OGLE-TR-113b
{{Short description|Extrasolar planet orbiting the star OGLE-TR-113}}
{{Infobox planet
| name = OGLE-TR-113b
| image = Exoplanet Comparison OGLE-TR-113 b.png
| caption = Size comparison of OGLE-TR-113b with Jupiter
| discovery_site = {{flag|Poland}}
| discovered = transit found in 2002,
proved to be a planet
on 14 April 2004
| apsis = astron
| semimajor = {{convert|0.0229|±|0.0002|AU|km|abbr=on}}
| period = 1.4324757 ± 0.0000013 d
| star = OGLE-TR-113
| mean_radius = 1.09 ±0.03 {{Jupiter radius|link=y}}
| mass = 1.32 ±0.19 {{Jupiter mass|link=y}}
}}
OGLE-TR-113b is an extrasolar planet orbiting the star OGLE-TR-113.
In 2002 the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming in the star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet, radial velocity measurements were necessary to calculate the mass of the body. In 2004, the object was proved to be a new transiting extrasolar planet.
The planet has a mass 1.32 times that of Jupiter. Since the planet's inclination is known, the value is exact. It orbits the star (OGLE-TR-113) in an extremely close orbit, even closer than the famous planets 51 Pegasi b and HD 209458 b. The planet races around the star every 1.43 days. The radius of the planet is only 9% larger than Jupiter's, despite the heating effect by the star. Planets of its kind are sometimes called "super-hot Jupiters".
See also
References
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External links
{{commonscat-inline|OGLE-TR-113 b}}
- {{cite web| url=http://media4.obspm.fr/exoplanets/base/planete.php?etoile=OGLE-TR-113&planete=b| title=OGLE-TR-113 b| work=Exoplanets| access-date=2010-01-20| archive-url=https://web.archive.org/web/20120401193427/http://media4.obspm.fr/exoplanets/base/planete.php?etoile=OGLE-TR-113&planete=b| archive-date=2012-04-01| url-status=dead}}
{{Sky|10|52|24.40|-|61|26|48.5|4892}}
{{DEFAULTSORT:Ogle-Tr-113b}}
Category:Transiting exoplanets
Category:Exoplanets discovered in 2002
Category:Carina (constellation)
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