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<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Earth Sci.</journal-id>
<journal-title>Frontiers in Earth Science</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Earth Sci.</abbrev-journal-title>
<issn pub-type="epub">2296-6463</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">1202477</article-id>
<article-id pub-id-type="doi">10.3389/feart.2023.1202477</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Earth Science</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Petrography, geochemistry and geochronology of igneous rocks from the Jiangnan Orogen, South China: constraints on the Early Paleozoic tectonic evolution of the South China Block</article-title>
<alt-title alt-title-type="left-running-head">Tang et al.</alt-title>
<alt-title alt-title-type="right-running-head">
<ext-link ext-link-type="uri" xlink:href="https://doi.org/10.3389/feart.2023.1202477">10.3389/feart.2023.1202477</ext-link>
</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Tang</surname>
<given-names>Yuanyuan</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<uri xlink:href="https://loop.frontiersin.org/people/2122663/overview"/>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Shi</surname>
<given-names>Yu</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Weng</surname>
<given-names>Boyin</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Zhou</surname>
<given-names>Yuxi</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Lan</surname>
<given-names>Yuanchun</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group>
<aff id="aff1">
<sup>1</sup>
<institution>Guangxi Key Laboratory of Hidden Metal Mineral Exploration</institution>, <institution>Guilin University of Technology</institution>, <addr-line>Guilin</addr-line>, <country>China</country>
</aff>
<aff id="aff2">
<sup>2</sup>
<institution>Collaborative Innovation Center for Exploration of Nonferrous Metal Deposits and Efficient Utilization of Resources</institution>, <institution>Guilin University of Technology</institution>, <addr-line>Guilin</addr-line>, <country>China</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1401736/overview">Tatsuki Tsujimori</ext-link>, Tohoku University, Japan</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/2278960/overview">Zheng Liu</ext-link>, Yunnan University, China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/825009/overview">Guoguang Wang</ext-link>, Nanjing University, China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/938712/overview">Xiao-Ping Xia</ext-link>, Chinese Academy of Sciences (CAS), China</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Yu Shi, <email>shiyu_61@163.com</email>
</corresp>
</author-notes>
<pub-date pub-type="epub">
<day>01</day>
<month>06</month>
<year>2023</year>
</pub-date>
<pub-date pub-type="collection">
<year>2023</year>
</pub-date>
<volume>11</volume>
<elocation-id>1202477</elocation-id>
<history>
<date date-type="received">
<day>08</day>
<month>04</month>
<year>2023</year>
</date>
<date date-type="accepted">
<day>22</day>
<month>05</month>
<year>2023</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2023 Tang, Shi, Weng, Zhou and Lan.</copyright-statement>
<copyright-year>2023</copyright-year>
<copyright-holder>Tang, Shi, Weng, Zhou and Lan</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/">
<p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p>
</license>
</permissions>
<abstract>
<p>The Early Paleozoic tectonic evolution of the South China Block (SCB) remains controversial related to intracontinental orogenic and oceanic subduction processes. We present whole-rock major and trace elemental data, LA-ICP-MS zircon U-Pb age and Lu-Hf isotopic data for the Early Paleozoic igneous rocks including granodiorites from the Yuechengling pluton and volcanic breccias from the Damingshan pluton from the western segment of the Jiangnan Orogen in the SCB. LA-ICP-MS zircon U-Pb dating yielded emplacement ages for the Yuechengling S-type granitoids of 438&#x2013;436&#xa0;Ma and the deposited age for the Damingshan volcaniclastic rocks to be later than 451&#xa0;Ma. The Yuechengling granitoids have consistent SiO<sub>2</sub>, TiO<sub>2</sub>, Fe<sub>2</sub>O<sub>3</sub>
<sup>T</sup>, MgO, and P<sub>2</sub>O<sub>5</sub> contents, higher Al<sub>2</sub>O<sub>3</sub> contents, and Na<sub>2</sub>O &#x2b; K<sub>2</sub>O values, but lower Mg<sup>&#x23;</sup> values, compared with those of the Damingshan volcaniclastic rocks. All the studied samples exhibit enrichment in LREEs and moderate negative Eu anomalies (&#x3b4;Eu &#x3d; 0.63&#x2013;0.75), with negative Ba, Sr, Nb, Ta, P, and Ti anomalies, and positive Rb, Th, U, Pb, and K anomalies. The granitoids have variable CaO/Na<sub>2</sub>O ratios of 0.22&#x2013;1.11, negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values of &#x2212;11.98 to &#x2212;0.90, and corresponding T<sub>DM2</sub> ages distributed from 2.37 to 1.55&#xa0;Ga. The petrographic and geochemical characteristics of the Yuechengling granitoids indicate that their parental magma was derived from a crustal meta-greywacke and meta-pelite components in the Paleoproterozoic basement, and have undergone some degree of fractional crystallization. The volcaniclastic rocks have mostly negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values with partially positive (&#x2212;27.54 to 8.73), and zircons with negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values (&#x2212;27.54 to &#x2212;0.14) show T<sub>DM2</sub> ages of 3.79 to 1.63&#xa0;Ga. Combined with petrographic and geochemical data, we suggest that the Damingshan volcaniclastic rocks were derived from Neoarchean-Neoproterozoic crustal materials and the felsic parental magma has undergone some degree of magma mixing with mantle material, and deposited soon after a Late Ordovician volcanic eruption (later than 451&#xa0;Ma). Integrated with previous studies, our new data support the intracontinental orogenic model to account for the Early Paleozoic tectonic evolution. Thus, we suggest that the Early Paleozoic tectonic setting of the SCB was intracontinental orogeny rather than oceanic subduction-collision.</p>
</abstract>
<kwd-group>
<kwd>the South China Block</kwd>
<kwd>igneous rock</kwd>
<kwd>zircon U-Pb geochronology</kwd>
<kwd>geochemistry</kwd>
<kwd>Hf isotope</kwd>
</kwd-group>
<contract-sponsor id="cn001">Guilin University of Technology<named-content content-type="fundref-id">10.13039/501100003457</named-content>
</contract-sponsor>
<custom-meta-wrap>
<custom-meta>
<meta-name>section-at-acceptance</meta-name>
<meta-value>Petrology</meta-value>
</custom-meta>
</custom-meta-wrap>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>The SCB, a major continental block of East Asia, is located in southeast Eurasia and the convergence area of Eurasian and Pacific Plates (<xref ref-type="fig" rid="F1">Figure 1A</xref>). The block consists of the Yangtze Block to the northwest and the Cathaysia Block to the southeast, which were welded together during the Neoproterozoic along the Jiangnan fold belt (the Jiangnan Orogen, <xref ref-type="fig" rid="F1">Figure 1B</xref>) (<xref ref-type="bibr" rid="B13">Charvet, 2013</xref>; <xref ref-type="bibr" rid="B99">Yao et al., 2014</xref>; <xref ref-type="bibr" rid="B74">Shu et al., 2015</xref>). The SCB had undergone three episodes of tectonic evolution of the Proto-(Early Paleozoic), the Paleo-(Late Paleozoic) and the Neo-(Mesozoic-Cenozoic) Tethys since Neoproterozoic, corresponding to three tectonic evolution stages of the Caledonian (Early Paleozoic), Indosinian (Early Mesozoic) and Yanshanian-Himalayan (Late Mesozoic-Cenozoic) (<xref ref-type="bibr" rid="B109">Zhang et al., 2013</xref>). As the first extensive tectono-thermal event in the SCB since the Neoproterozoic break-up of the Rodinia supercontinent (<xref ref-type="bibr" rid="B86">Wang et al., 2011</xref>; <xref ref-type="bibr" rid="B35">Huang et al., 2013</xref>; <xref ref-type="bibr" rid="B106">Yu et al., 2016</xref>), the Early Paleozoic orogeny strongly affected the final tectonic framework of the SCB (<xref ref-type="bibr" rid="B71">Shu, 2012</xref>; <xref ref-type="bibr" rid="B109">Zhang et al., 2013</xref>), which is characterized by high-grade metamorphism, intensive deformation, wide-spread magmatism and unconformities (<xref ref-type="bibr" rid="B11">Charvet et al., 2010</xref>; <xref ref-type="bibr" rid="B50">Liu et al., 2010</xref>; <xref ref-type="bibr" rid="B86">Wang et al., 2011</xref>; <xref ref-type="bibr" rid="B110">Zhang et al., 2015</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref>).</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>
<bold>(A)</bold> Simplified tectonic map of Eurasia showing the major tectonic units and the location of the SCB (modified after <xref ref-type="bibr" rid="B80">Wang et al., 2018</xref>). <bold>(B)</bold> Distribution of the Early Paleozoic igneous rocks in the SCB and location of the Jiangnan Orogen (modified after <xref ref-type="bibr" rid="B114">Zhao et al., 2022</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref>). &#x2460; CLF-the Chenzhou-Linwu fault (after <xref ref-type="bibr" rid="B113">Zhao, 2015</xref>), &#x2461; PNF-the Pingxiang-Gongcheng-Nanning fault (after <xref ref-type="bibr" rid="B121">Zhou and Wen, 2021</xref>), &#x2462; SLF-the Shizong-Mile-Luodian fault (after <xref ref-type="bibr" rid="B22">Dong et al., 2015</xref>). The numbers stand for ages with the unit of Ma.</p>
</caption>
<graphic xlink:href="feart-11-1202477-g001.tif"/>
</fig>
<p>Despite decades of considerable research, the Early Paleozoic orogeny remains uncertain with regard to its tectonic setting and geodynamic driving force (<xref ref-type="bibr" rid="B11">Charvet et al., 2010</xref>; <xref ref-type="bibr" rid="B87">Wang et al., 2010</xref>; <xref ref-type="bibr" rid="B35">Huang et al., 2013</xref>; <xref ref-type="bibr" rid="B73">Shu et al., 2014</xref>; <xref ref-type="bibr" rid="B106">Yu et al., 2016</xref>). Two opposing tectonic setting models of oceanic subduction-collision and intracontinental orogeny are proposed, controversy still exists regarding the Early Paleozoic &#x201c;Huanan Ocean&#x201d; in the SCB. Some researchers proposed that the Yangtze and Cathaysia Blocks were amalgamated together into the ancient South China continent during the amalgamation process of the Rodinia supercontinent in the Late Neoproterozoic and the Early Paleozoic &#x201c;Huanan Ocean&#x201d; did not exist (e.g., <xref ref-type="bibr" rid="B11">Charvet et al., 2010</xref>; <xref ref-type="bibr" rid="B35">Huang et al., 2013</xref>; <xref ref-type="bibr" rid="B93">Xia et al., 2014</xref>; <xref ref-type="bibr" rid="B74">Shu et al., 2015</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref>). While others believed that the &#x201c;Huanan Ocean&#x201d; existed in the Early Paleozoic and the oceanic subduction occurred (e.g., <xref ref-type="bibr" rid="B34">Hs&#xfc; et al., 1990</xref>; <xref ref-type="bibr" rid="B63">Qin et al., 2011</xref>; <xref ref-type="bibr" rid="B60">Peng et al., 2016a</xref>; <xref ref-type="bibr" rid="B61">Peng et al., 2016b</xref>; <xref ref-type="bibr" rid="B51">Liu et al., 2018</xref>). Based on the Early Paleozoic ultramafic-mafic rocks (e.g., <xref ref-type="bibr" rid="B100">Yao et al., 2012</xref>; <xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>; <xref ref-type="bibr" rid="B110">Zhang et al., 2015</xref>) and I-type granitoids (e.g., <xref ref-type="bibr" rid="B35">Huang et al., 2013</xref>; <xref ref-type="bibr" rid="B110">Zhang et al., 2015</xref>; <xref ref-type="bibr" rid="B106">Yu et al., 2016</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref>), a model of the Early Paleozoic magmatic activity in the SCB was related to the partially molten SCLM (Sub-Continental Lithospheric Mantle) heated by upwelling asthenosphere triggered by lithospheric delamination is proposed. However, there was no consensus concerning the geodynamic framework of the Early Paleozoic orogeny.</p>
