The Kepler-319 system contains 3 exoplanets. It is located 1641.99 light years away from the solar system.
Mass | 0.96 solar masses |
Radius | 0.9 solar radiae |
Temperature | 5526 kelvin |
Stellar Metallicity | -0.015 decimal exponent |
Age | 3.55 billion years |
At 3.307 Earth masses, Kepler-319 b is a so called Super Earth. Super Earths could be terrestrial worlds like Earth, but they could also be ocean worlds or terrestrial worlds wrapped in a substantial atmosphere, in which case some refer to them as Mini Neptunes.
Mass | 3.290 Earth masses |
Density | 4.170 grams per cubic centimeter |
Radius | 1.630 Earth radiae |
Semi-major Axis | 0.051 AU |
Eccentricity | 0 |
Orbital Period | 4.363 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-319 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 | 7.410 Earth masses |
Density | 2.240 grams per cubic centimeter |
Radius | 2.630 Earth radiae |
Semi-major Axis | 0.069 AU |
Eccentricity | 0 |
Orbital Period | 6.941 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-319 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 | 5.860 Earth masses |
Density | 2.680 grams per cubic centimeter |
Radius | 2.290 Earth radiae |
Semi-major Axis | 0.191 AU |
Eccentricity | 0 |
Orbital Period | 31.782 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 |