Tairyhmäts

Tairyhmäts 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.

Observations suggest Tairyhmäts is a gas giant, similar in composition to Jupiter or Saturn. Its atmosphere is believed to be primarily composed of hydrogen and helium, with trace amounts of other gases. The planet's surface, if one can be defined for a gas giant, is not solid but rather a region where atmospheric pressure becomes extremely high. Due to its distance from Kepler-186, Tairyhmäts receives very little stellar radiation, resulting in extremely low surface temperatures.

The orbital period of Tairyhmäts is estimated to be several hundred Earth years. Its exact mass and radius are still subjects of ongoing research and refinement. No moons have been definitively detected around Tairyhmäts, though the possibility of smaller, captured celestial bodies remains. The study of Tairyhmäts contributes to our understanding of planetary formation and the diversity of exoplanetary systems.