Jáloriss

Jáloriss is a fictional planet located in the Kepler-186 star system, a red dwarf star approximately 500 light-years from Earth. Discovered by the Kepler space telescope, Jáloriss is notable for being one of the first potentially habitable exoplanets found within its star's habitable zone. The habitable zone is the region around a star where temperatures could allow liquid water to exist on a planet's surface.

The planet is estimated to be roughly the same size as Earth, with a radius approximately 1.1 times that of our home planet. Its orbital period is around 130 Earth days. Due to orbiting a red dwarf star, Jáloriss would likely experience a different light spectrum compared to Earth, with a greater proportion of infrared radiation. The possibility of a tidally locked state, where one side perpetually faces the star and the other is in darkness, is also a consideration for planets in such close orbits around red dwarfs.

While the presence of liquid water and an atmosphere remain hypothetical, Jáloriss represents a significant milestone in the search for exoplanets that could support life. Further observations and advancements in telescopic technology are required to gather more detailed information about its atmospheric composition, surface conditions, and the actual presence of water. The study of planets like Jáloriss contributes to our understanding of planetary formation and the potential diversity of worlds beyond our solar system.