Lävmiin

Lävmiin 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 at a distance of approximately 500 light-years from Earth. Lävmiin is notable for being a rocky planet within the habitable zone of its star, meaning it could potentially support liquid water on its surface.

The planet's estimated size is about 1.1 times that of Earth. Its orbital period is roughly 130 days. Due to its orbit around a red dwarf star, Lävmiin likely receives less intense light than Earth does from the Sun. The nature of its atmosphere, if any, and its surface conditions remain theoretical, as direct observation is limited. Scientists speculate about the possibility of life given its location within the habitable zone, but no definitive evidence exists. The Kepler-186 system itself consists of four other known planets, all of which are closer to the star and are likely gas or ice giants. Lävmiin's discovery was part of the Kepler Space Telescope's mission to identify exoplanets. Further research and advancements in telescopic technology are required to gather more detailed information about Lävmiin's composition, climate, and potential habitability.