The Kepler-198 system contains 3 exoplanets. It is located 1615.64 light years away from the solar system.
Mass | 0.97 solar masses |
Radius | 0.94 solar radiae |
Temperature | 5574 kelvin |
Stellar Metallicity | 0.114 decimal exponent |
Age | 3.72 billion years |
At more than 10 Earth masses, Kepler-198 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 | 8.350 Earth masses |
Density | 2.050 grams per cubic centimeter |
Radius | 2.820 Earth radiae |
Semi-major Axis | 0.131 AU |
Eccentricity | 0 |
Orbital Period | 17.790 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-198 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 | 6.660 Earth masses |
Density | 2.430 grams per cubic centimeter |
Radius | 2.470 Earth radiae |
Semi-major Axis | 0.259 AU |
Eccentricity | 0 |
Orbital Period | 49.567 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 2.957 Earth masses, Kepler-198 d is a so called Super Earth. Super Earths could be terrestrial worlds like Earth, but they could also be ocean worlds or terrestrial worlds wrapped in a substantial atmosphere, in which case some refer to them as Mini Neptunes.
Mass | 2.960 Earth masses |
Density | 4.540 grams per cubic centimeter |
Radius | 1.530 Earth radiae |
Semi-major Axis | 0.0229 AU |
Eccentricity | 0 |
Orbital Period | 1.312 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2016-05 |
Reference | Morton et al. 2016 |