The Kepler-325 system contains 3 exoplanets. It is located 2685.05 light years away from the solar system.
Mass | 0.92 solar masses |
Radius | 1 solar radiae |
Temperature | 5752 kelvin |
Stellar Metallicity | 0.017 decimal exponent |
Age | 8.2 billion years |
At more than 10 Earth masses, Kepler-325 b 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 | 8.800 Earth masses |
Density | 1.960 grams per cubic centimeter |
Radius | 2.910 Earth radiae |
Semi-major Axis | 0.053 AU |
Eccentricity | 0 |
Orbital Period | 4.544 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-325 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 | 6.990 Earth masses |
Density | 2.340 grams per cubic centimeter |
Radius | 2.540 Earth radiae |
Semi-major Axis | 0.105 AU |
Eccentricity | 0 |
Orbital Period | 12.762 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-325 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 | 8.200 Earth masses |
Density | 2.070 grams per cubic centimeter |
Radius | 2.790 Earth radiae |
Semi-major Axis | 0.22 AU |
Eccentricity | 0 |
Orbital Period | 38.715 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 |