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Tau1 Aquarii : ウィキペディア英語版 | Tau1 Aquarii
Tau1 Aquarii (τ1 Aqr, τ1 Aquarii) is the Bayer designation for a star in the equatorial constellation of Aquarius. With an apparent visual magnitude of 5.66,〔 it is a faint naked eye that requires dark suburban skies for viewing. Parallax measurements made during the Hipparcos mission yield a distance estimate of roughly from Earth.〔 τ1 Aquarii has a stellar classification of B9 V;〔 right along the borderline between a B- and A-type main sequence star. It is around 100〔 million years old and has twice the Sun's radius.〔 When examined in the infrared band, it displays an excess emission that is a characteristic of stars with an orbiting debris disk. Indeed, the model that best fits the data suggests there are two concentric circumstellar disks.〔 ==References==
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「Tau1 Aquarii」の詳細全文を読む
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