The Kepler-1336 system contains 2 exoplanets. It is located 3674.60 light years away from the solar system.
| Mass | 0.94 solar masses |
| Radius | 1.3 solar radiae |
| Temperature | 5512 kelvin |
| Stellar Metallicity | 0.05 decimal exponent |
| Age | 12.3 billion years |
With a mass below 5 Earth masses, a density of 3.24, and a semi-major axis of 0.1595 astronomical units, Kepler-1336 b could, potentially, be an ocean world - a planet with no dry land.
| Mass | 4.580 Earth masses |
| Density | 3.240 grams per cubic centimeter |
| Radius | 1.980 Earth radiae |
| Semi-major Axis | 0.1595 AU |
| Eccentricity | 0 |
| Orbital Period | 23.199 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 3.562 Earth masses, Kepler-1336 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 | 3.570 Earth masses |
| Density | 3.920 grams per cubic centimeter |
| Radius | 1.710 Earth radiae |
| Semi-major Axis | 0.0631 AU |
| Eccentricity | 0 |
| Orbital Period | 5.777 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 |