HD 106906 b
| Discovery | |
|---|---|
| Discovered by | Vanessa Bailey, et al. |
| Discovery site | Magellan Telescopes at the Las Campanas Observatory in Chile |
| Discovery date | December 4, 2013 (published) |
| Direct imaging | |
| Orbital characteristics | |
Mean orbit radius | 738 AU (110 billion km) |
| 8,910.501 years | |
| Star | HD 106906 |
| Physical characteristics | |
| 1.54+0.04 −0.05 RJ | |
| Mass | 11±2 MJup |
| Temperature | ≈1,800 K (1,500 °C; 2,800 °F) |
HD 106906 b is a directly imaged planetary-mass companion and exoplanet orbiting the star HD 106906, in the constellation Crux at about 336 ± 13 light-years (103 ± 4 pc) from Earth. It is estimated to be about eleven times the mass of Jupiter and is located about 738 AU away from its host star. HD 106906 b is an oddity; while its mass estimate is nominally consistent with identifying it as an exoplanet, it appears at a much wider separation from its parent star than thought possible for in-situ formation from a protoplanetary disk.