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|
|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|
|Orbital Period||38.097 days|
|Discovery Telescope||0.95 m Kepler Telescope|
|Discovery Instrument||Kepler CCD Array|
|Reference||Torres et al. 2017|