<p>The Jiangnan Orogen is located in the southeastern margin of the Yangtze Block and is bound on its southeastern side by the Cathaysia Block along the Jiangshan-Shaoxing fault as the eastern boundary, with a width of ca. 120&#xa0;km and length of ca. 1,500&#xa0;km (<xref ref-type="fig" rid="F1">Figure 1B</xref>; <xref ref-type="bibr" rid="B82">Wang X. L. et al., 2007</xref>; <xref ref-type="bibr" rid="B99">Yao et al., 2014</xref>), which could be divided into the eastern and western segments by the border of Hunan and Jiangxi provinces. Due to poor exposure and thermo-tectonic modification (<xref ref-type="bibr" rid="B46">Li et al., 2010</xref>; <xref ref-type="bibr" rid="B71">Shu, 2012</xref>), the southwestern boundary of the western segment is unclear and several faults have been proposed, such as the Pingxiang-Gongcheng-Nanning fault (e.g., <xref ref-type="bibr" rid="B121">Zhou and Wen, 2021</xref>), the Chenzhou-Linwu fault (e.g., <xref ref-type="bibr" rid="B113">Zhao, 2015</xref>), and the Shizong-Mile-Luodian fault (e.g., <xref ref-type="bibr" rid="B22">Dong et al., 2015</xref>). The Jiangnan Orogen is considered to represent the subductional-collisional suture between the Yangtze and Cathaysia Blocks (<xref ref-type="bibr" rid="B99">Yao et al., 2014</xref>), which is a key to understanding the assembly and evolution of the SCB (<xref ref-type="bibr" rid="B82">Wang X. L. et al., 2007</xref>; <xref ref-type="bibr" rid="B48">Lin et al., 2008</xref>; <xref ref-type="bibr" rid="B11">Charvet et al., 2010</xref>; <xref ref-type="bibr" rid="B116">Zhao et al., 2016</xref>). Therefore, the temporal-spatial pattern and petrogenesis of the Early Paleozoic igneous rocks in the western segment can provide particular constraints on the tectonic setting and evolution of the Early Paleozoic orogeny (<xref ref-type="bibr" rid="B87">Wang et al., 2010</xref>; <xref ref-type="bibr" rid="B83">Wang et al., 2013a</xref>; <xref ref-type="bibr" rid="B118">Zhong et al., 2013</xref>; <xref ref-type="bibr" rid="B73">Shu et al., 2014</xref>; <xref ref-type="bibr" rid="B74">Shu et al., 2015</xref>). Moreover, previous studies are mostly focused on the granitoids in the SCB (e.g., <xref ref-type="bibr" rid="B35">Huang et al., 2013</xref>; <xref ref-type="bibr" rid="B115">Zhao et al., 2013</xref>; <xref ref-type="bibr" rid="B118">Zhong et al., 2013</xref>; <xref ref-type="bibr" rid="B106">Yu et al., 2016</xref>; <xref ref-type="bibr" rid="B6">Cai et al., 2017</xref>; <xref ref-type="bibr" rid="B95">Xin et al., 2020</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref>), while less attention has been paid on the Early Paleozoic volcanic-volcaniclastic rocks. Consequently, we studied the Early Paleozoic intrusive and extrusive rocks located in northeastern and central Guangxi province in the western segment, which are of great significance for constraining the Early Paleozoic magmatism, tectonic evolution, and geodynamic driving force of the SCB. Based on field geological investigation, we present new zircon U-Pb ages, Hf isotopic compositions, and whole-rock geochemical data for the Early Paleozoic igneous rocks to reveal their petrogenesis, and further offer new perspectives on the Early Paleozoic tectonic setting of the SCB.</p>
</sec>
<sec id="s2">
<title>2 Geological setting and sample descriptions</title>
<p>The Yangtze and Cathaysia Blocks were amalgamated and separated in multiple tectonic evolutions from the Mesoproterozoic to Neoproterozoic (<xref ref-type="bibr" rid="B12">Charvet et al., 1996</xref>; <xref ref-type="bibr" rid="B86">Wang et al., 2011</xref>; <xref ref-type="bibr" rid="B71">Shu, 2012</xref>; <xref ref-type="bibr" rid="B73">Shu et al., 2014</xref>; <xref ref-type="bibr" rid="B74">Shu et al., 2015</xref>). The basement of the Yangtze Block is Archean tonalitic-trondhjemitic-granodioritic (TTG) gneisses with ages of 3.2&#x2013;2.9&#xa0;Ga in the north (e.g., the Kongling Group) and Paleoproterozoic strata in the west (e.g., the Hekou Group), overlain by a Neoproterozoic to Cenozoic cover (<xref ref-type="bibr" rid="B64">Qiu et al., 2000</xref>; <xref ref-type="bibr" rid="B38">Jiao et al., 2009</xref>; <xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref>). The basement of the Cathaysia Block has a Paleoproterozoic origin (1.8&#x2013;2.0&#xa0;Ga), which is dominantly composed of schist, gneiss, amphibolite, migmatite and volcaniclastics (<xref ref-type="bibr" rid="B49">Liu et al., 2009</xref>; <xref ref-type="bibr" rid="B102">Yu et al., 2009</xref>; <xref ref-type="bibr" rid="B101">Yu et al., 2010</xref>; <xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>), while the Jiangnan Orogen consists mostly of the Paleoproterozoic to Early Neoproterozoic sedimentary strata and igneous rocks (<xref ref-type="bibr" rid="B81">Wang et al., 2008</xref>; <xref ref-type="bibr" rid="B74">Shu et al., 2015</xref>; <xref ref-type="bibr" rid="B114">Zhao et al., 2022</xref>).</p>
<p>Most of the Early Paleozoic igneous rocks in the SCB are distributed in southeastern margin of the Yangtze Block (the Jiangnan Orogen) and northwestern-western margin of the Cathaysia Block (<xref ref-type="fig" rid="F1">Figure 1B</xref>). Recently, the increasing discovery of S-type (e.g., <xref ref-type="bibr" rid="B86">Wang et al., 2011</xref>; <xref ref-type="bibr" rid="B108">Zhang et al., 2012</xref>; <xref ref-type="bibr" rid="B74">Shu et al., 2015</xref>), I-type (e.g., <xref ref-type="bibr" rid="B35">Huang et al., 2013</xref>; <xref ref-type="bibr" rid="B118">Zhong et al., 2013</xref>; <xref ref-type="bibr" rid="B110">Zhang et al., 2015</xref>; <xref ref-type="bibr" rid="B106">Yu et al., 2016</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref>), and A-type (<xref ref-type="bibr" rid="B25">Feng et al., 2014</xref>; <xref ref-type="bibr" rid="B6">Cai et al., 2017</xref>; <xref ref-type="bibr" rid="B95">Xin et al., 2020</xref>) granitoids, ultramafic-mafic (<xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>; <xref ref-type="bibr" rid="B118">Zhong et al., 2013</xref>; <xref ref-type="bibr" rid="B117">Zhong et al., 2014</xref>; <xref ref-type="bibr" rid="B116">Zhong et al., 2016</xref>; <xref ref-type="bibr" rid="B110">Zhang et al., 2015</xref>), and intermediate (<xref ref-type="bibr" rid="B119">Zhong et al., 2016</xref>) intrusive rocks, volcanic rocks (<xref ref-type="bibr" rid="B100">Yao et al., 2012</xref>; <xref ref-type="bibr" rid="B112">Zhang X. S. et al., 2017</xref>; <xref ref-type="bibr" rid="B62">Qin et al., 2017</xref>; <xref ref-type="bibr" rid="B51">Liu et al., 2018</xref>), and metamorphic rocks (<xref ref-type="bibr" rid="B84">Wang Y. J. et al., 2007</xref>; <xref ref-type="bibr" rid="B42">Li et al., 2011</xref>) from the SCB have been reported. Geochronological studies indicate that the magmatism in the Early Paleozoic initiated in the Late Ordovician (ca. 460&#xa0;Ma) and lasted until the Late Devonian (ca. 390&#xa0;Ma) (<xref ref-type="bibr" rid="B42">Li et al., 2011</xref>; <xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>; <xref ref-type="bibr" rid="B95">Xin et al., 2020</xref>; <xref ref-type="bibr" rid="B40">Kong et al., 2021</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref> and the related references).</p>
<p>In this study, granitoids from the Yuechengling pluton and volcaniclastic rocks from the Damingshan pluton located in the western segment of the Jiangnan Orogen were studied (<xref ref-type="fig" rid="F1">Figure 1B</xref>), aiming to constrain the petrogenesis of the igneous rocks and offer new perspectives on the tecno-thermal evolution and tectonic setting of the Early Paleozoic magmatic activity in the SCB. The sampling locations and mineral compositions of the samples are shown in <xref ref-type="fig" rid="F2">Figure 2</xref> and <xref ref-type="table" rid="T1">Table 1</xref>.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>Simplified geological map of <bold>(A)</bold> Yuechengling (modified after <xref ref-type="bibr" rid="B26">Feng et al., 2022</xref>) and <bold>(B)</bold> Damingshan area and sampling locations. 1-Quaternary, 2-Paleogene, 3-Cretaceous, 4-Triassic, 5-Permian, 6-Carboniferous, 7-Devonian, 8-Ordovician, 9-Cambrian, 10-Proterozoic, 11-Early Paleozoic granitoid, 12-Early Mesozoic granitoid, 13-Late Mesozoic granitoid, 14-fault, 15-sampling location, XZF-the Xin-Zi fault, NBF-the Nandan-Binyang fault.</p>
</caption>
<graphic xlink:href="feart-11-1202477-g002.tif"/>
</fig>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>The sampling location, lithology and mineral assemblages of the Yuechengling granitoids and the Damingshan volcaniclastic rocks.</p>
</caption>
<table>
<thead valign="top">
<tr>
<th align="left">Pluton</th>
<th align="left">Sample NO.</th>
<th align="left">Lithology</th>
<th align="left">Location</th>
<th align="left">Mineralogy</th>
</tr>
</thead>
<tbody valign="top">
<tr>
<td rowspan="3" align="left">Yuechengling</td>
<td align="left">21LDT-1</td>
<td align="left">granodiorite</td>
<td align="left">N25&#xb0;47&#x2032;4.6&#x2033;, E110&#xb0;40&#x2032;42.3&#x2033;</td>
<td align="left">quartz (50%) &#x2b; plagioclase (40%) &#x2b; K-feldspar (5%) &#x2b; biotite (5%)</td>
</tr>
<tr>
<td align="left">21LDT-2-01</td>
<td align="left">granodiorite</td>
<td align="left">N25&#xb0;47&#x2032;16.2&#x2033;, E110&#xb0;40&#x2032;37.2&#x2033;</td>
<td align="left">quartz (40%) &#x2b; plagioclase (20%) &#x2b; K-feldspar (20%) &#x2b; biotite (20%)</td>
</tr>
<tr>
<td align="left">21LDT-2-02</td>
<td align="left">granodiorite</td>
<td align="left">N25&#xb0;47&#x2032;14.4&#x2033;, E110&#xb0;40&#x2032;37.3&#x2033;</td>
<td align="left">quartz (45%) &#x2b; K-feldspar (30%) &#x2b; plagioclase (15%&#x2013;20%) &#x2b; biotite (5%&#x2013;10%)</td>
</tr>
<tr>
<td rowspan="3" align="left">Damingshan</td>
<td align="left">21DMS-1</td>
<td align="left">volcanic breccia</td>
<td rowspan="3" align="left">N23&#xb0;23&#x2032;04&#x2033;, E108&#xb0;28&#x2032;01&#x2033;</td>
<td align="left">detritus (60%): quartz (70%) &#x2b; plagioclase (20%) &#x2b; biotite (10%); matrix (40%): quartz &#x2b; sericite</td>
</tr>
<tr>
<td align="left">21DMS-2</td>
<td align="left">volcanic breccia</td>
<td align="left">detritus (50%): quartz (50%) &#x2b; biotite (10%) &#x2b; calcite (20%) &#x2b; feldspar (20%); matrix (50%): quartz &#x2b; calcite &#x2b; sericite</td>
</tr>
<tr>
<td align="left">21DMS-4</td>
<td align="left">volcanic breccia</td>
<td align="left">detritus (70%): quartz (90%) &#x2b; feldspar (5%) &#x2b; muscovite (5%) &#x2b; detritus (&#x3c;1%); matrix (30%): quartz &#x2b; sericite</td>
</tr>
</tbody>
</table>
</table-wrap>
<sec id="s2-1">
<title>2.1 The Yuechengling pluton</title>
<p>The Yuechengling pluton is located in the border region of Guangxi and Hunan Provinces, which is mainly composed of the Early Paleozoic granitoids with a surface area of more than 3,000&#xa0;km<sup>2</sup> (<xref ref-type="bibr" rid="B92">Wu et al., 2012</xref>; <xref ref-type="bibr" rid="B15">Chen et al., 2016</xref>). It showed a NEE-trending distribution with the outcropped strata of Proterozoic (Pt), Cambrian (&#x404;), Ordovician (O), Devonian (D), Carboniferous (C), Permian (P), Cretaceous (K), and Quaternary (Q) (<xref ref-type="fig" rid="F2">Figure 2A</xref>). There are two episodes of granitic magmatic activities and the Early Paleozoic (435&#x2013;422&#xa0;Ma) granite (<xref ref-type="bibr" rid="B115">Zhao et al., 2013</xref>; <xref ref-type="bibr" rid="B3">Bai et al., 2015</xref>; <xref ref-type="bibr" rid="B15">Chen et al., 2016</xref> and the related references) in the south and associated Early Mesozoic (236&#x2013;222&#xa0;Ma) granite (<xref ref-type="bibr" rid="B19">Chu et al., 2012</xref>; <xref ref-type="bibr" rid="B26">Feng et al., 2022</xref> and the related references) in the north were produced respectively. Many deposits of W-Sn-Mo-Pb-Zn-Cu are surrounding the contact zone between the pluton and strata, forming an ore-rich belt around the Yuechengling pluton (<xref ref-type="bibr" rid="B92">Wu et al., 2012</xref>; <xref ref-type="bibr" rid="B15">Chen et al., 2016</xref>). Many scholars have constrained the geochronological, lithological, geochemical, petrogenesis (e.g., <xref ref-type="bibr" rid="B115">Zhao et al., 2013</xref>; <xref ref-type="bibr" rid="B3">Bai et al., 2015</xref>; <xref ref-type="bibr" rid="B15">Chen et al., 2016</xref>) and mineralization of non-ferrous metals (e.g., <xref ref-type="bibr" rid="B15">Chen et al., 2016</xref>; <xref ref-type="bibr" rid="B111">Zhang W. L. et al., 2017</xref>; <xref ref-type="bibr" rid="B16">Chen et al., 2018</xref>) for the Early Paleozoic and Early Mesozoic granites in the study area. Despite numerous studies are available, disputes still exit and further work is needed to refine the tecno-thermal evolution and tectonic setting.</p>
