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<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>
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<article-id pub-id-type="publisher-id">1487090</article-id>
<article-id pub-id-type="doi">10.3389/feart.2024.1487090</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>Early paleozoic evolution of the South Bainaimiao Ocean: constraints from the Chegendalai ophiolite m&#xe9;lange</article-title>
<alt-title alt-title-type="left-running-head">Feng 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.2024.1487090">10.3389/feart.2024.1487090</ext-link>
</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname>Feng</surname>
<given-names>Chenfei</given-names>
</name>
<uri xlink:href="https://loop.frontiersin.org/people/2827305/overview"/>
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<role content-type="https://credit.niso.org/contributor-roles/investigation/"/>
<role content-type="https://credit.niso.org/contributor-roles/methodology/"/>
<role content-type="https://credit.niso.org/contributor-roles/visualization/"/>
<role content-type="https://credit.niso.org/contributor-roles/writing-original-draft/"/>
</contrib>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Wang</surname>
<given-names>Guosheng</given-names>
</name>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<role content-type="https://credit.niso.org/contributor-roles/conceptualization/"/>
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<contrib contrib-type="author">
<name>
<surname>Zhou</surname>
<given-names>Zhiguang</given-names>
</name>
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<contrib contrib-type="author">
<name>
<surname>Gao</surname>
<given-names>Shen</given-names>
</name>
<role content-type="https://credit.niso.org/contributor-roles/Writing - review &#x26; editing/"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname>Chen</surname>
<given-names>Jianfeng</given-names>
</name>
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<contrib contrib-type="author">
<name>
<surname>Hu</surname>
<given-names>Hao</given-names>
</name>
<uri xlink:href="https://loop.frontiersin.org/people/2863730/overview"/>
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<aff>
<institution>School of Earth Sciences and Resources</institution>, <institution>China University of Geosciences, Beijing</institution>, <addr-line>Beijing</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/111619/overview">Derek Keir</ext-link>, University of Southampton, United Kingdom</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/728142/overview">Junpeng Wang</ext-link>, China University of Geosciences Wuhan, China</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/2842231/overview">Darko Spahi&#x107;</ext-link>, Institute for Multidisciplinary Research, University of Belgrade, Serbia</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Guosheng Wang, <email>wanggsh@cugb.edu.cn</email>
</corresp>
</author-notes>
<pub-date pub-type="epub">
<day>21</day>
<month>11</month>
<year>2024</year>
</pub-date>
<pub-date pub-type="collection">
<year>2024</year>
</pub-date>
<volume>12</volume>
<elocation-id>1487090</elocation-id>
<history>
<date date-type="received">
<day>27</day>
<month>08</month>
<year>2024</year>
</date>
<date date-type="accepted">
<day>31</day>
<month>10</month>
<year>2024</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2024 Feng, Wang, Zhou, Gao, Chen and Hu.</copyright-statement>
<copyright-year>2024</copyright-year>
<copyright-holder>Feng, Wang, Zhou, Gao, Chen and Hu</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>
<sec>
<title>Introduction</title>
<p>Arc-continent collision contributes to the accretion of continental crust in the Central Asian Orogenic Belt. The Chegendalai ophiolitic m&#x00E9;lange, located between the Bainaimiao arc and the North China Craton, is important to understanding the early Paleozoic evolution of the South Bainaimiao Ocean and arc-continent collision processes.</p>
</sec>
<sec>
<title>Methods</title>
<p>In this study, we provide Early Paleozoic geochronological and geochemical data from the Chegendalai ophiolitic m&#x00E9;lange and island arc magmatic rocks in northern Damaoqi.</p>
</sec>
<sec>
<title>Results</title>
<p>Zircon U-Pb dating of ultrabasic rocks and diabase porphyrite from the Chegendalai ophiolitic m&#x00E9;lange yielded ages of 424 Ma and 431.9 Ma, respectively. Schist has an age of 421 Ma. Zircon U-Pb ages of island arc magmatic rocks are 425.7 Ma for tonalite, and 431 &#x00B1; 11 Ma and 433.2 &#x00B1; 4.4 Ma for granodiorite. Gabbro and ultrabasic rocks were formed in a volcanic arc basalt or mid-ocean ridge setting, displaying a tholeiitic basalt signature. These rocks likely derived from the lithospheric mantle with assimilation of crustal materials. Intermediate-acid magmatic rocks in northern Damaoqi are geochemically classified as I-type granites and exhibit characteristics of adakites.</p>
