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HD 81040 b

Gas giant

HD 81040 b

Gas giant

FieldValue
extrasolarplanetyes
nameHD 81040 b
imageHD 81040 Radial Velocity.png
image_scale1.5
image_altRadial velocity curve of HD 81040 b
captionRadial velocity curve of HD 81040 b
discovererSozzetti et al.
discovery_siteObservatoire de Haute-Provence
in France
discoveredNovember 24, 2005
discovery_methodDoppler Spectroscopy
apsisastron
semimajor1.946 ±
eccentricity
period1004.7 ±
inclination
asc_node
time_periastron
arg_peri
semi-amplitude168 ± 9
starHD 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.

Astrometric orbit of HD 81040 b<ref name=&quot;IOW20220131&quot;/>

References

References

  1. (2006). "A massive planet to the young disc star HD 81040". Astronomy and Astrophysics.
  2. (2021). "Precise Masses and Orbits for Nine Radial-velocity Exoplanets". The Astronomical Journal.
  3. (31 January 2022). "Image of the Week: Astrometric Orbit of the Exoplanet-Host Star HD81040". [[ESA]]/Gaia/DPAC/CU4-CU3.
  4. (2023). "''Gaia'' Data Release 3". Astronomy & Astrophysics.
  5. (August 2022). "3D Selection of 167 Substellar Companions to Nearby Stars". [[The Astrophysical Journal Supplement Series]].
  6. Winn, Joshua N.. (September 2022). "Joint Constraints on Exoplanetary Orbits from Gaia DR3 and Doppler Data". The Astronomical Journal.
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