Potenssius

Potenssius is a fictional planet located in the Kepler-186 system. It is the fifth and outermost known planet orbiting the red dwarf star Kepler-186, situated in the habitable zone of its star. This placement suggests that Potenssius could potentially harbor liquid water on its surface, a key ingredient for life as we know it.

The planet's estimated size is roughly 1.1 times that of Earth, making it a terrestrial or "super-Earth" type planet. Its orbital period is approximately 130 days. Due to orbiting a red dwarf star, Potenssius receives less stellar radiation than Earth receives from the Sun, but its closer proximity to Kepler-186 compensates for this. The conditions on Potenssius are theorized to be cooler than Earth's, and its atmosphere, if present, would play a crucial role in regulating its temperature.

Research into Potenssius focuses on its potential habitability and the possibility of extraterrestrial life. Further observations and analysis are needed to determine the planet's atmospheric composition, the presence of water, and its geological activity. Potenssius represents one of the most promising exoplanet candidates for astrobiological study currently known.