The Kepler-1464 system contains 2 exoplanets. It is located 3756.44 light years away from the solar system.
| Mass | 1.02 solar masses |
| Radius | 1.01 solar radiae |
| Temperature | 5828 kelvin |
| Stellar Metallicity | 0.03 decimal exponent |
| Age | 3.89 billion years |
At 3.403 Earth masses, Kepler-1464 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 | 3.390 Earth masses |
| Density | 4.070 grams per cubic centimeter |
| Radius | 1.660 Earth radiae |
| Semi-major Axis | 0.1803 AU |
| Eccentricity | 0 |
| Orbital Period | 31.779 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-1464 c is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 0.972 Earth masses |
| Density | 5.340 grams per cubic centimeter |
| Radius | 1.000 Earth radiae |
| Semi-major Axis | 0.0548 AU |
| Eccentricity | 0 |
| Orbital Period | 5.328 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 |