The Kepler-750 system contains 2 exoplanets. It is located 4227.05 light years away from the solar system.
| Mass | 1.15 solar masses |
| Radius | 1.23 solar radiae |
| Temperature | 6160 kelvin |
| Stellar Metallicity | 0.03 decimal exponent |
| Age | 3.09 billion years |
At more than 10 Earth masses, Kepler-750 b is an ice giant, a planet that is made up mostly of volatiles like water, amonia and methane, and enveloped by a dense hydrogen and helium atmosphere, much like Uranus and Neptune.
| Mass | 9.640 Earth masses |
| Density | 1.830 grams per cubic centimeter |
| Radius | 3.070 Earth radiae |
| Semi-major Axis | 0.093 AU |
| Eccentricity | 0 |
| Orbital Period | 9.429 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 3.244 Earth masses, Kepler-750 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 | 3.260 Earth masses |
| Density | 4.210 grams per cubic centimeter |
| Radius | 1.620 Earth radiae |
| Semi-major Axis | 0.0533 AU |
| Eccentricity | 0 |
| Orbital Period | 4.089 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 |