Английская Википедия:Alpha Lupi

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Шаблон:Short description Шаблон:Starbox begin Шаблон:Starbox image Шаблон:Starbox observe Шаблон:Starbox character Шаблон:Starbox astrometry Шаблон:Starbox detail Шаблон:Starbox catalog Шаблон:Starbox reference Шаблон:Starbox end Alpha Lupi (α Lupi, α Lup) is a blue giant star, and the brightest star in the southern constellation of Lupus. According to the Bortle Dark-Sky Scale, its apparent visual magnitude of 2.3[1] makes it readily visible to the naked eye even from highly light-polluted locales. Based upon parallax measurements made during the Hipparcos mission,[2] the star is around Шаблон:Convert from the solar system.[3] It is one of the nearest supernova candidates.[4]

Characteristics

Файл:AlphaLupLightCurve.png
A light curve for Alpha Lupi, plotted from Hipparcos data[5]

Alpha Lupi is a giant star with a stellar classification of B1.5 III.[6] It has about ten times the mass of the sun (~Шаблон:Solar mass)[7] yet is radiating 25,000 times the Sun's luminosity.[8] The outer atmosphere has an effective temperature of 21,820 K,[9] 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,[10] which means it undergoes periodic changes in luminosity because of pulsations in the atmosphere. The variability period is 0.29585 days,[11] or just over 7 hours, 6 minutes. The magnitude varies by about 0.05 magnitudes, or about 5% of its brightness. A 14th magnitude star situated 26" from Alpha Lupi is listed as a companion in double star catalogues.[12]

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.[8] 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.[13]

Visibility

Visible from the Southern Hemisphere for much of the year, it can also be viewed for a shorter season from the northern tropics and from parts of the northern subtropical latitudes.

Nomenclature

α Lupi (Latinised to Alpha Lupi) is the star's Bayer designation.

In Chinese, Kekouan Шаблон:Lang (Шаблон:Lang), 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.[14] Consequently, the Chinese name for α Lupi itself is Шаблон:Lang (Шаблон:Lang, Шаблон:Lang-en.).[15]

R. H. Allen described this star as having the Chinese name Yang Mun or Men(南門), meaning "the South Gate", in his work Star-Names and their Meanings.[16] In Chinese astronomy, 南門 is located in Horn mansion and consisted of α and ε Centauri. It was referred to as Yang Mun, meaning "the south Gate". Allen also suggested that the Babylonian name for the star was "Kakkab Su-gub Gud-Elim" (Star Left Hand of the Horned Bull).[16]

References

Шаблон:Reflist

Шаблон:Stars of Lupus

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