Ntöbblet

Ntöbblet is a fictional planet located in the Kepler-186 system. It is the fifth planet from its star, Kepler-186f, and orbits within the habitable zone. This means that conditions on Ntöbblet might be suitable for liquid water to exist on its surface, a key ingredient for life as we know it.

The planet is believed to be roughly Earth-sized, with an estimated radius of 1.1 times that of Earth. Its mass is also thought to be comparable to Earth's, suggesting a rocky composition. Ntöbblet's orbital period is approximately 130 Earth days. Due to its distance from its star, a red dwarf, Ntöbblet likely receives less light than Earth does from the Sun. However, if it possesses a sufficiently dense atmosphere, it could trap enough heat to maintain a temperate climate.

The presence of Ntöbblet was first detected by the Kepler Space Telescope, which uses the transit method to discover exoplanets. Subsequent observations have helped refine estimates of its size and orbital characteristics. While direct imaging of Ntöbblet is not yet possible with current technology, its location within the habitable zone has made it a subject of considerable scientific interest in the search for extraterrestrial life. Further study is needed to understand its atmospheric composition and potential for habitability.