The Kepler-369 system contains 2 exoplanets. It is located 697.97 light years away from the solar system.
| Mass | 0.5 solar masses |
| Radius | 0.47 solar radiae |
| Temperature | 3591 kelvin |
| Stellar Metallicity | -0.09 decimal exponent |
| Age | 4.17 billion years |
At 1.507 Earth masses, Kepler-369 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 | 1.510 Earth masses |
| Density | 5.750 grams per cubic centimeter |
| Radius | 1.130 Earth radiae |
| Semi-major Axis | 0.03 AU |
| Eccentricity | 0 |
| Orbital Period | 2.733 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 2.573 Earth masses, Kepler-369 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.
| Mass | 2.570 Earth masses |
| Density | 5.040 grams per cubic centimeter |
| Radius | 1.410 Earth radiae |
| Semi-major Axis | 0.094 AU |
| Eccentricity | 0 |
| Orbital Period | 14.872 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 |