Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/106937
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Type: Journal article
Title: Constraining the timing of shale detachment faulting: a geochemical approach
Author: Hansberry, R.
Zwingmann, H.
Loehr, S.
Collins, A.
King, R.
Morley, C.
Drysdale, R.
Citation: Lithosphere, 2017; 9(3):431-440
Publisher: Geological Society of America
Issue Date: 2017
ISSN: 1941-8264
1947-4253
Statement of
Responsibility: 
Rowan L. Hansberry, Horst Zwingmann, Stefan Loehr, Alan S. Collins, Rosalind C. King, Christopher K. Morley, and Russell N. Drysdale
Abstract: K-Ar dating of illite in fault gouges is a useful tool for constraining the timing of brittle fault movement; however, this can be problematic in fault gouges hosted in clay-rich rocks due to the influence of host-rock material. Therefore, this study employs a multianalytical geochemical approach to unravel the influence of host-rock mineralogy, as well as fault zone development, on ages from fault-gouge samples in a shale detachment zone. K-Ar dating of the ≥2 μm fraction of 6 samples from the Sap Bon Formation detachment zone and associated fault zones in the Khao Khwang fold-thrust belt of central Thailand yielded an age range of 262 ± 5.4 to 208 ± 4.6 Ma. Carbon and oxygen stable isotope analysis along with X-ray diffraction mineralogy indicate that the samples with the youngest K-Ar ages are characterized by higher grade clay mineralogy, and hotter, orogenic fluid temperatures. Using these proxies and comparison to existing geochronology of the study area, we correlated K-Ar illite ages to one of three stages of fault zone evolution: detrital, diagenetic (burial), and authigenic (fault movement). The youngest K-Ar dates in the Sap Bon Formation are contemporaneous with recently published zircon province data indicating that faulting and detachment zone formation in the Sap Bon Formation were occurring by the mid-Late Triassic, with deformation continuing as late as the Rhaetian.
Rights: © 2017 Geological Society of America For permission to copy, contact editing@geosociety.org
RMID: 0030071313
DOI: 10.1130/L612.1
Grant ID: http://purl.org/au-research/grants/arc/FT120100340
http://purl.org/au-research/grants/arc/DP120101460
Appears in Collections:Geology & Geophysics publications

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