K2-72b

K2-72b is an exoplanet orbiting the red dwarf star K2-72, located approximately 227 light-years away in the constellation Aquarius. Discovered by NASA's Kepler spacecraft during its K2 mission, it is notable for its potentially rocky composition and position within the habitable zone of its star.

K2-72b has a radius approximately 1.3 times that of Earth. While its exact mass is not precisely known, estimates suggest it is likely more massive than Earth. Due to its size and proximity to its star, it is considered a super-Earth.

The exoplanet orbits K2-72 at a relatively close distance, completing one orbit in about 24 Earth days. This places K2-72b within the habitable zone, meaning it could potentially have liquid water on its surface, depending on its atmospheric properties. However, orbiting a red dwarf presents challenges for habitability, including the possibility of strong stellar flares and tidal locking, where one side of the planet always faces the star.

Further observations and studies are needed to determine the precise composition and atmospheric characteristics of K2-72b, which will help scientists better understand its potential for harboring life.