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Vista Variables in the Via Lactea : ウィキペディア英語版 | Vista Variables in the Via Lactea
== ''The VVV Survey'' == VISTA Variables in the Via Lactea (The VVV Survey) is an astronomical survey to map the Milky Way's bulge and a disk area close to the center of the galaxy. It uses the capabilities of the VISTA telescope at the VLT site in Paranal, Chile, to make observations in 5 bands in the near infrared. The survey started in February 2010 and will be completed in 2015.
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「Vista Variables in the Via Lactea」の詳細全文を読む
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