This is a double-lined spectroscopic binary system with an orbital period of nearly two days in a circular orbit. It is classified as a rotating ellipsoidal variable star and its brightness varies by 0.02 magnitudes with a period of 23.57 hours, which equals half of its orbital period.
This is a double-lined spectroscopic binary system with an orbital period of nearly two days in a circular orbit. It is categorized as a rotating ellipsoidal variable star and its brightness fluctuates by 0.02 magnitudes with a period of 23.57 hours, which corresponds to half of its orbital period.