"galaxy:andromeda-galaxy","type":"studies","confidence":"confirmed","domain":"science"},{"id":"space_telescope:hubble-space-telescope|studies|nebula:crab-nebula","from":"space_telescope:hubble-space-telescope","to":"nebula:crab-nebula","type":"studies","confidence":"confirmed","domain":"science"},{"id":"space_telescope:hubble-space-telescope|studies|nebula:eagle-nebula","from":"space_telescope:hubble-space-telescope","to":"nebula:eagle-nebula","type":"studies","confidence":"confirmed","domain":"science","note":"Hubble's 1995 image of the Eagle Nebula — the 'Pillars of Creation'."},{"id":"space_telescope:james-webb-space-telescope|studies|nebula:eagle-nebula","from":"space_telescope:james-webb-space-telescope","to":"nebula:eagle-nebula","type":"studies","confidence":"confirmed","domain":"science","note":"Webb re-imaged the Pillars of Creation in 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1610."},{"id":"comet:halleys-comet|named_after|astronomer:edmond-halley","from":"comet:halleys-comet","to":"astronomer:edmond-halley","type":"named_after","confidence":"confirmed","domain":"science","note":"Halley computed the comet's orbit and predicted its 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2 is the only spacecraft to visit Uranus and Neptune."},{"id":"galaxy:andromeda-galaxy|scientifically_related_to|galaxy:milky-way","from":"galaxy:andromeda-galaxy","to":"galaxy:milky-way","type":"scientifically_related_to","confidence":"confirmed","domain":"science","note":"The nearest large galaxy to the Milky Way."},{"id":"galaxy:triangulum-galaxy|scientifically_related_to|galaxy:milky-way","from":"galaxy:triangulum-galaxy","to":"galaxy:milky-way","type":"scientifically_related_to","confidence":"confirmed","domain":"science","note":"A member of the Local Group with the Milky Way."},{"id":"galaxy:large-magellanic-cloud|scientifically_related_to|galaxy:milky-way","from":"galaxy:large-magellanic-cloud","to":"galaxy:milky-way","type":"scientifically_related_to","confidence":"confirmed","domain":"science","note":"A satellite galaxy of the Milky 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