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Unravelling Complex Geologic Histories Using U–Pb and Trace Element Systematics of TitaniteUnravelling the spatio-temporal evolution of orogenic terranes requires a comprehensive understanding of the duration and extent of metamorphic events and hydrothermal alteration. Commonly used minerals such as zircon and monazite may not fully record geological histories in complex tectonic settings because their elemental constituents do not react under many metamorphic and metasomatic conditions. Here, we complement the current geochronological record of the Capricorn Orogen, Western Australia, with titanite U–Pb geochronology and geochemistry of felsic intrusive rocks to draw conclusions about the use of titanite in understanding the evolution of orogenic terranes. Because titanite usually incorporates common-Pb and may be variably reset by multiple metamorphic and hydrothermal events, a workflow is provided here for the systematic and robust interpretation of titanite U-Pb data. The addition of trace element data in titanite is particularly effective for differentiating whether a grain is igneous, recrystallized or metamorphic. We have developed several petrogenetic indices to differentiate these three types of titanite using Zr-in-titanite temperature, Th/U, Th/Pb, Al/(Al + Fe), light to heavy rare earth element ratio, and Eu anomalies. The addition of trace element geochemistry can also highlight anomalously radiogenic (sup 207)Pb/(sup 206)Pb reservoirs. Utilization of our workflow in the Capricorn Orogen reveals that titanite ages from the same samples as published zircon U–Pb data range from coeval to several hundreds of Myr of age difference between the two minerals. Titanite geochronology and trace element geochemistry indicates ~20 Myr of previously unrecognized prolonged cooling for the Capricorn Orogeny to ca. 1750 Ma. The spatial extent of the ca. 1210–1170 Ma part of the Mutherbukin Tectonic Event is also broadened significantly farther north and south than previously recognized. Incorporating titanite geochronology and trace geochemistry with more commonly used techniques (e.g., zircon and monazite petrochronology) extends our ability to resolve the complete history of large-scale orogenic terranes.
Document ID
20190002202
Acquisition Source
Johnson Space Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
Hugo K. H. Olierook
(Curtin University Perth, Western Australia, Australia)
Richard J. M. Taylor
(University of Cambridge Cambridge, United Kingdom)
Timmons M Erickson
(Jacobs (United States) Dallas, Texas, United States)
Chris Clark
(Curtin University Perth, Western Australia, Australia)
Steven M. Reddy
(Curtin University Perth, Western Australia, Australia)
Christopher L. Kirkland
(Curtin University Perth, Western Australia, Australia)
Inalee Jahn
(Curtin University Perth, Western Australia, Australia)
Milo Barham
(Curtin University Perth, Western Australia, Australia)
Date Acquired
April 5, 2019
Publication Date
January 20, 2019
Publication Information
Publication: Chemical Geology
Publisher: Elsevier
Volume: 504
Issue Publication Date: January 20, 2019
ISSN: 0009-2541
Subject Category
Geophysics
Report/Patent Number
JSC-E-DAA-TN64249
ISSN: 0009-2541
Report Number: JSC-E-DAA-TN64249
Funding Number(s)
CONTRACT_GRANT: UAP-RP04-063
CONTRACT_GRANT: NNJ13HA01C
Distribution Limits
Public
Copyright
Public Use Permitted.
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