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#REDIRECT [[VB 10#Claims of a planetary system]]
{{Planetbox begin
| name = VB 10b
}}
{{Planetbox image
| image = 352344main A-VB10b art-516.jpg
| caption = An artist's impression of VB 10b<br>showing the relative size of its parent star.
}}
{{Planetbox star
| star = [[VB 10]]
| constell = [[Aquila (constellation)|Aquila]]
| RA = {{RA|19|16|57.62}}
| DEC = {{DEC|+05|09|02.2}}
| app_mag = 17.30
| dist_ly = 19.85
| dist_pc = 6.09
| class = M8V
}}
{{Planetbox orbit
| semimajor = 0.360 ({{±|0.016|0.006}})
| semimajor_mas = 59.1
| periastron =
| apastron =
| eccentricity = <0.98
| inclination = 96.9 ({{±|7.4|1.8}})
| period = 271.56 ({{±|6.9|3}})
| arg_peri = 38.7 ({{±|4.8|3.3}})
| t_peri =
| semi-amp =
}}
{{Planetbox character
| mass = 6.4 ({{±|2.6|3.1}})
| radius =
| temperature =
}}
{{Planetbox discovery
| discovery_date = May 2009
| discoverers = Pravdo and Shaklan of [[JPL]]
| discovery_method = [[Methods_of_detecting_extrasolar_planets#Astrometry|Astrometry]]
| discovery_site = [[Pasadena, California]]
| discovery_status = Announced (Preprint)
}}
{{Planetbox catalog
| names = Gliese 752 Bb
}}
{{Planetbox reference
| star = VB+10
| planet = b
}}
{{Planetbox end}}


[[Category:Disproven exoplanets]]
In May of 2009 astronomers from [[NASA|NASA's]] [[Jet Propulsion Laboratory]], [[Pasadena, California]] announced the [[Methods_of_detecting_extrasolar_planets#Astrometry|astrometric discovery]] of a planet, '''VB 10b''', orbiting a nearby [[red dwarf]], using the {{convert|200|in|m|abbr=on}} [[Hale telescope]] at the [[Palomar Observatory]]. If confirmed, the [[extrasolar planet]] will be the first discovered using this method, and the star, [[VB 10]], will be the least massive to known to host a planet.<ref name="disc">{{cite journal
| title = An Ultracool Star's Candidate Planet
| url = http://steps.jpl.nasa.gov/links/docs/pravdoshaklan09vb10b.pdf
| year = 2009
| journal = Submitted to the [[Astrophysical Journal]]
| last1 = Pravdo ''et al.''
| accessdate = 2009-05-30}}</ref><ref name="announce">{{cite web
| title=Planet-Hunting Method Succeeds at Last
| url=http://www.nasa.gov/topics/universe/features/exoplanet-20090528.html
| work=NASA NEWS, NEWS RELEASE: 2009-090
| accessdate=2009-05-28}}</ref>

VB 10b is reported to be a [[gas giant]] orbiting the star [[VB 10]] in the [[constellation]] of [[Aquila (constellation)|Aquila]]. It is reported to be approximately six times the mass of [[Jupiter]] and is about 20 [[light years]] away from Earth.<ref name="announce" /><ref>{{cite news|url=http://www.newscientist.com/article/dn17208-exoplanet-found-by-measuring-stars-sideways-shift.html|title=Exoplanet found by measuring star's sideways shift |last= McKee|first=Maggie |date=28 May 2009|publisher=New Scientist}}</ref>
This planetary system is also unique in the ratio of the mass of the planet to the mass of the star. Up to 10% of the mass of this entire star-planet system could be in the planet.<ref name="disc"/>

==Past claims based on astrometry==
{{main|Methods of detecting extrasolar planets#Astrometry|l1=Astrometry as an extrasolar planet detection method}}
VB 10b is not the first extrasolar planet claimed to be found by astrometry. In 1969 [[Peter Van de Kamp]] claimed that a planet was orbiting [[Barnard's Star]], and in 1996 a claim of planets orbiting the nearby star [[Lalande 21185]] appeared in the popular press.<ref>{{cite news|title=Data Seem to Show a Solar System Nearly in the Neighborhood|publisher=The New York Times|author=John Wilford|date=1996-06-12|accessdate=2009-05-29|page=1|url=http://www.nytimes.com/1996/06/12/us/data-seem-to-show-a-solar-system-nearly-in-the-neighborhood.html}}</ref> Subsequent analysis and further observations of those stars showed both claims to be erroneous.<ref name="sky">{{cite web
| title=Astronomers Pioneer New Method for Finding Exoplanets
| url=http://www.skyandtelescope.com/news/46462532.html
| publisher=[[Sky and Telescope]]
| accessdate=2009-05-29
}}</ref>

==References==
{{reflist}}

[[Category:Aquila constellation]]
[[Category:Extrasolar planets]]
[[Category:Exoplanets discovered in 2009]]
[[Category:Gas giant planets]]

{{Sky|19|16|58|+|05|09|02|19.85}}

{{Extrasolar-planet-stub}}

[[fr:VB 10b]]
[[fi:VB 10b]]

Latest revision as of 17:18, 17 January 2021