GJ 682 b · Asteria Star

Scientific overview

GJ 682 b is a super-earth orbiting GJ 682, completing an orbit every 17 days, about 16 light-years from Earth. It was discovered in 2014 using the radial velocity method.

Host star

GJ 682

Spectral type

M3.5 V

Temperature

3,028 K

Mass

0.27 M☉

Planetary system — GJ 682 system

View the GJ 682 system (2 known planets).

Planet	Class	Radius (R⊕)	Period (d)	Distance (ly)
GJ 682 bRadial Velocity · 2014	Super-Earth	1.93	17.478	16
GJ 682 cRadial Velocity · 2014	Mini-Neptune	2.89	57.32	16

Discovery and detection

Detection method

Radial Velocity Method

Discovery year

2014

Knowledge connections

OrbitsGJ 682
Member of systemGJ 682 system
Discovered by methodRadial Velocity Method
Catalogued inNASA Exoplanet Archive

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