- OGLE-2005-BLG-071Lb
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OGLE-2005-BLG-071Lb Extrasolar planet List of extrasolar planets
Artist's conception of OGLE-05-071Lb. Parent star Star OGLE-2005-BLG-071L Constellation Scorpius Right ascension (α) 17h 50m 09s Declination (δ) –34° 40′ 23″ Distance approx. 11000 ly
(approx. 3300 pc)Spectral type M? Observed separation Projected separation (d) 3.6 ± 0.2 AU Physical characteristics Mass (m) 3.5 ± 0.3 MJ Discovery information Discovery date 27 May 2005 Discoverer(s) Udalski et al. Detection method Gravitational microlensing Discovery status Published Other designations EWS 2005-BUL-071Lb, EWS 2005-BLG-071LbDatabase references Extrasolar Planets
Encyclopaediadata SIMBAD data OGLE-2005-BLG-071Lb is an planet discovered by the Optical Gravitational Lensing Experiment (OGLE) and others in 2005, using gravitational microlensing.[1] According to the best fit model, it has about 3.5 times the mass of Jupiter and a projected separation of 3.6 astronomical units from the star. This would result in an effective temperature around 50 K, similar to that of Neptune. However, an alternative model which gives a slightly lower mass of 3.3 times that of Jupiter and a projected separation of 2.1 AU is only slightly less likely. It may be the most massive planet currently known around a red dwarf star (though only lower limits are known for those planets detected by the radial velocity method).[2]
See also
References
- ^ Udalski, A. et al. (2005). "A Jovian-Mass Planet in Microlensing Event OGLE-2005-BLG-071". The Astrophysical Journal 628 (2): L109–L112. arXiv:astro-ph/0505451. Bibcode 2005ApJ...628L.109U. doi:10.1086/432795.
- ^ Dong et al; Gould, Andrew; Udalski, Andrzej; Anderson, Jay; Christie, G. W.; Gaudi, B. S.; Jaroszyński, M.; Kubiak, M. et al. (2009). "OGLE-2005-BLG-071Lb, THE MOST MASSIVE M DWARF PLANETARY COMPANION?". The Astrophysical Journal 695 (2): 970–987. Bibcode 2009ApJ...695..970D. doi:10.1088/0004-637X/695/2/970. http://www.iop.org/EJ/abstract/0004-637X/695/2/970.
Coordinates:
17h 50m 09s, −34° 40′ 23″
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