The Kepler-1652 system contains 1 exoplanet. It is located 821.91 light years away from the solar system.
| Mass | 0.4 solar masses |
| Radius | 0.38 solar radiae |
| Temperature | 3638 kelvin |
| Stellar Metallicity | -0.3 decimal exponent |
| Age | 3.2 billion years |
At 3.180 Earth masses, Kepler-1652 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. Kepler-1652 b orbits within the habitable zone of its parent star and could, potentially, be a habitable planet with stable bodies of liquid water on its surface, like Earth.
| Mass | 3.190 Earth masses |
| Density | 4.280 grams per cubic centimeter |
| Radius | 1.600 Earth radiae |
| Semi-major Axis | 0.1654 AU |
| Eccentricity | 0 |
| Orbital Period | 38.097 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2017-12 |
| Reference | Torres et al. 2017 |