Rrühmastian

Rrühmastian 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 approximately 500 light-years from Earth. Rrühmastian is believed to be a rocky planet, similar in size and mass to Earth, though its exact composition is still under scientific investigation.

The planet resides within the habitable zone of its star, the region where conditions might be suitable for liquid water to exist on the surface. This makes Rrühmastian a subject of interest in the search for exoplanets that could potentially harbor life. However, the presence of liquid water is not confirmed, and the planet's atmosphere, if any, is unknown.

Due to the nature of its host star, Kepler-186, Rrühmastian receives less stellar radiation than Earth receives from the Sun. The light on Rrühmastian would likely appear redder and dimmer. Scientists hypothesize that if an atmosphere exists, it might need to be thicker than Earth's to maintain a sufficient surface temperature for liquid water. Further observations and analysis are required to determine the true characteristics of Rrühmastian.