| Discovery | |
|---|---|
| Discovery date | 2015 November 17 |
| radial velocity method | |
| Orbital characteristics | |
| Apastron | 0.1679 (± 0.00908) AU |
| Periastron | 0.1246 (± 0.00908) AU |
| 0.1463 (± 0.0018)[1] 0.14574 (± 2e-05)[2] AU | |
| Eccentricity | 0.148 (± 0.047)[1] |
| 22.805 (± 0.005)[1] d | |
| Inclination | ?[1] |
| Star | HD 219134 |
| Physical characteristics | |
| >1.31 (± 0.02)[1] R🜨 | |
| Mass | >7.30 (± 0.40)[1] ME |
Mean density | <17.9 g cm−3 |
| <4.25 g | |
| Temperature | 522.6 K (249.5 °C; 481.0 °F) |
HD 219134 f, also known as HR 8832 f, is an exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia. It is a Super-Earth with a minimum mass of over 7 times that of Earth. Unlike HD 219134 b and HD 219134 c it was not observed by the Spitzer Space Telescope and thus its radius and density are unknown. Only a minimum radius can be given.
- ^ a b c d e f "HD 219134". exoplanetarchive.ipac.caltech.edu. Retrieved 2017-12-24.
- ^ "HD 219134 f". exoplanetarchive.ipac.caltech.edu. Retrieved 2017-12-24.
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