The Kepler-107 system contains 4 exoplanets. It is located 1715.57 light years away from the solar system.
| Mass | 1.24 solar masses |
| Radius | 1.45 solar radiae |
| Temperature | 5854 kelvin |
| Stellar Metallicity | 0.321 decimal exponent |
| Age | 4.29 billion years |
At 3.511 Earth masses, Kepler-107 b is a so called Super Earth. Super Earths could be terrestrial worlds like Earth, but they could also be ocean worlds or terrestrial worlds wrapped in a substantial atmosphere, in which case some refer to them as Mini Neptunes.
| Mass | 3.510 Earth masses |
| Density | 5.300 grams per cubic centimeter |
| Radius | 1.536 Earth radiae |
| Semi-major Axis | 0.04544 AU |
| Eccentricity | 0 |
| Orbital Period | 3.180 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-107 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 | 9.390 Earth masses |
| Density | 12.650 grams per cubic centimeter |
| Radius | 1.597 Earth radiae |
| Semi-major Axis | 0.06064 AU |
| Eccentricity | 0 |
| Orbital Period | 4.901 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 3.803 Earth masses, Kepler-107 d is a so called Super Earth. Super Earths could be terrestrial worlds like Earth, but they could also be ocean worlds or terrestrial worlds wrapped in a substantial atmosphere, in which case some refer to them as Mini Neptunes.
| Mass | 3.800 Earth masses |
| Density | 33.100 grams per cubic centimeter |
| Radius | 0.860 Earth radiae |
| Semi-major Axis | 0.08377 AU |
| Eccentricity | 0 |
| Orbital Period | 7.958 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-107 e 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 | 8.600 Earth masses |
| Density | 2.000 grams per cubic centimeter |
| Radius | 2.903 Earth radiae |
| Semi-major Axis | 0.12639 AU |
| Eccentricity | 0 |
| Orbital Period | 14.749 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 |