Unravelling 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 Pb-207/Pb-206 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 similar to 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.
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CUNY Queens Coll, Sch Earth & Environm Sci, 6530 Kissena Blvd, Flushing, NY 11367 USA
Amer Museum Nat Hist, Dept Earth & Planetary Sci, New York, NY 10024 USACUNY Queens Coll, Sch Earth & Environm Sci, 6530 Kissena Blvd, Flushing, NY 11367 USA
Marsh, Jeffrey H.
Smye, Andrew J.
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Penn State Univ, Dept Geosci, 332 Deike Bldg, University Pk, PA 16802 USACUNY Queens Coll, Sch Earth & Environm Sci, 6530 Kissena Blvd, Flushing, NY 11367 USA
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Univ Lyon 1, ENS Lyon, LGL TPE, CNRS UMR, F-5276 Villeurbanne, FranceUniv Arizona, Dept Geosci, Tucson, AZ 85721 USA
Triantafyllou, Antoine
Ducea, Mihai N.
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Univ Arizona, Dept Geosci, Tucson, AZ 85721 USA
Univ Bucharest, Fac Geol & Geophys, Bucharest 010040, RomaniaUniv Arizona, Dept Geosci, Tucson, AZ 85721 USA
Ducea, Mihai N.
Jepson, Gilby
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Univ Arizona, Dept Geosci, Tucson, AZ 85721 USA
Univ Oklahoma, Sch Geosci, Norman, OK 73019 USAUniv Arizona, Dept Geosci, Tucson, AZ 85721 USA
Jepson, Gilby
McClelland, William
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Univ Iowa, Dept Earth & Environm Sci, Iowa City, IA 52242 USAUniv Arizona, Dept Geosci, Tucson, AZ 85721 USA
McClelland, William
Giesler, Dominique
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Univ Arizona, Dept Geosci, Tucson, AZ 85721 USAUniv Arizona, Dept Geosci, Tucson, AZ 85721 USA
Giesler, Dominique
Gehrels, George E.
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Univ Arizona, Dept Geosci, Tucson, AZ 85721 USAUniv Arizona, Dept Geosci, Tucson, AZ 85721 USA
Gehrels, George E.
Fellah, Clementine
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Univ Lyon 1, ENS Lyon, LGL TPE, CNRS UMR, F-5276 Villeurbanne, FranceUniv Arizona, Dept Geosci, Tucson, AZ 85721 USA