The Kepler-920 system contains 2 exoplanets. It is located 3267.04 light years away from the solar system.
| Mass | 0.89 solar masses |
| Radius | 0.85 solar radiae |
| Temperature | 5403 kelvin |
| Stellar Metallicity | 0 decimal exponent |
| Age | 4.37 billion years |
At more than 10 Earth masses, Kepler-920 b is an ice giant, a planet that is made up mostly of volatiles like water, amonia and methane, and enveloped by a dense hydrogen and helium atmosphere, much like Uranus and Neptune.
| Mass | 6.440 Earth masses |
| Density | 2.500 grams per cubic centimeter |
| Radius | 2.420 Earth radiae |
| Semi-major Axis | 0.065 AU |
| Eccentricity | 0 |
| Orbital Period | 6.532 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2016-05 |
| Reference | Morton et al. 2016 |
At more than 10 Earth masses, Kepler-920 c is an ice giant, a planet that is made up mostly of volatiles like water, amonia and methane, and enveloped by a dense hydrogen and helium atmosphere, much like Uranus and Neptune.
| Mass | 13.800 Earth masses |
| Density | 1.380 grams per cubic centimeter |
| Radius | 3.800 Earth radiae |
| Semi-major Axis | 0.4029 AU |
| Eccentricity | 0 |
| Orbital Period | 100.827 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2016-05 |
| Reference | Morton et al. 2016 |