Planet TOI-677 b
| Name | TOI-677 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2019 | ||
| Mass | 1.236 (± 0.069) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.1038 (± 0.0017) AU | |
|
| Orbital Period | 11.2366 (± 0.00011) day | |
|
| Eccentricity | 0.435 (± 0.024) | |
|
| ω | 70.1 (± 3.6) deg | |
|
| Tperi | — | ||
| Radius | 1.179 (± 0.03) RJ | |
|
| Inclination | 87.63 (± 0.11) deg | |
|
| Update | 2019-11-14 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Spectrum | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2458547.47448 (± 0.000289) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 0.723 ( -0.024 +0.018 ) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | 1252.0 K | |
|
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
TOI-677| Name | TOI-677 | ||
| Distance | 143.0 (± 5.0) pc | |
|
| Spectral type | — | ||
| Apparent magnitude V | 9.7 | ||
| Mass | 1.18 (± 0.058) MSun | |
|
| Age | 2.92 ( -0.73 +0.8 ) Gyr | |
|
| Effective temperature | 6295.0 (± 77.0) K | |
|
| Radius | 1.28 (± 0.03) RSun | |
|
| Metallicity [Fe/H] | 0.0 | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 16:32:18.0 | ||
| Dec2000 | -22:21:30 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Related publications
Orbital alignment of the eccentric warm Jupiter TOI-677 b
2023
SEDAGHATI E., JORDAN A., BRAHM R., MUÑOZ D., PETROVICH C. & HOBSON M.
Astron. J., 166, 130
paper arxiv
TOI-677 b: A Warm Jupiter (P=11.2d) on an eccentric orbit transiting a late F-type star
2019
JORDAN A., BRAHM R., ESPINOZA N., HENNING Th., JONES M. et al.
Astron. J., 159, 145
paper arxiv
