Astronomy:OGLE-2005-BLG-071L

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OGLE-2005-BLG-071L
Observation data
Equinox J2000.0]] (ICRS)
Constellation Scorpius
Right ascension  17h 50m 09.77s[1]
Declination –34° 40′ 23.5″[1]
Apparent magnitude (V) 19.5
Characteristics
Spectral type M5[1]
Astrometry
Distance3,500±300[2] pc
Details
Mass0.426±0.037[2] M☉
Other designations
EWS 2005-BUL-71, EWS 2005-BLG-71
Database references
SIMBADdata
Extrasolar Planets
Encyclopaedia		data

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] the second planet found by this method.[2] The planet was later confirmed by the Keck telescope and its properties were refined.[2]

The OGLE-2005-BLG-071L planetary system[1]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b 3.8 +0.3−0.4
or 3.4 ± 0.3 MJ 		3.6 ± 0.2
or 2.1 ± 0.1 		— — — —

See also

References

  1. ↑ 1.0 1.1 1.2 1.3 Dong, Subo et al. (2009). "OGLE-2005-BLG-071Lb, the Most Massive M Dwarf Planetary Companion?". The Astrophysical Journal 695 (2): 970–987. doi:10.1088/0004-637X/695/2/970. Bibcode: 2009ApJ...695..970D. 
  2. ↑ 2.0 2.1 2.2 2.3 Bennett, David P.; Bhattacharya, Aparna; Beaulieu, Jean-Philippe; Blackman, Joshua W.; Vandorou, Aikaterini; Terry, Sean K.; Cole, Andrew A.; Henderson, Calen B. et al. (2020). "Keck Observations Confirm a Super-Jupiter Planet Orbiting M Dwarf OGLE-2005-BLG-071L". The Astronomical Journal 159 (2): 68. doi:10.3847/1538-3881/ab6212. Bibcode: 2020AJ....159...68B. 
  3. ↑ Udalski, A. et al. (2005). "A Jovian-Mass Planet in Microlensing Event OGLE-2005-BLG-071". The Astrophysical Journal 628 (2): L109–L112. doi:10.1086/432795. Bibcode: 2005ApJ...628L.109U. 

Coordinates: Sky map 17h 50m 09s, −34° 40′ 23″




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