The Kepler-332 system contains 3 exoplanets. It is located 1122.60 light years away from the solar system.
Mass | 0.8 solar masses |
Radius | 0.72 solar radiae |
Temperature | 4955 kelvin |
Stellar Metallicity | -0.1 decimal exponent |
Age | 2.82 billion years |
At 1.708 Earth masses, Kepler-332 b 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 | 1.710 Earth masses |
Density | 5.870 grams per cubic centimeter |
Radius | 1.170 Earth radiae |
Semi-major Axis | 0.07 AU |
Eccentricity | 0 |
Orbital Period | 7.626 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-332 c is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
Mass | 1.320 Earth masses |
Density | 5.600 grams per cubic centimeter |
Radius | 1.090 Earth radiae |
Semi-major Axis | 0.114 AU |
Eccentricity | 0 |
Orbital Period | 15.996 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 1.759 Earth masses, Kepler-332 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 | 1.760 Earth masses |
Density | 5.890 grams per cubic centimeter |
Radius | 1.180 Earth radiae |
Semi-major Axis | 0.189 AU |
Eccentricity | 0 |
Orbital Period | 34.212 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 |