APOLLO 11: SOIL MECHANICS RESULTS

DATA WERE EXTRACTED FROM ASTRONAUT OBSERVATIONS, TELEVISION COVERAGE OF THE MOON WALK, AND RETURNED PHOTOGRAPHS AND SAMPLES. IT HAS BEEN DETERMINED THAT THE UPPER FEW CENTIMETERS OF THE LUNAR SOIL IN THE VICINITY OF TRANQUILLITY BASE ARE CHARACTERIZED BY A BROWNISH, MEDIUM-GRAY, SLIGHTLY COHESIVE GRANULAR SOIL COMPOSED LARGELY OF BULKY GRAINS IN THE SILT-TO-FINE-SAND SIZE RANGE, WITH ANGULAR TO SUBROUNDED ROCK FRAGMENTS RANGING UP TO 1 M IN SIZE DISTRIBUTED THROUGHOUT THE AREA. THE LUNAR SURFACE AT THIS SITE IS SOFT TO DEPTHS OF 5 CM TO 20 CM, BELOW WHICH THE RESISTANCE TO PENETRATION INCREASES CONSIDERABLY. ALTHOUGH THE SOIL DIFFERS CONSIDERABLY IN COMPOSITION AND RANGE OF PARTICLE SHAPES FROM A TERRESTRIAL SOIL OF THE SAME PARTICLE SIZE DISTRIBUTION, IT DOES NOT APPEAR TO DIFFER SIGNIFICANTLY IN ITS MECHANICAL BEHAVIOR. THE SOIL, WHILE BASICALLY FRICTIONAL IN BEHAVIOR, EXHIBITS A SMALL AMOUNT OF COHESION AND STRONG ADHESIVE PROPERTIES. PRELIMINARY ESTIMATES OF THE IN SITU SOIL DENSITY GAVE A VALUE OF 1.6 G PER CU CM. /AUTHOR/

  • Supplemental Notes:
    • Vol 96, No SM6, PROC PAPER NO 7704 PP 2045-2080, 7 FIG,
  • Authors:
    • Costes, N C
    • Carrier, W D
    • Mitchell, J K
    • Scott, R F
  • Publication Date: 1970-11

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Filing Info

  • Accession Number: 00237934
  • Record Type: Publication
  • Files: TRIS
  • Created Date: May 3 1971 12:00AM