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・ Alpha Octantis
・ Alpha Omega (album)
・ Alpha Omega (Cheek album)
・ Alpha Omega Alpha
・ Alpha Omega Epsilon
・ Alpha Omega Fraternity
・ Alpha Omicron Pi
・ Alpha operon ribosome binding site
・ Alpha Ophiuchi
・ Alpha Oumar Barry
・ Alpha Oumar Konaré
・ Alpha oxidation
・ Alpha particle
・ Alpha particle X-ray spectrometer
・ Alpha Pavonis
Alpha Coronae Australis
・ Alpha Coronae Borealis
・ Alpha Corvi
・ Alpha course
・ Alpha Crateris
・ Alpha Crucis
・ Alpha Crucis (research vessel)
・ Alpha Cygni variable
・ Alpha Data
・ Alpha decay
・ Alpha defensin
・ Alpha Delphini
・ Alpha Delta
・ Alpha Delta Chi
・ Alpha Delta Gamma


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Alpha Coronae Australis : ウィキペディア英語版
Alpha Coronae Australis


Alpha Coronae Australis (α CrA, α Coronae Australis) is a star in the constellation Corona Australis. It is the only star in the constellation with a proper name, Alphekka Meridiana (Alphekka South), after the brightest star in Corona Borealis, Alphecca. In Chinese astronomy, it is known as 鱉六 (the Sixth Star of the River Turtle). It is a Class A star like Vega, rotating extremely fast on its axis, close to its breakup velocity.
== Properties ==

Alpha Coronae Australis belongs to the spectral class A2Va and has apparent magnitude +4.10.〔 Located about 125 light years from Earth, the star's mass and radius are estimated at 2.3 times solar. With an effective temperature of roughly 9,100 K, the star radiates a total luminosity of about 31 times solar.〔 This star is roughly 254 million years old.〔 A rapidly rotating star, it spins at almost 200 km per second at the equator, making a complete revolution in approximately 14 hours.〔 Like the star Vega, it has excess infrared radiation, which indicates it may be ringed by a disk of dust.〔

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「Alpha Coronae Australis」の詳細全文を読む



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