The Kepler-267 system contains 3 exoplanets. It is located 864.29 light years away from the solar system.
Mass | 0.54 solar masses |
Radius | 0.56 solar radiae |
Temperature | 4258 kelvin |
Stellar Metallicity | -0.18 decimal exponent |
Age | 3.31 billion years |
At more than 10 Earth masses, Kepler-267 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 | 37.900 Earth masses |
Density | 26.800 grams per cubic centimeter |
Radius | 1.980 Earth radiae |
Semi-major Axis | 0.037 AU |
Eccentricity | 0 |
Orbital Period | 3.354 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-267 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 | 5.180 Earth masses |
Density | 2.950 grams per cubic centimeter |
Radius | 2.130 Earth radiae |
Semi-major Axis | 0.06 AU |
Eccentricity | 0 |
Orbital Period | 6.877 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-267 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 | 5.770 Earth masses |
Density | 2.710 grams per cubic centimeter |
Radius | 2.270 Earth radiae |
Semi-major Axis | 0.154 AU |
Eccentricity | 0 |
Orbital Period | 28.465 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 |