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Transport and emplacement of crater and basin depositsMaterial is ejected from impact craters in ballastic trajectories; it impacts first near the crater rim and then at progressively greater ranges. Ejecta from craters smaller than approximately 1 km are laid predominantly on top of the surrounding surface. With increasing crater size, more and more surrounding surface will be penetrated by secondary cratering action, and these preexisting materials will be mixed with primary crater ejecta. Ejecta from large craters, and especially basin-forming events, not only excavate preexisting local materials, but also are capable of moving large amounts of material away from the crater. Thus mixing and lateral transport give rise to continuous deposits that contain materials from within and outside the primary crater. As a consequence, ejecta of basins and large highland craters have eroded and mixed highland materials throughout geologic time and deposited them in depressions inside and between older crater structures.
Document ID
19750061675
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Oberbeck, V. R.
(NASA Ames Research Center Moffett Field, Calif., United States)
Morrison, R. H.
(LFE Corp. Moffett Field, Calif., United States)
Hoerz, F.
(NASA Johnson Space Center Houston, Tex., United States)
Date Acquired
August 8, 2013
Publication Date
July 1, 1975
Subject Category
Lunar And Planetary Exploration
Accession Number
75A45747
Distribution Limits
Public
Copyright
Other

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