Astronomy:81 Ceti b
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Short description: Extrasolar planet in the constellation Cetus
Discovery | |
---|---|
Discovered by | Sato et al. |
Discovery date | July 2, 2008 |
Doppler Spectroscopy | |
Orbital characteristics | |
2.5 AU (370,000,000 km) | |
Eccentricity | 0.206 ± 0.029 |
Orbital period | 952.7 ± 8.8 d |
astron|astron|helion}} | 2486 ± 26 |
175 ± 69 | |
Star | 81 Ceti |
Physical characteristics | |
Mean radius | 1.14 |♃|J}}}}}} Estimate |
Mass | 5.30 |♃|J}}}}}}[1][2] |
81 Ceti b (abbreviated 81 Cet b) is an extrasolar planet approximately 331 light years away in the constellation of Cetus. It is estimated to be 5.3 times the mass of Jupiter which also makes it a gas giant.[1][2] It orbits the G-type giant star 81 Ceti at an average distance of 2.5 AU, taking about 2.6 years to revolve with an eccentricity of 20.6.[3]
Discovery
The preprint announcing this planet was submitted to the arXiv electronic repository on July 2, 2008, by Bun'ei Sato and collaborators, who discovered it using the Doppler Spectroscopy method, during the Okayama Planet Search radial velocity survey of G and K giants at Okayama Astrophysical Observatory.[3]
See also
References
- ↑ 1.0 1.1 NASA 7012
- ↑ 2.0 2.1 81 Ceti b
- ↑ 3.0 3.1 Sato, Bun'ei et al. (2008). "Planetary Companions to Evolved Intermediate-Mass Stars: 14 Andromedae, 81 Ceti, 6 Lyncis, and HD167042". Publications of the Astronomical Society of Japan 60 (6): 1317–1326. doi:10.1093/pasj/60.6.1317. Bibcode: 2008PASJ...60.1317S. https://academic.oup.com/pasj/article/60/6/1317/1391840.
External links
- Jean Schneider (2011). "Notes for Planet 81 Cet b". Extrasolar Planets Encyclopaedia. https://exoplanet.eu/catalog/81_cet_b--490/.
- "81 Ceti". Exoplanets. http://media4.obspm.fr/exoplanets/base/etoile.php?nom=81+Cet.
Coordinates: 02h 37m 41.8003s, −03° 23′ 46.229″
Original source: https://en.wikipedia.org/wiki/81 Ceti b.
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