T217 How Old, How Long, and How Fast: Establishing the Timing, Duration, and Rates of Mid- to Lower-Crustal Deformation
Tuesday, 24 September 2019
1:30 PM - 5:30 PM
Room 229B, North Building
TITANITE U-PB PETROCHRONOLOGY REVEALS ~26 MILLION YEARS OF DEFORMATION IN A MID-CRUSTAL HIGH-TEMPERATURE SHEAR ZONE
Paper number: T217-4
Program: Technical Sessions
Time: 2:15 PM – 2:30 PM
Authors
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Mark SchmitzBoise State University, Boise, ID
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Maureen KahnUniversity of Wisconsin-Madison, Madison, WI
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Basil TikoffUniversity of Wisconsin-Madison, Madison, WI
Abstract
We dated zircon and titanite using a sequential textural characterization, in situ analysis, microsampling, and isotope dilution petrochronology workflow for plutons within the WISZ and inboard of the arc-continent transition. Zircon ages, a proxy for magmatism, range from 105.23 ± 0.12 Ma to 82.50 ± 0.08 Ma. Ages for recrystallized and neoblastic titanite, a proxy for fabric development during deformation, range from 103.30 ± 0.26 Ma to 77.34 ± 0.65 Ma. Some peaks in the probability density function of titanite ages correlate with peaks in the probability density function of zircon ages, suggesting that titanite records localized zones of increased strain resulting from adjacent pluton intrusion. However, most titanite ages lag and/or are uncorrelated with zircon ages, suggesting that titanite also records ongoing strain accumulation in the shear zone. Overall, activity in the WISZ lasted ~26 million years, with multiple episodes of magmatism and changes in rates of deformation.
Our results reveal that deformation in the WISZ does not consistently migrate eastward with time, contrary to previous models. Rather, the locus of deformation moves back and forth across a 15 km wide shear zone, which is at least partially controlled by magmatism. This study illustrates how titanite and zircon petrochronology can parse the spatial-temporal patterns of fabric development within high-temperature shear zones.
Geological Society of America Abstracts with Programs. Vol. 51, No. 5
doi: 10.1130/abs/2019AM-340946
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