Vetewia

Vetewia is a fictional planet located in the Kepler-186 star system, approximately 500 light-years from Earth. It is the fifth and outermost known planet in its system, orbiting a red dwarf star. Vetewia is classified as a terrestrial planet and is believed to be within its star's habitable zone, meaning conditions might be suitable for liquid water to exist on its surface.

The planet's diameter is estimated to be about 1.2 times that of Earth, and its mass is thought to be slightly greater. Due to its orbit around a dimmer red dwarf star, Vetewia receives less light than Earth, resulting in a cooler overall climate. Scientists hypothesize that the planet may possess a thicker atmosphere, which could help trap heat and maintain a more stable temperature.

Initial observations suggest that Vetewia has a rocky composition, similar to other terrestrial planets in our solar system. Evidence points towards the presence of a substantial atmosphere, though its exact composition is not yet known. Further research is required to determine if Vetewia harbors any form of life or possesses other significant geological features. Its discovery is part of ongoing efforts to find exoplanets that could potentially support life beyond Earth.