The lunar dust environment: concerns for Moon-based astronomy

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)’.

Astronomy from the Moon: the next decades (part 2)

“…Perhaps the most worrying obstacle to developing lunar telescopes is the abrasive dust that pervades the lunar environment. Mihaly Horanyi [ 11 ] (University of Colorado) describes some of these challenges. The meteoroid flux near the poles needs to be evaluated as does the role of electrostatic levitation of dust and deposition in dark craters where telescopes may be sited.…”