<p>The granodiorite samples (21LDT-1, 21LDT-2-01, and 21LDT-2-02) were collected from south of the Yuechengling pluton (<xref ref-type="fig" rid="F2">Figure 2A</xref>), which have typical granitic textures (<xref ref-type="fig" rid="F3">Figure 3</xref>). These rocks consist mainly of quartz, plagioclase, K-feldspar, and biotite, while the accessory minerals are mainly magnetite and apatite (<xref ref-type="fig" rid="F3">Figure 3</xref>; <xref ref-type="table" rid="T1">Table 1</xref>). They have experienced variable degrees of alteration, and exhibit kaolinization and chloritization of K-feldspar and biotite, and sericitization of plagioclase, respectively (<xref ref-type="fig" rid="F3">Figure 3</xref>).</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Field, Hand specimen and microscopic photographs of the Yuechengling granitoids <bold>(A&#x2013;I)</bold> and the Damingshan volcaniclastic rocks <bold>(J&#x2013;O)</bold>. Abbreviations: Qtz-quartz, Pl-plagioclase, Kfs-K-feldspar, Bt-biotite, Mic-microcline, Chl-chlorite, Ser-sericite, Amp-amphibole, Fsp-feldspar.</p>
</caption>
<graphic xlink:href="feart-11-1202477-g003.tif"/>
</fig>
<sec id="s2-1-1">
<title>2.2 The Damingshan pluton</title>
<p>The Damingshan pluton is located in the southeastern margin of Youjiang rift basin, central Guangxi Province. The NW-SE trending Nandan-Binyang fault is the main fault, which passes across the Damingshan composite anticline from northwest to southeast. The strata outcropped are from Cambrian (&#x404;) to Quaternary (Q), with Silurian (S) and Jurassic (J) are missing (<xref ref-type="fig" rid="F2">Figure 2B</xref>). Ordovician distributed in the southwest of the Damingshan anticline in an NW-trending strip (<xref ref-type="fig" rid="F2">Figure 2B</xref>), with lithology of greywacke, shale, mudstone, pyroclastic rock, etc., and shows parallel unconformity with the underlying Cambrian strata and angular unconformity with the overlaying Devonian strata. Ordovician only outcropped at the Huang&#x2019;ai formation (O1<italic>h</italic>), which distributed in Longtoushan, Shanglin County. Previous studies for the Damingshan pluton mainly focused on deposits (<xref ref-type="bibr" rid="B7">Cai, 2012</xref>; <xref ref-type="bibr" rid="B30">Gan et al., 2022</xref>) by using geochronology (<xref ref-type="bibr" rid="B98">Yang et al., 2011</xref>) or geochemistry (<xref ref-type="bibr" rid="B120">Zhou, 2020</xref>) methods, only a few systematic chronology and geochemistry studies had been conducted on the igneous rocks (<xref ref-type="bibr" rid="B14">Chen, 2018</xref>; <xref ref-type="bibr" rid="B88">Wang et al., 2020</xref>).</p>
<p>The volcaniclastic samples (21DMS-1, 21DMS-2, and 21DMS-4) were collected from the Ordovician strata. The detritus consists of quartz, feldspar, calcite, biotite, and muscovite, most of the quartz and feldspar minerals have been sericitized (<xref ref-type="table" rid="T1">Table 1</xref>; <xref ref-type="fig" rid="F3">Figure 3</xref>). The component of the matrix is mainly quartz and sericite, with calcite only appearing in sample 21DMS-2 (<xref ref-type="table" rid="T1">Table 1</xref>; <xref ref-type="fig" rid="F3">Figure 3</xref>).</p>
</sec>
</sec>
</sec>
<sec id="s3">
<title>3 Analytical methods</title>
<p>Whole-rock major and trace element compositions were determined for the granitoid and volcaniclastic samples. The zircons from these samples were used for laser ablation-inductively coupled plasma-mass spectrometer (LA-ICP-MS) zircon U-Pb dating and multicollector-inductively coupled plasma-mass spectrometer (MC-ICP-MS) zircon Lu-Hf isotope analyses.</p>
<p>Major and trace element compositions were undertaken at Guangxi Key Laboratory of Exploration for Hidden Metallic ore Deposits, Guilin University of Technology. Major element compositions were determined using a ZSX Primus II X-ray fluorescence spectrometer (XRF) and the analytical accuracy was better than 2%. Trace element compositions were determined using an Agilent 7500cx inductively coupled plasma mass spectrometry (ICP-MS) and the analytical accuracy was better than 2%. The analytical procedures have been described by <xref ref-type="bibr" rid="B52">Liu X. J. et al. (2020)</xref>.</p>
<p>Zircon U-Pb dating and Hf isotope analyses were performed at Guangxi Key Laboratory of Hidden Metal Mineral Exploration at Guilin University of Technology. The instrument used for the zircon U-Pb dating was LA-ICP-MS, with a laser beam spot diameter of 32&#xa0;&#x3bc;m and a frequency of 6&#xa0;Hz. To ensure reliability of the analyses and stability of the instruments, standard samples were analyzed before and after each group of analyses, using the American national standard silicate glass NIST610. The external standard 91,500 was analyzed twice before and after each group of eight analyses, and internal standard samples were limited by GJ. The measured data were processed using ICPMSDataCal10.2 software, and the U-Pb harmonic graphs and age-weighted average graphs of samples were drawn using Isoplot v4.15. The zircon <italic>in situ</italic> Hf isotope analyses were performed using a high-resolution multi-receiver ICP-MS system equipped with an ESI New Wave 193 Ar F excimer laser. The methods were described by <xref ref-type="bibr" rid="B5">Bouvier et al. (2008)</xref>. Standard zircon GJ whose <sup>176</sup>Hf/<sup>177</sup>Hf value is &#x3d; 0.282000 &#xb1; 50 (2&#x3c3;) was used for external correction, initial <sup>176</sup>Hf/<sup>177</sup>Hf values calculations were based on Lu decay constant of 1.865 &#xd7; 10<sup>&#x2212;11</sup> yr<sup>&#x2212;1</sup> (<xref ref-type="bibr" rid="B70">Scherer et al., 2001</xref>). Model ages and <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values were calculated under the supposition that the <sup>176</sup>Lu/<sup>177</sup>Hf of average crust is 0.015, the <sup>176</sup>Hf/<sup>177</sup>Hf and <sup>176</sup>Lu/<sup>177</sup>Hf ratios of chondrite are 0.282772 and 0.0332, and ratios of depleted mantle at the present are 0.28325 and 0.0384, respectively (<xref ref-type="bibr" rid="B4">Blichert Toft and Albar&#xe8;de, 1997</xref>; <xref ref-type="bibr" rid="B31">Griffin et al., 2004</xref>).</p>
</sec>
<sec id="s4">
<title>4 Analytical results</title>
<sec id="s4-1">
<title>4.1 Zircon characteristics and U-Pb dating results</title>
<sec id="s4-1-1">
<title>4.1.1 The Yuechengling granitoids</title>
<p>Zircon U-Pb ages were obtained and shown in <xref ref-type="sec" rid="s12">Supplementary Table S1</xref>. Zircon grains of sample 21LDT-1, 21LDT-2&#x2013;01, and 21LDT-2&#x2013;02 are mostly shaped in prismatic and euhedral, only a few are irregular anhedral and ellipse shapes, mostly 80&#x2013;210&#xa0;&#x3bc;m long and 40&#x2013;80&#xa0;&#x3bc;m wide, with length/width ratios of 1:1&#x2013;4:1. As shown in the cathode luminescence (CL) images (<xref ref-type="fig" rid="F4">Figures 4A&#x2013;C</xref>), most of the zircon grains display a clear oscillatory zonation, which is typical of magmatic origin zircons.</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>Cathode luminescence (CL) images of zircons from the Yuechengling granitoids <bold>(A&#x2013;C)</bold> and the Damingshan volcaniclastic rocks <bold>(D&#x2013;F)</bold>.</p>
</caption>
<graphic xlink:href="feart-11-1202477-g004.tif"/>
</fig>
<p>Twenty-two spot analyses were conducted in sample 21LDT-1 (granodiorite) and the CL images show that most of the zircons have magmatic oscillatory zoning (<xref ref-type="fig" rid="F4">Figure 4A</xref>). 22 zircon grains exhibit Th/U values of &#x3e; 0.2 and 18 of them display age data with &#x2265; 90% concordance, giving a weighted mean age of 437.0 &#xb1; 2.7&#xa0;Ma (MSWD &#x3d; 2.9, <xref ref-type="fig" rid="F5">Figure 5A</xref>). The remaining four concordant grains show older <sup>206</sup>Pb/<sup>238</sup>U age of 859&#x2013;549&#xa0;Ma (<xref ref-type="sec" rid="s12">Supplementary Table S1</xref>), which are probably inherited or captured zircons.</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>Concordant zircon U-Pb dating diagrams of igneous rocks from the Yuechengling pluton <bold>(A&#x2013;C)</bold> and the Damingshan pluton <bold>(D&#x2013;F)</bold>.</p>
</caption>
<graphic xlink:href="feart-11-1202477-g005.tif"/>
</fig>
<p>A total of 17 analyses in sample 21LDT-2-01 (granodiorite) exhibit well-developed magmatic oscillatory zoning (<xref ref-type="fig" rid="F4">Figure 4B</xref>) and show concordant ages with &#x2265; 90% concordance and Th/U values of &#x3e; 0.2. Five zircon grains have consistent <sup>206</sup>Pb/<sup>238</sup>U ages ranging from 475&#xa0;Ma to 467&#xa0;Ma (<xref ref-type="sec" rid="s12">Supplementary Table S1</xref>), with a weighted mean age of 470.7 &#xb1; 2.9&#xa0;Ma (MSWD &#x3d; 0.62, <xref ref-type="fig" rid="F5">Figure 5B</xref>). 11 zircon grains have younger ages ranging from 431&#xa0;Ma to 440&#xa0;Ma, with a weighted mean age of 436.0 &#xb1; 1.8&#xa0;Ma (MSWD &#x3d; 0.55, <xref ref-type="fig" rid="F5">Figure 5B</xref>). The remaining one inherited zircon grains was formed in Neoproterozoic (754&#xa0;Ma).</p>
<p>Zircons from sample 21LDT-2-02 (granodiorite) exhibit magmatic oscillatory zoning in CL images (<xref ref-type="fig" rid="F4">Figure 4C</xref>) and Th/U values of &#x3e; 0.2. 20 zircon grains show concordant ages with &#x2265;90% concordance and 16 of them have consistent <sup>206</sup>Pb/<sup>238</sup>U ages ranging from 445&#xa0;Ma to 436&#xa0;Ma (<xref ref-type="sec" rid="s12">Supplementary Table S1</xref>), with a weighted mean age of 437.8 &#xb1; 1.4&#xa0;Ma (MSWD &#x3d; 0.92, <xref ref-type="fig" rid="F5">Figure 5C</xref>). The remaining four zircon grains show older age of 481&#x2013;462&#xa0;Ma.</p>
</sec>
<sec id="s4-1-2">
<title>4.1.2 The Damingshan volcaniclastic rocks</title>
<p>Zircon grains in sample 21DMS-1, 21DMS-2, and 21DMS-4 are mostly shaped in irregular anhedral and round-ellipse in shapes. They feature in size of 50&#x2013;320&#xa0;&#x3bc;m long and 45&#x2013;160&#xa0;&#x3bc;m wide, with length/width ratios of 1:1&#x2013;4:1. As shown in the CL images (<xref ref-type="fig" rid="F4">Figures 4D&#x2013;F</xref>), most of the zircon grains display a clear oscillatory zonation, which is typical of magmatic origin zircons.</p>
<p>A total of 31 analyses were conducted on zircon grains from sample 21DMS-1 (volcanic breccia), and all have concordant ages with &#x2265; 90% concordance and Th/U values of &#x3e; 0.2, defining an age range from 2,478&#xa0;Ma to 521&#xa0;Ma (<xref ref-type="sec" rid="s12">Supplementary Table S1</xref>; <xref ref-type="fig" rid="F5">Figure 5D</xref>). These grains define two detrital zircon age modes at ca. 970&#xa0;Ma and 540&#xa0;Ma. The oldest zircon grains have an Early Paleoproterozoic age (2,478&#xa0;Ma) and some detrital zircons define Mesoproterozoic-Neoproterozoic ages (1703&#x2013;645&#xa0;Ma). Eight zircons were formed in the Early Paleozoic (542&#x2013;521&#xa0;Ma) with the youngest age of 521 &#xb1; 6&#xa0;Ma (96% concordance), which is interpreted to be a maximum depositional age of the rock.</p>
