HD 136352 b · Asteria Star

Scientific overview

HD 136352 b is a super-earth orbiting HD 136352, completing an orbit every 12 days, about 48 light-years from Earth. It was discovered in 2019 using the radial velocity method.

Host star

HD 136352

Spectral type

G4 V

Temperature

5,664 K

Mass

0.87 M☉

Planetary system — HD 136352 system

View the HD 136352 system (3 known planets).

Planet	Class	Radius (R⊕)	Period (d)	Distance (ly)
HD 136352 bRadial Velocity · 2019	Super-Earth	1.66	11.578	48
HD 136352 cRadial Velocity · 2019	Mini-Neptune	2.92	27.5922	48
HD 136352 dRadial Velocity · 2019	Mini-Neptune	2.56	107	48

Discovery and detection

Detection method

Radial Velocity Method

Discovery year

2019

Discovered at

La Silla Observatory

Knowledge connections

OrbitsHD 136352
Member of systemHD 136352 system
Discovered by methodRadial Velocity Method
Discovered atLa Silla Observatory
Catalogued inNASA Exoplanet Archive

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