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HD 163607 c 
Summary
HD 163607 c is the outermost planet discovered to orbit a star HD 163607, a star somewhat brighter and older than the Sun. It was discovered using the radial velocity method, and was initially observed as part of the N2K Program. Its minimum mass is at least 2.4 of Jupiter's. It is located in its host star's habitable zone.[1]
| Discovery[1] | |
|---|---|
| Discovered by | Giguere et al. |
| Discovery site | Keck Observatory |
| Discovery date | 2011 |
| Doppler spectroscopy | |
| Orbital characteristics[2] | |
| 2.39±0.11 AU | |
| Eccentricity | 0.080±0.014 |
| 1272.0±4.4 d | |
| 2455111±40 JD | |
| 274±12 º | |
| Semi-amplitude | 38.37±0.65 m/s |
| Star | HD 163607 |
| Physical characteristics[2] | |
| Mass | ≥2.201±0.037 MJ |
See also edit
References edit
- ^ a b Giguere, Matthew J.; et al. (2012). "A High-eccentricity Component in the Double-planet System around HD 163607 and a Planet around HD 164509". The Astrophysical Journal. 744 (1): 4–13. arXiv:1109.2955. Bibcode:2012ApJ...744....4G. doi:10.1088/0004-637X/744/1/4.
- ^ a b Luhn, Jacob K.; et al. (2019). "Retired A Stars and Their Companions. VIII. 15 New Planetary Signals around Subgiants and Transit Parameters for California Planet Search Planets with Subgiant Hosts". The Astronomical Journal. 157 (4). 149. arXiv:1811.03043. Bibcode:2019AJ....157..149L. doi:10.3847/1538-3881/aaf5d0.
External links edit
- Notes on the planet HD 163607 c