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Preliminary stratigraphy of the Apollo 15 drill coreThe crew of Apollo 15 collected a 242-cm-long core of the regolith developed on the surface of Palus Putredinus (3 deg 39 min 20 sec E, 26 deg 26 min 00 sec N). This core consists of 42 major textural units, which range from a few millimeters to 13 cm thick. The regolith at this site was deposited layer by layer, each layer having been reworked, to some degree, by micrometeorite bombardment. The particle composition of six layers for which samples were obtained varies in a random fashion, thus supporting the heterogeneous, layered model of the regolith. The ratio of lithic fragments derived from the Apennine Front to that derived from the mare surface is about 1:1. This lithic ratio, in a regolith section 3.75 km from the base of the front, is an indication of the efficiency of lateral transport of soil by impact processes and mass wasting.
Document ID
19740040069
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Heiken, G.
Duke, M.
Mckay, D. S.
Clanton, U. S.
(NASA Johnson Space Center Houston, Tex., United States)
Fryxell, R.
(Washington State University Pullman, Wash., United States)
Nagle, J. S.
(Northrop Services, Inc. Houston, Tex., United States)
Scott, R.
(California Institute of Technology Pasadena, Calif., United States)
Sellers, G. A.
(U.S. Geological Survey Washington, D.C., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Subject Category
Space Sciences
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 5, 1973
End Date: March 8, 1973
Accession Number
74A22819
Distribution Limits
Public
Copyright
Other

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