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 |
3 Sep 2012: The TTVs constrain the planet mass (Ragozzine et al. 2012)
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