HD 121504 b explained

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HD 121504 b
Discovered:August 7, 2000
Discovery Method:Radial velocity
(CORALIE)
Discovery Site:La Silla Observatory
Discoverer:Mayor et al.
Alt Names:HIP 68162 b
Semimajor:0.33 AU
49 Gm
Apsis:astron
Aphelion:0.34
50 Gm
Perihelion:0.32
48 Gm
Eccentricity:0.03 ± 0.01
Period:63.33 ± 0.03 d
0.1734 year
Angular Dist:7 mas
Long Periastron:265° ± 12°
Time Periastron:2,451,450 ± 2 JD
Semi-Amplitude:50.8 ± 0.9 m/s
Mass:>1.22 MJ
>388 ME
Star:HD 121504

HD 121504 b is an exoplanet that is likely to be slightly less massive than Jupiter. Although the radial velocity method that was used to detect the planet can only measure the minimum mass of the planet, it is very unlikely that its true mass would be much higher.

HD 121504 b orbits the star at a distance of about one third of Earth's distance from the Sun, and has a slightly eccentric orbit.

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