Valniran

Valniran is a fictional planet located in the Kepler-186 star system. It is the fifth planet from its star, Kepler-186f, a red dwarf. Valniran is considered to be within the habitable zone of its star, meaning conditions may be suitable for liquid water to exist on its surface. The planet is approximately 500 light-years from Earth.

Initial observations suggest Valniran is a terrestrial planet, meaning it is rocky and has a solid surface. Its size is estimated to be slightly larger than Earth, with a radius roughly 1.1 times that of our planet. The planet's mass is not precisely known, but it is inferred to be similar to Earth's. Valniran's orbital period is approximately 130 Earth days.

Due to the dim nature of its red dwarf star, Kepler-186f, Valniran receives less stellar energy than Earth does from the Sun. However, its closer proximity to its star may compensate for this, potentially allowing for surface temperatures conducive to liquid water. The exact atmospheric composition of Valniran remains unknown, which is a critical factor in determining its habitability. Future observations, possibly with advanced telescopes, are needed to gather more detailed information about Valniran's atmosphere, surface features, and potential for life. The Kepler-186 system is of significant interest to astronomers searching for exoplanets that could support life.