Kepler 69c is an Exoplanets

Kepler-69c is an exoplanet located approximately 2,700 light-years away from Earth in the constellation Cygnus. It was discovered by NASA's Kepler spacecraft and confirmed as an exoplanet in 2013.

Kepler-69c is considered a "super-Earth" due to its size, with an estimated diameter around 1.7 times that of Earth. It orbits its host star, Kepler-69, at a distance that places it within the star's habitable zone, where conditions may be suitable for liquid water to exist on its surface.

The planet has a relatively long orbital period, completing one orbit around its star in about 242 Earth days. Its distance from its host star, along with the composition of its atmosphere and other factors, contribute to its overall climate and potential habitability.

While Kepler-69c's mass and composition are not precisely known, its size suggests that it could have a rocky or a combination of rocky and gaseous composition.

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