The Kepler-384 system contains 2 exoplanets. It is located 2921.31 light years away from the solar system.
| Mass | 0.97 solar masses |
| Radius | 0.88 solar radiae |
| Temperature | 5577 kelvin |
| Stellar Metallicity | -0.459 decimal exponent |
| Age | 1.5 billion years |
At less than 1.5 Earth masses, Kepler-384 b is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 1.460 Earth masses |
| Density | 5.710 grams per cubic centimeter |
| Radius | 1.120 Earth radiae |
| Semi-major Axis | 0.148 AU |
| Eccentricity | 0 |
| Orbital Period | 22.597 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 1.507 Earth masses, Kepler-384 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 | 1.510 Earth masses |
| Density | 5.750 grams per cubic centimeter |
| Radius | 1.130 Earth radiae |
| Semi-major Axis | 0.236 AU |
| Eccentricity | 0 |
| Orbital Period | 45.348 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 |