Structural and chemical resetting processes in white mica and their effect on K-Ar data during low temperature metamorphism
White mica has been widely used to date microstructures and tectonic events in faults, shear-zones and folds because of its suitability for radiogenic dating. However, complex (i) microstructural evolution, (ii) individual chemical evolution of the K-bearing phases, (iii) mixing of ‘detrital grains’...
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description | White mica has been widely used to date microstructures and tectonic events in faults, shear-zones and folds because of its suitability for radiogenic dating. However, complex (i) microstructural evolution, (ii) individual chemical evolution of the K-bearing phases, (iii) mixing of ‘detrital grains’ with newly formed and/or recrystallized or chemically reset grains as well as (iv) volume diffusion may result in apparent K-Ar ages. Here, specimens from a prograde sediment sequence of the exhumed fossil European Alpine accretionary wedge were used to investigate resetting processes of white mica by the type and intensity of deformation as well as peak metamorphic conditions. We combine the K-Ar system with mass and mineral quantities from grain size fractions to calculate the amount of recrystallized white mica in each grain size fraction along the metamorphic gradient. Increasing recrystallization with increasing metamorphic grade is related to thermally activated pressure solution and dissolution-precipitation creep, as seen by the formation of a spaced cleavage of recrystallized phyllosilicates documented through Synchrotron X-ray Fluorescence Microscopy and Scanning Electron Microscope imaging techniques. Increasing recrystallization by dissolution-precipitation processes induces chemical resetting of the isotopic system, resulting in a prograde decrease of apparent K-Ar ages. We demonstrate that Ar volume diffusion does not play a significant role for the low-temperature samples, promoting recrystallization as the important physico-chemical process for age resetting. However, white mica chemistry reveals that no simple relation between isotopic resetting and grain size exists along the prograde path. Reliable age information can therefore only be obtained in the case of (nearly) complete resetting, which accounts only for the smallest grain size fraction at the highest metamorphic temperature. These findings could shed new light on accurate dating of mica-rich fault rocks, where the time constraints depend not only on the temperature, but also on the amount and type of deformation.
•We investigate resetting mechanisms in white mica from a prograde sediment sequence.•Isotopic resetting is related to ductile dissolution-precipitation processes.•No simple relation between isotopic resetting and grain size exists.•Reliable age information is only obtained in case of complete resetting.•Complete resetting is reported for smallest grains at highest metamorphi |
doi_str_mv | 10.1016/j.tecto.2020.228708 |
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•We investigate resetting mechanisms in white mica from a prograde sediment sequence.•Isotopic resetting is related to ductile dissolution-precipitation processes.•No simple relation between isotopic resetting and grain size exists.•Reliable age information is only obtained in case of complete resetting.•Complete resetting is reported for smallest grains at highest metamorphic grade.