Gamma Cephei B
Gamma Cephei B is a star located in the constellation Cepheus, approximately 45 light-years away from Earth. It is part of a binary system, orbiting around its companion star, Gamma Cephei A. This system is notable for its relatively close proximity to our solar system.
Gamma Cephei B is classified as a K-type main-sequence star, which means it is cooler and less luminous than our Sun. It has a lower mass and temperature, making it an interesting object for astronomers studying stellar evolution and the characteristics of different types of stars in the universe.