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Apollo 11 Soil Mechanics Investigation

Costes, N. C. and Carrier, W. D. and Mitchell, J. K. and Scott, R. F. (1970) Apollo 11 Soil Mechanics Investigation. Science, 167 (3918). pp. 739-741. ISSN 0036-8075. https://resolver.caltech.edu/CaltechAUTHORS:20150211-104950108

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Abstract

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.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1126/science.167.3918.739DOIArticle
http://www.sciencemag.org/content/167/3918/739PublisherArticle
http://www.jstor.org/stable/1728832JSTORArticle
Additional Information:© 1970 American Association for the Advancement of Science. 7 January 1970.
Issue or Number:3918
Record Number:CaltechAUTHORS:20150211-104950108
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150211-104950108
Official Citation:Costes, N. C., Carrier, W. D., Mitchell, J. K., & Scott, R. F. (1970). Apollo 11 Soil Mechanics Investigation. Science, 167(3918), 739-741. doi: 10.1126/science.167.3918.739
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:54717
Collection:CaltechAUTHORS
Deposited By: Joanne McCole
Deposited On:11 Feb 2015 19:56
Last Modified:03 Oct 2019 08:00

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