The Kepler-382 system contains 2 exoplanets. It is located 3051.01 light years away from the solar system.
| Mass | 0.88 solar masses |
| Radius | 0.94 solar radiae |
| Temperature | 5600 kelvin |
| Stellar Metallicity | 0.082 decimal exponent |
| Age | 11.3 billion years |
At 2.302 Earth masses, Kepler-382 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 | 0.055 AU |
| Eccentricity | 0 |
| Orbital Period | 5.262 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 3.158 Earth masses, Kepler-382 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 | 3.150 Earth masses |
| Density | 4.310 grams per cubic centimeter |
| Radius | 1.590 Earth radiae |
| Semi-major Axis | 0.097 AU |
| Eccentricity | 0 |
| Orbital Period | 12.163 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 |