The Kepler-104 system contains 3 exoplanets. It is located 1307.18 light years away from the solar system.
Mass | 0.81 solar masses |
Radius | 1.35 solar radiae |
Temperature | 5711 kelvin |
Stellar Metallicity | -0.38 decimal exponent |
Age | 12.9 billion years |
At more than 10 Earth masses, Kepler-104 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 | 19.600 Earth masses |
Density | 3.620 grams per cubic centimeter |
Radius | 3.100 Earth radiae |
Semi-major Axis | 0.094 AU |
Eccentricity | 0 |
Orbital Period | 11.428 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-104 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 | 9.960 Earth masses |
Density | 1.780 grams per cubic centimeter |
Radius | 3.130 Earth radiae |
Semi-major Axis | 0.153 AU |
Eccentricity | 0 |
Orbital Period | 23.668 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-104 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 | 12.500 Earth masses |
Density | 1.500 grams per cubic centimeter |
Radius | 3.580 Earth radiae |
Semi-major Axis | 0.257 AU |
Eccentricity | 0 |
Orbital Period | 51.755 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 |