Premium
Weak Dust Activity Near a Geologically Young Surface Revealed by Chang'E‐3 Mission
Author(s) -
Yan Qi,
Zhang Xiaoping,
Xie Lianghai,
Guo Dawei,
Li Yong,
Xu Yi,
Xiao Zhiyong,
Di Kaichang,
Xiao Long
Publication year - 2019
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2019gl083611
Subject(s) - regolith , astrobiology , geology , deposition (geology) , earth science , geomorphology , physics , sediment
In spite of great scientific and engineering interests in lunar exploration, natural dust activity near the Moon surface remains unclear. According to distinct reflectance features of lunar rocks and regolith observed by Chang'E‐3 mission, long‐term dust activity near a young surface is quantified with a new method. We found that a dust deposition upper line on rocks is about 28 cm above the ground. Below this line, the quantity of dust deposits becomes smaller as the altitude ascends, whereas above the line, no visible or only negligible amount of dust is distributed on the rocks. This dust distribution pattern could be explained by dust electrostatic levitation process. The results indicate distinctively weak long‐term dust activity near the young surface and suggest possible selection of geologically young regions as landing sites or lunar bases to minimize the effect of dust grains.