Discovery | |
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Discovered by | Jones, et al. |
Discovery site | Australia |
Discovery date | 17 September 2002 |
Detection method | Doppler spectroscopy |
Orbital characteristics | |
Semi-major axis | 2.561 AU (383.1 million km) |
Eccentricity | 0.0703 ± 0.0781 |
Orbital period (sidereal) | 1,311 ± 49 d |
Time of periastron | 2,450,870 ± 210 |
Argument of periastron | 99.8 |
Semi-amplitude | 19.6 ± 1.5 |
Star | Tau Gruis |
Tau Gruis b, also known as HD 216435 b, is an extrasolar planet approximately 109 light-years away in the constellation of Grus (the Crane). The planet was discovered orbiting the star Tau Gruis in September 2002. It was calculated that the planet orbits its sun at an average distance of 2.7 astronomical units. The planet is over 1.25 times as massive as Jupiter.
See also
References
- Jones; Butler, R. Paul; Tinney, C. G.; Marcy, Geoffrey W.; Penny, Alan J.; McCarthy, Chris; Carter, Brad D. (2003). "An exoplanet in orbit around τ1 Gruis". Monthly Notices of the Royal Astronomical Society. 341 (3): 948–952. arXiv:astro-ph/0209302. Bibcode:2003MNRAS.341..948J. doi:10.1046/j.1365-8711.2003.06481.x. S2CID 1575040. (web Preprint)
External links
- "Notes for planet HD 216435 b". Extrasolar Planets Encyclopaedia. Retrieved 2008-06-22.
- "Tau1 Gruis". Solstation. Retrieved 2008-06-22.
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