阿波罗
地质学
土力学
地球科学
天体生物学
土壤科学
物理
生物
土壤水分
生态学
作者
N. C. Costes,W. D. Carrier,J. K. Mitchell,Ronald F. Scott
出处
期刊:Science
[American Association for the Advancement of Science]
日期:1970-01-30
卷期号:167 (3918): 739-741
被引量:64
标识
DOI:10.1126/science.167.3918.739
摘要
The fine-grained surface material at the Apollo 11 landing site is a brownish, medium-gray, slightly cohesive granular soil, with bulky grains in the silt-to-fine-sand range, having a specific gravity of 3.1 and exhibiting adhesive characteristics. Within the upper few centimeters, the lunar soil has an average density of about 1.6 grams per cubic centimeter and is similar in appearance and behavior to the soils studied at the Surveyor equatorial landing sites. Although considerably different in composition and in range of particle shapes, it is similar in its mechanical behavior to terrestrial soils of the same grain size distribution.
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