跳到主要导航 跳到搜索 跳到主要内容

Review of research on lunar dust dynamics

  • Kun Yang
  • , Weiming Feng*
  • , Luyuan Xu
  • , Xiaodong Liu*
  • *此作品的通讯作者
  • Shandong University
  • Macau University of Science and Technology
  • CNSA Macau Center for Space Exploration and Science
  • Sun Yat-Sen University

科研成果: 期刊稿件文献综述同行评审

摘要

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.

源语言英语
文章编号67
期刊Astrophysics and Space Science
367
7
DOI
出版状态已出版 - 7月 2022
已对外发布

学术指纹

探究 'Review of research on lunar dust dynamics' 的科研主题。它们共同构成独一无二的学术指纹。

引用此