Planet HD 202696 c
| Name | HD 202696 c | ||
| Planet Status | Confirmed | ||
| Discovered in | 2018 | ||
| Mass | — | ||
| Mass*sin(i) | 1.917 ( -0.212 +0.116 ) MJ |  |
|
| Semi-Major Axis | 2.36 ( -0.04 +0.003 ) AU | |
|
| Orbital Period | 958.0 ( -26.4 +2.2 ) day | |
|
| Eccentricity | 0.265 ( -0.23 +0.05 ) | |
|
| ω | 140.0 ( -44.9 +88.7 ) deg | |
|
| Tperi | — | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2019-01-09 | ||
| Detection Method | Radial Velocity | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | — | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 26.6 ( -3.5 +1.1 ) m/s | |
|
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
HD 202696| Name | HD 202696 | ||
| Distance | 188.5 (± 1.6) pc | |
|
| Spectral type | KOIII | ||
| Apparent magnitude V | 8.23 | ||
| Mass | 1.91 ( -0.14 +0.09 ) MSun | |
|
| Age | 1.32 ( -0.25 +0.35 ) Gyr | |
|
| Effective temperature | 5040.0 ( -85.0 +71.0 ) K | |
|
| Radius | 6.01 ( -0.19 +0.33 ) RSun | |
|
| Metallicity [Fe/H] | 0.02 (± 0.04) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 21:16:54.0 | ||
| Dec2000 | +27:15:29 | ||
| Alternate Names | |||
| Planetary system | 2 planets |
Related publications
A general stability-driven approach for the refinement of multi-planet systems
2022
STALPORT M., DELISLE J.-B., UDRY S., MATTHEWS E., BOURRIER V. & LELEU A.
Astron. & Astrophys., accepted
arxiv
Two Jovian planets around the giant star HD202696. A growing population of packed massive planetary pairs around massive stars?
2019
TRIFONOV T., STOCK S., HENNING Th., REFFERT S., KUERTSER M. et al.
Astron. J., 157, 93
paper arxiv
