The Kepler-225 system contains 2 exoplanets. It is located 1830.06 light years away from the solar system.
| Mass | 0.59 solar masses |
| Radius | 0.48 solar radiae |
| Temperature | 3682 kelvin |
| Stellar Metallicity | -0.04 decimal exponent |
| Age | 2.88 billion years |
At 1.870 Earth masses, Kepler-225 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 | 1.870 Earth masses |
| Density | 5.950 grams per cubic centimeter |
| Radius | 1.200 Earth radiae |
| Semi-major Axis | 0.056 AU |
| Eccentricity | 0 |
| Orbital Period | 6.739 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 4.039 Earth masses, Kepler-225 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 | 4.040 Earth masses |
| Density | 3.560 grams per cubic centimeter |
| Radius | 1.840 Earth radiae |
| Semi-major Axis | 0.111 AU |
| Eccentricity | 0 |
| Orbital Period | 18.794 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 |