Planet Kepler-435 b
| Name | Kepler-435 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2015 | ||
| Mass | 0.84 ( -0.15 +0.15 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 0.0948 (± 0.0018) AU | ||
| Orbital Period | 8.6001536 (± 1.8e-06) day | |
|
| Eccentricity | 0.114 (± 0.077) | |
|
| ω | 104.0 ( -36.0 +36.0 ) deg | |
|
| Tperi | — | ||
| Radius | 1.99 ( -0.18 +0.18 ) RJ | |
|
| Inclination | 85.51 (± 0.52) deg | |
|
| Update | 2021-02-05 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | 2455010.64241 (± 0.0004) JD | |
|
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | 0.448 ( -0.024 +0.024 ) | |
|
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | 64.0 ( -12.0 +12.0 ) m/s | |
|
| Calculated temperature | 1729.0 ( -70.0 +70.0 ) K | |
|
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | KOI-680 b, 2MASS J19290895+4311502 b, K00680.01, KIC 7529266 b, KOI-680.01, WISE J192908.95+431150.1 b |
Star
Kepler-435| Name | Kepler-435 | ||
| Distance | 2070.0 (± 200.0) pc | |
|
| Spectral type | |||
| Apparent magnitude V | 14.0 | ||
| Mass | 1.54 ( -0.09 +0.09 ) MSun | ||
| Age | 2.25 (± 0.42) Gyr | |
|
| Effective temperature | 6161.0 (± 94.0) K | |
|
| Radius | 3.21 (± 0.3) RSun | |
|
| Metallicity [Fe/H] | -0.18 (± 0.11) | |
|
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 19:29:09.0 | ||
| Dec2000 | +43:11:50 | ||
| Alternate Names | KOI-680, 2MASS J19290895+4311502, KIC 7529266, WISE J192908.95+431150.1 | ||
| Planetary system | 1 planet |
Observability Predictor 
Remarks
Alias KOI-680.01Related publications
SOPHIE velocimetry of Kepler transit candidates. XV. KOI-614b, KOI-206b, and KOI-680b: a massive warm Jupiter orbiting a G0 metallic dwarf and two highly inflated planets with a distant companion around evolved F-type stars
2015
ALMENARA J., DAMIANI C., BOUCHY F., HAVEL M., BRUNO G. et al.
Astron. & Astrophys., 575, A71
paper arxiv ADS
Limits on surface gravities of Kepler planet-candidate host stars from non-detection of solar-like oscillations
2014
CAMPANTE T., CHAPLIN W., LUND M., HUBER D., HEKKER S. et al.
ApJ, 783, 123
paper arxiv
