HD 50499 b is an extrasolar planet approximately 154 light-years away in the constellation of Puppis. The planet is suspected to be a gas giant with mass of 1.7 times Jupiter. It is a long period, taking 351 weeks to orbit the star. The planet's eccentric orbit passes through the average distance of 574 Gm.
| Discovery | |
|---|---|
| Discovered by | Vogt, Butler, Marcy, and Fischer et al. |
| Discovery site |  United States |
| Discovery date | 5 June 2005 |
| Radial velocity | |
| Orbital characteristics | |
| 3.84 ± 0.04 AU (574,500,000 ± 6,000,000 km) | |
| Eccentricity | 0.25 ± 0.20 |
| 2458 ± 38 d | |
| 2451220 ± 77 | |
| 259 ± 36 | |
| Semi-amplitude | 23.0 ± 1.1 |
| Star | HD 50499 |
The planet was discovered by four team members including Steve Vogt in 2005 using their radial velocity method, which used to measure changes in red- and blue-shifting of the star that indicate the presence of planets caused by gravitational tug.[1] He also indicated the existence of two additional outer planets.
See also edit
References edit
- ^ Vogt, Steven S.; et al. (2005). "Five New Multicomponent Planetary Systems" (PDF). The Astrophysical Journal. 632 (1): 638–658. Bibcode:2005ApJ...632..638V. doi:10.1086/432901. S2CID 16509245.
 | This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it. |