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X-ray diffractometer studies of shocked materialsThis study explores the utility of X-ray diffractometer scans for determination of shock pressure histories of geological materials from meteorite impact sites. The technique is based on quantification of increased crystal lattice disorder with increasing shock pressure as expressed by decreasing diffraction peak amplitude and pronounced line-broadening caused by decreasing mosaic domain size and increasing strain. The ratio of peak height (PH) to half width (HW) decreases systematically with increasing shock pressure. Data are given for experimentally shocked quartz, feldspars, pyroxene and olivine along with data for granitic materials from the Piledriver nuclear event and from the Ries Crater, Germany. Although the technique in principle may be capable of yielding relatively accurate pressure determinations, its application to naturally shocked materials may be severely limited.
Document ID
19790055237
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Hanss, R. E.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Montague, B. R.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Davis, M. K.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Galindo, C.
(St. Mary's University San Antonio, Tex., United States)
Hoerz, F.
(NASA Johnson Space Center Houston, Tex., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1978
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Start Date: March 13, 1978
End Date: March 17, 1978
Accession Number
79A39250
Funding Number(s)
CONTRACT_GRANT: NSG-9039
Distribution Limits
Public
Copyright
Other

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