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{{Infobox planet
| name = HD 88133 b
| discoverer = Fischer, Laughlin,
Butler et al.
| discovery_site = California
| discovered = September 6, 2004
| discovery_method = Radial velocity
(N2K Consortium)
| apsis = astron
| semimajor = {{val|0.0479|0.0032}} AU
| eccentricity = 0 (fixed)[1]
| period = {{val|3.414887|0.000045}}[1] d
| time_periastron = {{val|2463014.948|s=(fixed)}}[1]
| arg_peri = {{val|205.3|3.3}}[1]
| semi-amplitude = {{val|32.7|1.0}}[1]
| star = HD 88133
}}HD 88133 b is an extrasolar planet orbiting the star HD 88133. It is probably less massive than Jupiter and even Saturn. It orbits the star in a very tight orbit, completing one revolution around the star in every three and half days or so. Despite the relatively large radius of the star (about 2 times Solar), no transits have been detected.References1. ^1 2 3 4 5 {{cite journal | title=Radial Velocities from the N2K Project: Six New Cold Gas Giant Planets Orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810 | last1=Ment | first1=Kristo | last2=Fischer | first2=Debra A. | last3=Bakos | first3=Gaspar | last4=Howard | first4=Andrew W. | last5=Isaacson | first5=Howard | display-authors=1 | journal=The Astronomical Journal | volume=156 | issue=5 | at=213 | year=2018 | arxiv=1809.01228 | bibcode=2018AJ....156..213M | doi=10.3847/1538-3881/aae1f5 }}
[1]
}}External links- {{cite web | url=http://media4.obspm.fr/exoplanets/base/etoile.php?nom=HD+88133 | title=HD 88133 | work=Exoplanets}}
{{Sky|10|10|07.68|+|18|11|12.74|242.7}}{{DEFAULTSORT:Hd 88133 B}}{{extrasolar-planet-stub}} 6 : Exoplanets|Hot Jupiters|Exoplanets discovered in 2004|Giant planets|Leo (constellation)|Exoplanets detected by radial velocity |