The Kepler-1322 system is known to contain 1 exoplanet in orbit around it. It is located 4404.15 light years away from the solar system.
| Mass | 0.9 solar masses |
| Radius | 0.87 solar radiae |
| Temperature | 5488 kelvin |
| Stellar Metallicity | -0.07 Decimal exponent |
| Age | 4.47 billion years |
At 3.212 Earth masses, Kepler-1322 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. No Super Earths are known to exist in our solar system, but if it exists, the so-called Planet Nine could very well be a super Earth, as it is hypothesized to have a mass between five and ten Earth masses.
| Mass | 3.220 Earth masses |
| Density | 4.240 Grams per cubic centimeter |
| Radius | 1.610 Earth radiae |
| Semi-major Axis | 0.0183 AU |
| Eccentricity | 0 |
| Orbital Period | 0.963 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 |