The Kepler-350 system contains 3 exoplanets. It is located 3120.85 light years away from the solar system.
Mass | 1.19 solar masses |
Radius | 1.53 solar radiae |
Temperature | 6186 kelvin |
Stellar Metallicity | 0.041 decimal exponent |
Age | 4 billion years |
At 4.070 Earth masses, Kepler-350 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 | 4.080 Earth masses |
Density | 3.540 grams per cubic centimeter |
Radius | 1.850 Earth radiae |
Semi-major Axis | 0.104 AU |
Eccentricity | 0 |
Orbital Period | 11.190 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-350 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 | 6.100 Earth masses |
Density | 1.130 grams per cubic centimeter |
Radius | 3.100 Earth radiae |
Semi-major Axis | 0.1385 AU |
Eccentricity | 0 |
Orbital Period | 17.849 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2014-02 |
Reference | Xie 2014 |
At more than 10 Earth masses, Kepler-350 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 | 14.900 Earth masses |
Density | 3.730 grams per cubic centimeter |
Radius | 2.800 Earth radiae |
Semi-major Axis | 0.1786 AU |
Eccentricity | 0 |
Orbital Period | 26.136 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2014-02 |
Reference | Xie 2014 |