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Lunar ash flows.Softened appearance of certain large lunar craters explained by ash flow theory
Document ID
19660056161
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Okeefe, J. A.
Date Acquired
August 3, 2013
Publication Date
January 1, 1966
Subject Category
Space Sciences
Accession Number
66A35451
Distribution Limits
Public
Copyright
Other
Keywords
LUNAR CRATER
SURFACE EROSION

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