Planet LTT 3780 b
| Name | LTT 3780 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2020 | ||
| Mass | 0.00982 (± 0.0016) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.012 AU | |
|
| Orbital Period | 0.7683881 (± 8.4e-05) day | |
|
| Eccentricity | 0.064 ( -0.046 +0.075 ) | |
|
| ω | 251.0 (± 66.0) deg | |
|
| Tperi | — | ||
| Radius | 0.11883 (± 0.00669) RJ | |
|
| Inclination | 85.9 ( -0.5 +0.59 ) deg | ||
| Update | 2020-03-04 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Spectrum | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2458543.91281 ( -0.00052 +0.00048 ) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 0.518 ( -0.089 +0.059 ) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | 892.0 K | |
|
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | TOI-732 b, LP 729-54 b |
Star
LTT 3780| Name | LTT 3780 | ||
| Distance | 21.981 (± 0.04) pc | |
|
| Spectral type | M4V | ||
| Apparent magnitude V | 13.0 | ||
| Mass | 0.401 (± 0.012) MSun | |
|
| Age | — | ||
| Effective temperature | 3360.0 (± 51.0) K | |
+ |
| Radius | 0.374 (± 0.011) RSun | |
|
| Metallicity [Fe/H] | 0.28 (± 0.13) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 10:18:35.0 | ||
| Dec2000 | -11:43:04 | ||
| Alternate Names | TOI-732, LP 729-54 | ||
| Planetary system | 2 planets |
Related publications
The Thermal Emission Spectrum of the Closest M Dwarf Transiting Rocky Planet
2021
BERTA-THOMPSON Z. et al.
JWST GO Programme
abstract
A pair of TESS planets spanning the radius valley around the nearby mid-M dwarf LTT 3780
2020
CLOUTIER R., EASTMAN J., RODRIGUEZ J., ASTUDILLO-DEFRU N., BONFILS X. et al.
Astron. J., 160, 3
paper arxiv
The CARMENES search for exoplanets around M dwarfs. Two planets on the opposite sides of the radius gap transiting the nearby M dwarf LP 729-54
2020
NOWAK G., LUQUE R., PARVIAINEN H., PALLE E., MOLAVERDIKHANI K. et al.
Astron. & Astrophys., 642, A173
paper arxiv