<p>Almost all the 31 zircons in the 21DMS-2 (volcanic breccia) define concordant ages with &#x2265; 90% concordance. The high Th/U ratios suggest most of magmatic origin. The zircon grains show a wide age range spanning from 2,644&#xa0;Ma to 451&#xa0;Ma (<xref ref-type="sec" rid="s12">Supplementary Table S1</xref>; <xref ref-type="fig" rid="F5">Figure 5E</xref>), with a major Neoproterozoic peak (&#x223c;970&#xa0;Ma) and minor Early Paleozoic peak (&#x223c;530&#xa0;Ma). Three young zircon grains yield Early Paleozoic ages from 543&#xa0;Ma to 451&#xa0;Ma, the youngest age of 451 &#xb1; 4&#xa0;Ma (98% concordance) constraining the timing of deposition to be later than 451&#xa0;Ma.</p>
<p>All of the 24 zircon grains in sample 21DMS-4 (volcanic breccia) show concordant ages with &#x2265; 90% concordance. The zircon grains also define a broad age ranging from 2,610&#xa0;Ma to 540&#xa0;Ma (<xref ref-type="sec" rid="s12">Supplementary Table S1</xref>; <xref ref-type="fig" rid="F5">Figure 5F</xref>) with a peak at &#x223c;970&#xa0;Ma and also carry an Early Paleozoic peak at &#x223c;540&#xa0;Ma. Nine youngest concordant zircons show ages of Early Paleozoic between 552&#xa0;Ma and 540&#xa0;Ma with a weighted mean age of 542.7 &#xb1; 3.4&#xa0;Ma (MSWD &#x3d; 0.57, <xref ref-type="fig" rid="F5">Figure 5F</xref>), suggesting the maximum depositional age.</p>
</sec>
</sec>
<sec id="s4-2">
<title>4.2 Whole-rock major and trace elements</title>
<sec id="s4-2-1">
<title>4.2.1 Major elements</title>
<p>Whole-rock major and trace element compositions are presented in <xref ref-type="sec" rid="s12">Supplementary Table S2</xref>.</p>
<p>Granitoids from the Yuechengling pluton have SiO<sub>2</sub> contents of 66.12&#x2013;67.32&#xa0;wt%, low Fe<sub>2</sub>O<sub>3</sub>
<sup>T</sup> &#x2b; MgO contents of 5.98&#x2013;6.31&#xa0;wt% and Mg<sup>&#x23;</sup> values [Mg<sup>&#x23;</sup> &#x3d; atomic Mg/(Mg &#x2b; Fe)] of 48&#x2013;49, TiO<sub>2</sub> of 0.45&#x2013;0.48&#xa0;wt%, P<sub>2</sub>O<sub>5</sub> of 0.11&#x2013;0.13&#xa0;wt% and high Al<sub>2</sub>O<sub>3</sub> contents of 14.97&#x2013;16.30&#xa0;wt%. They have total alkali (ALK &#x3d; Na<sub>2</sub>O&#x2b; K<sub>2</sub>O) values of 6.10&#x2013;6.59&#xa0;wt% and A/CNK [A/CNK &#x3d; molar Al<sub>2</sub>O<sub>3</sub>/(CaO &#x2b; Na<sub>2</sub>O&#x2b; K<sub>2</sub>O)] values of 1.18&#x2013;1.55 with strongly peraluminous characteristics and plot in the granodiorite and high-K calc-alkaline series fields in the total alkali <italic>vs.</italic> alkali (TAS) and SiO<sub>2</sub> vs. K<sub>2</sub>O diagrams (<xref ref-type="fig" rid="F6">Figures 6A, B</xref>). Most of the samples have loss on ignition (L.O.I.) values of &#x3c;2.5&#xa0;wt% (1.02&#x2013;2.44&#xa0;wt%), indicating weak weathering or secondary alteration.</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>
<bold>(A)</bold> TAS diagram (after <xref ref-type="bibr" rid="B41">Le Maitre et al., 2005</xref>), <bold>(B)</bold> K<sub>2</sub>O vs. SiO<sub>2</sub> plot (after <xref ref-type="bibr" rid="B66">Rickwood, 1989</xref>), <bold>(C)</bold> primitive mantle-normalized trace element spider diagrams, and <bold>(D)</bold> chondrite-normalized REE patterns of the Yuechengling granitoids and the Damingshan volcaniclastic rocks.</p>
</caption>
<graphic xlink:href="feart-11-1202477-g006.tif"/>
</fig>
<p>In contrast, volcaniclastic rocks from the Damingshan pluton have variable SiO<sub>2</sub> contents of 61.23&#x2013;74.07&#xa0;wt%, CaO of 0.74&#x2013;2.91&#xa0;wt%, Fe<sub>2</sub>O<sub>3</sub>
<sup>T</sup> &#x2b; MgO of 4.34&#x2013;9.70&#xa0;wt% and Mg<sup>&#x23;</sup> values of 47&#x2013;56, ALK values of 4.95&#x2013;6.08&#xa0;wt%, low TiO<sub>2</sub> of 0.44&#x2013;0.62&#xa0;wt% and relatively high Al<sub>2</sub>O<sub>3</sub> of 11.44&#x2013;14.00&#xa0;wt%. The samples have relatively high L.O.I. values ranging from 2.46&#xa0;wt% to 4.77&#xa0;wt%, probably caused by calcites filled in rock fissures. In the TAS (<xref ref-type="fig" rid="F6">Figure 6A</xref>) and SiO<sub>2</sub> vs. K<sub>2</sub>O (<xref ref-type="fig" rid="F6">Figure 6B</xref>) diagrams, the samples fall into the dacite-rhyolite field and show calc-alkaline to high-K calc-alkaline characteristics.</p>
</sec>
<sec id="s4-2-2">
<title>4.2.2 Trace elements</title>
<p>Samples from the Yuechengling and Damingshan plutons have similar trace element compositions, which suggests the similarity of their petrogenesis. In the primitive mantle-normalized trace element spider diagrams (<xref ref-type="fig" rid="F6">Figure 6C</xref>), all the samples show relatively enrichment of large ion lithophile elements (LILEs, e.g., Rb, Th, U, K) and Pb, relative depletion of Ba, Sr, and high field strength elements (HFSEs, e.g., Nb, Ta, P, Ti), and no Zr and Hf anomalies. These features are similar to those of Early Paleozoic granitoids from Yuechengling (<xref ref-type="bibr" rid="B47">Lin et al., 2017</xref>).</p>
<p>The samples have total rare Earth element (&#x3a3;REE) values of 124&#x2013;181&#xa0;ppm, relatively enrichment in light rare Earth elements (LREEs, <xref ref-type="fig" rid="F6">Figure 6D</xref>), and relatively depletion in heavy rare Earth elements (HREEs, <xref ref-type="fig" rid="F6">Figure 6D</xref>), with the LREE/HREE ratios ranging from 7.53 to 10.43 (<xref ref-type="sec" rid="s12">Supplementary Table S2</xref>). The chondrite-normalized REE patterns (<xref ref-type="fig" rid="F6">Figure 6D</xref>) show that the samples have right-inclined HREE patterns, with La<sub>N</sub>/Yb<sub>N</sub> ratios ranging from 8.72 to 12.24, which indicate weak-moderate fractionation between HREEs and LREEs. Besides, the samples exhibit moderate negative Eu anomalies with &#x3b4;Eu values of 0.63&#x2013;0.75 [<xref ref-type="fig" rid="F6">Figure 6D</xref>, <xref ref-type="sec" rid="s12">Supplementary Table S2</xref>, &#x3b4;Eu &#x3d; Eu<sub>N</sub>/(Sm &#xd7; Gd)<sup>1/2</sup>], which suggest that there might be plagioclase residue in the source area or its parental magma suffered plagioclase fractionation during its evolution.</p>
</sec>
</sec>
<sec id="s4-3">
<title>4.3 Zircon Lu-Hf isotope</title>
<p>As shown in <xref ref-type="sec" rid="s12">Supplementary Table S3</xref>, <italic>In situ</italic> Lu-Hf isotope analyses of zircons that have &#x2265; 90% concordance U-Pb ages have been carried out. <sup>176</sup>Lu/<sup>177</sup>Hf ratios of the zircon grains range from 0.000015 to 0.002425. Most of them have <sup>176</sup>Lu/<sup>177</sup>Hf ratios less than 0.002, indicating no accumulation of radiogenic Hf after zircon formation and the ratios of Hf isotopes are not affected by later episodes of partial melting and fractional crystallization, the ratios can essentially represent the Lu-Hf system when the zircon formed (<xref ref-type="bibr" rid="B91">Wu et al., 2007</xref>).</p>
<sec id="s4-3-1">
<title>4.3.1 The Yuechengling granitoids</title>
<p>Thirteen zircons from sample 21LDT-1 (granodiorite) with concordant ages of 460&#x2013;432&#xa0;Ma display uniform (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> (initial ratio) values of 0.282298&#x2013;0.282422 (<xref ref-type="fig" rid="F7">Figure 7A</xref>), negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values ranging from &#x2212;7.49 to &#x2212;3.12, and two-stage Hf isotope model ages (T<sub>DM2</sub>) of 1.88&#x2013;1.60&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>). Two inherited or captured zircons with ages of 549 and 859&#xa0;Ma yielded (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> values of 0.282414 and 0.281963 (<xref ref-type="fig" rid="F7">Figure 7A</xref>), negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values of &#x2212;0.90 and &#x2212;9.89, T<sub>DM2</sub> ages of 2.37 and 1.55&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>), respectively.</p>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>Diagrams of Lu-Hf isotopic data for zircons from the Yuechengling granitoids and the Damingshan volcaniclastic rocks. Plots of <bold>(A)</bold> U-Pb ages vs. (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub>, <bold>(B)</bold> U-Pb ages vs. <italic>&#x3b5;</italic>
<sub>Hf</sub>(t), Histograms of <bold>(C)</bold> <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values and <bold>(D)</bold> Hf isotope two-stage model ages.</p>
</caption>
<graphic xlink:href="feart-11-1202477-g007.tif"/>
</fig>
<p>The Lu-Hf analyses were performed on 14 Early Paleozoic (475&#x2013;431&#xa0;Ma) zircons from sample 21LDT-2&#x2013;01 (granodiorite), and these zircons show (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> values of 0.282278&#x2013;0.282388 (<xref ref-type="fig" rid="F7">Figure 7A</xref>), corresponding to negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values of &#x2212;8.24 to &#x2212;4.33 and T<sub>DM2</sub> age of 1.92&#x2013;1.68&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>). The oldest zircon (754&#xa0;Ma) display relatively high (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> value of 0.282188 (<xref ref-type="fig" rid="F7">Figure 7A</xref>), negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) value of &#x2212;4.28, and T<sub>DM2</sub> age of 1.93&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>).</p>
<p>Fifteen zircons from sample 21LDT-2-02 (granodiorite) with the ages of 481&#x2013;439&#xa0;Ma were analyzed, results show that they have similar characteristics to the granitoid samples above, which contains (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> values of 0.282171&#x2013;0.282379 (<xref ref-type="fig" rid="F7">Figure 7A</xref>) that correspond to negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values ranging from &#x2212;11.98 to &#x2212;4.43 and T<sub>DM2</sub> ages of 2.16 to 1.70&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>).</p>
</sec>
<sec id="s4-3-2">
<title>4.3.2 The Damingshan volcaniclastic rocks</title>
<p>Five zircons with the ages of 542&#x2013;521&#xa0;Ma from sample 21DMS-1 (volcanic breccia) show consistent (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> values ranging from 0.282090 to 0.282125 (<xref ref-type="fig" rid="F7">Figure 7A</xref>), with negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values of &#x2212;12.53 to &#x2212;11.27, and T<sub>DM2</sub> ages of 2.28 to 2.20&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>), while 13 Mesoproterozoic-Neoproterozoic (1703&#x2013;645&#xa0;Ma) zircons have (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> values ranging from 0.281646 to 0.282406 (<xref ref-type="fig" rid="F7">Figure 7A</xref>), with both negative and obviously positive <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values ranging from &#x2212;11.10 to 7.18, corresponding to variable T<sub>DM2</sub> ages ranging from 2.79 to 1.43&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>). The remaining Early Paleoproterozoic (2,455&#xa0;Ma) and Late Paleoproterozoic (1996&#xa0;Ma) zircons have (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> values of 0.280859 and 0.281099 (<xref ref-type="fig" rid="F7">Figure 7A</xref>), obviously negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values of &#x2212;12.48 and &#x2212;14.58, T<sub>DM2</sub> ages of 3.79 and 3.56&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>), respectively.</p>
<p>The youngest (451&#xa0;Ma) and the other Early Paleozoic (528&#xa0;Ma) zircons from sample 21DMS-2 (volcanic breccia) display (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> values of 0.282404&#x2013;0.282142 (<xref ref-type="fig" rid="F7">Figure 7A</xref>), corresponding to negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values of &#x2212;3.42 to &#x2212;10.99 and T<sub>DM2</sub> ages of 2.17&#x2013;1.63&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>). 15 zircons with Mesoproterozoic-Neoproterozoic ages (1712&#x2013;608&#xa0;Ma) yielded higher (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> values vary from 0.281422 to 0.282561 (<xref ref-type="fig" rid="F7">Figure 7A</xref>), extremely negative to obviously positive <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values of &#x2212;27.54 to 8.73, and variable T<sub>DM2</sub> ages vary from 3.26&#x2013;1.13&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>). The remaining three Neoarchean-Paleoproterozoic zircons with ages from 2,644&#xa0;Ma to 2028&#xa0;Ma show a narrow range of (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> values (0.281118&#x2013;0.281386) (<xref ref-type="fig" rid="F7">Figure 7A</xref>), corresponding to both negative and positive <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values of &#x2212;3.63 to 2.22, and T<sub>DM2</sub> ages of 3.08&#x2013;2.82&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>).</p>
