The Kepler-152 system contains 2 exoplanets. It is located 1438.64 light years away from the solar system.
| Mass | 0.83 solar masses |
| Radius | 0.72 solar radiae |
| Temperature | 5088 kelvin |
| Stellar Metallicity | -0.16 decimal exponent |
| Age | 2 billion years |
At more than 10 Earth masses, Kepler-152 b is an ice giant, a planet that is made up mostly of volatiles like water, amonia and methane, and enveloped by a dense hydrogen and helium atmosphere, much like Uranus and Neptune.
| Mass | 8.200 Earth masses |
| Density | 2.070 grams per cubic centimeter |
| Radius | 2.790 Earth radiae |
| Semi-major Axis | 0.124 AU |
| Eccentricity | 0 |
| Orbital Period | 18.208 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 more than 10 Earth masses, Kepler-152 c is an ice giant, a planet that is made up mostly of volatiles like water, amonia and methane, and enveloped by a dense hydrogen and helium atmosphere, much like Uranus and Neptune.
| Mass | 6.300 Earth masses |
| Density | 2.540 grams per cubic centimeter |
| Radius | 2.390 Earth radiae |
| Semi-major Axis | 0.356 AU |
| Eccentricity | 0 |
| Orbital Period | 88.255 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 |