The Kepler-112 system contains 2 exoplanets. It is located 1673.85 light years away from the solar system.
| Mass | 0.78 solar masses |
| Radius | 0.84 solar radiae |
| Temperature | 5544 kelvin |
| Stellar Metallicity | -0.522 decimal exponent |
| Age | 9.4 billion years |
At more than 10 Earth masses, Kepler-112 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 | 6.170 Earth masses |
| Density | 2.580 grams per cubic centimeter |
| Radius | 2.360 Earth radiae |
| Semi-major Axis | 0.076 AU |
| Eccentricity | 0 |
| Orbital Period | 8.409 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-03 |
| Reference | Rowe et al. 2014 |
At more than 10 Earth masses, Kepler-112 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 | 6.350 Earth masses |
| Density | 2.520 grams per cubic centimeter |
| Radius | 2.400 Earth radiae |
| Semi-major Axis | 0.172 AU |
| Eccentricity | 0 |
| Orbital Period | 28.574 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-03 |
| Reference | Rowe et al. 2014 |