The Kepler-275 system contains 3 exoplanets. It is located 6634.83 light years away from the solar system.
Mass | 1.16 solar masses |
Radius | 1.38 solar radiae |
Temperature | 6165 kelvin |
Stellar Metallicity | 0 decimal exponent |
Age | 0.31 billion years |
At more than 10 Earth masses, Kepler-275 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 | 6.080 Earth masses |
Density | 2.610 grams per cubic centimeter |
Radius | 2.340 Earth radiae |
Semi-major Axis | 0.098 AU |
Eccentricity | 0 |
Orbital Period | 10.301 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-275 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 | 11.400 Earth masses |
Density | 1.620 grams per cubic centimeter |
Radius | 3.380 Earth radiae |
Semi-major Axis | 0.132 AU |
Eccentricity | 0 |
Orbital Period | 16.088 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-275 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 | 11.100 Earth masses |
Density | 1.650 grams per cubic centimeter |
Radius | 3.330 Earth radiae |
Semi-major Axis | 0.224 AU |
Eccentricity | 0 |
Orbital Period | 35.676 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 |