Gamma Velorum is a binary star system located in the constellation Vela, which is part of the larger Argo Navis constellation. It is approximately 80 light-years away from Earth and consists of two stars: Gamma Velorum A, a bright blue giant, and Gamma Velorum B, a smaller companion star. The system is known for its brightness and is often used in astronomical studies. The primary star, Gamma Velorum A, is classified as a B-type star, indicating it is hot and luminous. It has a surface temperature of around 25,000 Kelvin, making it much hotter than our Sun. The system is also notable for its rapid rotation and strong stellar winds, contributing to its dynamic nature.