The Kepler-373 system contains 2 exoplanets. It is located 3556.57 light years away from the solar system.
| Mass | 0.93 solar masses |
| Radius | 0.84 solar radiae |
| Temperature | 5787 kelvin |
| Stellar Metallicity | 0.07 decimal exponent |
| Age | 0.5 billion years |
At 2.420 Earth masses, Kepler-373 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 | 2.420 Earth masses |
| Density | 5.290 grams per cubic centimeter |
| Radius | 1.360 Earth radiae |
| Semi-major Axis | 0.06 AU |
| Eccentricity | 0 |
| Orbital Period | 5.535 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-373 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 | 0.126 AU |
| Eccentricity | 0 |
| Orbital Period | 16.726 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 |