Provenance of a Late Permian retroarc foreland basin along the eastern Gondwanan margin: northern Sydney Basin, eastern Australia
The Upper Permian sedimentary successions in the northern Sydney Basin have been the subject of several stratigraphic, sedimentological and coal petrographic studies, and recently, extensive U-Pb zircon dating has been carried out on tuffs in the Newcastle Coal Measures. However, detailed petrograph...
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Veröffentlicht in: | Geological magazine 2023-08, Vol.160 (8), p.1535-1555 |
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description | The Upper Permian sedimentary successions in the northern Sydney Basin have been the subject of several stratigraphic, sedimentological and coal petrographic studies, and recently, extensive U-Pb zircon dating has been carried out on tuffs in the Newcastle Coal Measures. However, detailed petrographic and geochemical studies of these successions are lacking. These are important because a major change in tectonic setting occurred prior to the Late Permian because of the Hunter-Bowen Orogeny that caused the uplift of the Carboniferous and Devonian successions in the Tamworth Group and Tablelands Complex adjacent to the Sydney Basin. This should be reflected in the detrital makeup of the Upper Permian rocks. This study provides data that confirms major changes did take place at this time. Petrographic analysis indicates that the source area is composed of sedimentary, felsic volcanic and plutonic and low-grade metamorphic rocks. Conglomerate clast composition analysis confirms these results, revealing a source region that is composed of felsic volcanics, cherts, mudstones and sandstones. Geochemical analysis suggests that the sediments are geochemically mature and have undergone a moderate degree of weathering. The provenance data presented in this paper indicate that the southern New England Orogen is the principal source of detritus in the basin. Discrimination diagrams confirm that the source rocks derive from an arc-related, contractional setting and agree with the provenance analyses that indicate sediment deposition in a retroarc foreland basin. This study offers new insights on the provenance and tectonic setting of the Northern Sydney Basin, eastern Australia. |
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However, detailed petrographic and geochemical studies of these successions are lacking. These are important because a major change in tectonic setting occurred prior to the Late Permian because of the Hunter-Bowen Orogeny that caused the uplift of the Carboniferous and Devonian successions in the Tamworth Group and Tablelands Complex adjacent to the Sydney Basin. This should be reflected in the detrital makeup of the Upper Permian rocks. This study provides data that confirms major changes did take place at this time. Petrographic analysis indicates that the source area is composed of sedimentary, felsic volcanic and plutonic and low-grade metamorphic rocks. Conglomerate clast composition analysis confirms these results, revealing a source region that is composed of felsic volcanics, cherts, mudstones and sandstones. Geochemical analysis suggests that the sediments are geochemically mature and have undergone a moderate degree of weathering. The provenance data presented in this paper indicate that the southern New England Orogen is the principal source of detritus in the basin. Discrimination diagrams confirm that the source rocks derive from an arc-related, contractional setting and agree with the provenance analyses that indicate sediment deposition in a retroarc foreland basin. This study offers new insights on the provenance and tectonic setting of the Northern Sydney Basin, eastern Australia.</description><identifier>ISSN: 0016-7568</identifier><identifier>EISSN: 1469-5081</identifier><identifier>DOI: 10.1017/S0016756823000535</identifier><language>eng</language><publisher>Cambridge, UK: Cambridge University Press</publisher><subject>Analysis ; Basins ; Carboniferous ; Coal ; Conglomerates ; Dating ; Detritus ; Devonian ; Geochemistry ; Geochronometry ; Gondwana ; Metamorphic rocks ; Original Article ; Orogeny ; Permian ; Radiometric dating ; Sandstone ; Sediment ; Sediments ; Stratigraphy ; Tectonics ; Uplift ; Zircon</subject><ispartof>Geological magazine, 2023-08, Vol.160 (8), p.1535-1555</ispartof><rights>The Author(s), 2023. Published by Cambridge University Press</rights><rights>The Author(s), 2023. Published by Cambridge University Press. This work is licensed under the Creative Commons Attribution License This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited. (the “License”). 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Mag</addtitle><description>The Upper Permian sedimentary successions in the northern Sydney Basin have been the subject of several stratigraphic, sedimentological and coal petrographic studies, and recently, extensive U-Pb zircon dating has been carried out on tuffs in the Newcastle Coal Measures. However, detailed petrographic and geochemical studies of these successions are lacking. These are important because a major change in tectonic setting occurred prior to the Late Permian because of the Hunter-Bowen Orogeny that caused the uplift of the Carboniferous and Devonian successions in the Tamworth Group and Tablelands Complex adjacent to the Sydney Basin. This should be reflected in the detrital makeup of the Upper Permian rocks. This study provides data that confirms major changes did take place at this time. Petrographic analysis indicates that the source area is composed of sedimentary, felsic volcanic and plutonic and low-grade metamorphic rocks. Conglomerate clast composition analysis confirms these results, revealing a source region that is composed of felsic volcanics, cherts, mudstones and sandstones. Geochemical analysis suggests that the sediments are geochemically mature and have undergone a moderate degree of weathering. The provenance data presented in this paper indicate that the southern New England Orogen is the principal source of detritus in the basin. Discrimination diagrams confirm that the source rocks derive from an arc-related, contractional setting and agree with the provenance analyses that indicate sediment deposition in a retroarc foreland basin. This study offers new insights on the provenance and tectonic setting of the Northern Sydney Basin, eastern Australia.