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Soil mechanical properties at the Apollo 14 site

Mitchell, James K. and Bromwell, Leslie G. and Carrier, W. David, III and Costes, Nicholas C. and Scott, Ronald F. (1972) Soil mechanical properties at the Apollo 14 site. Journal of Geophysical Research, 77 (29). pp. 5641-5664. ISSN 0148-0227. http://resolver.caltech.edu/CaltechAUTHORS:20141106-164832874

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Abstract

The Apollo 14 lunar landing provided a greater amount of information on the mechanical properties of the lunar soil than previous missions because of the greater area around the landing site that was explored and because a simple penetrometer device, a special soil mechanics trench, and the modularized equipment transporter (Met) provided data of a type not previously available. The characteristics of the soil at shallow depths varied more than anticipated in both lateral and vertical directions. While blowing dust caused less visibility impairment during landing than on previous missions, analysis shows that eroded particles were distributed over a large area around the final touchdown point. Measurements on core-tube samples and the results of transporter track analyses indicate that the average density of the soil in the Fra Mauro region is in the range of 1.45 to 1.60 g/cm^3. The soil strength appears to be higher in the vicinity of the site of the Apollo 14 lunar surface experiments package, and trench data suggest that strength increases with depth. Lower-bound estimates of soil cohesion give values of 0.03 to 0.10 kN/m^2, which are lower than values of 0.35 to 0.70 kN/m^2 estimated for soils encountered in previous missions. The in situ modulus of elasticity, deduced from the measured seismic-wave velocity, is compatible with that to be expected for a terrestrial silty fine sand in the lunar gravitational field.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1029/JB077i029p05641DOIArticle
http://onlinelibrary.wiley.com/doi/10.1029/JB077i029p05641/abstractPublisherArticle
Additional Information:Copyright 1972 by the American Geophysical Union. (Received December 10, 1971; revised June 15, 1972.) Professor W. N. Houston, Dr. H. J. Hovland, and H. T. Durgunoglu assisted in simulation studies and data analyses at the University of California, Berkeley. Dr. Stewart W. Johnson, Richard A. Werner, and Ralf Schmitt participated in phases of the work carried out at the Manned Spacecraft Center, Houston. G. T. Cohron assisted in the transporter-track analyses, which were done at the Marshall Space Flight Center, Huntsville, Ala. The assistance of these individuals is gratefully acknowledged. The studies reported herein were supported, in part, by NASA contract NAS 9-11266, principal investigator support for soil mechanics experiment (S-200), and NASA contract NAS 9-11454, co-investigator support for soil mechanics experiment (S-200).
Funders:
Funding AgencyGrant Number
NASANAS 9-11266
NASANAS 9-11454
Subject Keywords:Engineering Geology; Moon; Soils
Record Number:CaltechAUTHORS:20141106-164832874
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20141106-164832874
Official Citation:Mitchell, J. K., L. G. Bromwell, W. D. Carrier III, N. C. Costes, and R. F. Scott (1972), Soil mechanical properties at the Apollo 14 site, J. Geophys. Res., 77(29), 5641–5664, doi:10.1029/JB077i029p05641.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:51409
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:07 Nov 2014 16:10
Last Modified:13 Feb 2019 18:06

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