Almelia

Almelia is a fictional planet located in the Kepler-186 star system. It is the fifth planet from its star, Kepler-186f, and resides within the habitable zone. This means that Almelia is theoretically capable of supporting liquid water on its surface, a key ingredient for life as we know it.

The planet is believed to be rocky and terrestrial, similar in composition to Earth. Its diameter is estimated to be roughly 1.1 times that of Earth, suggesting a slightly larger gravitational pull. Almelia's atmosphere is a subject of ongoing scientific speculation. While its exact composition is unknown, it is hypothesized to be dense enough to retain heat and shield the surface from harmful radiation from its host star.

The Kepler-186 star is a red dwarf, meaning it is smaller and cooler than our Sun. This affects Almelia's illumination, with the planet likely receiving less light than Earth. The color of the sky on Almelia is also debated, with some models suggesting it could be a pale orange or even reddish hue due to the red dwarf's light spectrum.

Due to its distance from Earth, direct observation of Almelia is currently limited. Much of what is known or theorized about the planet comes from data gathered by space telescopes such as Kepler and its successor, TESS. Future missions aim to provide more detailed information about Almelia's surface conditions, atmospheric makeup, and potential for extraterrestrial life.