The Kepler-219 system contains 3 exoplanets. It is located 2567.08 light years away from the solar system.
Mass | 1.17 solar masses |
Radius | 1.49 solar radiae |
Temperature | 5786 kelvin |
Stellar Metallicity | 0.361 decimal exponent |
Age | 4 billion years |
At more than 10 Earth masses, Kepler-219 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 | 9.010 Earth masses |
Density | 1.930 grams per cubic centimeter |
Radius | 2.950 Earth radiae |
Semi-major Axis | 0.057 AU |
Eccentricity | 0 |
Orbital Period | 4.586 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-219 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 | 12.500 Earth masses |
Density | 1.500 grams per cubic centimeter |
Radius | 3.580 Earth radiae |
Semi-major Axis | 0.165 AU |
Eccentricity | 0 |
Orbital Period | 22.715 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-219 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 | 19.100 Earth masses |
Density | 4.730 grams per cubic centimeter |
Radius | 2.810 Earth radiae |
Semi-major Axis | 0.272 AU |
Eccentricity | 0 |
Orbital Period | 47.904 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 |