Ákófs

Ákófs 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, approximately 500 light-years from Earth. The planet's existence was theorized based on gravitational perturbations observed in the orbits of its neighboring planets, Kepler-186f and Kepler-186g. Subsequent telescopic observations and spectral analysis have provided some limited data about its characteristics.

Ákófs is believed to be a gas giant, similar in size and mass to Neptune. Its atmosphere is thought to be composed primarily of hydrogen and helium, with trace amounts of methane and ammonia, giving it a distinctive blue-green hue when viewed from space. The planet's orbital period is estimated to be around 130 Earth days, and it possesses a complex system of rings, likely composed of ice and rock particles.

Due to its distance from Kepler-186, Ákófs receives very little stellar radiation, resulting in extremely low surface temperatures. Scientists speculate that it may possess a rocky core, but no direct evidence of a solid surface has been found. The presence of moons orbiting Ákófs is currently unconfirmed, though theoretical models suggest it is likely to have several small, icy satellites. Research into Ákófs continues as astronomers seek to refine their understanding of planetary formation and composition in systems outside our own.