Planet OGLE-2012-BLG-0950L b
| Name | OGLE-2012-BLG-0950L b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2016 | ||
| Mass | 0.11 ( -0.028 +0.053 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 2.7 ( -0.7 +0.6 ) AU | |
|
| Orbital Period | — | ||
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2023-04-17 | ||
| 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 | MOA-2012- BLG-527 b |
Star
OGLE-2012-BLG-0950L| Name | OGLE-2012-BLG-0950L | ||
| Distance | 3000.0 ( -1100.0 +800.0 ) pc | ||
| Spectral type | M | ||
| Apparent magnitude V | — | ||
| Mass | 0.56 ( -0.16 +0.12 ) MSun | ||
| Age | — | ||
| Effective temperature | 5500.0 K | ||
| Radius | — | ||
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 18:08:04.6 | ||
| Dec2000 | -29:43:54 | ||
| Alternate Names | MOA-2012- BLG-527 | ||
| Planetary system | 1 planet |
Related publications
Adaptive Optics Imaging Can Break the Central Caustic Cusp Approach Degeneracy in High Magnification Microlensing Events
2022
TERRY S. K., BENNETT D. P., BHATTACHARYA A., KOSHIMOTO N., BEAULIEU J. et al.
Astron. J., 164, 217
paper arxiv
Adaptive Optics Imaging Can Break the Central Caustic Cusp Approach Degeneracy in High-magnification Microlensing Events
2022
TERRY S., BENNETT D., BHATTACHARYA A., KOSHIMOTO N., BEAULIEU J.-Ph. et al.
Astron. J., 164, 217
paper
MASADA: From Microlensing Planet Mass-Ratio Function to Planet Mass Function
2022
GOULD A.
arxiv
WFIRST Exoplanet Mass Measurement Method Finds a Planetary Mass of 39±8M⊕ for OGLE-2012-BLG-0950Lb
2018
BHATTACHARYA A., BEAULIEU J.-Ph., BENNET D., ANDERSON J., KOSHIMOTO N. et al
Astron. J., 156, 289
paper arxiv
OGLE-2012-BLG-0950Lb: The First Planet Mass Measurement from Only Microlens Parallax and Lens Flux
2017
KOSHIMOTO N., UDALSKI A., BEAULIEU J., SUMI T., BENNETT D. et al.
Astron. J., 153, 1
paper arxiv ADS
