The Kepler-969 system contains 2 exoplanets. It is located 1273.16 light years away from the solar system.
| Mass | 0.92 solar masses |
| Radius | 0.82 solar radiae |
| Temperature | 5214 kelvin |
| Stellar Metallicity | 0.22 decimal exponent |
| Age | 1.51 billion years |
With a mass below 5 Earth masses, a density of 3.06, and a semi-major axis of 0.2027 astronomical units, Kepler-969 b could, potentially, be an ocean world - a planet with no dry land.
| Mass | 4.940 Earth masses |
| Density | 3.060 grams per cubic centimeter |
| Radius | 2.070 Earth radiae |
| Semi-major Axis | 0.2027 AU |
| Eccentricity | 0 |
| Orbital Period | 34.173 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-969 c is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 0.937 Earth masses |
| Density | 5.310 grams per cubic centimeter |
| Radius | 0.990 Earth radiae |
| Semi-major Axis | 0.0272 AU |
| Eccentricity | 0 |
| Orbital Period | 1.683 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 |