天体生物学
月球土壤
纹理(宇宙学)
扫描电子显微镜
纵横比(航空)
材料科学
表征(材料科学)
矿物学
地质学
复合材料
纳米技术
物理
计算机科学
图像(数学)
人工智能
作者
Yang Liu,Jae‐Sung Park,D. W. Schnare,Eddy Hill,L. A. Taylor
出处
期刊:Journal of Aerospace Engineering
[American Society of Civil Engineers]
日期:2008-09-15
卷期号:21 (4): 272-279
被引量:86
标识
DOI:10.1061/(asce)0893-1321(2008)21:4(272)
摘要
The morphology (shape and texture) of dust fractions of five Apollo lunar soils and a lunar dust simulant, JSC-1Avf, was studied using scanning electron microscopy. Shape (aspect ratio and complexity) of particles was described based on the two-dimensional projection images. The distributions of aspect ratio and complexity of particles are reported. It was determined that the Apollo lunar dust particles consist mainly of impact-produced glass, with complicated morphologies, extensive surface areas per grain, and sharp, jagged edges. Importantly, many grains contain elaborate vesicular textures, representing minute agglutinates. Dust simulant JSC-1Avf also has similar shapes as lunar dust, but differs in surface texture and area (smooth and nonvesicular). These data provide information for toxicity studies of lunar dust and for selecting a suitable lunar dust simulant.
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