The Kepler-368 system contains 2 exoplanets. It is located 2514.59 light years away from the solar system.
| Mass | 0.97 solar masses |
| Radius | 2.02 solar radiae |
| Temperature | 5502 kelvin |
| Stellar Metallicity | 0.03 decimal exponent |
| Age | 10.47 billion years |
At more than 10 Earth masses, Kepler-368 b 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 | 10.700 Earth masses |
| Density | 1.700 grams per cubic centimeter |
| Radius | 3.260 Earth radiae |
| Semi-major Axis | 0.186 AU |
| Eccentricity | 0 |
| Orbital Period | 26.848 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-368 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 | 14.300 Earth masses |
| Density | 1.350 grams per cubic centimeter |
| Radius | 3.880 Earth radiae |
| Semi-major Axis | 0.36 AU |
| Eccentricity | 0 |
| Orbital Period | 72.379 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 |