The Kepler-1067 system contains 2 exoplanets. It is located 2177.72 light years away from the solar system.
| Mass | 0.95 solar masses |
| Radius | 0.93 solar radiae |
| Temperature | 5592 kelvin |
| Stellar Metallicity | 0.03 decimal exponent |
| Age | 4.79 billion years |
At less than 1.5 Earth masses, Kepler-1067 b is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 0.437 Earth masses |
| Density | 4.690 grams per cubic centimeter |
| Radius | 0.800 Earth radiae |
| Semi-major Axis | 0.0162 AU |
| Eccentricity | 0 |
| Orbital Period | 0.762 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 3.689 Earth masses, Kepler-1067 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 | 3.700 Earth masses |
| Density | 3.810 grams per cubic centimeter |
| Radius | 1.747 Earth radiae |
| Semi-major Axis | 0.0601 AU |
| Eccentricity | 0 |
| Orbital Period | 5.426 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 |