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Review of research on lunar dust dynamics

  • Kun Yang
  • , Weiming Feng*
  • , Luyuan Xu
  • , Xiaodong Liu*
  • *Corresponding author for this work
  • Shandong University
  • Macau University of Science and Technology
  • CNSA Macau Center for Space Exploration and Science
  • Sun Yat-Sen University

Research output: Contribution to journalReview articlepeer-review

Abstract

Lunar dust particles are generated by hypervelocity impacts of interplanetary micrometer meteoroids onto the surface of the Moon, which seriously threatens the security of explorations. Studying the lunar dust dynamics helps to understand the origin and migration mechanism of lunar dust, and to provide the theoretical guidelines for the orbital design of lunar space missions. This paper reviews previous research on the lunar dust dynamics, including the interplanetary impactor environment of the Earth–Moon system, the mass production rate, the initial mass, speed and ejecta angle distributions, the related space exploration missions, the dynamical model, and spatial distribution of dust particles originating from the lunar surface in the whole Earth–Moon system.

Original languageEnglish
Article number67
JournalAstrophysics and Space Science
Volume367
Issue number7
DOIs
StatePublished - Jul 2022
Externally publishedYes

Keywords

  • Celestial mechanics
  • Moon
  • Planets and satellites: rings
  • Zodiacal dust

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