HD 23127 b
HD 23127 b is a jovian extrasolar planet orbiting the star HD 23127 at the distance of 2.29 AU, taking 3.32 years to orbit. The orbit is very eccentric, a so-called "eccentric Jupiter". At periastron, the distance is 1.28 AU, and at apastron, the distance is 3.30 AU. The mass is at least 1.37 times Jupiter. Only the minimum mass is known because the inclination is not known.[1]
| Discovery | |
|---|---|
| Discovered by | O'Toole et al. |
| Discovery site | .svg.png){kind=small} |
| Discovery date | February 9, 2007 |
| radial velocity | |
| Orbital characteristics | |
| 2.29 AU (343,000,000 km) | |
| Eccentricity | 0.44 ± 0.07 |
| 1214 ± 9 d 3.32 y | |
| 2,400,229 ± 19 | |
| 190 ± 6 | |
| Semi-amplitude | 27.5 ± 1 |
| Star | HD 23127 |
References
- O'Toole, Simon J.; et al. (2007). "New Planets around Three G Dwarfs". The Astrophysical Journal. 660 (2): 1636–1641. arXiv:astro-ph/0702213. Bibcode:2007ApJ...660.1636O. doi:10.1086/513563.
Constellation of Reticulum | |||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| Stars |
| ||||||||||
| |||||||||||
| Galaxies |
| ||||||||||
| |||||||||||
 | |||||||||||
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.