Oleltis

Oleltis is a fictional planetary body located within the Kepler-186 star system, approximately 500 light-years from Earth. It is the fifth planet from the star Kepler-186, a red dwarf star. Oleltis resides within the habitable zone of its star, meaning that conditions on its surface might be suitable for liquid water to exist. This characteristic has made it a subject of interest in astrobiological studies and science fiction narratives.

The planet is believed to be rocky, with an estimated radius similar to that of Earth. Its orbital period around Kepler-186 is approximately 130 Earth days. Due to its distance from Earth, direct observation of Oleltis's atmosphere or surface features is currently limited. However, based on its position within the habitable zone and its rocky composition, scientists speculate about the potential for various geological processes and possibly even life.

The Kepler-186 system is notable for hosting multiple planets, and Oleltis is one of the outer members of this planetary family. The nature of its star, Kepler-186, being a red dwarf, means that any potential life on Oleltis would need to be adapted to the different light spectrum and potential stellar activity characteristic of such stars. Further research and advancements in observational technology are needed to provide more definitive information about Oleltis.