</description><identifier>ISSN: 0040-1951</identifier><identifier>EISSN: 1879-3266</identifier><identifier>DOI: 10.1016/j.tecto.2020.228708</identifier><language>eng</language><publisher>Amsterdam: Elsevier B.V</publisher><subject>Accretion ; Chemical evolution ; Chemical precipitation ; Deformation ; Diffusion ; Dissolution ; Dissolving ; Evolution ; Fluorescence ; Fluorescence microscopy ; Fossils ; Geological faults ; Grain size ; Imaging techniques ; K-Ar ; Low temperature ; Metamorphism ; Mica ; Microstructure ; Particle size ; Phyllosilicates ; Precipitation ; Precipitation processes ; Recrystallization ; Solifluction ; Synchrotron radiation ; Synchrotrons ; Tectonics ; Temperature effects ; X-ray fluorescence</subject><ispartof>Tectonophysics, 2021-02, Vol.800, p.228708, Article 228708</ispartof><rights>2021</rights><rights>Copyright Elsevier BV Feb 5, 2021</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a399t-d2c56897bd21b9ab8f4aa79743aef903a7052f6b02eb332ebffc6470f05888783</citedby><cites>FETCH-LOGICAL-a399t-d2c56897bd21b9ab8f4aa79743aef903a7052f6b02eb332ebffc6470f05888783</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/S0040195120303917$$EHTML$$P50$$Gelsevier$$Hfree_for_read</linktohtml><link.rule.ids>314,776,780,3537,27901,27902,65306</link.rule.ids></links><search><creatorcontrib>Akker, Ismay Vénice</creatorcontrib><creatorcontrib>Berger, Alfons</creatorcontrib><creatorcontrib>Zwingmann, Horst</creatorcontrib><creatorcontrib>Todd, Andrew</creatorcontrib><creatorcontrib>Schrank, Christoph E.</creatorcontrib><creatorcontrib>Jones, Michael W.M.</creatorcontrib><creatorcontrib>Kewish, Cameron M.</creatorcontrib><creatorcontrib>Schmid, Timothy C.</creatorcontrib><creatorcontrib>Herwegh, Marco</creatorcontrib><title>Structural and chemical resetting processes in white mica and their effect on K-Ar data during low temperature metamorphism</title><title>Tectonophysics</title><description>White mica has been widely used to date microstructures and tectonic events in faults, shear-zones and folds because of its suitability for radiogenic dating. However, complex (i) microstructural evolution, (ii) individual chemical evolution of the K-bearing phases, (iii) mixing of ‘detrital grains’ with newly formed and/or recrystallized or chemically reset grains as well as (iv) volume diffusion may result in apparent K-Ar ages. Here, specimens from a prograde sediment sequence of the exhumed fossil European Alpine accretionary wedge were used to investigate resetting processes of white mica by the type and intensity of deformation as well as peak metamorphic conditions. We combine the K-Ar system with mass and mineral quantities from grain size fractions to calculate the amount of recrystallized white mica in each grain size fraction along the metamorphic gradient. Increasing recrystallization with increasing metamorphic grade is related to thermally activated pressure solution and dissolution-precipitation creep, as seen by the formation of a spaced cleavage of recrystallized phyllosilicates documented through Synchrotron X-ray Fluorescence Microscopy and Scanning Electron Microscope imaging techniques. Increasing recrystallization by dissolution-precipitation processes induces chemical resetting of the isotopic system, resulting in a prograde decrease of apparent K-Ar ages. We demonstrate that Ar volume diffusion does not play a significant role for the low-temperature samples, promoting recrystallization as the important physico-chemical process for age resetting. However, white mica chemistry reveals that no simple relation between isotopic resetting and grain size exists along the prograde path. Reliable age information can therefore only be obtained in the case of (nearly) complete resetting, which accounts only for the smallest grain size fraction at the highest metamorphic temperature. These findings could shed new light on accurate dating of mica-rich fault rocks, where the time constraints depend not only on the temperature, but also on the amount and type of deformation.
