Planet Kepler-80 c
| Name | Kepler-80 c | ||
| Planet Status | Confirmed | ||
| Discovered in | 2012 | ||
| Mass | 0.0212 ( -0.0027 +0.00387 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | — | ||
| Orbital Period | 9.52 day | |
|
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | 0.23 RJ | |
|
| Inclination | — | ||
| Update | 2016-07-27 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | TTV | ||
| Radius Detection Method | Primary Transit | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | KOI-500 c |
Star
Kepler-80| Name | Kepler-80 | ||
| Distance | — | ||
| Spectral type | |||
| Apparent magnitude V | 15.0 | ||
| Mass | — | ||
| Age | — | ||
| Effective temperature | 4250.0 K | ||
| Radius | 0.738 RSun | ||
| Metallicity [Fe/H] | -0.56 | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 19:44:27.0 | ||
| Dec2000 | +39:58:44 | ||
| Alternate Names | KOI-500 | ||
| Planetary system | 6 planets |
Remarks
Alias KIC 4852528Alias 2MASS 19442701+3958436
More data
- Simbad
- Most recent references (ADS)
Observability Predictor 
Remarks
Alias KOI-500.023 Sep 2012: The TTVs constrain the planet mass (Ragozzine et al. 2012)
Related publications
Identifying Exoplanets with Deep Learning: A Five Planet Resonant Chain around Kepler-80 and an Eighth Planet around Kepler-90
2018
SHALLUE Ch. & VANDERBURG A.
Astron. J., 155, 94
paper arxiv
On the formation of compact planetary systems via concurrent core accretion and migration
2016
COLEMAN G. & NELSON R.
MNRAS, 457, 2480
paper arxiv ADS
A Dynamical Analysis of the Kepler-80 System of Five Transiting Planets
2016
MACDONALD, M., RAGOZZINE, D., FABRYCKY, D., FORD, E., HOLMAN, M. & 8 additional authors
Astron. J., accepted
arxiv
paper
ADS
The Very Compact Five Exoplanet System KOI-500: Mass Constraints from TTVs, Resonances, and Implications
2012
RAGOZZINE D. & Kepler Team
BAAS, 44, no 5, 200.04
abstract
