Hypothetical view of 83 Leonis Bb rendered by Celestia | |
| Discovery | |
|---|---|
| Discovered by | Marcy, Butler, Vogtet al. |
| Discovery site | United States |
| Discovery date | 25 January 2005 |
| Doppler spectroscopy | |
| Orbital characteristics | |
| 0.12186 ± 0.00002 AU (18,230,000 ± 3,000 km)[1] | |
| Eccentricity | 0.13 ± 0.07[1] |
| 17.054 ± 0.003[1]d | |
| 2,450,449 ± 2[1] | |
| 196 ± 32[1] | |
| Semi-amplitude | 7.9 ± 0.6[1] |
| Star | 83 Leonis B |
83 Leonis Bb, also catalogued asHD 99492 b or abbreviated83 Leo Bb, is anextrasolar planet with a minimum mass of 1.5 Neptune mass. It is located approximately 59light-years away in theconstellation ofLeo (theLion). The planet was discovered in January 2005 by theCalifornia and Carnegie Planet Search team, who use theDoppler spectroscopy method to detect planets.[2] It orbits in a close orbit around the star, completing one orbit in about 17days.[1] The HARPS-N spectrograph discovered a second Neptune-like exoplanet in 2022 orbiting at 95 days.
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