OGLE-TR-56
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Observation data Epoch J2000.0 |
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Constellation (pronunciation) |
Sagittarius |
Right ascension | 17h 56m 35.51s [1] |
Declination | -29° 32' 21.2" [1] |
Apparent magnitude (V) | 16.6 [1] |
Distance | ~4,900 ly (~1,500 [2] pc) |
Spectral type | G? |
OGLE-TR-56 is a star similar to the sun[2] in the constellation Sagittarius. In 2003, an extrasolar planet was discovered orbiting the star.
[edit] OGLE-TR-56b
Discovery
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Discovered by | Konacki et al. |
Discovery date | Nov 3, 2002 (confirmed: Jan 4, 2003) |
Detection method | Transit |
Semi-major axis | 0.0225 ± 0.0004 AU |
Eccentricity | 0 |
Orbital period | 1.211909 ± 0.000001 d[3] |
Inclination | 78.8 ± 0.5° |
Angular distance | 0.015 mas |
Physical characteristics
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Mean radius | 1.30 ± 0.05 RJ[3] |
Mass | 1.29 ± 0.12 MJ[3] |
OGLE-TR-56b is an extrasolar hot jupiter discovered in 2002[1] by the OGLE project using the transit method and confirmed in 2003 by the Doppler technique.[2] As of 2007 it has the shortest orbital period of any known extrasolar planet.
[edit] References
- ^ a b c d Udalski et al. (2002). "The Optical Gravitational Lensing Experiment. Search for Planetary and Low-Luminosity Object Transits in the Galactic Disk. Results of 2001 Campaign - Supplement". Acta Astronomica 52: 115.(web Preprint)
- ^ a b c Konacki et al. (2003). "An extrasolar planet that transits the disk of its parent star". Nature 421: 507–509. doi: .(web Preprint)
- ^ a b c Pont et al. (2007). "The "666" collaboration on OGLE transits I. Accurate radius of the planets OGLE-TR-10b and OGLE-TR-56b with VLT deconvolution photometry". Astronomy and Astrophysics 465: 1069–1074. doi: .(web Preprint)
[edit] External links
- OGLE-TR-56 (Extrasolar Visions)
- OGLE-TR-56b (Extrasolar Visions)
- Planet: OGLE-TR-56b (The Extrasolar Planets Encyclopaedia)