HD 27631 b

HD 27631 b^[1]
Discovery
Discovered by	Marmier et al.
Discovery site	HARPS
Discovery date	Sept. 13, 2011
Detection method	Doppler spectroscopy
Orbital characteristics
Semi-major axis	3.22+0.065; −0.064 AUえーゆー
Eccentricity	0.163±0.057
Orbital period (sidereal)	2173+47; −44 d; 5.95+0.13; −0.12 yr
Inclination	74°+11°; −15° or 106°+15°; −11°
Longitude of ascending node	91°+63°; −66°
Time of periastron	2456110+158; −147
Argument of periastron	128°+28°; −27°
Star	HD 27631
Physical characteristics
Mass	1.56+0.2; −0.15 MJ

HD 27631 b is an extrasolar planet that has more mass than Jupiter. It orbits 3.25 AUえーゆー from the star, taking six years to revolve around the parent star HD 27631. Its orbit is eccentric, around 12%.^[1] In 2023, the inclination and true mass of HD 27631 b were determined via astrometry.^[2]

References

^ ^a ^b ^c Marmier, M.; et al. (2013). "The CORALIE survey for southern extrasolar planets XVII. New and updated long period and massive planets". Astronomy and Astrophysics. 551. A90. arXiv:1211.6444. Bibcode:2013A&A...551A..90M. doi:10.1051/0004-6361/201219639. S2CID 59467665.
^ ^a ^b ^c Xiao, Guang-Yao; Liu, Yu-Juan; et al. (March 2023). "The Masses of a Sample of Radial-Velocity Exoplanets with Astrometric Measurements". Research in Astronomy and Astrophysics. arXiv:2303.12409.

External links

"HD 27631". Exoplanets. Archived from the original on 2016-11-30. Retrieved 2012-11-29.

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[Marmier2013-1] Marmier, M.; et al. (2013). "The CORALIE survey for southern extrasolar planets XVII. New and updated long period and massive planets". Astronomy and Astrophysics. 551. A90. arXiv:1211.6444. Bibcode:2013A&A...551A..90M. doi:10.1051/0004-6361/201219639. S2CID 59467665.

[Xiao2023-2] Xiao, Guang-Yao; Liu, Yu-Juan; et al. (March 2023). "The Masses of a Sample of Radial-Velocity Exoplanets with Astrometric Measurements". Research in Astronomy and Astrophysics. arXiv:2303.12409.

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