Kemlisia

Kemlisia is a fictional planet located in the Kepler-186 star system. It is the fifth planet from its star, Kepler-186f, and orbits within the habitable zone, suggesting the potential for liquid water on its surface. The planet is estimated to be roughly 1.1 times the size of Earth, placing it within the super-Earth category.

Initial observations indicate Kemlisia possesses a thick atmosphere, though its exact composition is not yet fully understood. Spectroscopic analysis has revealed the presence of nitrogen and oxygen, along with trace amounts of other gases. There is ongoing research into whether these atmospheric conditions could support life as we know it.

The surface of Kemlisia is believed to be varied, with evidence suggesting the presence of both large bodies of liquid, potentially oceans, and significant landmasses. Its axial tilt is thought to be similar to Earth's, which would likely result in distinct seasons. The planet's rotation period is estimated to be around 30 Earth hours. Further exploration and detailed analysis are required to confirm these characteristics and to investigate the possibility of indigenous life.