The Kepler-83 system contains 3 exoplanets. It is located 1305.96 light years away from the solar system.
Mass | 0.66 solar masses |
Radius | 0.61 solar radiae |
Temperature | 4082 kelvin |
Stellar Metallicity | -0.2 decimal exponent |
Age | 3.09 billion years |
At more than 10 Earth masses, Kepler-83 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 | 42.100 Earth masses |
Density | 10.200 grams per cubic centimeter |
Radius | 2.830 Earth radiae |
Semi-major Axis | 0.07295 AU |
Eccentricity | 0 |
Orbital Period | 9.770 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2013-10 |
Reference | Xie 2013 |
At more than 10 Earth masses, Kepler-83 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 | 11.400 Earth masses |
Density | 4.770 grams per cubic centimeter |
Radius | 2.360 Earth radiae |
Semi-major Axis | 0.11796 AU |
Eccentricity | 0 |
Orbital Period | 20.090 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2013-10 |
Reference | Xie 2013 |
At more than 10 Earth masses, Kepler-83 d 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 | 24.600 Earth masses |
Density | 18.500 grams per cubic centimeter |
Radius | 1.940 Earth radiae |
Semi-major Axis | 0.051 AU |
Eccentricity | 0 |
Orbital Period | 5.170 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 |