Planet OGLE-2014-BLG-0124L b
| Name | OGLE-2014-BLG-0124L b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2014 | ||
| Mass | 0.64 ( -0.044 +0.044 ) MJ | ||
| Mass*sin(i) | — | ||
| Semi-Major Axis | 3.48 (± 0.22) AU |  |
+ |
| Orbital Period | — | ||
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2017-09-05 | ||
| Detection Method | Microlensing | ||
| Mass Detection Method | Microlensing | ||
| Radius Detection Method | — | ||
| Molecules | — | ||
| 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
OGLE-2014-BLG-0124L| Name | OGLE-2014-BLG-0124L | ||
| Distance | 3600 (± 300) pc | |
+ |
| Spectral type | |||
| Apparent magnitude V | — | ||
| Mass | 0.89 (± 0.05) MSun | |
+ |
| Age | — | ||
| Effective temperature | — | ||
| Radius | — | ||
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 18:02:29.0 | ||
| Dec2000 | -28:23:47 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Related publications
Combining Spitzer parallax and Keck II adaptive optics imaging to measure the mass of a solar-like star orbited by a cold gaseous planet discovered by microlensing
2017
BEAULIEU J.-Ph., BATISTA V., BENNETT D., MARQUETTE J.-B., BLACKMAN J. et al.
ApJ, 155, 78
paper arxiv
Is the Galactic bulge devoid of planets?
2016
PENNY M., HENDERSON C. & CLANTON Ch.
ApJ, 830, 150
arxiv
paper
ADS
Planet Sensitivity from Combined Ground- and Space-based Microlensing Observations
2015
ZHU W., GOULD A., BEICHMAN C., NOVATI S., CAREY S. et al.
ApJ, 814, 129
paper arxiv
ADS
Spitzer as Microlens Parallax Satellite: Mass Measurement for the OGLE-2014-BLG-0124L Planet and its Host Star
2014
UDALSKI A., YEE J., GOULD A., CAREY S., ZHU W. et al.
ApJ, submitted
arxiv
