The Kepler-1050 system contains 2 exoplanets. It is located 1599.76 light years away from the solar system.
| Mass | 1.09 solar masses |
| Radius | 1.13 solar radiae |
| Temperature | 6010 kelvin |
| Stellar Metallicity | 0.03 decimal exponent |
| Age | 3.55 billion years |
At 3.180 Earth masses, Kepler-1050 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 | 3.190 Earth masses |
| Density | 4.280 grams per cubic centimeter |
| Radius | 1.600 Earth radiae |
| Semi-major Axis | 0.1313 AU |
| Eccentricity | 0 |
| Orbital Period | 15.379 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 2.795 Earth masses, Kepler-1050 c 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 | 2.790 Earth masses |
| Density | 4.730 grams per cubic centimeter |
| Radius | 1.480 Earth radiae |
| Semi-major Axis | 0.1622 AU |
| Eccentricity | 0 |
| Orbital Period | 21.128 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 |