Planet TOI-132 b
| Name | TOI-132 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2019 | ||
| Mass | 0.07183 (± 0.0057) MJ | ||
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.026 ( -0.003 +0.002 ) AU | ||
| Orbital Period | 2.1097008 (± 1.2e-05) day | ||
| Eccentricity | 0.087 ( -0.057 +0.054 ) | ||
| ω | 125.47 ( -54.0 +110.0 ) deg | ||
| Tperi | — | ||
| Radius | 0.306 (± 0.0125) RJ | ||
| Inclination | 84.63 ( -5.63 +1.58 ) deg | ||
| Update | 2019-11-07 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Spectrum | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2458343.77954 (± 0.00093) JD | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 0.583 ( -0.15 +0.11 ) | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 11.58 (± 0.78) m/s | ||
| Calculated temperature | 1384.0 ( -75.0 +53.0 ) K | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
TOI-132| Name | TOI-132 | ||
| Distance | 164.47 (± 27.32) pc |  |
|
| Spectral type | G8V | ||
| Apparent magnitude V | 11.3 | ||
| Mass | 0.97 (± 0.06) MSun | |
|
| Age | 6.34 ( -2.35 +0.42 ) Gyr | |
|
| Effective temperature | 5397.0 (± 46.0) K | ||
| Radius | 0.9 (± 0.02) RSun | |
|
| Metallicity [Fe/H] | 0.16 (± 0.1) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 22:33:36.0 | ||
| Dec2000 | -43:26:12 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Related publications
Mass loss by atmospheric escape from extremely close-in planets
2022
KOSKINEN T., LAVVAS P., HUANG Ch., BERGSTEN G., FERNANDES R. & YOUNG M.
ApJ, 929, 52
paper arxiv
TOI-132 b: A short-period planet in the Neptune desert transiting a V=11.3 G-type star
2020
DIAZ M., JENKINS J., GANDOLFI D., LOPEZ E., SOTO M. et al.
MNRAS, 493, 973
paper arxiv
