Planet MOA-2011-BLG-262L b
| Name | MOA-2011-BLG-262L b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2013 | ||
| Mass | 0.0566340496492 ( -0.0314633609162 +0.0880974105654 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.84 ( -0.25 +0.14 ) AU | |
|
| Orbital Period | — | ||
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2014-05-22 | ||
| Detection Method | Microlensing | ||
| Mass Detection Method | — | ||
| Radius Detection Method | — | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
MOA-2011-BLG-262L| Name | MOA-2011-BLG-262L | ||
| Distance | 7350.0 (± 350.0) pc | |
|
| Spectral type | |||
| Apparent magnitude V | — | ||
| Mass | 0.12 ( -0.19 +0.06 ) MSun | |
|
| Age | — | ||
| Effective temperature | — | ||
| Radius | — | ||
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 18:00:23.0 | ||
| Dec2000 | -30:45:17 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Remarks
31 Jan 2014: An alternate model leads to a host mass of ~ 4 MJup (Bennett et al. 2014)More data
- Simbad
- Most recent references (ADS)
Observability Predictor 
Remarks
31 Jan 2014: An alternate model gives a sub Earth mass of 0.540.300.19 MEarth at a projected separation of 0.130.190.04 AU (Bennett et al.2014)Related publications
Is the Galactic bulge devoid of planets?
2016
PENNY M., HENDERSON C. & CLANTON Ch.
ApJ, 830, 150
arxiv
paper
ADS
MOA-2011-BLG262L b: A Sub-Earth-Mass Moon Orbiting a Gas Giant Primary or a High Velocity Planetary System in the Galactic Bulge
2014
BENNETT D., BATISTA V., BOND I., BENNETT C., SUZUKI D. et al.
ApJ, 785, 155
paper arxiv
New Method to Measure Proper Motions of Microlensed Sources: Application to Candidate Free-Floating-Planet Event MOA-2011-BLG-262
2014
SKOWRON J., UDALSKI A., SZYMANSKI M., KUBIAK M., PIETRZYNSKI G. et al.
ApJ, 785, 156
paper arxiv
