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Apollo 14 active seismic experiment.Explosion seismic refraction data indicate that the lunar near-surface rocks at the Apollo 14 site consist of a regolith 8.5 meters thick and characterized by a compressional wave velocity of 104 meters per second. The regolith is underlain by a layer with a compressional wave velocity of 299 meters per second. The thickness of this layer, which we interpret to be the Fra Mauro Formation, is between 16 and 76 meters. The layer immediately beneath this has a velocity greater than 370 meters per second. We found no evidence of permafrost.
Document ID
19720039829
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Watkins, J. S.
(North Carolina, University Chapel Hill, N.C., United States)
Kovach, R. L.
(Stanford University Stanford, Calif., United States)
Date Acquired
August 6, 2013
Publication Date
March 17, 1972
Publication Information
Publication: Science
Volume: 175
Subject Category
Space Sciences
Accession Number
72A23495
Funding Number(s)
CONTRACT_GRANT: NAS9-5632
Distribution Limits
Public
Copyright
Other

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