The primary component of this system is a variable star of the Beta Cephei type with a period of just 3h 22m. It has nearly nine times the mass of the Sun and more than six times the Sun's radius.
At its heart lies a variable star of the Beta Cephei type, known for its brief orbital cycle of around 3 hours and 22 minutes. This massive celestial body has a mass roughly nine times that of the Sun and a diameter greater than six times that of our solar system's central star.