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位于月球极地的由6.5米望远镜组成的600米阵列。

A 600 m array of 6.5 m telescopes at the lunar pole.

作者信息

Angel Roger

机构信息

Steward Observatory, University of Arizona, Tucson, AZ, USA.

Department of Optical Sciences, University of Arizona, Tucson, AZ, USA.

出版信息

Philos Trans A Math Phys Eng Sci. 2024 May 9;382(2271):20230076. doi: 10.1098/rsta.2023.0076. Epub 2024 Mar 25.

Abstract

The proposed lunar telescope for optical and infrared astronomy aims at very large aperture, 600 m, at a fundable cost. It comprises an array of 18 separate telescopes, each of 6.5 m aperture. The 200 m diameter array will be located within 1/2° (15 km) of a lunar pole on approximately level ground, with a perimeter screen deployed to provide shade and cooling to cryogenic temperature. The 500 m diameter screen will allow unobscured access down to 8° elevation. All 18 telescopes will reflect light into a central beam combiner to form a single image covering wavelengths from 0.4 µm to 10 µm. The initial instrument complement will include high-resolution and multi-object spectrographs to exploit the single combined field of view of two arcminute diameter, with the diffraction limited resolution of 6.5 m aperture. Scientific applications include the search for molecular biosignatures in transiting exoplanets, and the study of galaxy evolution using red-shifted spectra to beyond  = 10. The array cost, including delivery to the Moon by SpaceX Starship for installation using lunar base infrastructure, is around $10 billion, similar to that of the 25 m JWST. To test the concept, first a single prototype 6.5 m unit would be operated at the lunar south pole. This article is part of a discussion meeting issue 'Astronomy from the Moon: the next decades (part 2)'.

摘要

提议用于光学和红外天文学的月球望远镜旨在以可承受的成本实现600米的超大口径。它由18个独立的望远镜阵列组成,每个望远镜的口径为6.5米。直径200米的阵列将位于月球极点附近约1/2°(15公里)范围内的大致平坦地面上,并部署一个周边屏幕,为低温设备提供遮阳和冷却,使其达到低温状态。直径500米的屏幕将允许无障碍观测低至8°仰角的区域。所有18台望远镜将把光线反射到一个中央光束合成器中,以形成一个覆盖0.4微米至10微米波长的单一图像。初始仪器配置将包括高分辨率和多目标光谱仪,以利用两弧分直径的单一组合视场,其衍射极限分辨率为6.5米口径。科学应用包括在凌日系外行星中寻找分子生物特征,以及利用红移光谱研究星系演化,直至红移  = 10以上。该阵列的成本,包括由SpaceX星际飞船运送到月球并使用月球基地基础设施进行安装,约为100亿美元,与25米口径的詹姆斯·韦伯太空望远镜(JWST)的成本相似。为了测试该概念,首先将在月球南极运行一个6.5米的单一原型单元。本文是一次研讨会“月球天文学:未来几十年(第二部分)”的一部分。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/a6c6/10961182/a6c3d184c3bb/rsta20230076f01.jpg

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