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MOA-2011-BLG-262L

Artist's impression showing the two models of the MOA-2011-BLG-262L system
Observation data
Epoch J2000       Equinox J2000
Constellation Sagittarius [1]
Right ascension 18h 00m 23.48s [2]
Declination −31° 14′ 42.93″ [2]
Astrometry
Distance~1,800 or ~23,000  ly
(~560 or ~7,200 [2]  pc)
Details [2]
Mass0.11+0.21
−0.06
or 0.003  M
Mass115.2327 or 3.6+2.0
−1.7
  MJup
Database references
SIMBAD data

MOA-2011-BLG-262L is an astronomical object of uncertain nature with an orbiting companion, detected through the gravitational microlensing event MOA-2011-BLG-262 in the constellation Sagittarius. Two different models fit the observation equally well - an object of ~3.2  MJ, likely a rogue planet, at a distance of about 0.56 kiloparsecs (1,800 light-years) and orbited by a ~0.47  M🜨 exomoon; or an object of ~0.11  M, likely a red dwarf star, at a distance of about 7.2 kiloparsecs (23,000 light-years) in the galactic bulge, and orbited by a ~17 M🜨 planet. The discovery team considers the latter scenario to be more likely, but the former is a better fit. [2] [3]

Planetary system

The MOA-2011-BLG-262L planetary system [2]
Companion
(in order from star)
Mass Semimajor axis
( AU)
Orbital period
( days)
Eccentricity Inclination Radius
b 18+28
−10
or 0.54+0.30
−0.19
  M🜨
0.84+0.25
−0.14
or 0.13+0.06
−0.04

References

  1. ^ "Finding the constellation which contains given sky coordinates". djm.cc. 2 August 2008.
  2. ^ a b c d e f Bennett, D.P.; Batista, V.; et al. (13 December 2013). "A Sub-Earth-Mass Moon Orbiting a Gas Giant Primary or a High Velocity Planetary System in the Galactic Bulge". The Astrophysical Journal. 785 (2): 155. arXiv: 1312.3951. Bibcode: 2014ApJ...785..155B. doi: 10.1088/0004-637X/785/2/155. S2CID  118327512.
  3. ^ Clavin, Whitney (10 April 2014). "Faraway Moon or Faint Star? Possible Exomoon Found". NASA. Archived from the original on 12 April 2014. Retrieved 19 February 2023.