The Kepler-336 system contains 3 exoplanets. It is located 2507.68 light years away from the solar system.
Mass | 1.09 solar masses |
Radius | 1.3 solar radiae |
Temperature | 5867 kelvin |
Stellar Metallicity | 0.337 decimal exponent |
Age | 4.9 billion years |
At less than 1.5 Earth masses, Kepler-336 b is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 1.040 Earth masses |
Density | 5.390 grams per cubic centimeter |
Radius | 1.020 Earth radiae |
Semi-major Axis | 0.033 AU |
Eccentricity | 0 |
Orbital Period | 2.025 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-336 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 | 5.060 Earth masses |
Density | 3.000 grams per cubic centimeter |
Radius | 2.100 Earth radiae |
Semi-major Axis | 0.092 AU |
Eccentricity | 0 |
Orbital Period | 9.600 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-336 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 | 6.210 Earth masses |
Density | 2.560 grams per cubic centimeter |
Radius | 2.370 Earth radiae |
Semi-major Axis | 0.154 AU |
Eccentricity | 0 |
Orbital Period | 20.679 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 |