Planet TOI-849 b
| Name | TOI-849 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2020 | ||
| Mass | 0.12299 ( -0.00802 +0.00837 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.01598 ( -0.00014 +0.00013 ) AU | |
|
| Orbital Period | 0.76552414 ( -2.79e-06 +2.62e-06 ) day | |
|
| Eccentricity | 0.0 (± 0.0) | ||
| ω | 360.0 (± 0.0) deg | ||
| Tperi | — | ||
| Radius | 0.30726 ( -0.01026 +0.01401 ) RJ | |
|
| Inclination | 86.8 ( -2.4 +2.1 ) deg | ||
| Update | 2021-03-30 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2458394.73768 ( -0.00099 +0.00091 ) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 0.212 ( -0.14 +0.145 ) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 28.64 ( -0.00182 +0.00187 ) m/s | |
|
| Calculated temperature | 1800.0 K | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
TOI-849| Name | TOI-849 | ||
| Distance | 225.2 ( -5.8 +6.1 ) pc | |
|
| Spectral type | G | ||
| Apparent magnitude V | 11.98 | ||
| Mass | 0.929 (± 0.023) MSun | |
|
| Age | 6.7 ( -2.4 +2.8 ) Gyr | |
|
| Effective temperature | 5375.3 ( -41.4 +41.8 ) K | |
|
| Radius | 0.919 ( -0.022 +0.031 ) RSun | |
|
| Metallicity [Fe/H] | 0.19 (± 0.03) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 01:54:51.8 | ||
| Dec2000 | -29:25:18 | ||
| Alternate Names | TIC 33595516 | ||
| Planetary system | 1 planet |
Observability Predictor 
Remarks
Armstrong et al. (2020) : TOI-489 b is probably a remnant planetary core. The equilibrium telmperature is computed assuming an albedo of 0.3.Related publications
Removal of Hot Saturns in Mass-Radius Plane by Runaway Mass Loss
2023
THORNGREN D., LEE E. & LOPEZ E.
ApJ. Letters, 945, L36
paper arxiv
The mass-radius relation of intermediate-mass planets outlined by hydrodynamic escape and thermal evolution
2022
KUBYSHKINA D. & FOSSATI L.
Astron. & Astrophys., in press
paper
The key impact of the host star's rotational history on the evolution of TOI-849b
2021
PEZZOTTI C., ATTIA O., EGGENBERGER P., BULDGEN G. & BOURRIER V.
Astron. & Astrophys., 454, L5
paper arxiv
A remnant planetary core in the hot Neptunian desert
2020
ARMSTRONG D., LOPEZ Th., ADIBEKYAN V., BOOTH R., BRYANT E. et al.
Nature, 583, 39
paper
arxiv