</description><subject>Analysis</subject><subject>Basins</subject><subject>Carboniferous</subject><subject>Coal</subject><subject>Conglomerates</subject><subject>Dating</subject><subject>Detritus</subject><subject>Devonian</subject><subject>Geochemistry</subject><subject>Geochronometry</subject><subject>Gondwana</subject><subject>Metamorphic rocks</subject><subject>Original Article</subject><subject>Orogeny</subject><subject>Permian</subject><subject>Radiometric dating</subject><subject>Sandstone</subject><subject>Sediment</subject><subject>Sediments</subject><subject>Stratigraphy</subject><subject>Tectonics</subject><subject>Uplift</subject><subject>Zircon</subject><issn>0016-7568</issn><issn>1469-5081</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>IKXGN</sourceid><sourceid>8G5</sourceid><sourceid>BENPR</sourceid><sourceid>GUQSH</sourceid><sourceid>M2O</sourceid><recordid>eNp1kE9LAzEQxYMoWKsfwFvAq6v5s7vZeKuiVShYqJ6XySapW9qkJlulR7-5WVr0IJ6G4b3fG-YhdE7JFSVUXM8IoaUoyopxQkjBiwM0oHkps4JU9BANejnr9WN0EuMirZxU1QB9TYP_MA5cY7C3GPAEOoOnJqxacDiYLngIDbY-mCU4jRXE1mFYejfH3ZvBBmJngsNj7_QnpBy8gjBv3Q12PiRDkmZb7cwW3_bk5Q8w2sQuwLKFU3RkYRnN2X4O0evD_cvdYzZ5Hj_djSYZcF50GatyrYSyoKUEywppGqVYRYFYBpZQJYQoVc5AC4BcFEyCtJpJYYlQean5EF3sctfBv29M7OqF3wSXTtasElIyWQqeXHTnaoKPMRhbr0ObXtrWlNR90_WfphPD9wysVGj13PxG_099A6zSgek</recordid><startdate>20230801</startdate><enddate>20230801</enddate><creator>Maravelis, Angelos G.</creator><creator>Offler, Robin</creator><creator>Botziolis, Chrysanthos</creator><creator>Pantopoulos, George</creator><creator>Scott, Alexandra</creator><creator>Landenberger, Bill</creator><creator>Collins, William J.</creator><general>Cambridge University Press</general><scope>IKXGN</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7UA</scope><scope>7XB</scope><scope>88I</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>8G5</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F1W</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H96</scope><scope>HCIFZ</scope><scope>L.G</scope><scope>L6V</scope><scope>M2O</scope><scope>M2P</scope><scope>M7S</scope><scope>MBDVC</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PTHSS</scope><scope>Q9U</scope><scope>R05</scope><orcidid>https://orcid.org/0000-0002-9694-7500</orcidid></search><sort><creationdate>20230801</creationdate><title>Provenance of a Late Permian retroarc foreland basin along the eastern Gondwanan margin: northern Sydney Basin, eastern Australia</title><author>Maravelis, Angelos G. ; 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Mag</addtitle><date>2023-08-01</date><risdate>2023</risdate><volume>160</volume><issue>8</issue><spage>1535</spage><epage>1555</epage><pages>1535-1555</pages><issn>0016-7568</issn><eissn>1469-5081</eissn><abstract>The Upper Permian sedimentary successions in the northern Sydney Basin have been the subject of several stratigraphic, sedimentological and coal petrographic studies, and recently, extensive U-Pb zircon dating has been carried out on tuffs in the Newcastle Coal Measures. However, detailed petrographic and geochemical studies of these successions are lacking. These are important because a major change in tectonic setting occurred prior to the Late Permian because of the Hunter-Bowen Orogeny that caused the uplift of the Carboniferous and Devonian successions in the Tamworth Group and Tablelands Complex adjacent to the Sydney Basin. This should be reflected in the detrital makeup of the Upper Permian rocks. This study provides data that confirms major changes did take place at this time. Petrographic analysis indicates that the source area is composed of sedimentary, felsic volcanic and plutonic and low-grade metamorphic rocks. Conglomerate clast composition analysis confirms these results, revealing a source region that is composed of felsic volcanics, cherts, mudstones and sandstones. Geochemical analysis suggests that the sediments are geochemically mature and have undergone a moderate degree of weathering. The provenance data presented in this paper indicate that the southern New England Orogen is the principal source of detritus in the basin. Discrimination diagrams confirm that the source rocks derive from an arc-related, contractional setting and agree with the provenance analyses that indicate sediment deposition in a retroarc foreland basin. This study offers new insights on the provenance and tectonic setting of the Northern Sydney Basin, eastern Australia.</abstract><cop>Cambridge, UK</cop><pub>Cambridge University Press</pub><doi>10.1017/S0016756823000535</doi><tpages>21</tpages><orcidid>https://orcid.org/0000-0002-9694-7500</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Analysis Basins Carboniferous Coal Conglomerates Dating Detritus Devonian Geochemistry Geochronometry Gondwana Metamorphic rocks Original Article Orogeny Permian Radiometric dating Sandstone Sediment Sediments Stratigraphy Tectonics Uplift Zircon |
title | Provenance of a Late Permian retroarc foreland basin along the eastern Gondwanan margin: northern Sydney Basin, eastern Australia |
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