The Kepler-913 system contains 2 exoplanets. It is located 3234.22 light years away from the solar system.
| Mass | 0.63 solar masses |
| Radius | 0.61 solar radiae |
| Temperature | 4687 kelvin |
| Stellar Metallicity | -0.52 decimal exponent |
| Age | 5.62 billion years |
With a mass below 5 Earth masses, a density of 3.08, and a semi-major axis of 0.1009 astronomical units, Kepler-913 b could, potentially, be an ocean world - a planet with no dry land.
| Mass | 4.900 Earth masses |
| Density | 3.080 grams per cubic centimeter |
| Radius | 2.060 Earth radiae |
| Semi-major Axis | 0.1009 AU |
| Eccentricity | 0 |
| Orbital Period | 10.297 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2016-05 |
| Reference | Morton et al. 2016 |
At more than 10 Earth masses, Kepler-913 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 | 14.200 Earth masses |
| Density | 1.360 grams per cubic centimeter |
| Radius | 3.858 Earth radiae |
| Semi-major Axis | 0.0699 AU |
| Eccentricity | 0 |
| Orbital Period | 5.939 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2022-02 |
| Reference | Valizadegan et al. 2022 |