HD 86264 b
HD 86264 b is an extrasolar planet which orbits the F-type main sequence star HD 86264, located approximately 237 light years away in the constellation Hydra.[1] The planet is considered to orbit in an eccentric path around the star with a period of about four years. This planet can be as close as 0.86 AU to as far as 4.86 AU. It has minimum mass seven Jupiter masses and orbits at a distance of 2.86 astronomical units. This planet was detected by radial velocity method on August 13, 2009.
Discovery | |
---|---|
Discovery date | August 13, 2009 |
Radial velocity | |
Orbital characteristics | |
Apastron | 4.86 AU (727,000,000 km) |
Periastron | 0.86 AU (129,000,000 km) |
2.86 ± 0.07 AU (428,000,000 ± 10,000,000 km) | |
Eccentricity | 0.7 ± 0.2 |
1475 ± 55 d 4.04 ± 0.15 y | |
15172 ± 114 | |
306 ± 10 | |
Star | HD 86264 |
An estimate of the planet's inclination and true mass (~9.81 MJ) via astrometry, though with high error, was published in 2022.[2]
References
- Fischer, Debra; et al. (2009). "Five planets and an independent confirmation of HD 196885 Ab from Lick Observatory". The Astrophysical Journal. 703 (2): 1545–1556. arXiv:0908.1596. Bibcode:2009ApJ...703.1545F. doi:10.1088/0004-637X/703/2/1545. S2CID 15524804.
- 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.
External links
- PlanetQuest, HD 86264 b
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