The Kepler-190 system contains 2 exoplanets. It is located 1413.52 light years away from the solar system.
| Mass | 0.86 solar masses |
| Radius | 0.8 solar radiae |
| Temperature | 5106 kelvin |
| Stellar Metallicity | 0.02 decimal exponent |
| Age | 3.72 billion years |
At 3.056 Earth masses, Kepler-190 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 | 3.050 Earth masses |
| Density | 4.410 grams per cubic centimeter |
| Radius | 1.560 Earth radiae |
| Semi-major Axis | 0.03 AU |
| Eccentricity | 0 |
| Orbital Period | 2.020 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 2.732 Earth masses, Kepler-190 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 | 2.730 Earth masses |
| Density | 4.820 grams per cubic centimeter |
| Radius | 1.460 Earth radiae |
| Semi-major Axis | 0.045 AU |
| Eccentricity | 0 |
| Orbital Period | 3.763 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 |