A 600 m 2 array of 6.5 m telescopes at the lunar pole

Author:

Angel Roger12ORCID

Affiliation:

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

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

Abstract

The proposed lunar telescope for optical and infrared astronomy aims at very large aperture, 600 m 2 , 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 z  = 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 2 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)’.

Funder

College of Science, University of Arizona

Publisher

The Royal Society

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Astronomy from the Moon: the next decades (part 2);Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences;2024-03-25

2. Astronomy from the moon in the next decades: from exoplanets to cosmology in visible light and beyond;Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences;2024-03-25

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