The Kepler-374 system contains 3 exoplanets. It is located 4127.86 light years away from the solar system.
Mass | 1.04 solar masses |
Radius | 0.91 solar radiae |
Temperature | 5977 kelvin |
Stellar Metallicity | 0.111 decimal exponent |
Age | 1.5 billion years |
At less than 1.5 Earth masses, Kepler-374 b is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 1.080 Earth masses |
Density | 5.430 grams per cubic centimeter |
Radius | 1.030 Earth radiae |
Semi-major Axis | 0.029 AU |
Eccentricity | 0 |
Orbital Period | 1.898 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-374 c is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 1.370 Earth masses |
Density | 5.660 grams per cubic centimeter |
Radius | 1.100 Earth radiae |
Semi-major Axis | 0.042 AU |
Eccentricity | 0 |
Orbital Period | 3.283 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 2.271 Earth masses, Kepler-374 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 | 2.270 Earth masses |
Density | 5.550 grams per cubic centimeter |
Radius | 1.310 Earth radiae |
Semi-major Axis | 0.056 AU |
Eccentricity | 0 |
Orbital Period | 5.028 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 |