•We investigate resetting mechanisms in white mica from a prograde sediment sequence.•Isotopic resetting is related to ductile dissolution-precipitation processes.•No simple relation between isotopic resetting and grain size exists.•Reliable age information is only obtained in case of complete resetting.•Complete resetting is reported for smallest grains at highest metamorphic grade.</description><subject>Accretion</subject><subject>Chemical evolution</subject><subject>Chemical precipitation</subject><subject>Deformation</subject><subject>Diffusion</subject><subject>Dissolution</subject><subject>Dissolving</subject><subject>Evolution</subject><subject>Fluorescence</subject><subject>Fluorescence microscopy</subject><subject>Fossils</subject><subject>Geological faults</subject><subject>Grain size</subject><subject>Imaging techniques</subject><subject>K-Ar</subject><subject>Low temperature</subject><subject>Metamorphism</subject><subject>Mica</subject><subject>Microstructure</subject><subject>Particle size</subject><subject>Phyllosilicates</subject><subject>Precipitation</subject><subject>Precipitation processes</subject><subject>Recrystallization</subject><subject>Solifluction</subject><subject>Synchrotron radiation</subject><subject>Synchrotrons</subject><subject>Tectonics</subject><subject>Temperature effects</subject><subject>X-ray fluorescence</subject><issn>0040-1951</issn><issn>1879-3266</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNp9kE1P3DAQhq2qldhCfwEXSz1nO7YTfxx6QIhSBBIH4Gw5zrjr1SZZbKeo4s_Xy3Lm4pGl55lX8xJyzmDNgMkf23VBX-Y1Bw5rzrUC_YmsmFamEVzKz2QF0ELDTMdOyNectwAgWSdX5PWhpMWXJbkdddNA_QbH6OsnYcZS4vSH7tPsMWfMNE70ZRML0gPyhpcNxkQxhBpP54neNheJDq44OizpIO_mF1pw3GNyNaSaWNw4p_0m5vGMfAlul_Hb-zwlT7-uHi9_N3f31zeXF3eNE8aUZuC-k9qofuCsN67XoXVOGdUKh8GAcAo6HmQPHHsh6hOCl62CAJ3WWmlxSr4f99ZLnhfMxW7nJU010vIOBFO8NbJS4kj5NOecMNh9iqNL_ywDe2jZbu1by_bQsj22XK2fRwvrAX8jJpt9xMnjEFOF7TDHD_3_z0WIhQ</recordid><startdate>20210205</startdate><enddate>20210205</enddate><creator>Akker, Ismay Vénice</creator><creator>Berger, Alfons</creator><creator>Zwingmann, Horst</creator><creator>Todd, Andrew</creator><creator>Schrank, Christoph E.</creator><creator>Jones, Michael W.M.</creator><creator>Kewish, Cameron M.</creator><creator>Schmid, Timothy C.</creator><creator>Herwegh, Marco</creator><general>Elsevier B.V</general><general>Elsevier BV</general><scope>6I.</scope><scope>AAFTH</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7TN</scope><scope>8FD</scope><scope>F1W</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope></search><sort><creationdate>20210205</creationdate><title>Structural and chemical resetting processes in white mica and their effect on K-Ar data during low temperature metamorphism</title><author>Akker, Ismay Vénice ; Berger, Alfons ; Zwingmann, Horst ; Todd, Andrew ; Schrank, Christoph E. ; Jones, Michael W.M. ; Kewish, Cameron M. ; Schmid, Timothy C. ; Herwegh, Marco</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a399t-d2c56897bd21b9ab8f4aa79743aef903a7052f6b02eb332ebffc6470f05888783</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Accretion</topic><topic>Chemical evolution</topic><topic>Chemical precipitation</topic><topic>Deformation</topic><topic>Diffusion</topic><topic>Dissolution</topic><topic>Dissolving</topic><topic>Evolution</topic><topic>Fluorescence</topic><topic>Fluorescence microscopy</topic><topic>Fossils</topic><topic>Geological faults</topic><topic>Grain size</topic><topic>Imaging techniques</topic><topic>K-Ar</topic><topic>Low temperature</topic><topic>Metamorphism</topic><topic>Mica</topic><topic>Microstructure</topic><topic>Particle size</topic><topic>Phyllosilicates</topic><topic>Precipitation</topic><topic>Precipitation processes</topic><topic>Recrystallization</topic><topic>Solifluction</topic><topic>Synchrotron radiation</topic><topic>Synchrotrons</topic><topic>Tectonics</topic><topic>Temperature effects</topic><topic>X-ray fluorescence</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Akker, Ismay Vénice</creatorcontrib><creatorcontrib>Berger, Alfons</creatorcontrib><creatorcontrib>Zwingmann, Horst</creatorcontrib><creatorcontrib>Todd, Andrew</creatorcontrib><creatorcontrib>Schrank, Christoph E.</creatorcontrib><creatorcontrib>Jones, Michael W.M.</creatorcontrib><creatorcontrib>Kewish, Cameron M.</creatorcontrib><creatorcontrib>Schmid, Timothy C.