The Kepler-262 system contains 2 exoplanets. It is located 1999.76 light years away from the solar system.
| Mass | 0.99 solar masses |
| Radius | 0.88 solar radiae |
| Temperature | 5841 kelvin |
| Stellar Metallicity | -0.338 decimal exponent |
| Age | 3.55 billion years |
At 2.420 Earth masses, Kepler-262 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 | 2.420 Earth masses |
| Density | 5.290 grams per cubic centimeter |
| Radius | 1.360 Earth radiae |
| Semi-major Axis | 0.108 AU |
| Eccentricity | 0 |
| Orbital Period | 13.061 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 3.339 Earth masses, Kepler-262 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 | 3.330 Earth masses |
| Density | 4.150 grams per cubic centimeter |
| Radius | 1.640 Earth radiae |
| Semi-major Axis | 0.152 AU |
| Eccentricity | 0 |
| Orbital Period | 21.854 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 |