Qlähdettä

Qlähdettä is a fictional celestial body located within the Kepler-186 system. Its designation, Kepler-186f, places it as the fifth and outermost known planet orbiting the red dwarf star Kepler-186. Discovered by NASA's Kepler Space Telescope, Qlähdettä gained significant attention due to its location within the habitable zone of its star. This means the planet receives an amount of stellar radiation that could potentially allow liquid water to exist on its surface, a key ingredient for life as we understand it.

The planet is estimated to be roughly 1.1 times the size of Earth, suggesting it is a terrestrial, or rocky, planet. Its orbital period is approximately 130 Earth days. While its size and habitable zone location are promising indicators for potential habitability, many factors remain unknown. These include its atmospheric composition, the presence of a magnetic field, and the actual existence of surface water. Further observations and analysis are required to determine the true nature of Qlähdettä and its potential to harbor life. The discovery of Qlähdettä is a significant step in the ongoing search for exoplanets that could potentially support life beyond Earth.