The Kepler-58 system contains 3 exoplanets. It is located 3161.27 light years away from the solar system.
| Mass | 0.95 solar masses |
| Radius | 1.03 solar radiae |
| Temperature | 5843 kelvin |
| Stellar Metallicity | 0.09 decimal exponent |
| Age | 2.14 billion years |
At more than 10 Earth masses, Kepler-58 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 | 35.500 Earth masses |
| Density | NaN grams per cubic centimeter |
| Radius | 2.780 Earth radiae |
| Semi-major Axis | 0.0927 AU |
| Eccentricity | 0 |
| Orbital Period | 10.218 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 50 Earth masses, Kepler-58 c is a gas giant, a planet whose mass is mostly made up of hydrogen and helium, like Jupiter and Saturn.
| Mass | 53.000 Earth masses |
| Density | NaN grams per cubic centimeter |
| Radius | 2.860 Earth radiae |
| Semi-major Axis | 0.1228 AU |
| Eccentricity | 0 |
| Orbital Period | 15.574 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-58 d 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 | 8.960 Earth masses |
| Density | 1.940 grams per cubic centimeter |
| Radius | 2.940 Earth radiae |
| Semi-major Axis | 0.236 AU |
| Eccentricity | 0 |
| Orbital Period | 40.101 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 |