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Preliminary geologic investigation of the Apollo 17 landing siteA geological investigation of the Apollo 17 lunar landing site was conducted. The Taurus-Littrow valley is interpreted as a deep graben formed by structural adjustment of lunar crustal material to the Serenitatis impact. Materials of the valley fill were sampled at many stations. Ejecta around many craters on the valley floor consist of basalt, showing that the graben was partly filled by lava flows. The geological objectives of the Apollo 17 mission are divided into orbital and lunar surface data collection. The data obtained for both types of investigation are presented in tables, photographs, and drawings.
Document ID
19740010323
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Muehlberger, W. R.
(Tex. Univ. Austin, United States)
Batson, R. M.
(Geological Survey Washington, DC, United States)
Cernan, E. A.
(NASA Johnson Space Center Washington, DC, United States)
Freeman, V. L.
(Geological Survey Washington, DC, United States)
Hait, M. H.
(Geological Survey Washington, DC, United States)
Holt, H. E.
(Geological Survey Washington, DC, United States)
Howard, K. A.
(Geological Survey Washington, DC, United States)
Jackson, E. D.
(Geological Survey Washington, DC, United States)
Larson, K. B.
(Geological Survey Washington, DC, United States)
Reed, V. S.
(Geological Survey)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Publication Information
Publication: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.
Subject Category
Space Sciences
Accession Number
74N18436
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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