The Kepler-326 system contains 3 exoplanets. It is located 1590.58 light years away from the solar system.
Mass | 0.85 solar masses |
Radius | 0.8 solar radiae |
Temperature | 5105 kelvin |
Stellar Metallicity | 0.239 decimal exponent |
Age | 14 billion years |
At more than 10 Earth masses, Kepler-326 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 | 44.600 Earth masses |
Density | 69.800 grams per cubic centimeter |
Radius | 1.520 Earth radiae |
Semi-major Axis | 0.032 AU |
Eccentricity | 0 |
Orbital Period | 2.248 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-326 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 | 17.400 Earth masses |
Density | 34.800 grams per cubic centimeter |
Radius | 1.400 Earth radiae |
Semi-major Axis | 0.051 AU |
Eccentricity | 0 |
Orbital Period | 4.580 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-326 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 | 6.900 Earth masses |
Density | 21.400 grams per cubic centimeter |
Radius | 1.210 Earth radiae |
Semi-major Axis | 0.066 AU |
Eccentricity | 0 |
Orbital Period | 6.767 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 |