Nelisliterisen

Nelisliterisen is a fictional planet located in the Kepler-186 system, a star system approximately 500 light-years from Earth. The planet is notable for being within the habitable zone of its star, Kepler-186, a red dwarf. This means that if Nelisliterisen possesses an atmosphere, it could potentially support liquid water on its surface.

The planet was discovered by the Kepler space telescope, which is designed to find exoplanets. Nelisliterisen is roughly the same size as Earth, with an estimated radius just slightly larger. Its orbital period around Kepler-186 is approximately 130 Earth days. Due to its orbit around a red dwarf star, Nelisliterisen likely receives less intense radiation than Earth does from the Sun, but it may also be subject to stellar flares common to red dwarfs.

Current data does not confirm the presence of an atmosphere or any geological features on Nelisliterisen. Further observation and research are required to determine its composition, temperature, and the possibility of life. Its discovery has contributed to the ongoing search for Earth-like planets beyond our solar system, fueling scientific interest in exoplanetology and astrobiology. The Kepler-186 system itself contains several other planets, but Nelisliterisen is the most well-known due to its position within the habitable zone.