Plánetunnis

Plánetunnis is a celestial body located in the Kepler-186 solar system, approximately 500 light-years from Earth. It is the fifth and outermost known planet orbiting the red dwarf star Kepler-186. Discovered by the Kepler Space Telescope, Plánetunnis has garnered interest due to its potential for harboring liquid water, a key ingredient for life as we know it.

The planet resides within the habitable zone of its star, meaning the temperature range on its surface could allow for liquid water to exist. However, its exact surface conditions remain largely unknown. Plánetunnis is believed to be a rocky planet, similar in size to Earth, although its mass and composition are still subjects of ongoing research. Its orbital period is approximately 130 Earth days.

Due to the dim nature of its host star, Kepler-186, Plánetunnis receives less stellar radiation than Earth does from the Sun. This could lead to a cooler climate, but atmospheric composition, if any, would significantly influence its temperature. Scientists are actively analyzing data from various telescopes to learn more about Plánetunnis's atmosphere, potential geological activity, and the possibility of it being a habitable world. Further observations are required to confirm its characteristics and assess its potential for supporting life.