Sárrs

Sárrs is a fictional planet located in the Kepler-186 star system, approximately 500 light-years from Earth. It is the fifth and outermost known planet in this system, orbiting a red dwarf star. The planet is characterized by its relatively low surface temperature, due to the dimmer nature of its parent star and its orbital distance. Data suggests Sárrs has a thick atmosphere, primarily composed of nitrogen and methane, contributing to a significant greenhouse effect that moderates its otherwise frigid conditions. Its surface is believed to be dominated by vast, frozen oceans and extensive tundra-like landscapes.

Evidence gathered from remote sensing indicates the presence of complex geological formations, including mountain ranges and large impact craters. While direct observation of life is currently impossible, theoretical models suggest that if life exists on Sárrs, it would likely be extremophilic, adapted to the cold and low-light environment. The planet's orbit is nearly circular, resulting in minimal seasonal variation. Further study of Sárrs is a priority for astrobiologists and planetary scientists seeking to understand the diversity of planetary environments within our galaxy.