Cannabaceae

HD 180902 b
Discovery[1]
Discovered byJohnson et al.
Discovery siteKeck Observatory
Discovery date2010
Doppler spectroscopy
Orbital characteristics[2]
1.40±0.11 AU
Eccentricity0.107±0.022
510.9±1.5 d
2455055±17 JD
181±12 º
Semi-amplitude34.25±0.84 m/s
StarHD 180902
Physical characteristics[2]
Mean radius
1.221 RJ
Mass≥1.685±0.041 MJ

HD 180902 b is an extrasolar planet orbiting the K-type star HD 180902 approximately 342 light years away[3] in the constellation Sagittarius.[1]

Discovery[edit]

HD 180902 b, along with other planets, was discovered in 2010 by scientists at the Keck Observatory. These planets were discovered via doppler spectroscopy, which is detecting exoplanets using the star's wobble.

Properties[edit]

Orbit

HD 180902 b takes 510 days to orbit its parent star, which is longer than Earth's orbital period, which is 365 days. It orbits at a distance similar to Earth from the sun. HD 180902 orbits with mild eccentricity.

Characteristics[edit]

HD 180902 b has a minimum mass of 1.685 times the mass of Jupiter, but since its inclination is not known, the true mass of the planet cannot be detected. According to a theoretical search by the observatory, it may have a radius that is 22.1% larger than Jupiter.

Size comparison
Jupiter HD 180902 b
Jupiter Exoplanet

See also[edit]

References[edit]

External links[edit]

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