Gamma Corvi is a star located in the constellation Corvus, which is known as the Crow. It is classified as a B-type main-sequence star, meaning it is hotter and more massive than our Sun. Gamma Corvi is approximately 165 light-years away from Earth and has a brightness that makes it one of the more prominent stars in its constellation. This star has a surface temperature of around 15,000 Kelvin, giving it a bluish hue. Gamma Corvi is also known for its rapid rotation, completing a full spin in just a few days. Its characteristics make it an interesting object of study for astronomers.