The Kepler-232 system contains 2 exoplanets. It is located 4400.27 light years away from the solar system.
| Mass | 0.97 solar masses |
| Radius | 0.97 solar radiae |
| Temperature | 5847 kelvin |
| Stellar Metallicity | 0.03 decimal exponent |
| Age | 1.4 billion years |
At more than 10 Earth masses, Kepler-232 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 | 9.690 Earth masses |
| Density | 1.820 grams per cubic centimeter |
| Radius | 3.080 Earth radiae |
| Semi-major Axis | 0.054 AU |
| Eccentricity | 0 |
| Orbital Period | 4.431 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-232 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 | 14.000 Earth masses |
| Density | 1.370 grams per cubic centimeter |
| Radius | 3.830 Earth radiae |
| Semi-major Axis | 0.101 AU |
| Eccentricity | 0 |
| Orbital Period | 11.379 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 |