<p>In sample 21DMS-4 (volcanic breccia), 7 zircons with the ages of 552&#xa0;Ma to 540&#xa0;Ma have (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> values of 0.282065&#x2013;0.282177 (<xref ref-type="fig" rid="F7">Figure 7A</xref>), obviously negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values of &#x2212;13.38 to &#x2212;9.43, and T<sub>DM2</sub> ages of 2.33&#x2013;2.08 (<xref ref-type="fig" rid="F7">Figure 7B</xref>), respectively. 12 Mesoproterozoic-Neoproterozoic (1708&#x2013;737&#xa0;Ma) zircons exhibit variable (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> values (0.281573&#x2013;0.282242) (<xref ref-type="fig" rid="F7">Figure 7A</xref>) that correspond to obviously negative to positive <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values of &#x2212;15.26 to 5.08 and variable T<sub>DM2</sub> ages (2.69&#x2013;1.59&#xa0;Ga) (<xref ref-type="fig" rid="F7">Figure 7B</xref>). The oldest zircon with a Neoarchean age of 2,610&#xa0;Ma shows the lowest (<sup>176</sup>Lu/<sup>177</sup>Hf)<sub>i</sub> value of 0.281260, corresponding to the highest positive <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) value of 5.45 and the oldest T<sub>DM2</sub> age of 2.78&#xa0;Ga (<xref ref-type="fig" rid="F7">Figure 7B</xref>).</p>
</sec>
</sec>
</sec>
<sec sec-type="discussion" id="s5">
<title>5 Discussion</title>
<sec id="s5-1">
<title>5.1 Formation age of the igneous rocks</title>
<p>Salient information from previous geochronological studies of the Early Paleozoic igneous rocks from the SCB have been reported in the past few years, showing that the igneous rocks were formed between ca. 460&#xa0;Ma and ca. 390&#xa0;Ma, and peaked at ca. 440&#x2013;420&#xa0;Ma (<xref ref-type="bibr" rid="B42">Li et al., 2011</xref>; <xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>; <xref ref-type="bibr" rid="B95">Xin et al., 2020</xref>; <xref ref-type="bibr" rid="B40">Kong et al., 2021</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref> and the related references). Previous studies based on the Early Paleozoic granitoids from the Yuechengling pluton were aged by using LA-ICP-MS zircon U-Pb (<xref ref-type="bibr" rid="B115">Zhao et al., 2013</xref>; <xref ref-type="bibr" rid="B15">Chen et al., 2016</xref>; <xref ref-type="bibr" rid="B47">Lin et al., 2017</xref>; <xref ref-type="bibr" rid="B16">Chen et al., 2018</xref>), zircon SHRIMP U-Pb (<xref ref-type="bibr" rid="B3">Bai et al., 2015</xref>), and SIMS zircon U-Pb (<xref ref-type="bibr" rid="B19">Chu et al., 2012</xref>) dating methods and obtained age data displaying a wide emplacement age peaked at 435&#x2013;422&#xa0;Ma. Our new LA-ICP-MS zircon U-Pb age data further constrain the emplacement age of the granitoids from the Yuechengling pluton to be 438&#x2013;436&#xa0;Ma.</p>
<p>In contrast, very few geochronological studies have been conducted for the Early Paleozoic igneous rocks from the Damingshan area, with the reported ages of 441&#x2013;432&#xa0;Ma for the granitoids (<xref ref-type="bibr" rid="B14">Chen, 2018</xref>; <xref ref-type="bibr" rid="B88">Wang et al., 2020</xref>), but a vacancy for the volcaniclastic rocks. In this study, zircons from the volcaniclastic rocks are mainly inherited or captured zircons, and the youngest concordant zircons from three samples are 521 &#xb1; 6, 451 &#xb1; 4, and 540 &#xb1; 6&#xa0;Ma, respectively. Since the volcaniclastic rocks are commonly deposited soon after a volcanic eruption, its deposited age would be close to the volcanic eruption age. And the volcanic eruption age could be constrained by the youngest group or single igneous zircon age in the volcaniclastic rocks. Consequently, we suggest that the volcaniclastic rocks should be formed by an Early Paleozoic volcanic eruption which is later than 451&#xa0;Ma. In addition, the inherited zircons from Neoarchean to Neoproterozoic indicated that ancient materials might exist in their source region.</p>
<p>In summary, the emplacement age of the Yuechengling granitoids constrained to be ca. 437&#xa0;Ma while the deposited age of the Damingshan volcaniclastic rocks to be later than 451&#xa0;Ma.</p>
</sec>
<sec id="s5-2">
<title>5.2 Genetic type of the Yuechengling granitoids</title>
<p>The granites are commonly divided into I-, S-, and A-types according to the nature of protolith and petrographical and geochemical features (<xref ref-type="bibr" rid="B10">Chappell and White, 1974</xref>; <xref ref-type="bibr" rid="B54">Loiselle and Wones, 1979</xref>). Studies have shown that feldspar is mostly alkali feldspar in A-type granites, often albite-orthoclase solid solutions or intergrowths, and micrographic intergrowths of quartz and alkali feldspars are very common (<xref ref-type="bibr" rid="B21">Collins et al., 1982</xref>). However, the Yuechengling granitoids consist of quartz, plagioclase, K-feldspar, biotite, magnetite, and apatite, being inconsistent with the typical petrographic characteristics of A-type granites. Compared with I-type and S-type granites, A-type granites can be distinguished from their high Zr &#x2b; Nb &#x2b; Ce &#x2b; Y contents (average value &#x3d; 350&#xa0;ppm) and FeO<sup>T</sup>/MgO ratios (average value &#x3d; 10), and enrichment in HFSEs (e.g., Nb and Ta) (<xref ref-type="bibr" rid="B89">Whalen et al., 1987</xref>). Geochemical data of the Yuechengling granitoids display low Zr &#x2b; Nb &#x2b; Ce &#x2b; Y contents (246&#x2013;275&#xa0;ppm; average value &#x3d; 257) and low FeO<sup>T</sup>/MgO ratios (1.84&#x2013;1.93; average value &#x3d; 1.87) (<xref ref-type="sec" rid="s12">Supplementary Table S2</xref>), lower than the limit and being inconsistent with the Fe-rich characteristics of A-type granites (<xref ref-type="bibr" rid="B89">Whalen et al., 1987</xref>). The depletion of HFSEs (Nb, Ta, P, Ti) is also different from typical A-type granites but similar to I- and S-type granites (<xref ref-type="fig" rid="F6">Figure 6C</xref>). Moreover, all the granitoids from this study fall in the range of unfractionated and fractionated I- and S-type granites on the Zr &#x2b; Nb &#x2b; Ce &#x2b; Y <italic>vs.</italic> FeO<sup>T</sup>/MgO (<xref ref-type="fig" rid="F8">Figure 8A</xref>) and Zr &#x2b; Nb &#x2b; Ce &#x2b; Y vs. (K<sub>2</sub>O &#x2b; Na<sub>2</sub>O)/CaO diagrams (<xref ref-type="fig" rid="F8">Figure 8B</xref>), which resembles the Yuechengling granitoids reported by <xref ref-type="bibr" rid="B15">Chen et al. (2016)</xref>, <xref ref-type="bibr" rid="B18">Cheng et al. (2016)</xref>, and <xref ref-type="bibr" rid="B16">Chen et al. (2018)</xref>, with only a few samples showing A-type characteristics which could be produced by strong fractionated S- or I- type granites (<xref ref-type="bibr" rid="B8">Champion and Bultitude, 2013</xref>).</p>
<fig id="F8" position="float">
<label>FIGURE 8</label>
<caption>
<p>Petrogenetic discrimination diagrams of the Yuechengling granitoids: <bold>(A)</bold> Zr &#x2b; Nb &#x2b; Ce &#x2b; Y vs. FeO<sup>T</sup>/MgO; <bold>(B)</bold> Zr &#x2b; Nb &#x2b; Ce &#x2b; Y vs. (K<sub>2</sub>O&#x2b; Na<sub>2</sub>O)/CaO, <bold>(C)</bold> SiO<sub>2</sub> vs. FeO<sup>T</sup>/(FeO<sup>T</sup> &#x2b; MgO), <bold>(D)</bold> ACF diagram. FG-fractionated M-, I-, and S-type granites; OGT-unfractionated M-, I-, and S-type granites. <bold>(A,B)</bold> are after <xref ref-type="bibr" rid="B89">Whalen et al. (1987)</xref>, <bold>(C)</bold> is after <xref ref-type="bibr" rid="B29">Frost et al. (2001)</xref>, <bold>(D)</bold> is after <xref ref-type="bibr" rid="B9">Chappell and White (1992)</xref>. Previous data of Yuechengling granitoids are from <xref ref-type="bibr" rid="B15">Chen et al. (2016)</xref>, <xref ref-type="bibr" rid="B18">Cheng et al. (2016)</xref>, and <xref ref-type="bibr" rid="B16">Chen et al. (2018)</xref>.</p>
</caption>
<graphic xlink:href="feart-11-1202477-g008.tif"/>
</fig>
<p>I-type and S-type granites have similar mineralogical and geochemical compositions, yet there are some differences. I-type granites contain hornblende and pyroxene, with normative mineral C (Corundum) content of &#x3c; 1 (<xref ref-type="bibr" rid="B10">Chappell and White, 1974</xref>). The granitoids from this study do not have a mineralogy typical of I-type granites, all the studied samples do not contain hornblende or pyroxene with normative mineral C contents of &#x3e; 1 (2.80&#x2013;5.87; average value &#x3d; 3.89). Furthermore, I-type granites are metaluminous to weakly peraluminous (A/CNK value &#x3c; 1.1) and have relatively high Na<sub>2</sub>O contents (&#x3e;3.2&#xa0;wt%; <xref ref-type="bibr" rid="B9">Chappell and White, 1992</xref>). The studied granitoids are all strongly peraluminous granitoids, with high A/CNK values of 1.18&#x2013;1.55 (average value &#x3d; 1.32, with all &#x3e; 1.1), A/NK values of &#x3e; 1.0 (1.77&#x2013;2.00; average value &#x3d; 1.85), and relatively low Na<sub>2</sub>O contents ranging from 2.78 to 3.13&#xa0;wt% (average value &#x3d; 2.90&#xa0;wt%, all &#x3c; 3.2&#xa0;wt%; <xref ref-type="sec" rid="s12">Supplementary Table S2</xref>), which are typical characteristics of S-type granites. Moreover, on the SiO<sub>2</sub> vs. FeO<sup>T</sup>/(FeO<sup>T</sup> &#x2b; MgO) (<xref ref-type="fig" rid="F8">Figure 8C</xref>) and ACF diagrams (<xref ref-type="fig" rid="F8">Figure 8D</xref>), the granitoids are all distributed in the S-type range, which is similar to previous studies from the Yuechengling pluton, furthering S-type affinity.</p>
</sec>
<sec id="s5-3">
<title>5.3 Origin of the Early Paleozoic igneous rocks</title>
<sec id="s5-3-1">
<title>5.3.1 The Yuechengling granitoids</title>
<p>S-type granites are usually characterized by felsic compositions with low Fe &#x2b; Mg contents less than 3%&#x2013;4% at reasonable crustal pressures and temperatures (<xref ref-type="bibr" rid="B8">Champion and Bultitude, 2013</xref> and references therein), while the Yuechengling granitoids display high-maficity feature with relatively high Fe &#x2b; Mg contents of 5.98&#x2013;6.31&#xa0;wt%. Several different mechanisms of this feature have been proposed, including 1) source heterogeneity, especially heterogeneous continental crustal material sources (e.g., <xref ref-type="bibr" rid="B79">Villaros et al., 2012</xref>); 2) magma mixing, incorporation of mantle-derived mafic magma will lead to mafic feature (<xref ref-type="bibr" rid="B20">Clemens et al., 2011</xref>; <xref ref-type="bibr" rid="B8">Champion and Bultitude, 2013</xref>); 3) selective entrainment of peritectic/restitic and accessory minerals, especially the peritectic garnet (e.g., <xref ref-type="bibr" rid="B122">Zhu et al., 2020</xref>; <xref ref-type="bibr" rid="B75">Song and Xu, 2022</xref>); 4) hydrothermal alteration, the hydrothermal fluids can bring Fe and Mg components into the granites (e.g., <xref ref-type="bibr" rid="B75">Song and Xu, 2022</xref>). Since no peritectic/restitic garnet was contained in the Yuechengling granitoids (<xref ref-type="table" rid="T1">Table 1</xref>), the mechanism of the entrainment of peritectic garnet was excluded. Thus, a full assessment of the partial melting, source heterogeneity, magma mixing, and fractional crystallization in the magmatic evolution process and the post-magmatic hydrothermal alteration could be accounted for petrogenesis and high-maficity feature of the Yuechengling granitoids.</p>
