MOA-2011-BLG-262L

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MOA-2011-BLG-262L
Discovery
Discovery date2013
Microlensing
Designations
MOA-2011-BLG-262
Orbital characteristics
PeriastronN/A
ApastronN/A
N/A AU
EccentricityN/A
N/A d
(N/A y)
N/A km/s
InclinationN/A
? mas
N/A°
N/A JD
Semi-amplitudeN/A m/s
StarN/A
Physical characteristics
Mass~4 MJ

MOA-2011-BLG-262L is a red dwarf[citation needed] or possibly a rogue planet[1] which may have an exomoon named MOA-2011-BLG-262L b. The exomoon is still most likely a Neptune-like planet.[2]

The MOA-2011-BLG-262L planetary system
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b 18 M⊕ ~1 — — — —

References[]

  1. ^ 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.
  2. ^ "Eyes on Exoplanets-MOA-2011-BLG-262Lb".


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