HD 106252 b
Discovery | |
---|---|
Discovered by | Geneva Extrasolar Planet Search |
Discovery site | La Silla Observatory |
Discovery date | April 4, 2001[1] |
radial velocity | |
Orbital characteristics[2] | |
2.655 ± 0.017 AU (397,200,000 ± 2,500,000 km) | |
Eccentricity | 0.480 ± 0.010 |
4.202+0.011 −0.010 yr | |
Inclination | 46.0+4.9 −4.1 or 134.0+4.1 −4.9 |
105.3+10 −6.1 | |
JD 246463.0+8.4 −8.6 | |
291.4 ± 1.5° | |
Semi-amplitude | 152 ± 21[3] |
Star | HD 106252 |
Physical characteristics | |
Mass | 10.00+0.78 −0.73[2] MJ |
HD 106252 b is a large gas giant extrasolar planet about 10 times more massive than Jupiter. It was announced in 2001 by the European Southern Observatory.[1] The discovery was confirmed by a different team using the Lick Telescope.[4]
Astrometry of HD 106252 has determined an orbital inclination of either 46° or 134°, depending on whether the solution is prograde or retrograde. This, combined with the minimum mass, gives a true mass of 10.0 MJ, larger than the minimum mass of 7.2 MJ.[2]
References
[edit]- ^ a b "Exoplanets: The Hunt Continues!" (Press release). Garching, Germany: European Southern Observatory. April 4, 2001. Retrieved December 27, 2012.
- ^ a b c Li, Yiting; Brandt, Timothy D.; Brandt, G. Mirek; Dupuy, Trent J.; Michalik, Daniel; Jensen-Clem, Rebecca; Zeng, Yunlin; Faherty, Jacqueline; Mitra, Elena L. (2021). "Precise Masses and Orbits for Nine Radial-velocity Exoplanets". The Astronomical Journal. 162 (6): 266. arXiv:2109.10422. Bibcode:2021AJ....162..266L. doi:10.3847/1538-3881/ac27ab. S2CID 237592581.
- ^ Butler, R. P.; et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal. 646 (1): 505–522. arXiv:astro-ph/0607493. Bibcode:2006ApJ...646..505B. doi:10.1086/504701. S2CID 119067572.
- ^ Fischer, Debra A.; et al. (2002). "Planetary Companions to HD 136118, HD 50554, and HD 106252". Publications of the Astronomical Society of the Pacific. 114 (795): 529–535. Bibcode:2002PASP..114..529F. doi:10.1086/341677.
External links
[edit]- "HD 106252". Exoplanets. Archived from the original on 2009-11-25. Retrieved 2008-10-31.