<sec id="s5-3-1-1">
<title>5.3.1.1 Partial melting and source heterogeneity</title>
<p>Zircon Lu-Hf isotope is of great significance for the study of magmatic evolution and source tracing, since it has extremely high closure temperature, which can maintain primitive Hf isotopic composition even under high-grade metamorphic conditions (<xref ref-type="bibr" rid="B91">Wu et al., 2007</xref>). The Yuechengling granitoids have negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values ranging from &#x2212;11.98 to &#x2212;0.90, and corresponding T<sub>DM2</sub> ages distributed from 2.37 to 1.55&#xa0;Ga (<xref ref-type="fig" rid="F7">Figures 7B&#x2013;D</xref>; <xref ref-type="sec" rid="s12">Supplementary Table S3</xref>), indicating that they might be derived from a crustal source of Paleoproterozoic basement. The granitoids have Rb/Sr ratios ranging from 0.95 to 1.25 (average value &#x3d; 1.1), which are higher than the mantle-derived granitoids (Rb/Sr &#x3c; 0.05) and crust-mantle-sourced granitoids (Rb/Sr &#x3d; 0.05&#x2013;0.50), but consistent with the range of crust-derived granites (Rb/Sr &#x3e; 0.5; <xref ref-type="bibr" rid="B76">Sylvester, 1998</xref>). They have Nb/Ta ratios (7.89&#x2013;8.4, average &#x3d; 8.21) that close to the average value of continental crust (Nb/Ta &#x3d; 11) and significantly less than the average value of primitive mantle (Nb/Ta &#x3d; 17.8; <xref ref-type="bibr" rid="B76">Sylvester, 1998</xref>). All the granitoids are characterized by depletion of Nb, Ti and enrichment of Pb (<xref ref-type="fig" rid="F6">Figure 6C</xref>), which furthered a crustal source.</p>
<p>There is little controversy about the sources of peraluminous, crustal-evolved, S-type granitic magma, which are derived from partial melting of meta-sedimentary rocks (<xref ref-type="bibr" rid="B20">Clemens et al., 2011</xref>). However, some scholars have shown that some S-type granitoids in the SCB are derived from a heterogeneous source (e.g., <xref ref-type="bibr" rid="B122">Zhu et al., 2020</xref>). The studied granitoids contained high Al<sub>2</sub>O<sub>3</sub> contents (14.97&#x2013;16.30&#xa0;wt%) and show peraluminous characteristics (A/CNK value &#x3d; 1.18&#x2013;1.55, <xref ref-type="sec" rid="s12">Supplementary Table S2</xref>), which can be produced by fractional crystallization of hornblende from subaluminous melts (A/CNK value &#x3c; 1, <xref ref-type="bibr" rid="B107">Zen, 1986</xref>) or partial melting of meta-igneous source rocks (<xref ref-type="bibr" rid="B65">Reichardt and Weinberg, 2012</xref>). However, combining with previous studies, the A/CNK values of the Yuechengling granitoids are constant with the increase of SiO<sub>2</sub> contents (<xref ref-type="fig" rid="F9">Figure 9A</xref>) and show negative Eu anomalies (<xref ref-type="fig" rid="F6">Figure 6D</xref>), being inconsistent with fractional crystallization of hornblende from subaluminous melts (<xref ref-type="bibr" rid="B37">Jiang and Zhu, 2017</xref>). Moreover, melts produced by partial melting of meta-igneous source rocks usually display enrichments in Na (K<sub>2</sub>O/Na<sub>2</sub>O &#x3c; 1), Sr (Sr/Rb &#x3e; 10), and Eu (&#x3b4;Eu &#x3e; 1) (<xref ref-type="bibr" rid="B65">Reichardt and Weinberg, 2012</xref>). Our samples contain high K<sub>2</sub>O/Na<sub>2</sub>O ratios (1.11&#x2013;1.26), low Sr/Rb ratios (0.8&#x2013;1.06) and display depletion in Eu (<xref ref-type="sec" rid="s12">Supplementary Table S2</xref>; <xref ref-type="fig" rid="F6">Figure 6C</xref>), excluding partial melting of meta-igneous source rocks. Generally, melts derived from metapelite show relatively low CaO/Na<sub>2</sub>O ratios of &#x3c; 0.3 and metagreywacke-derived melts contain higher CaO/Na<sub>2</sub>O ratios of 0.3&#x2013;1.5 (<xref ref-type="bibr" rid="B76">Sylvester, 1998</xref>), and granitoids of this study have variable CaO/Na<sub>2</sub>O ratios of 0.22&#x2013;1.11. Combining with previous data, on the Rb/Sr vs. CaO/Na<sub>2</sub>O and Rb/Sr vs. Rb/Ba diagrams (<xref ref-type="fig" rid="F9">Figures 9C, D</xref>), the Yuechengling granitoids are distributed both in the ranges of clay-poor and clay-rich sources, demonstrating the granitoids might be the products of pelite and greywacke melting. In summary, we suggest heterogeneity of meta-sedimentary sources may contribute to the granitoids, and they are derived from a crustal source with both meta-greywacke and meta-pelite components of the ancient basement.</p>
<fig id="F9" position="float">
<label>FIGURE 9</label>
<caption>
<p>Petrogenetic discrimination diagrams of the Yuechengling granitoids. <bold>(A)</bold> SiO<sub>2</sub> vs. A/CNK, <bold>(B)</bold> SiO<sub>2</sub> vs. K<sub>2</sub>O, <bold>(C)</bold> Rb/Sr vs. CaO/Na<sub>2</sub>O, <bold>(D)</bold> Rb/Sr vs. Rb/Ba. <bold>(C)</bold> is after <xref ref-type="bibr" rid="B44">Li et al. (2003)</xref>, <bold>(D)</bold> is after <xref ref-type="bibr" rid="B76">Sylvester (1998)</xref>. Previous data of Yuechengling granitoids are from <xref ref-type="bibr" rid="B15">Chen et al. (2016)</xref>, <xref ref-type="bibr" rid="B18">Cheng et al. (2016)</xref>, and <xref ref-type="bibr" rid="B16">Chen et al. (2018)</xref>.</p>
</caption>
<graphic xlink:href="feart-11-1202477-g009.tif"/>
</fig>
</sec>
<sec id="s5-3-1-2">
<title>5.3.1.2 Magma mixing and hydrothermal alteration</title>
<p>Recently, a growing number of the Early Paleozoic ultramafic-mafic rocks have been reported in the SCB (e.g., <xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>; <xref ref-type="bibr" rid="B118">Zhong et al., 2013</xref>; <xref ref-type="bibr" rid="B117">2014</xref>; <xref ref-type="bibr" rid="B119">2016</xref>; <xref ref-type="bibr" rid="B110">Zhang et al., 2015</xref>), indicating mantal-derived materials involved in generation of the subaluminous felsic magma, and the incorporation of mantle-derived mafic magma will trigger more mafic features such as high ferromagnesian contents of the melts (<xref ref-type="bibr" rid="B20">Clemens et al., 2011</xref>). Magma mixing process has been widely discussed on the genesis of the Early Paleozoic granitoids in the SCB, with inputting of mantle-derived materials (e.g., <xref ref-type="bibr" rid="B108">Zhang et al., 2012</xref>; <xref ref-type="bibr" rid="B93">Xia et al., 2014</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref>). Generally, variable zircon <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values ranging from negative to positive are considered as a result of mixing between crust-and mantle-derived magma (e.g., <xref ref-type="bibr" rid="B93">Xia et al., 2014</xref>). However, the Yuechengling granitoids have negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values (&#x2212;11.98 to &#x2212;0.90), which indicates that they were derived from a crustal source with no significant mixing between crust- and mantle-derived magma. Granitoids with high Mg<sup>&#x23;</sup> values (commonly &#x3e; 50) are possibly having a contribution of mantle-derived components to their parental magma (e.g., <xref ref-type="bibr" rid="B1">Abdallsamed et al., 2017</xref>). Samples of this study have Mg<sup>&#x23;</sup> values of 48&#x2013;49 (all &#x3c; 50), furthering no mixing occurred. Moreover, on the SiO<sub>2</sub> vs. A/CNK (<xref ref-type="fig" rid="F9">Figure 9A</xref>) diagram, they do not display an obvious trend of magma mixing combining our new data with previous studies. These evidences indicate no certain degree of magma mixing, suggesting that mantle-derived materials were not involved and the model of magma mixing is excluded.</p>
<p>Studies have shown that post-magmatic tectonic-thermal events can lead S-type granites to more mafic features, the hydrothermal fluids can bring Fe and Mg components into granites (e.g., <xref ref-type="bibr" rid="B75">Song and Xu, 2022</xref>). The granitoids from our study exhibit kaolinization and chloritization of K-feldspar and biotite, respectively, accompanied by sericitization of plagioclase. These petrographic characteristics indicate that they have been modified by variable degrees of intermediate- and low-temperature hydrothermal alteration. At the same time, hornblende can retrogress to biotite under hydrothermal conditions, which explains the absence of hornblende in the granodiorite samples. Moreover, most of the deposits in the Yuechengling area are considered related to magmatic-hydrothermal activities (<xref ref-type="bibr" rid="B92">Wu et al., 2012</xref>; <xref ref-type="bibr" rid="B15">Chen et al., 2016</xref>). Thus, the hydrothermal alteration can be the most reasonable explanation for the high-maficity feature of the granitoids in this paper. It should be noted that the proportion of Mg component in the hydrothermal fluids might be relatively high, by the reason of our samples contain relatively high Mg<sup>&#x23;</sup> values nearly close to 50 and no mantle-derived materials were involved in their magma source.</p>
<p>However, due to the existence of coetaneous mantle-derived magmatic products in the SCB, the high-maficity feature of the Yuechengling S-type granitoids is attributed to the involvement of mantle-derived materials or the alteration of hydrothermal fluids should be further examined in future studies.</p>
</sec>
<sec id="s5-3-1-3">
<title>5.3.1.3 Fractional crystallization</title>
<p>On the Zr &#x2b; Nb &#x2b; Ce &#x2b; Y vs. FeO<sup>T</sup>/MgO (<xref ref-type="fig" rid="F8">Figure 8A</xref>) and Zr &#x2b; Nb &#x2b; Ce &#x2b; Y <italic>vs.</italic> (K<sub>2</sub>O&#x2b;Na<sub>2</sub>O)/CaO diagrams (<xref ref-type="fig" rid="F8">Figure 8B</xref>), the samples all fall into the weakly fractionated granitoid field, indicating some degree of fractional crystallization. The granitoids have low contents of SiO<sub>2</sub> (66.12&#x2013;67.32&#xa0;wt%) and Differentiation index (DI) (73.46&#x2013;84.96) and ratios of Rb/Sr (0.95&#x2013;1.25), high ratios of K/Rb (135&#x2013;184) (<xref ref-type="sec" rid="s12">Supplementary Table S2</xref>), demonstrating a limited fractional crystallization (<xref ref-type="bibr" rid="B69">Sami et al., 2020</xref>).</p>
<p>Fractional crystallization or residual of plagioclase can be indicated by depletion of Eu (<xref ref-type="fig" rid="F6">Figure 6D</xref>). Nb and Ti are commonly hosted in Ti-bearing minerals (e.g., ilmenite and titanite), the depletion of Nb and Ti are indicative of the fractional crystallization of Ti-bearing minerals and a crustal magma source (<xref ref-type="fig" rid="F6">Figure 6C</xref>). The depletion of P (<xref ref-type="fig" rid="F6">Figure 6C</xref>) and low contents of P<sub>2</sub>O<sub>5</sub> (0.11&#x2013;0.13&#xa0;wt%, <xref ref-type="sec" rid="s12">Supplementary Table S2</xref>) are related to fractionation of apatite (<xref ref-type="bibr" rid="B33">Healy et al., 2004</xref>). Moreover, the increases in K<sub>2</sub>O contents with increasing SiO<sub>2</sub> contents show that there was no obvious fractional crystallization of K-feldspar and biotite (<xref ref-type="fig" rid="F9">Figure 9B</xref>). Therefore, the Yuechengling granitoids have undergone some degree of fractional crystallization of plagioclase, Ti-bearing minerals, and apatite.</p>
</sec>
</sec>
<sec id="s5-3-2">
<title>5.3.2 The Damingshan volcaniclastic rocks</title>
<sec id="s5-3-2-1">
<title>5.3.2.1 Weathering and sediment recycling.</title>
<p>The chemical index of alteration (CIA) [CIA &#x3d; molar Al<sub>2</sub>O<sub>3</sub>/(Al<sub>2</sub>O<sub>3</sub> &#x2b; CaO&#x2a; &#x2b; Na<sub>2</sub>O &#x2b; K<sub>2</sub>O) &#xd7; 100] is often used as an important parameter to reveal weathering degree of source rocks (<xref ref-type="bibr" rid="B59">Nesbitt and Young, 1982</xref>). Generally, rocks with CIA values of 45&#x2013;55 show low degree of weathering (CIA of the crust is ca. 47) and value of 100 to be intense degree of weathering, with the alkali and alkaline Earth elements no longer retained (<xref ref-type="bibr" rid="B55">McLennan et al., 1993</xref>). The Damingshan volcaniclastic rocks have CIA values ranging from 52 to 61 with an average value of 57 (<xref ref-type="sec" rid="s12">Supplementary Table S2</xref>), indicating incipient weathering conditions. These rocks have maturity index Al<sub>2</sub>O<sub>3</sub>/(Na<sub>2</sub>O &#x2b; K<sub>2</sub>O) values of limited variation of 2.30&#x2013;2.44, showing similar and low maturity and proximal sources.</p>
