The Kepler-310 system contains 3 exoplanets. It is located 1964.33 light years away from the solar system.
Mass | 0.91 solar masses |
Radius | 0.88 solar radiae |
Temperature | 5797 kelvin |
Stellar Metallicity | -0.07 decimal exponent |
Age | 1.9 billion years |
At 1.813 Earth masses, Kepler-310 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 | 1.810 Earth masses |
Density | 5.900 grams per cubic centimeter |
Radius | 1.190 Earth radiae |
Semi-major Axis | 0.111 AU |
Eccentricity | 0 |
Orbital Period | 13.931 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-310 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 | 1.620 grams per cubic centimeter |
Radius | 3.380 Earth radiae |
Semi-major Axis | 0.281 AU |
Eccentricity | 0 |
Orbital Period | 56.475 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-310 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 | 7.000 Earth masses |
Density | 3.300 grams per cubic centimeter |
Radius | 2.470 Earth radiae |
Semi-major Axis | 0.392 AU |
Eccentricity | 0 |
Orbital Period | 92.876 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 |