The Kepler-185 system contains 2 exoplanets. It is located 1522.28 light years away from the solar system.
| Mass | 0.81 solar masses |
| Radius | 0.81 solar radiae |
| Temperature | 5208 kelvin |
| Stellar Metallicity | 0.16 decimal exponent |
| Age | 11.9 billion years |
At 1.708 Earth masses, Kepler-185 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 | 1.710 Earth masses |
| Density | 5.870 grams per cubic centimeter |
| Radius | 1.170 Earth radiae |
| Semi-major Axis | 0.026 AU |
| Eccentricity | 0 |
| Orbital Period | 1.633 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 |
With a mass below 5 Earth masses, a density of 3.16, and a semi-major axis of 0.139 astronomical units, Kepler-185 c could, potentially, be an ocean world - a planet with no dry land.
| Mass | 4.740 Earth masses |
| Density | 3.160 grams per cubic centimeter |
| Radius | 2.020 Earth radiae |
| Semi-major Axis | 0.139 AU |
| Eccentricity | 0 |
| Orbital Period | 20.729 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 |