Planet TOI-1759 b
| Name | TOI-1759 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2022 | ||
| Mass | 0.0214 (± 0.006) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.1176 (± 0.0013) AU | |
|
| Orbital Period | 18.849975 (± 6e-06) day | |
|
| Eccentricity | 0.0 | |
|
| ω | — | ||
| Tperi | — | ||
| Radius | 0.273 (± 0.0196) RJ | |
|
| Inclination | 89.2 (± 0.5) deg | |
|
| Update | 2022-02-04 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2458745.4661 (± 0.001) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 0.5 (± 0.3) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 2.3 (± 0.7) m/s | |
|
| Calculated temperature | 433.0 (± 14.0) K | |
|
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
TOI-1759| Name | TOI-1759 | ||
| Distance | 40.12 (± 0.02) pc | |
|
| Spectral type | M0V | ||
| Apparent magnitude V | 11.0 | ||
| Mass | 0.61 (± 0.02) MSun | |
|
| Age | 5.0 (± 2.0) Gyr | |
|
| Effective temperature | 4036.0 (± 100.0) K | |
|
| Radius | 0.6 (± 0.03) RSun | |
|
| Metallicity [Fe/H] | 0.2 (± 0.4) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 21:47:24.0 | ||
| Dec2000 | +62:45:14 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Observability Predictor 
Remarks
04 Fev 2022Espinoza et al. (2022) find a slightly different planet mass of 10.8 #177; 0.1 M
Related publications
TOI-1759 b: a transiting sub-Neptune around a low mass star characterized with SPIRou and TESS
2022
MARTIOLI E., HEBRARD G., FOUQUE P., ARTIGAU E., DONATI J.-F. et al.
Astron. & Astrophys., 660, A86
paper arxiv
A transiting, temperate mini-Neptune orbiting the M dwarf TOI-1759 unveiled by TESS
2022
ESPINOZA N., PALLE E., KEMMER J., LUQUE R., CABALLERO J. et al.
Astron. J., 163, 133
paper arxiv
