The Kepler-1907 system contains 2 exoplanets. It is located 952.74 light years away from the solar system.
| Mass | 0.75 solar masses |
| Radius | 0.8 solar radiae |
| Temperature | 5159 kelvin |
| Stellar Metallicity | -0.16 decimal exponent |
| Age | 14 billion years |
At less than 1.5 Earth masses, Kepler-1907 b is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 0.589 Earth masses |
| Density | 4.920 grams per cubic centimeter |
| Radius | 0.870 Earth radiae |
| Semi-major Axis | 0.0565 AU |
| Eccentricity | 0 |
| Orbital Period | 5.652 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 |
At 1.631 Earth masses, Kepler-1907 c is a so called Super Earth. Super Earths could be terrestrial worlds like Earth, but they could also be ocean worlds or terrestrial worlds wrapped in a substantial atmosphere, in which case some refer to them as Mini Neptunes.
| Mass | 1.630 Earth masses |
| Density | 5.810 grams per cubic centimeter |
| Radius | 1.155 Earth radiae |
| Semi-major Axis | 0.1076 AU |
| Eccentricity | 0 |
| Orbital Period | 14.864 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 |