The Kepler-380 system contains 2 exoplanets. It is located 2653.97 light years away from the solar system.
| Mass | 1.08 solar masses |
| Radius | 1.22 solar radiae |
| Temperature | 6045 kelvin |
| Stellar Metallicity | -0.06 decimal exponent |
| Age | 4.43 billion years |
At 1.813 Earth masses, Kepler-380 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 | 1.810 Earth masses |
| Density | 5.900 grams per cubic centimeter |
| Radius | 1.190 Earth radiae |
| Semi-major Axis | 0.05 AU |
| Eccentricity | 0 |
| Orbital Period | 3.931 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 2.156 Earth masses, Kepler-380 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 | 2.150 Earth masses |
| Density | 5.770 grams per cubic centimeter |
| Radius | 1.270 Earth radiae |
| Semi-major Axis | 0.078 AU |
| Eccentricity | 0 |
| Orbital Period | 7.630 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 |