The Kepler-202 system contains 2 exoplanets. It is located 929.91 light years away from the solar system.
| Mass | 0.68 solar masses |
| Radius | 0.67 solar radiae |
| Temperature | 4668 kelvin |
| Stellar Metallicity | -0.263 decimal exponent |
| Age | 3.24 billion years |
At 3.307 Earth masses, Kepler-202 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 | 3.290 Earth masses |
| Density | 4.170 grams per cubic centimeter |
| Radius | 1.630 Earth radiae |
| Semi-major Axis | 0.045 AU |
| Eccentricity | 0 |
| Orbital Period | 4.069 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 4.070 Earth masses, Kepler-202 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 | 4.080 Earth masses |
| Density | 3.540 grams per cubic centimeter |
| Radius | 1.850 Earth radiae |
| Semi-major Axis | 0.113 AU |
| Eccentricity | 0 |
| Orbital Period | 16.282 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 |