81 Ceti b

{{Short description|Extrasolar planet in the constellation Cetus}}

{{Infobox planet

| name = 81 Ceti b

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| discoverer = Sato et al.

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| discovered = July 2, 2008

| discovery_method = Doppler Spectroscopy

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| apsis = astron

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| semimajor = {{convert|2.5|AU|km|abbr=on}}

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| eccentricity = 0.206 ± 0.029

| period = 952.7 ± 8.8 d

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| time_periastron = 2486 ± 26

| arg_peri = 175 ± 69

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| star = 81 Ceti

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| mean_radius = 1.14 {{Jupiter radius|link=y}} Estimate

| mass = 5.30 {{Jupiter mass|link=y}}[https://exoplanets.nasa.gov/exoplanet-catalog/7012/81-ceti-b/ NASA 7012][https://exoplanet.eu/catalog/81_cet_b--490/ 81 Ceti b]

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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. It orbits the K-type giant star 81 Ceti at an average distance of 2.5 AU, taking about 2.6 years to revolve with an eccentricity of 0.206.

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.

See also

References

{{Reflist|refs=

{{cite journal | title=Planetary Companions to Evolved Intermediate-Mass Stars: 14 Andromedae, 81 Ceti, 6 Lyncis, and HD167042 | url=https://academic.oup.com/pasj/article/60/6/1317/1391840 | last1=Sato | first1=Bun'ei | last2=Toyota | first2=Eri | last3=Omiya | first3=Masashi | last4=Izumiura | first4=Hideyuki | last5=Kambe | first5=Eiji | last6=Masuda | first6=Seiji | last7=Takeda | first7=Yoichi | last8=Itoh | first8=Yoichi | last9=Ando | first9=Hiroyasu | display-authors=1 | journal=Publications of the Astronomical Society of Japan | volume=60 | issue=6 | pages=1317–1326 | year=2008 | arxiv=0807.0268 | bibcode=2008PASJ...60.1317S | doi=10.1093/pasj/60.6.1317}}

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