The Kepler-192 system contains 3 exoplanets. It is located 2125.47 light years away from the solar system.
Mass | 0.94 solar masses |
Radius | 1.01 solar radiae |
Temperature | 5479 kelvin |
Stellar Metallicity | 0.357 decimal exponent |
Age | 0.5 billion years |
At more than 10 Earth masses, Kepler-192 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 | 7.950 Earth masses |
Density | 2.120 grams per cubic centimeter |
Radius | 2.740 Earth radiae |
Semi-major Axis | 0.09 AU |
Eccentricity | 0 |
Orbital Period | 9.927 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2014-03 |
Reference | Rowe et al. 2014 |
At more than 10 Earth masses, Kepler-192 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 | 8.200 Earth masses |
Density | 2.070 grams per cubic centimeter |
Radius | 2.790 Earth radiae |
Semi-major Axis | 0.15 AU |
Eccentricity | 0 |
Orbital Period | 21.223 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2014-03 |
Reference | Rowe et al. 2014 |
At less than 1.5 Earth masses, Kepler-192 d is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 1.040 Earth masses |
Density | 5.390 grams per cubic centimeter |
Radius | 1.020 Earth radiae |
Semi-major Axis | 0.0668 AU |
Eccentricity | 0 |
Orbital Period | 6.470 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 |