Eevaksis

Eevaksis is a fictional planet located in the Kepler-186 system, a star system approximately 500 light-years from Earth. It is the fifth planet from its star, Kepler-186f, and orbits within the habitable zone, the region around a star where liquid water could potentially exist on a planet's surface. Eevaksis is believed to be a terrestrial planet, meaning it is composed primarily of silicate rocks and metals.

Initial telescopic observations suggest Eevaksis is roughly Earth-sized, with a diameter estimated to be around 1.2 times that of our home planet. Its orbital period is approximately 130 Earth days. The planet's atmosphere is thought to be relatively dense, potentially contributing to a stable surface temperature. While direct evidence of life has not been found, its position within the habitable zone makes Eevaksis a prime candidate for further astrobiological investigation. Future missions are planned to analyze its atmospheric composition and search for biosignatures that could indicate the presence of microbial or more complex life forms. The planet's geology is largely unknown, but it is theorized to possess a rocky surface with possible oceans or large bodies of liquid.