The Kepler-392 system contains 2 exoplanets. It is located 2222.52 light years away from the solar system.
| Mass | 1.07 solar masses |
| Radius | 1.13 solar radiae |
| Temperature | 5938 kelvin |
| Stellar Metallicity | -0.436 decimal exponent |
| Age | 2.97 billion years |
At less than 1.5 Earth masses, Kepler-392 b is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 0.972 Earth masses |
| Density | 5.340 grams per cubic centimeter |
| Radius | 1.000 Earth radiae |
| Semi-major Axis | 0.059 AU |
| Eccentricity | 0 |
| Orbital Period | 5.342 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 less than 1.5 Earth masses, Kepler-392 c is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 1.370 Earth masses |
| Density | 5.660 grams per cubic centimeter |
| Radius | 1.100 Earth radiae |
| Semi-major Axis | 0.093 AU |
| Eccentricity | 0 |
| Orbital Period | 10.423 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 |