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Extrasolar planet orbiting the star OGLE-TR-113 From Wikipedia, the free encyclopedia
OGLE-TR-113b is an extrasolar planet orbiting the star OGLE-TR-113.
Discovery | |
---|---|
Discovered by | Konacki et al.[1] |
Discovery site | Poland[1] |
Discovery date | transit found in 2002, proved to be a planet on 14 April 2004[1] |
Transit[1] | |
Orbital characteristics | |
0.0229 ± 0.0002 AU (3,426,000 ± 30,000 km)[2] | |
Eccentricity | 0[2] |
1.4324757 ± 0.0000013[2] d | |
Inclination | 88.8[2] |
Star | OGLE-TR-113 |
Physical characteristics | |
1.09 ±0.03 RJ | |
Mass | 1.32 ±0.19 MJ |
In 2002 the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming in the star's light curve indicating a transiting, planetary-sized object.[3] 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.[1]
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".[2]
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