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contributor authorHoward A. Perko
contributor authorJohn D. Nelson
contributor authorWilly Z. Sadeh
date accessioned2017-05-08T21:27:13Z
date available2017-05-08T21:27:13Z
date copyrightApril 2001
date issued2001
identifier other%28asce%291090-0241%282001%29127%3A4%28371%29.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/52033
description abstractLunar soil consists of dry silty sand. Observations and measurements conducted during Surveyor, Apollo, and Luna missions indicated that the lunar soil is unusually cohesive. This is attributable to the fact that thick layers of adsorbed gases, which coat and lubricate soil particles on Earth, are absent in the ultrahigh vacuum on the Moon. “Surface cleanliness” is introduced as a new parameter for describing soils in different planetary environments. It is defined as the dimensionless inverse of adsorbate thickness on solid surfaces. By this definition, the ultrahigh vacuum on the Moon is associated with high surface cleanliness, while Earth's atmosphere is associated with low surface cleanliness. A model is developed to calculate surface cleanliness and its effect on shear strength in any planetary environment. Results obtained from the model compare well with data from previous ultrahigh vacuum and variable temperature laboratory experiments on Earth soils. It is shown that surface cleanliness is an important parameter with respect to lunar soil shear strength.
publisherAmerican Society of Civil Engineers
titleSurface Cleanliness Effect on Lunar Soil Shear Strength
typeJournal Paper
journal volume127
journal issue4
journal titleJournal of Geotechnical and Geoenvironmental Engineering
identifier doi10.1061/(ASCE)1090-0241(2001)127:4(371)
treeJournal of Geotechnical and Geoenvironmental Engineering:;2001:;Volume ( 127 ):;issue: 004
contenttypeFulltext


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