Template:Infobox Planet
HD 121504 b is an exoplanet that is likely 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.[1]
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.
References[]
- ↑ (2004). The CORALIE survey for southern extra-solar planets XII. Orbital solutions for 16 extra-solar planets discovered with CORALIE. Astronomy and Astrophysics 415 (1): 391–402.
External links[]
- HD 121504 b. The Extrasolar Planets Encyclopaedia.
- HD 121504. Exoplanets.
Coordinates: Sky map 13h 57m 17.2375s, −56° 02′ 24.153″
File:Iota-draconis-b.jpg | This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it. |