Alpha Lupi


Alpha Lupi is the brightest star in the southern constellation of Lupus. According to the Bortle Dark-Sky Scale, its apparent visual magnitude of 2.3 makes it readily visible to the naked eye even from highly light-polluted locales. Based upon parallax measurements made during the Hipparcos mission, the star is around from the solar system. It is one of the nearest soon supernova candidates, and is the brightest star without a pre-Bayer designation western classical/arabic world name, ranking 75 places below the sun.

Characteristics

Alpha Lupi is a giant star with a stellar classification of B1.5 III. It has about ten times the mass of the sun yet is radiating 25,000 times the Sun's luminosity. The outer atmosphere has an effective temperature of 21,820 K, which gives it the blue-white glow of a B-type star. In 1956 it was identified as a Beta Cephei variable by Bernard Pagel and colleagues, which means it undergoes periodic changes in luminosity because of pulsations in the atmosphere. The variability period is 0.29585 days, or just over 7 hours, 6 minutes. The magnitude varies by about 0.05, or about 5% of the total luminosity. A 14th magnitude star situated 26" from Alpha Lupi is listed as a companion in double star catalogues.
This star is a proper motion member of the Upper-Centaurus Lupus sub-group in the Scorpius-Centaurus OB association, the nearest such co-moving association of massive stars to the Sun. This is a gravitationally unbound stellar association with an estimated age of 16–20 million years. The association is also the source of a bubble of hot gas that contains the Sun, known as the Local Bubble.

Regions from which visible

Apart from the Southern Hemisphere for much of the year, it can be viewed for a shorter season from the northern tropics and from parts of the northern subtropical latitudes; it lies beyond much of the rest of its asterism, in turn south of Libra.

Etymology

In Chinese, Kekouan 騎官, meaning Imperial Guards, refers to an asterism consisting of α Lupi, γ Lupi, δ Lupi, κ Centauri, β Lupi, λ Lupi, ε Lupi, μ Lup, π Lupi, and ο Lupi. Consequently, the Chinese name for α Lupi itself is 騎官十.
R. H. Allen described this star as having the Chinese name Yang Mun or Men（南門), meaning "the South Gate", in his work . In Chinese astronomy, 南門 is located in Horn mansion and consisted of α and ε Centauri. Yang Mun was translated in Pinyin as 陽門, meaning "the Yang Gate", and refers to the asterism in Neck mansion, containing stars from the modern constellation Centaurus. Allen also suggested that the Babylonian name for the star was "Kakkab Su-gub Gud-Elim".