The Kepler-132 system contains 4 exoplanets. It is located 1140.08 light years away from the solar system.
| Mass | 0.98 solar masses |
| Radius | 1.18 solar radiae |
| Temperature | 6003 kelvin |
| Stellar Metallicity | -0.216 decimal exponent |
| Age | 4.37 billion years |
At 1.927 Earth masses, Kepler-132 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 | 1.920 Earth masses |
| Density | 5.960 grams per cubic centimeter |
| Radius | 1.210 Earth radiae |
| Semi-major Axis | 0.067 AU |
| Eccentricity | 0 |
| Orbital Period | 6.178 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 2.185 Earth masses, Kepler-132 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 | 2.180 Earth masses |
| Density | 5.710 grams per cubic centimeter |
| Radius | 1.280 Earth radiae |
| Semi-major Axis | 0.068 AU |
| Eccentricity | 0 |
| Orbital Period | 6.415 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 3.024 Earth masses, Kepler-132 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 | 3.020 Earth masses |
| Density | 4.460 grams per cubic centimeter |
| Radius | 1.550 Earth radiae |
| Semi-major Axis | 0.136 AU |
| Eccentricity | 0 |
| Orbital Period | 18.010 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-132 e 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 | 0.4393 AU |
| Eccentricity | 0 |
| Orbital Period | 110.287 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 |