The Kepler-339 system contains 3 exoplanets. It is located 2011.20 light years away from the solar system.
Mass | 0.93 solar masses |
Radius | 0.8 solar radiae |
Temperature | 5631 kelvin |
Stellar Metallicity | 0.033 decimal exponent |
Age | 4.37 billion years |
At 2.604 Earth masses, Kepler-339 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 | 2.600 Earth masses |
Density | 4.990 grams per cubic centimeter |
Radius | 1.420 Earth radiae |
Semi-major Axis | 0.055 AU |
Eccentricity | 0 |
Orbital Period | 4.978 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-339 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 | 7.300 Earth masses |
Density | 26.400 grams per cubic centimeter |
Radius | 1.150 Earth radiae |
Semi-major Axis | 0.069 AU |
Eccentricity | 0 |
Orbital Period | 6.988 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-339 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 | 14.700 Earth masses |
Density | 50.400 grams per cubic centimeter |
Radius | 1.170 Earth radiae |
Semi-major Axis | 0.091 AU |
Eccentricity | 0 |
Orbital Period | 10.558 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 |