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Chin. Phys. B, 2022, Vol. 31(4): 045201    DOI: 10.1088/1674-1056/ac2e61
PHYSICS OF GASES, PLASMAS, AND ELECTRIC DISCHARGES Prev   Next  

Distribution of charged lunar dust in the south polar region of the moon

Qing Xia(夏清)1, Ming-Hui Cai(蔡明辉)1,2,†, Liang-Liang Xu(许亮亮)1, Rui-Long Han(韩瑞龙)1,2, Tao Yang(杨涛)1, and Jian-Wei Han(韩建伟)1,2
1 National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China;
2 School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, China
Abstract  Lunar dust is one of the most threatening problems confronting the return of human beings to the moon. In this work we studied the spatial distribution behavior of charged lunar dust in the solar wind plasma environment in the south polar region of the moon and considered the influence of a mini-crater using Spacecraft Plasma Interactions Software. The distribution of dust and plasma at low solar altitude angles of 20° and 0° was studied, and the spatial density of lunar dust was ~1010.4 m-3 and ~1011.5 m-3, respectively. This is because a higher surface potential will result in transportation of small dust particles and photoelectrons can also neutralize positively charged lunar dust. The dust density in the plasma void region created by a mini-crater with a 5 m high wall was studied. We obtained a quasi-neutral electric environment in the plasma void region of the mini-crater, and the dust density was about a magnitude lower than that in other regions. The dust risk to a spacesuit is much lower on the nightside than on the dayside, but there is severe charged lunar dust transport in the region between light and shade, which is dominated by the difference in surface and plasma potential caused by photoelectrons.
Keywords:  lunar dust      south polar region      solar wind      mini-crater  
Received:  02 July 2021      Revised:  26 August 2021      Accepted manuscript online:  11 October 2021
PACS:  52.27.Lw (Dusty or complex plasmas; plasma crystals)  
Fund: Project supported by the National Key Research and Development Program of China (Grant No. 2020YFC2201300), the Strategic Priority Research Program of Chinese Academy of Sciences (Grant No. XDA17010301), and the Technical Basic Scientific Research Project (Grant No. JSZL2019903B001).
Corresponding Authors:  Ming-Hui Cai     E-mail:  caiminghui@nssc.ac.cn

Cite this article: 

Qing Xia(夏清), Ming-Hui Cai(蔡明辉), Liang-Liang Xu(许亮亮), Rui-Long Han(韩瑞龙), Tao Yang(杨涛), and Jian-Wei Han(韩建伟) Distribution of charged lunar dust in the south polar region of the moon 2022 Chin. Phys. B 31 045201

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