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contributor authorChristos Vrettos
date accessioned2017-05-08T21:47:27Z
date available2017-05-08T21:47:27Z
date copyrightApril 2012
date issued2012
identifier other%28asce%29gt%2E1943-5606%2E0000635.pdf
identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/62415
description abstractA class of granular materials is presented that was obtained from quarried intrusive igneous rock, further processed to match the grain-size distribution of typical Apollo samples. Texture, mineralogy, and chemical composition have been investigated; and the material is classified as basaltic andesite. A series of triaxial compression tests have been performed to assess the influence of confining stress on the shearing behavior at medium to low stress levels. A medium sand is used as reference. In one of the test series, corundum was added to simulate the glass particles found in the lunar regolith. Both stress-strain curves and volumetric strains are reported. All samples tested exhibit a purely dilatant behavior at low confining stress levels. Shear strength can be expressed either by a curved Mohr-Coulomb envelope or by a linear one with a cohesion intercept. Results are shown to agree well with those obtained on common lunar soil simulants.
publisherAmerican Society of Civil Engineers
titleShear Strength Investigations for a Class of Extraterrestrial Analogue Soils
typeJournal Paper
journal volume138
journal issue4
journal titleJournal of Geotechnical and Geoenvironmental Engineering
identifier doi10.1061/(ASCE)GT.1943-5606.0000619
treeJournal of Geotechnical and Geoenvironmental Engineering:;2012:;Volume ( 138 ):;issue: 004
contenttypeFulltext


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