The Kepler-363 system contains 3 exoplanets. It is located 2487.25 light years away from the solar system.
| Mass | 1.1 solar masses |
| Radius | 1.49 solar radiae |
| Temperature | 5593 kelvin |
| Stellar Metallicity | 0.397 decimal exponent |
| Age | 5.25 billion years |
At 1.657 Earth masses, Kepler-363 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 | 1.650 Earth masses |
| Density | 5.810 grams per cubic centimeter |
| Radius | 1.160 Earth radiae |
| Semi-major Axis | 0.048 AU |
| Eccentricity | 0 |
| Orbital Period | 3.615 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 50 Earth masses, Kepler-363 c is a gas giant, a planet whose mass is mostly made up of hydrogen and helium, like Jupiter and Saturn.
| Mass | 66.400 Earth masses |
| Density | 75.600 grams per cubic centimeter |
| Radius | 1.690 Earth radiae |
| Semi-major Axis | 0.079 AU |
| Eccentricity | 0 |
| Orbital Period | 7.542 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 3.1, and a semi-major axis of 0.107 astronomical units, Kepler-363 d could, potentially, be an ocean world - a planet with no dry land.
| Mass | 4.860 Earth masses |
| Density | 3.100 grams per cubic centimeter |
| Radius | 2.050 Earth radiae |
| Semi-major Axis | 0.107 AU |
| Eccentricity | 0 |
| Orbital Period | 11.932 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 |