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OGLE-2005-BLG-071L

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OGLE-2005-BLG-071L
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Scorpius
Right ascension 17 50 09.77
Declination –34° 40′ 23.5″
Apparent magnitude (V) 19.5
Characteristics
Spectral type M5
Astrometry
Distance3,500±300 pc
Details
Mass0.426±0.037 M
Other designations
EWS 2005-BUL-71, EWS 2005-BLG-71
Database references
SIMBADdata

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, the second planet found by this method. The planet was later confirmed by the Keck telescope and its properties were refined.

The OGLE-2005-BLG-071L planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 3.8
−0.4
or 3.4 ± 0.3 MJ
3.6 ± 0.2
or 2.1 ± 0.1

See also

References

  1. ^ 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.
  2. ^ 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.
  3. 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.

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