The Kepler-371 system contains 2 exoplanets. It is located 2652.27 light years away from the solar system.
| Mass | 0.93 solar masses |
| Radius | 0.99 solar radiae |
| Temperature | 5666 kelvin |
| Stellar Metallicity | -0.197 decimal exponent |
| Age | 0.3 billion years |
With a mass below 5 Earth masses, a density of 3.44, and a semi-major axis of 0.2 astronomical units, Kepler-371 b could, potentially, be an ocean world - a planet with no dry land.
| Mass | 4.230 Earth masses |
| Density | 3.440 grams per cubic centimeter |
| Radius | 1.890 Earth radiae |
| Semi-major Axis | 0.2 AU |
| Eccentricity | 0 |
| Orbital Period | 34.763 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 3.816 Earth masses, Kepler-371 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 | 3.820 Earth masses |
| Density | 3.720 grams per cubic centimeter |
| Radius | 1.780 Earth radiae |
| Semi-major Axis | 0.313 AU |
| Eccentricity | 0 |
| Orbital Period | 67.968 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 |