Planet KMT-2016-BLG-2142 b
| Name | KMT-2016-BLG-2142 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2018 | ||
| Mass | 15.49 ( -8.58 +24.99 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.83 ( -0.2 +0.15 ) AU | |
|
| Orbital Period | — | ||
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2018-06-29 | ||
| 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
KMT-2016-BLG-2142| Name | KMT-2016-BLG-2142 | ||
| Distance | 7010.0 ( -1160.0 +1010.0 ) pc | |
|
| Spectral type | |||
| Apparent magnitude V | — | ||
| Mass | 0.073 ( -0.04 +0.117 ) MSun | |
|
| Age | — | ||
| Effective temperature | — | ||
| Radius | — | ||
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 17:52:27.0 | ||
| Dec2000 | -29:23:04 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Related publications
KMT-2016-BLG-1820 and KMT-2016-BLG-2142: Two Microlensing Binaries Composed of Planetary-mass Companions and Very-Low-Mass Primaries
2018
JUNG Y., HWANG K.-H., RYU Y.-H., GOULD A., HAN Ch. et al.
Astron J., 156, 208
paper arxiv
