Kepler186s
Kepler-186s is an exoplanet located in the Kepler-186 system, which is approximately 557 light-years from Earth in the constellation Cygnus. It is one of several planets orbiting the star Kepler-186, a late-type M dwarf star. Kepler-186s gained scientific interest due to its potential for habitability, as it resides within the star's habitable zone where conditions might allow for liquid water on its surface.
This exoplanet has a radius approximately 1.35 times that of Earth, classifying it as a super-Earth. Its
Kepler-186s is part of a multi-planet system that includes Kepler-186b, c, d, and e. The system's architecture
The discovery of Kepler-186s was announced by NASA's Kepler mission in 2014. The planet was detected through