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High-explosive cratering analogs for bowl-shaped, central uplift, and multiring impact cratersThe paper describes six experimental explosion craters in terms of their basic morphology, subsurface structural deformation, and surrounding ejecta blanket. These craters exhibit one or more of the following features: bowl shapes with underlying breccia lens, central uplifts, multirings, terraced walls, rim strata, zones of concentric rim deformation, inner continuous ground cover of ejecta blankets formed by overturned flaps, secondary cratering, and fused alluvium. These craters were formed by large shock wave energy transfers at or near zero heights-of-burst, and it is possible that impact craters with analogous morphologic and structural features may have formed under similar surface energy transfer conditions.
Document ID
19770051970
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Roddy, D. J.
(U.S. Geological Survey Flagstaff, Ariz., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1976
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 15, 1976
End Date: March 19, 1976
Accession Number
77A34822
Funding Number(s)
CONTRACT_GRANT: NASA ORDER W-13130
Distribution Limits
Public
Copyright
Other

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