The Kepler-383 system contains 2 exoplanets. It is located 1532.93 light years away from the solar system.
| Mass | 0.67 solar masses |
| Radius | 0.67 solar radiae |
| Temperature | 4710 kelvin |
| Stellar Metallicity | -0.178 decimal exponent |
| Age | 13.9 billion years |
At 2.302 Earth masses, Kepler-383 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 | 2.300 Earth masses |
| Density | 5.500 grams per cubic centimeter |
| Radius | 1.320 Earth radiae |
| Semi-major Axis | 0.095 AU |
| Eccentricity | 0 |
| Orbital Period | 12.905 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 2.070 Earth masses, Kepler-383 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 | 2.070 Earth masses |
| Density | 5.970 grams per cubic centimeter |
| Radius | 1.240 Earth radiae |
| Semi-major Axis | 0.172 AU |
| Eccentricity | 0 |
| Orbital Period | 31.201 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 |