The K2-264 system contains 2 exoplanets. It is located 605.36 light years away from the solar system.
| Mass | 0.5 solar masses |
| Radius | 0.47 solar radiae |
| Temperature | 3660 kelvin |
| Stellar Metallicity | -0.013 decimal exponent |
| Age | - billion years |
At more than 10 Earth masses, K2-264 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 | 5.610 Earth masses |
| Density | 2.780 grams per cubic centimeter |
| Radius | 2.231 Earth radiae |
| Semi-major Axis | 0.05023 AU |
| Eccentricity | 0.5 |
| Orbital Period | 5.840 days |
| Discovery Method | Transit |
| Discovery Facility | K2 |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2018-11 |
| Reference | Rizzuto et al. 2018 |
At more than 10 Earth masses, K2-264 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 | 7.600 Earth masses |
| Density | 2.200 grams per cubic centimeter |
| Radius | 2.668 Earth radiae |
| Semi-major Axis | 0.11283 AU |
| Eccentricity | 0.45 |
| Orbital Period | 19.660 days |
| Discovery Method | Transit |
| Discovery Facility | K2 |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2018-11 |
| Reference | Rizzuto et al. 2018 |