The Kepler-625 system contains 2 exoplanets. It is located 2481.09 light years away from the solar system.
| Mass | 1.04 solar masses |
| Radius | 0.96 solar radiae |
| Temperature | 5789 kelvin |
| Stellar Metallicity | 0.1 decimal exponent |
| Age | 1.51 billion years |
With a mass below 5 Earth masses, a density of 3.22, and a semi-major axis of 0.0768 astronomical units, Kepler-625 b could, potentially, be an ocean world - a planet with no dry land.
| Mass | 4.620 Earth masses |
| Density | 3.220 grams per cubic centimeter |
| Radius | 1.990 Earth radiae |
| Semi-major Axis | 0.0768 AU |
| Eccentricity | 0 |
| Orbital Period | 7.752 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 less than 1.5 Earth masses, Kepler-625 c is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 1.160 Earth masses |
| Density | 5.510 grams per cubic centimeter |
| Radius | 1.050 Earth radiae |
| Semi-major Axis | 0.0508 AU |
| Eccentricity | 0 |
| Orbital Period | 4.165 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 |