Planet TOI-1235 b
| Name | TOI-1235 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2020 | ||
| Mass | 0.0186 (± 0.00195) MJ |  |
+ |
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.03826 (± 0.00049) AU | |
|
| Orbital Period | 3.444717 (± 4.2e-05) day | |
+ |
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | 0.15113 (± 0.0071) RJ | |
+ |
| Inclination | 88.9 ( -0.57 +0.62 ) deg | |
|
| Update | 2020-04-15 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2458683.6155 (± 0.0017) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 0.25 (± 0.14) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 3.4 (± 0.35) m/s | |
|
| Calculated temperature | 775.0 (± 13.0) K | |
|
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
TOI-1235| Name | TOI-1235 | ||
| Distance | 39.68 (± 0.048) pc | |
|
| Spectral type | M0.5V | ||
| Apparent magnitude V | 11.0 | ||
| Mass | 0.63 (± 0.024) MSun | |
|
| Age | 0.8 (± 0.2) Gyr | |
|
| Effective temperature | 3997.0 (± 51.0) K | |
|
| Radius | 0.619 (± 0.019) RSun | |
|
| Metallicity [Fe/H] | 0.33 (± 0.16) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 10:08:52.0 | ||
| Dec2000 | +69:16:36 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Related publications
Absence of extended atmospheres in low-mass star radius-gap planets GJ 9827 b, GJ 9827 d and TOI-1235 b
2023
KRISHNAMURTHY V., HIRANO T., GAIDOS E., SATO B., KOPPARAPU R. et al.
MNRAS, 521, 1210
paper arxiv
Precise mass and radius of a transiting super-Earth planet orbiting the M dwarf TOI-1235: a planet in the radius gap?
2020
BLUHM P., LUQUE R., ESPINOZA N., PALLE E., CABALLERO J. et al.
Astron. & Astrophys., 639, A132
paper arxiv
TOI-1235 b: a keystone super-Earth for testing radius valley emergence models around early M dwarfs
2020
CLOUTIER R., RODRIGUEZ J., IRWIN J., CHARBONNEAU D., STASSUN K. et al.
ApJ. Letters, submitted
arxiv
