Vyerpanas

Vyerpanas is a fictional planet located in the Kepler-186 system. It is the fifth and outermost planet in this system, orbiting a red dwarf star. Scientists first detected Vyerpanas through observations made by the Kepler Space Telescope. The planet is believed to be a rocky terrestrial world, similar in size to Earth, though its exact composition and atmospheric conditions remain largely unknown.

The orbit of Vyerpanas places it within the outer edge of its star's habitable zone. This means that while liquid water could potentially exist on its surface, conditions might be colder than on Earth due to the lower luminosity of its red dwarf host star. The planet's year is significantly longer than Earth's, taking approximately 130 Earth days to complete one orbit around Kepler-186.

Due to the dimness of the red dwarf star, Vyerpanas would likely receive less visible light than Earth. However, the specific spectrum of light emitted by a red dwarf might influence the types of life, if any, that could evolve there. Further research is required to determine the presence of an atmosphere, its composition, and the potential for Vyerpanas to harbor life. Its discovery highlights the growing number of exoplanets being found in habitable zones around stars other than our Sun.