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Impactite and pseudotachylite from Roter Kamm Crater, NamibiaPseudotachylite is known to occur in a variety of geologic settings including thrust belts (e.g., the Alps and the Himalayas) and impact craters such as Roter Kamm, Namibia. Controversy exists, however, as to whether pseudotachylite can be produced by shock brecciation as well as by tectonic frictional melting. Also open to debate is the question of whether pseudotachylites form by frictional fusion or by cataclasis. It was speculated that the pseudotachylite at Roter Kamm was formed by extensional settling and adjustment of basement blocks during 'late modification stage' of impact. The occurrence of pseudotachylite in association with rocks resembling quenched glass bombs and melt breccias in a relatively young crater of known impact origin offers a rare opportunity to compare features of these materials. Petrographic, x-ray diffraction, and electron microprobe analyses of the impactites and pseudotachylites are being employed to determine the modes of deformation and to assess the role of frictional melting and comminution of adjacent target rocks.
Document ID
19930000942
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Degenhardt, J. J., Jr.
(Texaco, Inc. Houston, TX., United States)
Buchanan, P. C.
(Houston Univ. TX, United States)
Reid, A. M.
(Houston Univ. TX, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: Lunar and Planetary Inst., International Conference on Large Meteorite Impacts and Planetary Evolution
Subject Category
Geophysics
Accession Number
93N10130
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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