The Kepler-414 system contains 2 exoplanets. It is located 1348.52 light years away from the solar system.
| Mass | 0.89 solar masses |
| Radius | 0.95 solar radiae |
| Temperature | 5536 kelvin |
| Stellar Metallicity | 0.05 decimal exponent |
| Age | 5.5 billion years |
At 3.498 Earth masses, Kepler-414 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 | 3.500 Earth masses |
| Density | 3.850 grams per cubic centimeter |
| Radius | 1.710 Earth radiae |
| Semi-major Axis | 0.0527 AU |
| Eccentricity | 0 |
| Orbital Period | 4.700 days |
| Discovery Method | Transit Timing Variations |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-05 |
| Reference | Hadden et al. 2014 |
At more than 10 Earth masses, Kepler-414 c is an ice giant, a planet that is made up mostly of volatiles like water, amonia and methane, and enveloped by a dense hydrogen and helium atmosphere, much like Uranus and Neptune.
| Mass | 29.900 Earth masses |
| Density | 6.020 grams per cubic centimeter |
| Radius | 3.010 Earth radiae |
| Semi-major Axis | 0.0699 AU |
| Eccentricity | 0 |
| Orbital Period | 7.171 days |
| Discovery Method | Transit Timing Variations |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-05 |
| Reference | Hadden et al. 2014 |