望远镜
主镜像
光学
有源光学
自适应光学
米
物理
第一道亮光
反射望远镜
构造(python库)
光学望远镜
遥感
天文
计算机科学
地质学
光源
程序设计语言
作者
E. C. Stone,Michael Bolte
出处
期刊:Current Science
[Indian Academy of Sciences]
日期:2017-08-25
卷期号:113 (04): 628-628
被引量:2
标识
DOI:10.18520/cs/v113/i04/628-630
摘要
The Thirty-Meter Telescope (TMT) project is a welladvanced
effort to construct one of the first of the next
generation of extremely large telescopes with primary
mirror diameter larger than 25 m. When used with an
adaptive optics systems capable of producing diffraction-
limited images, the science reach of a 30 m telescope is extraordinary with improvements in sensitivity over existing telescopes by as much as a factor of 80 for some kinds of observations. The TMT design extends that of the twin Keck 10 m telescopes now in operation and uses the same close-packed segmented primary mirror. The partnership that will finish the design, construct and operate the telescope is described.
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