The K2-24 system contains 2 exoplanets. It is located 556.30 light years away from the solar system.
| Mass | 1.07 solar masses |
| Radius | 1.16 solar radiae |
| Temperature | 5625 kelvin |
| Stellar Metallicity | 0.34 decimal exponent |
| Age | 5.1 billion years |
At more than 10 Earth masses, K2-24 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 | 19.000 Earth masses |
| Density | 0.640 grams per cubic centimeter |
| Radius | 5.400 Earth radiae |
| Semi-major Axis | 0.154 AU |
| Eccentricity | 0.06 |
| Orbital Period | 20.890 days |
| Discovery Method | Transit |
| Discovery Facility | K2 |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2016-02 |
| Reference | Petigura et al. 2016 |
At more than 10 Earth masses, K2-24 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 | 15.400 Earth masses |
| Density | 0.200 grams per cubic centimeter |
| Radius | 7.500 Earth radiae |
| Semi-major Axis | 0.247 AU |
| Eccentricity | 0.07 |
| Orbital Period | 42.339 days |
| Discovery Method | Transit |
| Discovery Facility | K2 |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2016-02 |
| Reference | Petigura et al. 2016 |