The Kepler-144 system contains 2 exoplanets. It is located 1255.43 light years away from the solar system.
| Mass | 1.15 solar masses |
| Radius | 1.24 solar radiae |
| Temperature | 6075 kelvin |
| Stellar Metallicity | -0.185 decimal exponent |
| Age | 0.94 billion years |
At 2.331 Earth masses, Kepler-144 b 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 | 2.330 Earth masses |
| Density | 5.440 grams per cubic centimeter |
| Radius | 1.330 Earth radiae |
| Semi-major Axis | 0.066 AU |
| Eccentricity | 0 |
| Orbital Period | 5.885 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-03 |
| Reference | Rowe et al. 2014 |
At 2.391 Earth masses, Kepler-144 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 | 2.390 Earth masses |
| Density | 5.340 grams per cubic centimeter |
| Radius | 1.350 Earth radiae |
| Semi-major Axis | 0.094 AU |
| Eccentricity | 0 |
| Orbital Period | 10.105 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-03 |
| Reference | Rowe et al. 2014 |