Planet NGTS-10 b
| Name | NGTS-10 b | ||
| Planet Status | Confirmed | ||
| Discovered in | — | ||
| Mass | 2.162 ( -0.107 +0.092 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.0143 (± 0.001) AU | |
|
| Orbital Period | 0.7668944 (± 3e-07) day | |
|
| Eccentricity | 0.0 | |
|
| ω | — | ||
| Tperi | — | ||
| Radius | 1.205 ( -0.083 +0.117 ) RJ | |
|
| Inclination | 79.0 (± 2.0) deg | |
|
| Update | 2019-09-30 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Spectrum | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2457518.84377 (± 0.00017) JD | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | |
|
| Velocity Semiamplitude K | 595.0 (± 7.0) m/s | |
|
| Calculated temperature | 1332.0 ( -54.0 +49.0 ) K | |
|
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
NGTS-10| Name | NGTS-10 | ||
| Distance | — | ||
| Spectral type | K5V | ||
| Apparent magnitude V | 14.3 | ||
| Mass | 0.696 (± 0.04) MSun | |
|
| Age | 10.4 (± 2.5) Gyr | |
+ |
| Effective temperature | 4400.0 (± 100.0) K | ||
| Radius | 0.697 (± 0.036) RSun | |
|
| Metallicity [Fe/H] | -0.02 (± 0.12) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 06:07:29.0 | ||
| Dec2000 | -25:35:42 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Remarks
Due to a software bug, the coodrinates are provisionnally incorrect
More data
- Simbad
- Most recent references (ADS)
Related publications
The impact of tidal friction evolution on the orbital decay of ultra-short period planets
2021
ALVARADO-MONTES J., SUCERQUIA M., GARCIA-CARMONA C., ZULUAGA J., SPITLER L. & SCHWAB Ch.
MNRAS, accepted
arxiv
From East to West: The First Simultaneous Temperature and Cloud Map of a Hot Jupiter
2021
PARMENTIER V. et al.
JWST GO Programme
abstract
NGTS-10b: The shortest period hot Jupiter yet discovered
2019
MCCORMAC J., GILLEN E., JACKMAN J., BROWN D., BAYLISS D. et al.
MNRAS, submitted
arxiv
