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Updated: Jun 30, 2025

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在月球极点的600米2的6.5米望远镜阵列
Roger Angel1,2
1Steward Observatory, University of Arizona, Tucson, AZ, USA.
概括
一个拟议的18个望远镜的月球望远镜阵列为光学和红外天文学提供600平方米的光圈. 这种具有成本效益的设计旨在寻找系外行星生物特征并研究星系进化.
科学领域:
- 天文学和天体物理学
- 光学和红外天文学
- 月球科学 月球科学
背景情况:
- 目前的天文天文台面临着光圈大小和成本的限制.
- 月球为先进的天文观测提供了一个稳定的平台,具有最小的大气层.
研究的目的:
- 提出一个具有非常大的光圈 (600 m2) 的具有成本效益的月球望远镜阵列,用于光学和红外天文学.
- 为了实现突破性的科学研究,包括系外行星生物特征检测和深层银河系进化研究.
主要方法:
- 一系列18个单独的6.5米孔径望远镜将在月球极附近部署.
- 一个周边屏幕将为望远镜提供阴影和冷冷却.
- 来自所有望远镜的光线将被组合在一起,形成一个用于分析的单一图像.
主要成果:
- 该阵列将达到600 m2的总收集面积.
- 该系统将覆盖从0.4μm到10μm的波长,分辨率有限.
- 最初的仪器将包括高分辨率和多物体光谱仪.
结论:
- 拟议的月球望远镜阵列提供了一种可行和可靠的方法,以实现天文学领域的极大光圈.
- 这个月球观测台有可能彻底改变我们对系外行星和早期宇宙的理解.
- 一个6.5米望远镜的原型将在月球南极进行测试,以验证这一概念.
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