OGLE-2005-BLG-071L is a distant, magnitude 19.5 galactic bulge star located in the constellation Scorpius , approximately 11,000 light years away from the Solar System . The star is probably a red dwarf with a mass 43% of that of the Sun .
Planetary system
In 2005 an exoplanet was discovered orbiting this star by the microlensing method,[ 3] [ 2] Keck telescope and its properties were refined.[ 2]
See also
References
^ a b c d Dong, Subo; et al. (2009). "OGLE-2005-BLG-071Lb, the Most Massive M Dwarf Planetary Companion?". The Astrophysical Journal . 695 (2): 970–987. arXiv :0804.1354 Bibcode :2009ApJ...695..970D . doi :10.1088/0004-637X/695/2/970 . S2CID 119186629 . ^ a b c d Bennett, David P.; Bhattacharya, Aparna; Beaulieu, Jean-Philippe; Blackman, Joshua W.; Vandorou, Aikaterini; Terry, Sean K.; Cole, Andrew A.; Henderson, Calen B.; Koshimoto, Naoki; Lu, Jessica R.; Baptiste Marquette, Jean; Ranc, Clément; Udalski, Andrzej (2020). "Keck Observations Confirm a Super-Jupiter Planet Orbiting M Dwarf OGLE-2005-BLG-071L" . The Astronomical Journal . 159 (2): 68. arXiv :1909.04740 Bibcode :2020AJ....159...68B . doi :10.3847/1538-3881/ab6212 S2CID 202558435 . ^ 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 . S2CID 7425167 .
External links
