The Kepler-1642 system contains 2 exoplanets. It is located 1349.87 light years away from the solar system.
| Mass | 0.88 solar masses |
| Radius | 0.84 solar radiae |
| Temperature | 5355 kelvin |
| Stellar Metallicity | -0.01 decimal exponent |
| Age | 4.47 billion years |
At more than 10 Earth masses, Kepler-1642 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 | 10.300 Earth masses |
| Density | 1.730 grams per cubic centimeter |
| Radius | 3.200 Earth radiae |
| Semi-major Axis | 0.1016 AU |
| Eccentricity | 0 |
| Orbital Period | 12.206 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-1642 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 | 7.560 Earth masses |
| Density | 2.210 grams per cubic centimeter |
| Radius | 2.660 Earth radiae |
| Semi-major Axis | 0.0678 AU |
| Eccentricity | 0 |
| Orbital Period | 6.651 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 |