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Implications for late Grenvillian (Rigolet Phase) construction of Rodinia using new U-Pb data from the Mars Hill Terrane, Tennessee and North Carolina, United States
New data for zircon (external morphology, cathodoluminescence zoning, and sensitive high resolution ion microprobe [SHRIMP] U-Pb ages) from the Carvers Gap granulite gneiss of the Mars Hill terrane (Tennessee and North Carolina, United States) require reevaluation of interpretations of the age and o...
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Published in: | Geology (Boulder) 2013-10, Vol.41 (10), p.1087-1090 |
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creator | Aleinikoff, John N Southworth, Scott Merschat, Arthur J |
description | New data for zircon (external morphology, cathodoluminescence zoning, and sensitive high resolution ion microprobe [SHRIMP] U-Pb ages) from the Carvers Gap granulite gneiss of the Mars Hill terrane (Tennessee and North Carolina, United States) require reevaluation of interpretations of the age and origin of this rock. The new results indicate that the zircon is detrital and that the sedimentary protolith of this gneiss (and related Cloudland gneiss) was deposited no earlier than ca. 1.02 Ga and was metamorphosed at ca. 0.98 Ga. Tectonic models that included the gneiss as a piece of 1.8 Ga Amazonian crust (perhaps as part of the hypothetical Columbia supercontinent) are now untenable. The remarkably fast cycle of exhumation, erosion, deposition, and deep burial also is characteristic of other late Grenvillian (post-Ottawan) Mesoproterozoic paragneisses that occur throughout the Appalachians. These rocks provide new evidence for the duration of the formation of the Rodinia supercontinent lasting until at least 0.98 Ma. |
doi_str_mv | 10.1130/G34779.1 |
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The new results indicate that the zircon is detrital and that the sedimentary protolith of this gneiss (and related Cloudland gneiss) was deposited no earlier than ca. 1.02 Ga and was metamorphosed at ca. 0.98 Ga. Tectonic models that included the gneiss as a piece of 1.8 Ga Amazonian crust (perhaps as part of the hypothetical Columbia supercontinent) are now untenable. The remarkably fast cycle of exhumation, erosion, deposition, and deep burial also is characteristic of other late Grenvillian (post-Ottawan) Mesoproterozoic paragneisses that occur throughout the Appalachians. These rocks provide new evidence for the duration of the formation of the Rodinia supercontinent lasting until at least 0.98 Ma.</description><identifier>ISSN: 0091-7613</identifier><identifier>EISSN: 1943-2682</identifier><identifier>DOI: 10.1130/G34779.1</identifier><language>eng</language><publisher>Boulder: Geological Society of America (GSA)</publisher><subject>absolute age ; Appalachians ; Blue Ridge Mountains ; Geochronology ; gneisses ; Grenvillian Orogeny ; Ions ; Luminescence ; Mars Hill Terrane ; Mesoproterozoic ; metamorphic rocks ; metamorphism ; metasedimentary rocks ; Morphology ; Neoproterozoic ; nesosilicates ; North America ; North Carolina ; orthosilicates ; paleogeography ; Plate tectonics ; Precambrian ; Proterozoic ; provenance ; Rigolet Phase ; Rocks ; Rodinia ; Sedimentary geology ; silicates ; Stratigraphy ; Tennessee ; U/Pb ; United States ; upper Precambrian ; zircon ; zircon group</subject><ispartof>Geology (Boulder), 2013-10, Vol.41 (10), p.1087-1090</ispartof><rights>GeoRef, Copyright 2022, American Geosciences Institute. 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The new results indicate that the zircon is detrital and that the sedimentary protolith of this gneiss (and related Cloudland gneiss) was deposited no earlier than ca. 1.02 Ga and was metamorphosed at ca. 0.98 Ga. Tectonic models that included the gneiss as a piece of 1.8 Ga Amazonian crust (perhaps as part of the hypothetical Columbia supercontinent) are now untenable. The remarkably fast cycle of exhumation, erosion, deposition, and deep burial also is characteristic of other late Grenvillian (post-Ottawan) Mesoproterozoic paragneisses that occur throughout the Appalachians. These rocks provide new evidence for the duration of the formation of the Rodinia supercontinent lasting until at least 0.98 Ma.</description><subject>absolute age</subject><subject>Appalachians</subject><subject>Blue Ridge Mountains</subject><subject>Geochronology</subject><subject>gneisses</subject><subject>Grenvillian Orogeny</subject><subject>Ions</subject><subject>Luminescence</subject><subject>Mars Hill Terrane</subject><subject>Mesoproterozoic</subject><subject>metamorphic rocks</subject><subject>metamorphism</subject><subject>metasedimentary rocks</subject><subject>Morphology</subject><subject>Neoproterozoic</subject><subject>nesosilicates</subject><subject>North America</subject><subject>North Carolina</subject><subject>orthosilicates</subject><subject>paleogeography</subject><subject>Plate tectonics</subject><subject>Precambrian</subject><subject>Proterozoic</subject><subject>provenance</subject><subject>Rigolet Phase</subject><subject>Rocks</subject><subject>Rodinia</subject><subject>Sedimentary geology</subject><subject>silicates</subject><subject>Stratigraphy</subject><subject>Tennessee</subject><subject>U/Pb</subject><subject>United States</subject><subject>upper Precambrian</subject><subject>zircon</subject><subject>zircon