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HD 81040 b
Gas giant
Gas giant
| Field | Value |
|---|---|
| extrasolarplanet | yes |
| name | HD 81040 b |
| image | HD 81040 Radial Velocity.png |
| image_scale | 1.5 |
| image_alt | Radial velocity curve of HD 81040 b |
| caption | Radial velocity curve of HD 81040 b |
| discoverer | Sozzetti et al. |
| discovery_site | Observatoire de Haute-Provence |
| in France | |
| discovered | November 24, 2005 |
| discovery_method | Doppler Spectroscopy |
| apsis | astron |
| semimajor | 1.946 ± |
| eccentricity | |
| period | 1004.7 ± |
| inclination | |
| asc_node | |
| time_periastron | |
| arg_peri | |
| semi-amplitude | 168 ± 9 |
| star | HD 81040 |
| mass |
in France | semi-amplitude = 168 ± 9
HD 81040 b is a massive gas giant exoplanet that orbits the star HD 81040, discovered in 2005 by radial velocity. Its orbital period is just over 1000 days. It has a semimajor axis of about 1.95 AU, and its orbit is quite eccentric, at a little over 0.5.
Astrometry of HD 81040 using Gaia, published in several papers, has determined an orbital inclination of about 111°. This, combined with the minimum mass, gives a true mass of . Since the inclination is high, there is a small chance that the planet transits.

References
References
- (2006). "A massive planet to the young disc star HD 81040". Astronomy and Astrophysics.
- (2021). "Precise Masses and Orbits for Nine Radial-velocity Exoplanets". The Astronomical Journal.
- (31 January 2022). "Image of the Week: Astrometric Orbit of the Exoplanet-Host Star HD81040". [[ESA]]/Gaia/DPAC/CU4-CU3.
- (2023). "''Gaia'' Data Release 3". Astronomy & Astrophysics.
- (August 2022). "3D Selection of 167 Substellar Companions to Nearby Stars". [[The Astrophysical Journal Supplement Series]].
- Winn, Joshua N.. (September 2022). "Joint Constraints on Exoplanetary Orbits from Gaia DR3 and Doppler Data". The Astronomical Journal.
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