The Kepler-967 system contains 2 exoplanets. It is located 1854.35 light years away from the solar system.
| Mass | 0.84 solar masses |
| Radius | 0.8 solar radiae |
| Temperature | 5178 kelvin |
| Stellar Metallicity | -0.03 decimal exponent |
| Age | 5.89 billion years |
At more than 10 Earth masses, Kepler-967 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 | 6.120 Earth masses |
| Density | 2.590 grams per cubic centimeter |
| Radius | 2.350 Earth radiae |
| Semi-major Axis | 0.1027 AU |
| Eccentricity | 0 |
| Orbital Period | 13.227 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-967 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 | 12.900 Earth masses |
| Density | 1.460 grams per cubic centimeter |
| Radius | 3.650 Earth radiae |
| Semi-major Axis | 0.6253 AU |
| Eccentricity | 0 |
| Orbital Period | 198.711 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 |