Micro-X-ray diffraction assessment of shock stage in enstatite chondrites

Matthew Richar Izawa, Roberta L. Flemming, Neil R. Banerjee, Philip J.A. Mccausland

Research output: Contribution to journalArticle

13 Citations (Scopus)

Abstract

A new method for assessing the shock stage of enstatite chondrites has been developed, using in situ micro-X-ray diffraction (μXRD) to measure the full width at half maximum (FWHMχ) of peak intensity distributed along the direction of the Debye rings, or chi angle (χ), corresponding to individual lattice reflections in two-dimensional XRD patterns. This μXRD technique differs from previous XRD shock characterization methods: it does not require single crystals or powders. In situ μXRD has been applied to polished thin sections and whole-rock meteorite samples. Three frequently observed orthoenstatite reflections were measured: (020), (610), and (131); these were selected as they did not overlap with diffraction lines from other phases. Enstatite chondrites are commonly fine grained, stained or darkened by weathering, shock-induced oxidation, and metal/sulfide inclusions; furthermore, most E chondrites have little olivine or plagioclase. These characteristics inhibit transmitted-light petrography, nevertheless, shock stages have been assigned MacAlpine Hills (MAC) 02837 (EL3) S3, Pecora Escarpment (PCA) 91020 (EL3) S5, MAC 02747 (EL4) S4, Thiel Mountains (TIL) 91714 (EL5) S2, Allan Hills (ALHA) 81021 (EL6) S2, Elephant Moraine (EET) 87746 (EH3) S3, Meteorite Hills (MET) 00783 (EH4) S4, EET 96135 (EH4-5) S2, Lewis Cliff (LEW) 88180 (EH5) S2, Queen Alexandra Range (QUE) 94204 (EH7) S2, LaPaz Icefield (LAP) 02225 (EH impact melt) S1; for the six with published shock stages, there is agreement with the published classification. FWHMχ plotted against petrographic shock stage demonstrates positive linear correlation. FWHMχ ranges corresponding to shock stages were assigned as follows: S1<0.7°, S2=0.7-1.2°, S3=1.2-2.3°, S4=2.3-3.5°, S5>3.5°, S6-not measured. Slabs of Abee (EH impact-melt breccia), and Northwest Africa (NWA) 2212 (EL6) were examined using μXRD alone; FWHMχ values place both in the S2 range, consistent with literature values. Micro-XRD analysis may be applicable to other shocked orthopyroxene-bearing rocks.

Original languageEnglish
Pages (from-to)638-651
Number of pages14
JournalMeteoritics and Planetary Science
Volume46
Issue number5
DOIs
Publication statusPublished - May 2011
Externally publishedYes

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enstatite chondrite
enstatite
chondrites
shock
X-ray diffraction
diffraction
x rays
impact melts
elephant
meteorites
moraine
meteorite
melt
Allan Hills meteorite
rocks
petrography
cliffs
escarpments
breccia
weathering

ASJC Scopus subject areas

  • Geophysics
  • Space and Planetary Science

Cite this

Micro-X-ray diffraction assessment of shock stage in enstatite chondrites. / Richar Izawa, Matthew; Flemming, Roberta L.; Banerjee, Neil R.; Mccausland, Philip J.A.

In: Meteoritics and Planetary Science, Vol. 46, No. 5, 05.2011, p. 638-651.

Research output: Contribution to journalArticle

Richar Izawa, Matthew ; Flemming, Roberta L. ; Banerjee, Neil R. ; Mccausland, Philip J.A. / Micro-X-ray diffraction assessment of shock stage in enstatite chondrites. In: Meteoritics and Planetary Science. 2011 ; Vol. 46, No. 5. pp. 638-651.
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