The Kepler-283 system contains 2 exoplanets. It is located 1526.72 light years away from the solar system.
| Mass | 0.6 solar masses |
| Radius | 0.57 solar radiae |
| Temperature | 4351 kelvin |
| Stellar Metallicity | -0.17 decimal exponent |
| Age | 3.09 billion years |
At more than 10 Earth masses, Kepler-283 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 | 5.180 Earth masses |
| Density | 2.950 grams per cubic centimeter |
| Radius | 2.130 Earth radiae |
| Semi-major Axis | 0.082 AU |
| Eccentricity | 0 |
| Orbital Period | 11.008 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 3.975 Earth masses, Kepler-283 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. Kepler-283 c 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 | 3.970 Earth masses |
| Density | 3.620 grams per cubic centimeter |
| Radius | 1.820 Earth radiae |
| Semi-major Axis | 0.341 AU |
| Eccentricity | 0 |
| Orbital Period | 92.744 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 |