group</subject><issn>0091-7613</issn><issn>1943-2682</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNpdkWFrFDEQhoMoeFbBnzDgl4rdmmyS3c1HOfRaaLXU3ucll8zepeSSM8la_EH-T1NOKPTTDMMzL-_MS8h7Rs8Z4_Tziou-V-fsBVkwJXjTdkP7kiwoVazpO8Zfkzc531PKhOyHBfl7uT94Z3RxMWSYYgKvC8IqYfjtvHc6wOmt20aPBW52OuNHMJUsaTaPKxAnuI3WBadhzi5sIeADrJubDVhdNEwp7qHsEK51ynBRFeEOU9IBz2oTAuaMCDpY-B5T2cFSp-hd0GewDq6ghZ-l2slvyatJ-4zv_tcTsv729W550Vz9WF0uv1w1ul5dGm1tJwdBB8snu1Fi6OrYtkz1m74XhoqhlagNo0IIuZFMTdryfkLVUTpR1fITcnrUPaT4a8Zcxr3LBr2vhuOcx_q0QXIpO1HRD8_Q-zinUN1Vig-DElL1T4ImxZwTTuMhub1Of0ZGx8e8xmNeI6vopyO6xZiNw2DwISZvn3RbyvhIO8U7yf8BcOaWIA</recordid><startdate>20131001</startdate><enddate>20131001</enddate><creator>Aleinikoff, John N</creator><creator>Southworth, Scott</creator><creator>Merschat, Arthur J</creator><general>Geological Society of America (GSA)</general><general>Geological Society of America</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7UA</scope><scope>C1K</scope><scope>F1W</scope><scope>H96</scope><scope>KL.</scope><scope>L.G</scope></search><sort><creationdate>20131001</creationdate><title>Implications for late Grenvillian (Rigolet Phase) construction of Rodinia using new U-Pb data from the Mars Hill Terrane, Tennessee and North Carolina, United States</title><author>Aleinikoff, John N ; Southworth, Scott ; Merschat, Arthur J</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a347t-add658408d3fdb9486347d2197b774c04825eac104445b519fad37fe9600f0923</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>absolute age</topic><topic>Appalachians</topic><topic>Blue Ridge Mountains</topic><topic>Geochronology</topic><topic>gneisses</topic><topic>Grenvillian Orogeny</topic><topic>Ions</topic><topic>Luminescence</topic><topic>Mars Hill Terrane</topic><topic>Mesoproterozoic</topic><topic>metamorphic rocks</topic><topic>metamorphism</topic><topic>metasedimentary rocks</topic><topic>Morphology</topic><topic>Neoproterozoic</topic><topic>nesosilicates</topic><topic>North America</topic><topic>North Carolina</topic><topic>orthosilicates</topic><topic>paleogeography</topic><topic>Plate tectonics</topic><topic>Precambrian</topic><topic>Proterozoic</topic><topic>provenance</topic><topic>Rigolet Phase</topic><topic>Rocks</topic><topic>Rodinia</topic><topic>Sedimentary geology</topic><topic>silicates</topic><topic>Stratigraphy</topic><topic>Tennessee</topic><topic>U/Pb</topic><topic>United States</topic><topic>upper Precambrian</topic><topic>zircon</topic><topic>zircon group</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Aleinikoff, John N</creatorcontrib><creatorcontrib>Southworth, Scott</creatorcontrib><creatorcontrib>Merschat, Arthur J</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Water Resources Abstracts</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><jtitle>Geology (Boulder)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Aleinikoff, John N</au><au>Southworth, Scott</au><au>Merschat, Arthur J</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Implications for late Grenvillian (Rigolet Phase) construction of Rodinia using new U-Pb data from the Mars Hill Terrane, Tennessee and North Carolina, United States</atitle><jtitle>Geology (Boulder)</jtitle><date>2013-10-01</date><risdate>2013</risdate><volume>41</volume><issue>10</issue><spage>1087</spage><epage>1090</epage><pages>1087-1090</pages><issn>0091-7613</issn><eissn>1943-2682</eissn><abstract>New data for zircon (external morphology, cathodoluminescence zoning, and sensitive high resolution ion microprobe [SHRIMP] U-Pb ages) from the Carvers Gap granulite gneiss of the Mars Hill terrane (Tennessee and North Carolina, United States) require reevaluation of interpretations of the age and origin of this rock. The new results indicate that the zircon is detrital and that the sedimentary protolith of this gneiss (and related Cloudland gneiss) was deposited no earlier than ca. 1.02 Ga and was metamorphosed at ca. 0.98 Ga. Tectonic models that included the gneiss as a piece of 1.8 Ga Amazonian crust (perhaps as part of the hypothetical Columbia supercontinent) are now untenable. The remarkably fast cycle of exhumation, erosion, deposition, and deep burial also is characteristic of other late Grenvillian (post-Ottawan) Mesoproterozoic paragneisses that occur throughout the Appalachians. These rocks provide new evidence for the duration of the formation of the Rodinia supercontinent lasting until at least 0.98 Ma.</abstract><cop>Boulder</cop><pub>Geological Society of America (GSA)</pub><doi>10.1130/G34779.1</doi><tpages>4</tpages></addata></record> |
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source | 地球科学世界出版社期刊(NSTL购买) |
subjects | absolute age Appalachians Blue Ridge Mountains Geochronology gneisses Grenvillian Orogeny Ions Luminescence Mars Hill Terrane Mesoproterozoic metamorphic rocks metamorphism metasedimentary rocks Morphology Neoproterozoic nesosilicates North America North Carolina orthosilicates paleogeography Plate tectonics Precambrian Proterozoic provenance Rigolet Phase Rocks Rodinia Sedimentary geology silicates Stratigraphy Tennessee U/Pb United States upper Precambrian zircon zircon group |
title | Implications for late Grenvillian (Rigolet Phase) construction of Rodinia using new U-Pb data from the Mars Hill Terrane, Tennessee and North Carolina, United States |
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