</creatorcontrib><creatorcontrib>Herwegh, Marco</creatorcontrib><collection>ScienceDirect Open Access Titles</collection><collection>Elsevier:ScienceDirect:Open Access</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>Technology Research Database</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Tectonophysics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Akker, Ismay Vénice</au><au>Berger, Alfons</au><au>Zwingmann, Horst</au><au>Todd, Andrew</au><au>Schrank, Christoph E.</au><au>Jones, Michael W.M.</au><au>Kewish, Cameron M.</au><au>Schmid, Timothy C.</au><au>Herwegh, Marco</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Structural and chemical resetting processes in white mica and their effect on K-Ar data during low temperature metamorphism</atitle><jtitle>Tectonophysics</jtitle><date>2021-02-05</date><risdate>2021</risdate><volume>800</volume><spage>228708</spage><pages>228708-</pages><artnum>228708</artnum><issn>0040-1951</issn><eissn>1879-3266</eissn><abstract>White mica has been widely used to date microstructures and tectonic events in faults, shear-zones and folds because of its suitability for radiogenic dating. However, complex (i) microstructural evolution, (ii) individual chemical evolution of the K-bearing phases, (iii) mixing of ‘detrital grains’ with newly formed and/or recrystallized or chemically reset grains as well as (iv) volume diffusion may result in apparent K-Ar ages. Here, specimens from a prograde sediment sequence of the exhumed fossil European Alpine accretionary wedge were used to investigate resetting processes of white mica by the type and intensity of deformation as well as peak metamorphic conditions. We combine the K-Ar system with mass and mineral quantities from grain size fractions to calculate the amount of recrystallized white mica in each grain size fraction along the metamorphic gradient. Increasing recrystallization with increasing metamorphic grade is related to thermally activated pressure solution and dissolution-precipitation creep, as seen by the formation of a spaced cleavage of recrystallized phyllosilicates documented through Synchrotron X-ray Fluorescence Microscopy and Scanning Electron Microscope imaging techniques. Increasing recrystallization by dissolution-precipitation processes induces chemical resetting of the isotopic system, resulting in a prograde decrease of apparent K-Ar ages. We demonstrate that Ar volume diffusion does not play a significant role for the low-temperature samples, promoting recrystallization as the important physico-chemical process for age resetting. However, white mica chemistry reveals that no simple relation between isotopic resetting and grain size exists along the prograde path. Reliable age information can therefore only be obtained in the case of (nearly) complete resetting, which accounts only for the smallest grain size fraction at the highest metamorphic temperature. These findings could shed new light on accurate dating of mica-rich fault rocks, where the time constraints depend not only on the temperature, but also on the amount and type of deformation.
•We investigate resetting mechanisms in white mica from a prograde sediment sequence.•Isotopic resetting is related to ductile dissolution-precipitation processes.•No simple relation between isotopic resetting and grain size exists.•Reliable age information is only obtained in case of complete resetting.•Complete resetting is reported for smallest grains at highest metamorphic grade.</abstract><cop>Amsterdam</cop><pub>Elsevier B.V</pub><doi>10.1016/j.tecto.2020.228708</doi><oa>free_for_read</oa></addata></record> |
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subjects | Accretion Chemical evolution Chemical precipitation Deformation Diffusion Dissolution Dissolving Evolution Fluorescence Fluorescence microscopy Fossils Geological faults Grain size Imaging techniques K-Ar Low temperature Metamorphism Mica Microstructure Particle size Phyllosilicates Precipitation Precipitation processes Recrystallization Solifluction Synchrotron radiation Synchrotrons Tectonics Temperature effects X-ray fluorescence |
title | Structural and chemical resetting processes in white mica and their effect on K-Ar data during low temperature metamorphism |
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