The Kepler-1693 system contains 2 exoplanets. It is located 2479.00 light years away from the solar system.
| Mass | 0.95 solar masses |
| Radius | 0.88 solar radiae |
| Temperature | 5432.34 kelvin |
| Stellar Metallicity | 0.026 decimal exponent |
| Age | 0.8 billion years |
At 2.210 Earth masses, Kepler-1693 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 | 2.210 Earth masses |
| Density | 5.670 grams per cubic centimeter |
| Radius | 1.289 Earth radiae |
| Semi-major Axis | 0.1011 AU |
| Eccentricity | 0 |
| Orbital Period | 12.100 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2021-07 |
| Reference | Armstrong et al. 2021 |
At less than 1.5 Earth masses, Kepler-1693 c is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 0.894 Earth masses |
| Density | 5.270 grams per cubic centimeter |
| Radius | 0.977 Earth radiae |
| Semi-major Axis | 0.0588 AU |
| Eccentricity | 0 |
| Orbital Period | 5.364 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2022-02 |
| Reference | Valizadegan et al. 2022 |