The Kepler-50 system contains 2 exoplanets. It is located 815.75 light years away from the solar system.
| Mass | 1.24 solar masses |
| Radius | 1.58 solar radiae |
| Temperature | 6225 kelvin |
| Stellar Metallicity | 0.03 decimal exponent |
| Age | 3.8 billion years |
At more than 10 Earth masses, Kepler-50 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 | 8.900 Earth masses |
| Density | NaN grams per cubic centimeter |
| Radius | 1.710 Earth radiae |
| Semi-major Axis | 0.077 AU |
| Eccentricity | 0 |
| Orbital Period | 7.813 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-01 |
| Reference | Steffen et al. 2013 |
At more than 10 Earth masses, Kepler-50 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 | 8.200 Earth masses |
| Density | NaN grams per cubic centimeter |
| Radius | 2.170 Earth radiae |
| Semi-major Axis | 0.087 AU |
| Eccentricity | 0 |
| Orbital Period | 9.376 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-01 |
| Reference | Steffen et al. 2013 |