| 词条 | HD 96167 b |
| 释义 |
| name = HD 96167 b | image = PlanetQuest-HD96167b.png | caption = HD 96167 b's orbit compared to the orbit of Mars (1.5AU) in the Solar System. This eccentric Jupiter has a comet-like orbit. | discoverer = Peek et al. | discovery_site = Lick and Keck Observatories | discovered = April 17, 2009 | discovery_method = radial velocity | apsis = astron | semimajor = {{val|1.332|0.092}} AU | eccentricity = {{val|0.681|0.033}} | period = {{val|498.1|0.81}} d | time_periastron = {{val|2463060.3|4.5}} | arg_peri = {{val|288.3|6.4}} | semi-amplitude = {{val|21.1|1.6}} | star = HD 96167 }} HD 96167 b is an extrasolar planet located approximately 280 light years away in the constellation of Crater, orbiting the 8th magnitude G-type subgiant HD 96167. It is a Jupiter-type planet that orbits at 1.3 AU in extremely elliptical orbit.[6] The planet was discovered on April 17, 2009. References1. ^1 {{cite journal | title=Old, rich, and eccentric: two jovian planets orbiting evolved metal-rich stars | last1=Peek | first1=John Asher | last2=Johnson | first2=Kathryn M. G. | last3=Fischer | first3=Debra A. | last4=Marcy | first4=Geoffrey W. | last5=Henry | first5=Gregory W. | last6=Howard | first6=Andrew W. | last7=Wright | first7=Jason T. | last8=Lowe | first8=Thomas B. | last9=Reffert | first9=Sabine | display-authors=1 | journal=Publications of the Astronomical Society of the Pacific | volume=121 | issue=880 | pages=613–620 | year=2009 | arxiv=0904.2786 | bibcode=2009PASP..121..613P | doi=10.1086/599862 }} [1]}}{{Sky|11|05|15.0681|-|10|17|28.681|274}}{{extrasolar-planet-stub}} 5 : Exoplanets|Exoplanets discovered in 2009|Giant planets|Crater (constellation)|Exoplanets detected by radial velocity |
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