description Kepler-1649c Overview
Kepler-1649c is an exoplanet roughly Earth-sized orbiting a red dwarf star named Kepler-1649. Its location within its star’s habitable zone—the region where liquid water could exist on the surface—makes it notable. Scientists study this super-Earth to assess the potential for habitability around M-dwarf stars and understand planetary formation processes. The planet is of interest to researchers investigating Earth analogs beyond our solar system.
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