The Kepler-124 system contains 3 exoplanets. It is located 1370.01 light years away from the solar system.
Mass | 0.84 solar masses |
Radius | 0.64 solar radiae |
Temperature | 4984 kelvin |
Stellar Metallicity | -0.46 decimal exponent |
Age | 1.82 billion years |
At less than 1.5 Earth masses, Kepler-124 b is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 0.315 Earth masses |
Density | 4.450 grams per cubic centimeter |
Radius | 0.730 Earth radiae |
Semi-major Axis | 0.039 AU |
Eccentricity | 0 |
Orbital Period | 3.410 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 3.721 Earth masses, Kepler-124 c 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 | 3.710 Earth masses |
Density | 3.800 grams per cubic centimeter |
Radius | 1.750 Earth radiae |
Semi-major Axis | 0.1 AU |
Eccentricity | 0 |
Orbital Period | 13.821 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 less than 1.5 Earth masses, Kepler-124 d is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 1.410 Earth masses |
Density | 5.670 grams per cubic centimeter |
Radius | 1.110 Earth radiae |
Semi-major Axis | 0.17 AU |
Eccentricity | 0 |
Orbital Period | 30.951 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 |