![]() Radial velocity curve of HD 81040 b [1] | |
Discovery | |
---|---|
Discovered by | Sozzetti et al. [2] |
Discovery site | Observatoire de Haute-Provence in France |
Discovery date | November 24, 2005 |
Doppler Spectroscopy | |
Orbital characteristics | |
1.946 ± 0.014 AU (291,100,000 ± 2,100,000 km) [3] | |
Eccentricity | 0.525+0.024 −0.026 [3] |
1,004.7 ± 3.0 days (2.7507 ± 0.0082 years) [4] | |
Inclination | 111.4°+4.4° −4.7° [4] |
19.2°+5.0° −4.8° [4] | |
245511.1+10 −8.7 [3] | |
73.1°±4.3° [4] | |
Semi-amplitude | 168 ± 9 [2] |
Star | HD 81040 |
Physical characteristics | |
Mass | 7.53±0.032 MJ [4] |
HD 81040 b is a massive gas giant exoplanet that orbits the star HD 81040, discovered in 2005 by radial velocity. [2] 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. [3] [4]
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 7.53 MJ. [3] [1] [5] [6] [4] Since the inclination is high, there is a small chance that the planet transits. [3]