The lunar dust environment: concerns for Moon-based astronomy.

Philos Trans A Math Phys Eng Sci

Laboratory for Atmospheric and Space Physics, and Department of Physics, University of Colorado, Boulder, CO, USA.

Published: May 2024

AI Article Synopsis

  • The Moon's lack of atmosphere makes it an ideal location for telescopes, especially radio telescopes, due to minimal interference from Earth.
  • Despite this advantage, the Moon's surface is constantly hit by interplanetary dust, damaging structures and altering the lunar regolith.
  • Additional concerns arise from human activities on the Moon, such as rocket launches and movement, which generate more dust and pose risks to sensitive astronomical equipment.

Article Abstract

The Moon has no atmosphere, hence, it offers a unique opportunity to place telescopes on its surface for astronomical observations. It is phase-locked with Earth, and its far side remains free from ground-based interference, enabling the optimal use of radio telescopes. However, the surface of the Moon, as any other airless planetary object in the solar system, is continually bombarded by interplanetary dust particles that cause impact damage and generate secondary ejecta particles that continually overturn the top layer of the lunar regolith. In addition, there is evidence, that small particles comprising the lunar regolith can be electrically charged, mobilized and transported, also representing a hazard for covering sensitive surfaces and interfering with exposed mechanical structures. In addition to the naturally occurring dust transport, rocket firings during landings and take-offs, pedestrian and motorized vehicle traffic will also liberate copious amounts of dust, representing a potential hazard for the safe and optimal use of optical platforms. This article is part of a discussion meeting issue 'Astronomy from the Moon: the next decades (part 2)'.

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Source
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC10961187PMC
http://dx.doi.org/10.1098/rsta.2023.0075DOI Listing

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