The Kepler-360 system contains 2 exoplanets. It is located 2857.27 light years away from the solar system.
| Mass | 0.95 solar masses |
| Radius | 1.06 solar radiae |
| Temperature | 6053 kelvin |
| Stellar Metallicity | 0.16 decimal exponent |
| Age | 3.4 billion years |
At 3.371 Earth masses, Kepler-360 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 | 3.360 Earth masses |
| Density | 4.110 grams per cubic centimeter |
| Radius | 1.650 Earth radiae |
| Semi-major Axis | 0.044 AU |
| Eccentricity | 0 |
| Orbital Period | 3.290 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-360 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 | 5.060 Earth masses |
| Density | 3.000 grams per cubic centimeter |
| Radius | 2.100 Earth radiae |
| Semi-major Axis | 0.075 AU |
| Eccentricity | 0 |
| Orbital Period | 7.186 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 |