The Kepler-100 system contains 3 exoplanets. It is located 993.62 light years away from the solar system.
| Mass | 1.08 solar masses |
| Radius | 1.49 solar radiae |
| Temperature | 5825 kelvin |
| Stellar Metallicity | 0.02 decimal exponent |
| Age | 6.46 billion years |
At more than 10 Earth masses, Kepler-100 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 | 7.340 Earth masses |
| Density | 14.250 grams per cubic centimeter |
| Radius | 1.320 Earth radiae |
| Semi-major Axis | 0.072 AU |
| Eccentricity | 0.13 |
| Orbital Period | 6.887 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-02 |
| Reference | Marcy et al. 2014 |
At more than 10 Earth masses, Kepler-100 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 | 7.050 Earth masses |
| Density | NaN grams per cubic centimeter |
| Radius | 2.200 Earth radiae |
| Semi-major Axis | 0.109 AU |
| Eccentricity | 0.02 |
| Orbital Period | 12.816 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-02 |
| Reference | Marcy et al. 2014 |
| Mass | 3.000 Earth masses |
| Density | NaN grams per cubic centimeter |
| Radius | 1.610 Earth radiae |
| Semi-major Axis | 0.2143 AU |
| Eccentricity | 0.38 |
| Orbital Period | 35.333 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-02 |
| Reference | Marcy et al. 2014 |