Lunar dust is regarded as the most crucial environmental problem on the Moon, and related research has crucially important scientific and technological interests. Here, we first reported the in situ measurements of lunar dust at the Chang'E-3 landing site in the northern Mare Imbrium using temperature-controlled sticky quartz crystal microbalance. The results showed that a total deposition mass at a height of 190 cm above the lunar surface during 12 lunar daytimes in the northern Mare Imbrium was about 0.0065 mg/cm(2), corresponding to an annual deposition rate of similar to 21.4 mu g/cm(2), which is comparable with that of Apollo's result to some extent. The present researches are strategically important for future human and robotic lunar expeditions, and can provide a valuable reference for the design of dust protection for onboard payloads long-term exposure to the lunar environment.
Publication name |
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS Volume: 124 Issue: 8 Pages: 2168-2177 DOI: 10.1029/2019JE006054 Published: AUG 2019 |
Author(s) |
Li, Detian; Wang, Yi; Zhang, He; Zhuang, Jianhong; Wang, Xiaojun; Wang, Yongjun; Yang, Shengsheng; Sun, Zezhou; Wang, Xianrong; Chen, Liping; Yao, Rijian; Zou, Xin; Ma, Jinan; Cui, Yang; Wang, Xilai; Li, Cunhui; Zhang, Haiyan; Li, Xiongyao; Gao, Xin; Cui, Xinyu; Zhang, Biao; Li, Wenfeng; Lin, Hongyu |
Corresponding author(s) |
LI Detian lidetian@hotmail.com -China Acad Space Technol, Sci & Technol Vacuum Technol & Phys Lab, Lanzhou Inst Phys, Lanzhou, Peoples R China. ZHUANG Jianhong zhuangjianhong@spacechina.com -China Acad Space Technol, Lanzhou Inst Phys, Sci & Technol Mat Performance Evaluating Space En, Lanzhou, Peoples R China. |
Author(s) from IGCAS |
Li Xiongyao | View here for the details
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