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・ Epsilon Pegasi
・ Epsilon Persei
・ Epsilon Phoenicis
・ Epsilon photography
・ Epsilon Pi Tau
・ Epsilon Piscis Austrini
・ Epsilon Piscium
・ Epsilon Pyxidis
・ Epsilon radiation
・ Epsilon Reticuli
・ Epsilon Reticuli b
・ Epsilon Sagittae
・ Epsilon Sagittarii
・ Epsilon Scorpii
・ Epsilon Sculptoris
Epsilon Scuti
・ Epsilon Serpentis
・ Epsilon Sextantis
・ Epsilon Sigma Alpha
・ Epsilon Tau Pi
・ Epsilon Tauri
・ Epsilon Tauri b
・ Epsilon Telescopii
・ Epsilon transition
・ Epsilon Trianguli
・ Epsilon Trianguli Australis
・ Epsilon Tucanae
・ Epsilon TV
・ Epsilon Ursae Majoris
・ Epsilon Ursae Minoris


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Epsilon Scuti : ウィキペディア英語版
Epsilon Scuti

Epsilon Scuti (ε Sct, ε Scuti) is a star system in the constellation Scutum. It is approximately 523 light years from Earth.
The primary component, Epsilon Scuti A, is a yellow G-type bright giant with an apparent magnitude of +4.88. It has at least three faint companions, two 14th magnitude stars, B and D, separated from the primary by 13.6 and 15.4 arcseconds respectively, and the 13th magnitude C, which is 38 arcseconds away.
Epsilon Scuti was a latter designation of 3 Aquilae.
==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「Epsilon Scuti」の詳細全文を読む



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