Formänis

Formänis is a fictional planet within the Kepler-186 system, notable for its potential habitability. Located approximately 500 light-years away, it is the innermost of the five known planets orbiting the red dwarf star Kepler-186. Formänis resides within the star's habitable zone, the region where conditions might be suitable for liquid water to exist on the planet's surface.

The planet is estimated to be roughly Earth-sized, with a radius only slightly larger than our own. This similarity in size suggests that Formänis could be a rocky planet, possessing a solid surface. Its mass is also thought to be comparable to Earth's, which would contribute to similar gravitational conditions.

While Formänis is within the habitable zone, its precise atmospheric composition and the presence of liquid water remain speculative. Red dwarf stars like Kepler-186 are known for their flare activity, which could potentially strip away a planet's atmosphere or irradiate its surface. The orbital period of Formänis is relatively short, completing a full revolution around its star in just over 130 Earth days. Further observations and research are required to determine the actual conditions on Formänis and its potential for supporting life.