HD 126614 Ab
Appearance
Discovery | |
---|---|
Discovered by | Howard et al. |
Discovery site | Keck Observatory |
Discovery date | November 13, 2009 |
Radial velocity | |
Orbital characteristics[1] | |
2.249+0.088 −0.096 | |
Eccentricity | 0.548+0.063 −0.062 |
3.442 ± 0.02 years (1,257.2 ± 7.3 d) | |
Inclination | 97.477°+35.340° −37.849° |
182.778°+120.999° −117.633° | |
2450124.747+26.090 −28.486 | |
304.917°+9.910° −12.242° | |
Semi-amplitude | 7.760+0.699 −0.516 m/s |
Star | HD 126614 A |
Physical characteristics[1] | |
Mass | 0.339+0.204 −0.019 MJ |
HD 126614 Ab, or simply HD 126614 b, (also known as HIP 70623 b) is an extrasolar planet which orbits the primary K-type star HD 126614 A, located approximately 240 light years away[2] in the constellation Virgo. It was discovered on November 13, 2009. However, this planet has a highly eccentric orbit around its parent star. The planetary distance ranges from 0.94
In 2022, the true mass and inclination of HD 126614 Ab were measured via astrometry.[1]
See also
[edit]Other planets that were discovered or confirmed on November 13, 2009:
References
[edit]- ^ a b c Feng, Fabo; Butler, R. Paul; et al. (August 2022). "3D Selection of 167 Substellar Companions to Nearby Stars". The Astrophysical Journal Supplement Series. 262 (21): 21. arXiv:2208.12720. Bibcode:2022ApJS..262...21F. doi:10.3847/1538-4365/ac7e57. S2CID 251864022.
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ Howard, Andrew W.; et al. (2010). "The California Planet Survey. I. Four New Giant Exoplanets". The Astrophysical Journal. 721 (2): 1467–1481. arXiv:1003.3488. Bibcode:2010ApJ...721.1467H. doi:10.1088/0004-637X/721/2/1467. S2CID 14147776.
- Jean Schneider (2011). "Notes for Planet HD 126614 b". Extrasolar Planets Encyclopaedia. Archived from the original on 2 June 2012. Retrieved 29 September 2011.