T27 Rates in Metamorphism and Tectonism: From Mineral Growth to Orogenesis
Sunday, 25 September 2016
8:00 AM - 12:00 PM
Mile High Ballroom 3B
ALLEGHANIAN-AGED HIGH-TEMPERATURE DEFORMATION CONDITIONS ASSOCIATED WITH FORMATION OF THE TALLULAH FALLS DOME, NORTHEASTERN GEORGIA
Paper number: T27-13
Program: Technical Sessions
Time: 11:05 AM – 11:20 AM
Authors
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Gabriele CasaleAppalachian State University, Boone, WA
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Jeffrey RahlWashington and Lee University, Lexington, VA
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Taylor D. CraigAppalachian State University, Boone, NC
Abstract
We have determined deformation conditions across the TFD based on both microstructural analysis and crystallographic preferred orientation of quartz using electron backscatter diffraction. All analyzed samples preserve quartz grains elongated parallel to the well-developed dome-defining foliation. In general, quartz grains are coarse, commonly forming ribbons with aspect ratios of up to 5:1, and preserve amoeboid grain boundaries and pinned micas characteristic of high-temperature grain boundary migration. The majority of our samples also display well-developed chessboard extinction, a texture consistent with the alpha-beta transition in quartz and deformation temperatures exceeding 650° C at moderate pressures. Quartz crystallographic preferred orientation patterns show large opening angles consistent with deformation at uppermost amphibolite-facies to granulite-facies conditions.
Regional isoclinal folding that predates and is interrupted by the TFD foliation has a maximum age of 335 Ma, as determined by the crystallization age of the deformed Rabun granite.40Ar/39Ar data from muscovite inside the dome record ages of 312 Ma. These age constraints indicate that rocks inside the dome cooled from the conditions we observe in deformation fabrics (>650 °C) to 340 °C in approximately 20 m.y. These timing constraints support previous interpretations that doming is Alleghanian rather than Neoacadian, but suggest substantially higher temperature (upper amphibolite-granulite-facies) conditions than previously suggested during this younger orogeny.
Geological Society of America Abstracts with Programs. Vol. 48, No. 7
doi: 10.1130/abs/2016AM-286683
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