The Kepler-722 system contains 2 exoplanets. It is located 4042.70 light years away from the solar system.
| Mass | 1.03 solar masses |
| Radius | 1.05 solar radiae |
| Temperature | 5863 kelvin |
| Stellar Metallicity | 0.02 decimal exponent |
| Age | 4.37 billion years |
At more than 10 Earth masses, Kepler-722 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 | 7.410 Earth masses |
| Density | 2.240 grams per cubic centimeter |
| Radius | 2.630 Earth radiae |
| Semi-major Axis | 0.0514 AU |
| Eccentricity | 0 |
| Orbital Period | 4.094 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 more than 10 Earth masses, Kepler-722 c 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 | 8.350 Earth masses |
| Density | 2.050 grams per cubic centimeter |
| Radius | 2.820 Earth radiae |
| Semi-major Axis | 0.4471 AU |
| Eccentricity | 0 |
| Orbital Period | 105.145 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 |