The Kepler-385 system contains 3 exoplanets. It is located 4672.54 light years away from the solar system.
Mass | 1.12 solar masses |
Radius | 1.13 solar radiae |
Temperature | 6326 kelvin |
Stellar Metallicity | 0.04 decimal exponent |
Age | 3.31 billion years |
At more than 10 Earth masses, Kepler-385 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 | 12.800 Earth masses |
Density | 3.460 grams per cubic centimeter |
Radius | 2.730 Earth radiae |
Semi-major Axis | 0.097 AU |
Eccentricity | 0 |
Orbital Period | 10.044 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-385 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 | 13.200 Earth masses |
Density | 2.580 grams per cubic centimeter |
Radius | 3.040 Earth radiae |
Semi-major Axis | 0.127 AU |
Eccentricity | 0 |
Orbital Period | 15.163 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-385 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 | 7.360 Earth masses |
Density | 2.250 grams per cubic centimeter |
Radius | 2.619 Earth radiae |
Semi-major Axis | 0.3024 AU |
Eccentricity | 0 |
Orbital Period | 56.416 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2021-07 |
Reference | Armstrong et al. 2021 |