Fulvian

Fulvian is a fictional planet located in the Kepler-186 system, approximately 500 light-years from Earth. It is the outermost planet in this system, orbiting its red dwarf star at a distance that places it within the habitable zone. This orbital position suggests the potential for liquid water to exist on its surface, a key ingredient for life as we know it.

The planet is estimated to be roughly 1.1 times the size of Earth and has a rocky composition. Its atmosphere is thought to be thicker than Earth's, potentially offering protection from stellar radiation. Early telescopic observations indicate the presence of cloud formations and a distinct coloration, suggesting a varied surface geology and possibly atmospheric composition.

Scientists are particularly interested in Fulvian due to its location within the habitable zone of a red dwarf star. While red dwarfs are known for their stellar flares, Kepler-186 is considered a relatively stable star, increasing the chances of a stable environment on Fulvian. Further research is needed to confirm atmospheric composition, the presence of water, and any potential signs of biosignatures. The planet's study contributes to the ongoing search for exoplanets that could harbor life.