The Kepler-334 system contains 3 exoplanets. It is located 1391.35 light years away from the solar system.
Mass | 1.07 solar masses |
Radius | 1.07 solar radiae |
Temperature | 5828 kelvin |
Stellar Metallicity | -0.012 decimal exponent |
Age | 1.6 billion years |
At less than 1.5 Earth masses, Kepler-334 b is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 1.460 Earth masses |
Density | 5.710 grams per cubic centimeter |
Radius | 1.120 Earth radiae |
Semi-major Axis | 0.061 AU |
Eccentricity | 0 |
Orbital Period | 5.470 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 2.636 Earth masses, Kepler-334 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 | 2.630 Earth masses |
Density | 4.940 grams per cubic centimeter |
Radius | 1.430 Earth radiae |
Semi-major Axis | 0.107 AU |
Eccentricity | 0 |
Orbital Period | 12.758 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 2.573 Earth masses, Kepler-334 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 | 2.570 Earth masses |
Density | 5.040 grams per cubic centimeter |
Radius | 1.410 Earth radiae |
Semi-major Axis | 0.168 AU |
Eccentricity | 0 |
Orbital Period | 25.098 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 |