The Kepler-1468 system is known to contain 2 exoplanets in orbit around it. It is located 6194.49 light years away from the solar system.
| Mass | 1.04 solar masses |
| Radius | 1.05 solar radiae |
| Temperature | 5893 kelvin |
| Stellar Metallicity | 0.03 Decimal exponent |
| Age | 3.55 billion years |
At 3.657 Earth masses, Kepler-1468 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. No Super Earths are known to exist in our solar system, but if it exists, the so-called Planet Nine could very well be a super Earth, as it is hypothesized to have a mass between five and ten Earth masses.
| Mass | 3.640 Earth masses |
| Density | 3.860 Grams per cubic centimeter |
| Radius | 1.730 Earth radiae |
| Semi-major Axis | 0.0817 AU |
| Eccentricity | 0 |
| Orbital Period | 8.240 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 |
At 1.606 Earth masses, Kepler-1468 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. No Super Earths are known to exist in our solar system, but if it exists, the so-called Planet Nine could very well be a super Earth, as it is hypothesized to have a mass between five and ten Earth masses.
| Mass | 1.600 Earth masses |
| Density | 5.780 Grams per cubic centimeter |
| Radius | 1.150 Earth radiae |
| Semi-major Axis | 0.0466 AU |
| Eccentricity | 0 |
| Orbital Period | 3.546 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 |