Pi Aquarii


Pi Aquarii, Latinized from π Aquarii, is the Bayer designation for a binary star in the equatorial constellation of Aquarius. This system has an apparent visual magnitude of a mean apparent magnitude of +4.57. Based upon parallax measurements, it is located at a distance of roughly from Earth.
This is a binary star system with an orbital period of 84.1 days. The primary component is a B1 giant or subgiant star. This is a large star with nearly eleven times the mass and over six times the radius of the Sun. Pi Aquarii shines about 7,300 times as brightly as the Sun. This energy is being radiated from its outer atmosphere at an effective temperature of 27,094, giving it the blue-hued glow of a B-type star. It is spinning rapidly with a projected rotational velocity of 215 km/s.
Pi Aquarii is notable for having undergone a transition from a Be star into an ordinary B-type star. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +4.45 to +4.71; a range of 0.28. The dominant variability period,, is nearly the same as the orbital period. Pi Aquarii has a reasonable chance of becoming a supernova some day.

In culture

Pi Aquarii was called Seat by Grotius in the 17th century, but the name has rarely been used since.
In Chinese, 墳墓, meaning Tomb, refers to an asterism consisting of π Aquarii, γ Aquarii, ζ Aquarii, η Aquarii. Consequently, the Chinese name for π Aquarii itself is 墳墓四
In the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Wasat al Achbiya, which was translated into Latin as Media Tabernaculorum, meaning the middle of luck of the homes . This star, along with γ Aqr, ζ Aqr and η Aqr, were al Aḣbiyah, the Tent.