The Kepler-183 system contains 2 exoplanets. It is located 3426.73 light years away from the solar system.
| Mass | 0.94 solar masses |
| Radius | 0.96 solar radiae |
| Temperature | 5888 kelvin |
| Stellar Metallicity | 0.101 decimal exponent |
| Age | 4.27 billion years |
With a mass below 5 Earth masses, a density of 3.08, and a semi-major axis of 0.064 astronomical units, Kepler-183 b could, potentially, be an ocean world - a planet with no dry land.
| Mass | 4.900 Earth masses |
| Density | 3.080 grams per cubic centimeter |
| Radius | 2.060 Earth radiae |
| Semi-major Axis | 0.064 AU |
| Eccentricity | 0 |
| Orbital Period | 5.688 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-183 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 | 35.700 Earth masses |
| Density | 16.800 grams per cubic centimeter |
| Radius | 2.270 Earth radiae |
| Semi-major Axis | 0.103 AU |
| Eccentricity | 0 |
| Orbital Period | 11.637 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 |