The K2-413 system contains 2 exoplanets. It is located 930.07 light years away from the solar system.
| Mass | 0.81 solar masses |
| Radius | 0.7 solar radiae |
| Temperature | 4116 kelvin |
| Stellar Metallicity | -0.205 decimal exponent |
| Age | - billion years |
At less than 1.5 Earth masses, K2-413 b is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 0.363 Earth masses |
| Density | 4.550 grams per cubic centimeter |
| Radius | 0.760 Earth radiae |
| Semi-major Axis | 0.0117 AU |
| Eccentricity | NaN |
| Orbital Period | 0.809 days |
| Discovery Method | Transit |
| Discovery Facility | K2 |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2022-10 |
| Reference | del Ser et al. 2022 |
At 2.048 Earth masses, K2-413 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 | 2.050 Earth masses |
| Density | 6.010 grams per cubic centimeter |
| Radius | 1.233 Earth radiae |
| Semi-major Axis | 0.0426 AU |
| Eccentricity | NaN |
| Orbital Period | 5.330 days |
| Discovery Method | Transit |
| Discovery Facility | K2 |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2022-10 |
| Reference | del Ser et al. 2022 |