Emärtämed

Emärtämed is a fictional celestial body located in the Kepler-186 system, approximately 500 light-years away from Earth. It is the fourth planet orbiting the M-class red dwarf star Kepler-186, and is known for its potential habitability. Discovered by the Kepler Space Telescope, Emärtämed resides within the habitable zone of its star, meaning conditions could be suitable for liquid water to exist on its surface.

The planet is estimated to be roughly Earth-sized, with a radius of approximately 1.1 times that of Earth. Its mass is not precisely known, but it is believed to be rocky, similar to terrestrial planets in our solar system. Emärtämed's orbital period is approximately 130 Earth days. Due to its star being a red dwarf, Emärtämed likely receives a different spectrum of light compared to Earth, and might be tidally locked, presenting one side perpetually facing its star.

The potential for an atmosphere and surface water on Emärtämed remains a subject of ongoing scientific inquiry. While its position in the habitable zone is promising, factors such as atmospheric composition, geological activity, and the star's activity levels would play crucial roles in determining its actual habitability. Further observations and analysis are required to understand the complex environmental conditions on Emärtämed and its potential to harbor life.