HD 149026 b · Asteria Star

Scientific overview

HD 149026 b is a hot jupiter orbiting HD 149026, completing an orbit every 3 days, about 247 light-years from Earth. It was discovered in 2005 using the radial velocity method.

Host star

Ogma

Spectral type

G0

Temperature

6,179 K

Mass

1.42 M☉

Discovery and detection

Detection method

Radial Velocity Method

Discovery year

2005

Discovered at

Subaru Telescope

Knowledge connections

OrbitsOgma
Discovered by methodRadial Velocity Method
Discovered atSubaru Telescope
Catalogued inNASA Exoplanet Archive

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