HD 1461 b · Asteria Star

Scientific overview

HD 1461 b is a mini-neptune orbiting HD 1461, completing an orbit every 6 days, about 76 light-years from Earth. It was discovered in 2010 using the radial velocity method.

Host star

HD 1461

Spectral type

G0 V

Temperature

5,765 K

Mass

1.02 M☉

Planetary system — HD 1461 system

View the HD 1461 system (2 known planets).

Planet	Class	Radius (R⊕)	Period (d)	Distance (ly)
HD 1461 bRadial Velocity · 2010	Mini-Neptune	2.42	5.7715	76
HD 1461 cRadial Velocity · 2015	Super-Earth	2.23	13.5052	76

Discovery and detection

Detection method

Radial Velocity Method

Discovery year

2010

Discovered at

W. M. Keck Observatory

Knowledge connections

OrbitsHD 1461
Member of systemHD 1461 system
Discovered by methodRadial Velocity Method
Discovered atW. M. Keck Observatory
Catalogued inNASA Exoplanet Archive

Loading…