The Kepler-348 system contains 2 exoplanets. It is located 1861.64 light years away from the solar system.
| Mass | 1.27 solar masses |
| Radius | 1.36 solar radiae |
| Temperature | 6177 kelvin |
| Stellar Metallicity | 0.07 decimal exponent |
| Age | 2.29 billion years |
At 2.926 Earth masses, Kepler-348 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 | 2.920 Earth masses |
| Density | 4.570 grams per cubic centimeter |
| Radius | 1.520 Earth radiae |
| Semi-major Axis | 0.076 AU |
| Eccentricity | 0 |
| Orbital Period | 7.057 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 2.331 Earth masses, Kepler-348 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 | 2.330 Earth masses |
| Density | 5.440 grams per cubic centimeter |
| Radius | 1.330 Earth radiae |
| Semi-major Axis | 0.138 AU |
| Eccentricity | 0 |
| Orbital Period | 17.265 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 |