<p>Th and Zr are incompatible elements in the symbiotic components of igneous rocks and are often enriched in felsic rocks, whereas Sc often contained as a compatible element in the mafic mineral components in the initial stage of magmatic evolution (<xref ref-type="bibr" rid="B56">McLennan and Taylor, 1991</xref>). The ratio of Th/Sc is considered to be an indicator of revealing average provenance and enrichment degree of zircon (heavy-mineral), which will increase with the sediment recycling process (<xref ref-type="bibr" rid="B55">McLennan et al., 1993</xref>). In the Zr/Sc vs. Th/Sc diagram (<xref ref-type="fig" rid="F10">Figure 10B</xref>), the volcaniclastic rocks are distributed along the compositional variation trend, indicating a low degree of sediment recycling and heavy-mineral sorting. Thus, the geochemistry data of the volcaniclastic rocks are valid for further discussion.</p>
<fig id="F10" position="float">
<label>FIGURE 10</label>
<caption>
<p>Diagrams of <bold>(A)</bold> Sc vs. Th, <bold>(B)</bold> Zr/Sc vs. Th/Sc, <bold>(C)</bold> Sc vs. Th/Sc, and <bold>(D)</bold> Ni vs. TiO<sub>2</sub>. <bold>(A)</bold> is after <xref ref-type="bibr" rid="B58">Nagarajan et al. (2015)</xref>, <bold>(B)</bold> is after <xref ref-type="bibr" rid="B55">McLennan et al. (1993)</xref>, averages of the rocks are after <xref ref-type="bibr" rid="B67">Roser et al. (2002)</xref>, <bold>(C)</bold> is after <xref ref-type="bibr" rid="B58">Nagarajan et al. (2015)</xref>, <bold>(D)</bold> is after <xref ref-type="bibr" rid="B27">Floyd et al. (1990)</xref>. PASS-Post-Archean Australian Shales; UCC-Upper Continental Crust.</p>
</caption>
<graphic xlink:href="feart-11-1202477-g010.tif"/>
</fig>
</sec>
<sec id="s5-3-2-2">
<title>5.3.2.2 Provenance</title>
<p>For clastic sedimentary rocks that have not undergone significant sediment recycling, their geochemistry characteristics can be used for distinguishing between mafic/ultramafic and felsic source materials (<xref ref-type="bibr" rid="B78">Taylor and McLennan, 1985</xref>; <xref ref-type="bibr" rid="B90">Wronkiewicz and Condie, 1987</xref>). Al<sub>2</sub>O<sub>3</sub>/TiO<sub>2</sub> ratios could be used to discriminate the characteristics of source rocks, with mafic rocks having low Al<sub>2</sub>O<sub>3</sub>/TiO<sub>2</sub> ratios of 3-8, intermediate rocks of 8&#x2013;21 and felsic rocks of higher ratios (21&#x2013;70) (<xref ref-type="bibr" rid="B32">Hayashi et al., 1997</xref>). Volcaniclastic rocks of this study have relatively high Al<sub>2</sub>O<sub>3</sub>/TiO<sub>2</sub> ratios of 19.4&#x2013;26.1, suggesting intermediate to felsic components in the source area. On the Th vs. Sc plot, the rocks concentrate in the field of continental sources (<xref ref-type="fig" rid="F10">Figure 10A</xref>). On the Th/Sc vs. Zr/Sc diagram (<xref ref-type="fig" rid="F10">Figure 10B</xref>), the samples distributed between the dacite and granite fields. On the Sc vs. Th/Sc diagram (<xref ref-type="fig" rid="F10">Figure 10C</xref>), they concentrate between andesite and granite which are closer to granite field. Combining with Ni vs. TiO<sub>2</sub> diagram (<xref ref-type="fig" rid="F10">Figure 10D</xref>), the rocks were suggested to be acidic rather than mafic. The REE contents and Eu anomalies of clastic sedimentary rocks are also important keys for source rock characteristics (<xref ref-type="bibr" rid="B94">Xiang et al., 2015</xref>). Mafic rocks have lower LREE/HREE ratios and no negative Eu anomalies, whereas felsic rocks generally have higher LREE/HREE ratios and negative Eu anomalies (<xref ref-type="bibr" rid="B97">Yan et al., 2012</xref>). The samples have relatively high LREE/HREE ratios ranging from 7.53 to 9.12 with average value of 8.27 (<xref ref-type="sec" rid="s12">Supplementary Table S2</xref>), and exhibit moderate negative Eu anomalies (<xref ref-type="fig" rid="F10">Figure 6D</xref>), also indicating mainly felsic sources. The plots are consistent with the interpretation that the principal source rocks were of felsic composition with some intermediate composition included. The inference is also supported by mineral assemblages (<xref ref-type="table" rid="T1">Table 1</xref>; <xref ref-type="fig" rid="F3">Figure 3</xref>).</p>
<p>Zircon grains from our samples exhibit mostly negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values with partially positive (&#x2212;27.54 to 8.73, <xref ref-type="fig" rid="F7">Figures 7B, C</xref>), indicating that they were dominantly derived from crustal material and may have undergone some degree of magma mixing with mantle-derived materials. Moreover, the relatively high Mg<sup>&#x23;</sup> values (47&#x2013;56, <xref ref-type="sec" rid="s12">Supplementary Table S2</xref>) of the samples also indicate the contribution of mantle-derived components. Zircons with negative <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) values (&#x2212;27.54 to &#x2212;0.14) show T<sub>DM2</sub> ages of 3.79 to 1.63&#xa0;Ga, suggesting that they were mainly derived from Archean-Mesoproterozoic crustal materials. Therefore, combined with petrographic and geochemical data, we suggest that the felsic parental magma was erupted to the surface in a Late Ordovician volcanic event (later than 451&#xa0;Ma) and deposited soon after the eruption.</p>
</sec>
</sec>
</sec>
<sec id="s5-4">
<title>5.4 Constraints on the Early Paleozoic tectonic evolution of the SCB</title>
<p>Controversy surrounds the tectonic evolution of the Early Paleozoic orogeny in the SCB and two disparate tectonic models have been presented: 1) intracontinental orogeny (<xref ref-type="bibr" rid="B11">Charvet et al., 2010</xref>; <xref ref-type="bibr" rid="B93">Xia et al., 2014</xref>; <xref ref-type="bibr" rid="B74">Shu et al., 2015</xref>; <xref ref-type="bibr" rid="B24">Faure et al., 2017</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref>), i.e., the Yangtze and Cathaysia Blocks were amalgamated together into the ancient South China continent during the amalgamation process of the Rodinia supercontinent in the Late Neoproterozoic, and the Early Paleozoic &#x201c;Huanan Ocean&#x201d; did not exist. 2) oceanic subduction-collision (<xref ref-type="bibr" rid="B63">Qin et al., 2011</xref>; <xref ref-type="bibr" rid="B60">Peng et al., 2016a</xref>; <xref ref-type="bibr" rid="B61">Peng et al., 2016b</xref>; <xref ref-type="bibr" rid="B51">Liu et al., 2018</xref>), i.e., the &#x201c;Huanan Ocean&#x201d; existed and oceanic subduction occurred in the SCB in the Early Paleozoic.</p>
<p>As absence of the Early Paleozoic ophiolites, island arc igneous rock, coeval HP/LT (high pressure-low temperature)-type metamorphic rocks and turbidite with &#x201c;Bouma sequence&#x201d; related to closure of the &#x201c;Huanan Ocean&#x201d; are lacking in the SCB, the intra-continental orogenic model has been widely accepted (e.g., <xref ref-type="bibr" rid="B11">Charvet et al., 2010</xref>; <xref ref-type="bibr" rid="B86">Wang et al., 2011</xref>; <xref ref-type="bibr" rid="B73">Shu et al., 2014</xref>). Meanwhile, some &#x201c;Early Paleozoic island arc igneous rock&#x201d; and &#x201c;ophiolite suites&#x201d; from the southwest segment of the Jiangnan Orogen have been reported recently. Based on geochemical, petrological and geochronological studies, the existence of the Early Paleozoic &#x201c;Huanan Ocean&#x201d; and several different subductional-collisional models have been proposed (<xref ref-type="bibr" rid="B60">Peng et al., 2016a</xref>; <xref ref-type="bibr" rid="B61">Peng et al., 2016b</xref>; <xref ref-type="bibr" rid="B62">Qin et al., 2017</xref>). However, the origin of igneous rock with subductional signature is uncertain. The Early Paleozoic igneous rocks in the SCB generally show depletion of HFSEs (e.g., Nb and Ta), which is geochemically similar to island arc magma, and were considered to be formed in a subductional-collisional setting (<xref ref-type="bibr" rid="B63">Qin et al., 2011</xref>; <xref ref-type="bibr" rid="B62">Qin et al., 2017</xref>). However, the interpretation of &#x201c;subductional signature&#x201d; is not only applied to island arc magma. In some cases, the depletion of Nb and Ta can be caused by some magmatism related to intra-plate rift (<xref ref-type="bibr" rid="B68">Rudnick and Gao, 2003</xref>; <xref ref-type="bibr" rid="B57">Murphy and Dostal, 2007</xref>), or magma derived from the melting of ancient island arc material (<xref ref-type="bibr" rid="B43">Li et al., 2005</xref>), lithosphere mantle, or contamination of crustal materials (<xref ref-type="bibr" rid="B112">Zhang X. S. et al., 2017</xref>). Furthermore, the complete sequence and age of the Early Paleozoic &#x201c;ophiolite suit&#x201d; are uncertain. Although a suit of the Early Paleozoic &#x201c;ophiolite&#x201d; was found in the Nuodong area of the SCB (<xref ref-type="bibr" rid="B60">Peng et al., 2016a</xref>), it lacks the ultramafic rock (mantle peridotite) unit and should be excluded from the standard ophiolite suit. In addition, some &#x201C;Early Paleozoic ophiolite&#x201D; in the SCB was confirmed to be formed in Neoproterozoic (<xref ref-type="bibr" rid="B43">Li et al., 2005</xref>; <xref ref-type="bibr" rid="B72">Shu et al., 2006</xref>). Thus, further work is needed to refine the integrity and age of the &#x201c;ophiolite suit&#x201d;.</p>
<p>Igneous rocks formed in the subductional-collisional setting generally display a linear distribution (<xref ref-type="bibr" rid="B109">Zhang et al., 2013</xref>). Compared with the Late Mesozoic granites in the SCB (<xref ref-type="bibr" rid="B45">Li and Li, 2007</xref>), the spatial and temporal distribution of the Early Paleozoic granites does not display a clear trend of gradually younger age from inland to coastal caused by the plate retracement (<xref ref-type="bibr" rid="B53">Liu X. et al., 2020</xref>). From southeast to northwest, the SCB displays uninterrupted detrital zircon ages and sedimentary facies of the Lower Paleozoic sedimentary rocks (<xref ref-type="bibr" rid="B87">Wang et al., 2010</xref>; <xref ref-type="bibr" rid="B105">Yu et al., 2015</xref>). Combining with biostratigraphy, paleocurrent, and paleoecology signature (<xref ref-type="bibr" rid="B17">Chen et al., 2010</xref>; <xref ref-type="bibr" rid="B73">Shu et al., 2014</xref>; <xref ref-type="bibr" rid="B105">Yu et al., 2015</xref>), it is suggested that the Yangtze and Cathaysia Blocks were not separated in the Early Paleozoic.</p>
<p>Moreover, there is no sufficient geochemical evidence for the existence of asthenosphere mantle-derived igneous rock. The Early Paleozoic mafic igneous rocks reported in the SCB are characterized by extremely low <italic>&#x3b5;</italic>
<sub>Hf</sub>(t) and <italic>&#x3b5;</italic>
<sub>Nd</sub>(t) values and show depletions in HFSEs (e.g., Nb and Ta), which is similar to igneous rocks of the lithospheric mantle source (<xref ref-type="bibr" rid="B36">Jia et al., 2017</xref>). Therefore, the Yuechengling granitoids and Damingshan volcaniclastic rocks were probably formed in an intra-continental setting rather than a subductional-collisional setting.</p>
