The Kepler-320 system contains 2 exoplanets. It is located 2696.05 light years away from the solar system.
| Mass | 1.33 solar masses |
| Radius | 1.11 solar radiae |
| Temperature | 6435 kelvin |
| Stellar Metallicity | -0.123 decimal exponent |
| Age | 2.14 billion years |
At 1.555 Earth masses, Kepler-320 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 | 1.550 Earth masses |
| Density | 5.750 grams per cubic centimeter |
| Radius | 1.140 Earth radiae |
| Semi-major Axis | 0.085 AU |
| Eccentricity | 0 |
| Orbital Period | 8.372 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 2.452 Earth masses, Kepler-320 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 | 2.450 Earth masses |
| Density | 5.240 grams per cubic centimeter |
| Radius | 1.370 Earth radiae |
| Semi-major Axis | 0.142 AU |
| Eccentricity | 0 |
| Orbital Period | 17.935 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 |