OGLE-2005-BLG-071L
This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "OGLE-2005-BLG-071L"
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content
OGLE-2005-BLG-071L
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Scorpius
Right ascension 17h 50m 09s
Declination –34° 40′ 23″
Apparent magnitude (V) 19.5
Distance approx. 11000 ly
(approx. 3300 pc)
Spectral type M?
Other designations
EWS 2005-BLG-071L
Database references
SIMBAD data
Extrasolar Planets
Encyclopaedia
data

OGLE-2005-BLG-071L is a distant, magnitude 19.5 star located in the constellation Scorpius, approximately 11000 light years away from the Solar System. The star is probably a red dwarf with a mass 46% of that of our Sun.1

The OGLE-2005-BLG-071L system
Companion Mass Observed separation
(AU)
b 3.5 ± 0.3 MJ 3.6 ± 0.2

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See also

Reference

  1. ^ Dong, S. et al. (2008). "OGLE-2005-BLG-071Lb, the Most Massive M-Dwarf Planetary Companion?" arxiv:0804.1354 [astro-ph]. Retrieved on 2008-08-22.
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