<p>According to the currently chronological data from the SCB, the Early Paleozoic orogeny in the SCB started in the Late Ordovician (ca. 460&#xa0;Ma), peaked at the Early-Mid Silurian (ca. 440&#x2013;420&#xa0;Ma), and ended in the Early Devonian (ca. 390&#xa0;Ma) (<xref ref-type="bibr" rid="B42">Li et al., 2011</xref>; <xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>; <xref ref-type="bibr" rid="B95">Xin et al., 2020</xref>; <xref ref-type="bibr" rid="B40">Kong et al., 2021</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref> and the related references). It has been accepted that the Early Paleozoic orogeny has undergone two episodes of tectonic stages, including the syn-collisional stage (ca. 460&#x2013;440&#xa0;Ma) and post-collisional stage (ca. 440&#x2013;400&#xa0;Ma) (<xref ref-type="bibr" rid="B93">Xia et al., 2014</xref>; <xref ref-type="bibr" rid="B106">Yu et al., 2016</xref>; <xref ref-type="bibr" rid="B6">Cai et al., 2017</xref>; <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref>).</p>
<p>Generally, the tectonic setting of granites and intermediate rocks has uncertainty, they can be formed in a compressional setting as well as an extensional setting (except for A-type granites). However, peraluminous S-type granites are generally found in settings associated with the syn-collisional or post-collisional stage (<xref ref-type="bibr" rid="B39">Kalsbeek et al., 2001</xref>; <xref ref-type="bibr" rid="B2">Atherton and Ghani, 2002</xref>). Generally, thickening of the crust, detachment of the subducted slab (<xref ref-type="bibr" rid="B2">Atherton and Ghani, 2002</xref>) and lithospheric delamination (<xref ref-type="bibr" rid="B76">Sylvester, 1998</xref>) are some of the mechanisms envisaged for the heat source that led to partial melting of sedimentary rocks to generate S-type granites. In contrast, ultramafic-mafic rocks are normally considered as products of a regional extensional setting, which are important manifestation of deep thermal-dynamic action on the surface. Recently, some mafic-intermediate rocks in the SCB have been reported, such as the Northern Guangdong high-magnesian andesites and dacites (ca. 435&#xa0;Ma) (<xref ref-type="bibr" rid="B100">Yao et al., 2012</xref>), Longhugang (423 &#xb1; 8&#xa0;Ma), Xinchuan (434 &#xb1; 6&#xa0;Ma) and Xinsi (420 &#xb1; 3&#xa0;Ma) gabbroic plutons (<xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>), Dakang gabbroic pluton (441.1 &#xb1; 4.7&#xa0;Ma) (<xref ref-type="bibr" rid="B110">Zhang et al., 2015</xref>), Taoyuan hornblende gabbro (409 &#xb1; 2&#xa0;Ma) (<xref ref-type="bibr" rid="B118">Zhong et al., 2013</xref>), and Daning lamprophyre (445 &#xb1; 4&#xa0;Ma) (<xref ref-type="bibr" rid="B36">Jia et al., 2017</xref>). A-type granites related to extensional setting are also found in the SCB, such as the South Fufang and Yingshang granitoids (ca. 414&#x2013;404&#xa0;Ma) (<xref ref-type="bibr" rid="B95">Xin et al., 2020</xref>), Xiqin granites (410&#xa0;Ma) (<xref ref-type="bibr" rid="B6">Cai et al., 2017</xref>), Huitong and Epo granites (414&#x2013;415&#xa0;Ma) (<xref ref-type="bibr" rid="B25">Feng et al., 2014</xref>). Thus, the tectonic setting of the Early Paleozoic orogeny was changed to a strongly extensional environment at least since ca. 445&#xa0;Ma, and the timing of tectonic transition might be further constrained to 445&#x2013;440&#xa0;Ma based on these Early Paleozoic ultramafic-mafic rocks and A-type granites in the SCB. It is suggested that the Damingshan volcaniclastic rocks (later than 451&#xa0;Ma) might be formed in the syn-collisional stage while the Yuechengling granitoids (&#x223c;437&#xa0;Ma) in the post-collisional stage.</p>
<p>Crustal shortening, deep metamorphism, crustal collapse and extension should be involved in an orogenic cycle (<xref ref-type="bibr" rid="B28">Froidevaux and Ricard, 1987</xref>). Recently, a model of the Early Paleozoic magmatic activity in the SCB was related to the partially molten SCLM heated by upwelling asthenosphere triggered by lithospheric delamination is proposed (e.g., <xref ref-type="bibr" rid="B100">Yao et al., 2012</xref>; <xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>; <xref ref-type="bibr" rid="B110">Zhang et al., 2015</xref>; <xref ref-type="bibr" rid="B36">Jia et al., 2017</xref>). The Early Paleozoic volcanic and mafic rocks are rarely reported compared to granites in response to the synchronous Early Paleozoic orogeny (<xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>), which is similar with areas suspected to have undergone recent delamination that characterized by insignificant mafic magmatism (<xref ref-type="bibr" rid="B23">Ducea, 2011</xref>). And that may be due to the formation of extensive intra-crustal felsic magma and the thick Cambrian-Ordovician strata in the SCB, which acted as barriers against the rise of mafic magma (<xref ref-type="bibr" rid="B96">Xu and Xu, 2015</xref>). Moreover, the melting temperature for the basaltic magma and the calculated mantle potential temperature are both ca. 1,300&#xb0;C, similar to that of a MORB (Mid Ocean Ridge Basalt)-like asthenospheric mantle (<xref ref-type="bibr" rid="B100">Yao et al., 2012</xref>), supporting the hypothesis that the partially molten SCLM was heated up by upwelling asthenosphere triggered by dropping of the delaminated lithosphere.</p>
<p>Based on previous studies and this study, the Early Paleozoic tectonic evolution process in the SCB is as follows:<list list-type="simple">
<list-item>
<p>(1) From 460 to 440&#xa0;Ma (<xref ref-type="fig" rid="F11">Figure 11A</xref>), the SCB has undergone crustal shortening and crustal thickening, leading to a peak metamorphic pressure of &#x3e;8&#xa0;GPa and temperature of 835&#xb0;C&#x2013;878&#xb0;C with a series of thrust faults developed (<xref ref-type="bibr" rid="B104">Yu et al., 2003</xref>; <xref ref-type="bibr" rid="B103">2007</xref>; <xref ref-type="bibr" rid="B46">Li et al., 2010</xref>; <xref ref-type="bibr" rid="B93">Xia et al., 2014</xref>). The induced metamorphism caused melting of meta-sedimentary rocks in the crust and formed the parental magma after some degree of magma mixing. Subsequently, formation of the thrust faults provided magma conduits for intrusion or eruption of the parental magma, the syn-collisional igneous rocks were formed (e.g., Tanghu granites, <xref ref-type="bibr" rid="B108">Zhang et al., 2012</xref>, and the Damingshan volcaniclastic rocks in this study).</p>
</list-item>
<list-item>
<p>(2) From 440 to 400&#xa0;Ma (<xref ref-type="fig" rid="F11">Figure 11B</xref>), the orogen gradually transforms from compression to extension. After peak metamorphism and exhumation, the extension led the metamorphism to an isothermal metamorphic temperature and decreasing pressure of ca. 4&#xa0;GPa (<xref ref-type="bibr" rid="B46">Li et al., 2010</xref>). Due to the decreasing metamorphic pressure, the SCLM have undergone delamination with rapid unroofing and collapsing, and leading to upwelling of the asthenosphere, which input thermal for partial melting of the SCLM above (<xref ref-type="bibr" rid="B46">Li et al., 2010</xref>; <xref ref-type="bibr" rid="B100">Yao et al., 2012</xref>; <xref ref-type="bibr" rid="B85">Wang et al., 2013b</xref>; <xref ref-type="bibr" rid="B93">Xia et al., 2014</xref>). The basaltic magma formed by the partially molten SCLM underplated the crust (e.g., <xref ref-type="bibr" rid="B36">Jia et al., 2017</xref>), causing partial melting of the meta-sedimentary rocks to form the felsic magma. At this stage, parental magmas of some granites were formed in the interaction of the basaltic and felsic magma (e.g., Daning and Guiling granites, <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref>). After undergoing some degree of assimilation fractional crystallization, the post-collision igneous rocks were produced (the Yuechengling granitoids in this study). Accompanied by cooling retrogression, the orogen gradually adjusted to the normal crustal thickness, and the Early Paleozoic orogeny ended in the Early Devonian (ca. 400&#x2013;390&#xa0;Ma).</p>
</list-item>
</list>
</p>
<fig id="F11" position="float">
<label>FIGURE 11</label>
<caption>
<p>Cartoon showing the petrogenetic mechanisms that led to the formation of the Early Paleozoic igneous rocks in the SCB during <bold>(A)</bold> 460 to 440&#xa0;Ma and <bold>(B)</bold> 440 to 400&#xa0;Ma (modified after <xref ref-type="bibr" rid="B77">Tang et al., 2021</xref> and <xref ref-type="bibr" rid="B100">Yao et al., 2012</xref>). ALF-the Anhua-Luocheng fault, CLF-the Chenzhou-Linwu fault (after <xref ref-type="bibr" rid="B113">Zhao, 2015</xref>), PNF-the Pingxiang-Gongcheng-Nanning fault (after <xref ref-type="bibr" rid="B121">Zhou and Wen, 2021</xref>), SLF-the Shizong-Mile-Luodian fault (after <xref ref-type="bibr" rid="B22">Dong et al., 2015</xref>), ZDF-the Zhenghe-Dapu fault.</p>
</caption>
<graphic xlink:href="feart-11-1202477-g011.tif"/>
</fig>
</sec>
</sec>
<sec sec-type="conclusion" id="s6">
<title>6 Conclusion</title>
<p>
<list list-type="simple">
<list-item>
<p>(1) The Yuechengling granitoids (438&#x2013;436&#xa0;Ma) are S-type granitoids. Their parental magma was derived from a crustal meta-greywacke and meta-pelite components in the Paleoproterozoic basement, and have undergone some degree of fractional crystallization.</p>
</list-item>
<list-item>
<p>(2) The Damingshan volcaniclastic rocks (later than 451&#xa0;Ma) are classified as strongly peraluminous, calc-alkaline to high-K calc-alkaline volcaniclastic rocks. Their parental magma was derived from Neoarchean-Neoproterozoic crustal materials, and has undergone some degree of magma mixing with mantle-derived magma. The felsic parental magma was erupted to the surface in a Late Ordovician volcanic event (later than 451&#xa0;Ma) and deposited soon after the eruption.</p>
</list-item>
<list-item>
<p>(3) Combining with the previous studies and our new evidence on the Early Paleozoic igneous rock in the SCB, we suggest that the Early Paleozoic tectonic setting of the SCB was intracontinental orogeny rather than oceanic subduction-collision. Granitoids and volcaniclastic rocks in this study recorded the transitional stage of syn-collision compressional (ca. 460&#x2013;440&#xa0;Ma) and the post-collision extensional setting (ca. 440&#x2013;400&#xa0;Ma) of the Early Paleozoic orogeny.</p>
</list-item>
</list>
</p>
</sec>
</body>
<back>
<sec sec-type="data-availability" id="s7">
<title>Data availability statement</title>
<p>The original contributions presented in the study are included in the article/<xref ref-type="sec" rid="s12">Supplementary Material</xref>, further inquiries can be directed to the corresponding author.</p>
</sec>
<sec id="s8">
<title>Author contributions</title>
<p>YT: writing-original draft, methodology. YS: supervision, conceptualization, reviewing, and editing manuscript. BW, YZ, and YL: experiment assistance, data curation. All authors contributed to the article and approved the submitted version.</p>
</sec>
<sec id="s9">
<title>Funding</title>
<p>This research was jointly supported by National Science Foundations of China (Grant No. 41862003) and Guangxi Natural Science Foundations of China for Distinguished Young Scholars (Grant No. 2019GXNSFFA245005).</p>
</sec>
<ack>
<p>We thank H. Xu for his assistance with fieldwork and the reviewers for their constructive feedback and advice greatly.</p>
</ack>
<sec sec-type="COI-statement" id="s10">
<title>Conflict of interest</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
<sec sec-type="disclaimer" id="s11">
<title>Publisher&#x2019;s note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
<sec id="s12">
<title>Supplementary material</title>
<p>The Supplementary Material for this article can be found online at: <ext-link ext-link-type="uri" xlink:href="https://www.frontiersin.org/articles/10.3389/feart.2023.1202477/full#supplementary-material">https://www.frontiersin.org/articles/10.3389/feart.2023.1202477/full&#x23;supplementary-material</ext-link>
</p>
<supplementary-material xlink:href="Table2.XLSX" id="SM1" mimetype="application/XLSX" xmlns:xlink="http://www.w3.org/1999/xlink"/>
<supplementary-material xlink:href="Table3.XLSX" id="SM2" mimetype="application/XLSX" xmlns:xlink="http://www.w3.org/1999/xlink"/>
<supplementary-material xlink:href="Table1.XLSX" id="SM3" mimetype="application/XLSX" xmlns:xlink="http://www.w3.org/1999/xlink"/>
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