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Influence of Deformation and Fluids on Ti Exchange in Natural Quartz

  • Michel Bestmann (Corresponding author)
  • , Giorgio Pennacchioni
  • , Bernhard Grasemann
  • , Benjamin Huet
  • , Michael W.M. Jones
  • , Cameron M. Kewish

Publications: Contribution to journalArticlePeer Reviewed

Abstract

Using a combination of microstructural, spectroscopic, and geochemical analyses, we investigate how subgrain rotation recrystallization and fluid migration affect Ti concentration [Ti] in naturally deformed quartz veins from the Prijakt Nappe (Austroalpine Unit, Eastern Alps). These coarse-grained quartz veins, that formed at amphibolite facies conditions, were overprinted by lower greenschist facies deformation to different degrees. During the overprint, subgrain rotation recrystallization was dominant during progressive deformation to ultramylonitic stages. The initial [Ti] (3.0–4.7 ppm) and cathodoluminescence (CL) signature of the vein crystals decrease during deformation mainly depending on the availability of fluids across the microstructure. The amount of strain played a subordinate role in resetting to lower [Ti] and corresponding darker CL shades. Using a microstructurally controlled analysis we find that the most complete re-equilibration in recrystallized aggregates ([Ti] of 0.2–0.6 p.m.) occurred (a) in strain shadows around quartz porphyroclasts, acting as fluid sinks, and (b) in localized microshear zones that channelized fluid percolation. [Ti] resetting is mainly observed along wetted high angle boundaries (misorientation angle >10–15°), with partial [Ti] resetting observed along dry low angle boundaries (<10–15°). This study shows for the first time that pure subgrain rotation recrystallization in combination with dissolution-precipitation under retrograde condition provide microstructural domains suitable for the application of titanium-in-quartz geothermobarometry at deformation temperatures down to 300–350°C.
Original languageEnglish
Article numbere2021JB022548
Number of pages26
JournalJournal of Geophysical Research: Solid Earth
Volume126
Issue number12
DOIs
Publication statusPublished - Dec 2021

Funding

This work was funded by the Deutsche Forschungsgemeinschaft DFG (BE 2413/3-1). GP acknowledge funding from the University of Padova (BIRD175145/17). Access to the SEM-EBSD facilities was provided by the Department of Werkstoffwissenschaften WW1, FAU Erlangen-N?rnberg, Germany. The Oxford Instruments CMOS-Symmetry EBSD detector was funded by the DFG (JA 2718/3-1). Jay Thomas is thanked for providing the synthetic Ti-doped quartz standard (QTiP-38, Ti 380 ppm), Djordje Grujic for the natural standard (TN-06, 0.3 ppm) and Steven Kidder for the Herkimer ?Diamond? used as a Ti blank. Cees-Jan De Hoog is thanked for conducting SIMS measurements and processing at the School of Geosciences of the University of Edinburgh. We acknowledge Holger St?nitz for discussion and providing access to the SEM-CL spectra facilities at the Department of Geosciences at the Arctic University of Norway (Troms?), and Amicia Lee and Tom-Ivar Eilertsen for their assistance. Christoph E. Schrank and Nicholas W. Phillips are thanked for their contribution with respect to the synchrotron data set. Part of this research was undertaken on the XFM beamline at the Australian Synchrotron, part of ANSTO. Rene Romer is thanked for support during electron microprobe analysis (chlorite thermometry) and Friederike Urban and Raphael Njul for sample preparation. Alexis Plunder is thanked for the chlorite thermometry blind test. We are grateful for constructive reviews of Steve Kidder and Leif Tokle and the assessment of an anonymous associated editor of JGR-Solid Earth. Open access funding enabled and organized by Projekt DEAL. This work was funded by the Deutsche Forschungsgemeinschaft DFG (BE 2413/3‐1). GP acknowledge funding from the University of Padova (BIRD175145/17). Access to the SEM‐EBSD facilities was provided by the Department of Werkstoffwissenschaften WW1, FAU Erlangen‐Nürnberg, Germany. The Oxford Instruments CMOS‐Symmetry EBSD detector was funded by the DFG (JA 2718/3‐1). Jay Thomas is thanked for providing the synthetic Ti‐doped quartz standard (QTiP‐38, Ti 380 ppm), Djordje Grujic for the natural standard (TN‐06, 0.3 ppm) and Steven Kidder for the Herkimer “Diamond” used as a Ti blank. Cees‐Jan De Hoog is thanked for conducting SIMS measurements and processing at the School of Geosciences of the University of Edinburgh. We acknowledge Holger Stünitz for discussion and providing access to the SEM‐CL spectra facilities at the Department of Geosciences at the Arctic University of Norway (Tromsö), and Amicia Lee and Tom‐Ivar Eilertsen for their assistance. Christoph E. Schrank and Nicholas W. Phillips are thanked for their contribution with respect to the synchrotron data set. Part of this research was undertaken on the XFM beamline at the Australian Synchrotron, part of ANSTO. Rene Romer is thanked for support during electron microprobe analysis (chlorite thermometry) and Friederike Urban and Raphael Njul for sample preparation. Alexis Plunder is thanked for the chlorite thermometry blind test. We are grateful for constructive reviews of Steve Kidder and Leif Tokle and the assessment of an anonymous associated editor of JGR‐Solid Earth. Open access funding enabled and organized by Projekt DEAL.

Austrian Fields of Science 2012

  • 105124 Tectonics

Keywords

  • cathodoluminescence
  • correlative data workflow
  • geochemical re-equilibration
  • Quartz
  • recrystallization processes
  • TitaniQ thermobarometry
  • AUSTROALPINE BASEMENT
  • ALPINE
  • TITANIUM
  • CHLORITE
  • PRESSURE
  • TEMPERATURE
  • DYNAMIC RECRYSTALLIZATION MECHANISMS
  • CONSTRAINTS
  • DIFFUSION
  • FAULT

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