The Kepler-69 system contains 2 exoplanets. It is located 2382.98 light years away from the solar system.
| Mass | 0.81 solar masses |
| Radius | 0.93 solar radiae |
| Temperature | 5638 kelvin |
| Stellar Metallicity | -0.29 decimal exponent |
| Age | 9.8 billion years |
At more than 10 Earth masses, Kepler-69 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 | 5.650 Earth masses |
| Density | 2.760 grams per cubic centimeter |
| Radius | 2.240 Earth radiae |
| Semi-major Axis | 0.094 AU |
| Eccentricity | 0.16 |
| Orbital Period | 13.722 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-05 |
| Reference | Barclay et al. 2013 |
At 3.562 Earth masses, Kepler-69 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. Kepler-69 c orbits within the habitable zone of its parent star and could, potentially, be a habitable planet with stable bodies of liquid water on its surface, like Earth.
| Mass | 3.570 Earth masses |
| Density | 3.920 grams per cubic centimeter |
| Radius | 1.710 Earth radiae |
| Semi-major Axis | 0.64 AU |
| Eccentricity | 0.14 |
| Orbital Period | 242.461 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-05 |
| Reference | Barclay et al. 2013 |