Alpha Canum Venaticorum, also known as Ain, is a binary star system located in the constellation Canes Venatici. It is approximately 81 light-years away from Earth and is one of the brightest stars in its constellation. Ain consists of two stars, a primary giant star and a secondary companion, which orbit each other. The primary star, classified as a G-type giant, is significantly larger and more luminous than our Sun. The system is notable for its relatively close proximity to Earth and its visibility to the naked eye, making it a popular target for amateur astronomers and stargazers.