GJ 676 A c · Asteria Star

Scientific overview

GJ 676 A c is a gas giant orbiting GJ 676 A, completing an orbit every 13921 days, about 52 light-years from Earth. It was discovered in 2016 using the radial velocity method.

Host star

GJ 676 A

Spectral type

M0

Temperature

3,734 K

Mass

0.626 M☉

Planetary system — GJ 676 A system

View the GJ 676 A system (4 known planets).

Planet	Class	Radius (R⊕)	Period (d)	Distance (ly)
GJ 676 A dRadial Velocity · 2012	Super-Earth	1.78	3.6008	52
GJ 676 A eRadial Velocity · 2012	Mini-Neptune	2.47	35.4736	52
GJ 676 A bRadial Velocity · 2010	Gas giant	12.8	1051	52
GJ 676 A cRadial Velocity · 2016	Gas giant	12.3	13921	52

Discovery and detection

Detection method

Radial Velocity Method

Discovery year

2016

Discovered at

Very Large Telescope (VLT)

Knowledge connections

OrbitsGJ 676 A
Member of systemGJ 676 A system
Discovered by methodRadial Velocity Method
Discovered atVery Large Telescope (VLT)
Catalogued inNASA Exoplanet Archive

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