</sec>
<sec>
<title>Discussion</title>
<p>These rocks formed by partial melting of subducted plates and interactions with crustal and mantle wedges in a volcanic arc setting. Based on these results, we propose a three-stage evolution model for the South Bainaimiao Ocean: (&#x0069;) Initial subduction during the Ordovician (&#x223C;450 Ma), where the Bainaimiao arc separated the South Bainaimiao Ocean from the PaleoAsian Ocean, with the former acting as a branch ocean basin of the latter; (&#x0069;&#x0069;) Northward subduction from the Ordovician to Late Silurian (450&#x2013;424 Ma), with the South Bainaimiao Ocean subducting northward. The subducted slab partially melted and interacted with the crust-mantle wedge, leading to the formation of subduction-related island arc magmatic rocks; (&#x0069;&#x0069;&#x0069;) Closure during the Late Silurian (424&#x2013;421 Ma), marked by the collision of the Bainaimiao arc with the North China Craton in an arc-continent collision, ending orogenesis with the Xibiehe Formation.</p>
</sec>
</abstract>
<kwd-group>
<kwd>central asian orogenic belt (CAOB)</kwd>
<kwd>south bainaimiao ocean</kwd>
<kwd>bainaimiao arc</kwd>
<kwd>arc-continent collision</kwd>
<kwd>ophiolitic m&#xe9;lange</kwd>
</kwd-group>
<contract-sponsor id="cn001">National Natural Science Foundation of China<named-content content-type="fundref-id">10.13039/501100001809</named-content>
</contract-sponsor>
<custom-meta-wrap>
<custom-meta>
<meta-name>section-at-acceptance</meta-name>
<meta-value>Structural Geology and Tectonics</meta-value>
</custom-meta>
</custom-meta-wrap>
</article-meta>
</front>
<body>
<sec id="s1">
<title>1 Introduction</title>
<p>The Central Asian Orogenic Belt (CAOB), located between the Siberian Craton, the North China Craton (NCC), and the Tarim Craton, serves as a prototypical accretionary orogenic belt since the Phanerozoic (<xref ref-type="fig" rid="F1">Figure 1A</xref>) (<xref ref-type="bibr" rid="B53">&#x15e;eng&#xf6;r et al., 1993</xref>). The accretionary orogenic process of the CAOB elucidates crustal accretion mechanisms driven by plate tectonics, although its modes of accretion remain contentious (<xref ref-type="bibr" rid="B53">&#x15e;eng&#xf6;r et al., 1993</xref>; <xref ref-type="bibr" rid="B73">Xiao et al., 2003</xref>; <xref ref-type="bibr" rid="B69">Windley et al., 2007</xref>; <xref ref-type="bibr" rid="B51">Safonova et al., 2011</xref>). Many researchers propose that the formation of the CAOB from the Neoproterozoic to Late Paleozoic can be explained by the models involving southwest Pacific-style island arc and microcontinent accretion (<xref ref-type="bibr" rid="B73">Xiao et al., 2003</xref>; <xref ref-type="bibr" rid="B69">Windley et al., 2007</xref>; <xref ref-type="bibr" rid="B51">Safonova et al., 2011</xref>; <xref ref-type="bibr" rid="B24">Kr&#xf6;ner et al., 2014</xref>). Arc-continent collision is a major mechanism of crustal accretion in the western Pacific region (<xref ref-type="bibr" rid="B5">Brown et al., 2006</xref>; <xref ref-type="bibr" rid="B68">Whattam, 2009</xref>; <xref ref-type="bibr" rid="B23">Konstantinovskaya, 2011</xref>). Recent reports highlight Paleozoic arc-continent collision events in the southern Urals, Kazakhstan, and southern Mongolia within the CAOB (<xref ref-type="bibr" rid="B2">Alvarez-Marron et al., 2000</xref>; <xref ref-type="bibr" rid="B5">Brown et al., 2006</xref>; <xref ref-type="bibr" rid="B11">Degtyarev and Ryazantsev, 2007</xref>; <xref ref-type="bibr" rid="B21">Johnson et al., 2007</xref>; <xref ref-type="bibr" rid="B26">Li et al., 2023</xref>; <xref ref-type="bibr" rid="B79">Zeng et al., 2023</xref>), indicating that arc-continent collision is a crucial mechanism for continental crust growth and the formation of the CAOB (<xref ref-type="bibr" rid="B53">&#x15e;eng&#xf6;r et al., 1993</xref>; <xref ref-type="bibr" rid="B25">Li, 2004</xref>; <xref ref-type="bibr" rid="B78">Yuan et al., 2009</xref>; <xref ref-type="bibr" rid="B8">Chen et al., 2021</xref>; <xref ref-type="bibr" rid="B72">Xiao et al., 2022</xref>; <xref ref-type="bibr" rid="B26">Li et al., 2023</xref>).</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>
<bold>(A)</bold> The geotectonic location of the Central Asian orogenic belt (<xref ref-type="bibr" rid="B17">Hu et al., 2022</xref>); <bold>(B)</bold> Tectonic unit division of the XMOB (<xref ref-type="bibr" rid="B73">Xiao et al., 2003</xref>; <xref ref-type="bibr" rid="B81">Zhang et al., 2018</xref>).</p>
</caption>
<graphic xlink:href="feart-12-1487090-g001.tif"/>
</fig>
<p>The southern margin of CAOB adjacent to the NCC is characterized by the Bainaimiao arc. Previous studies suggest that the Bainaimiao arc is an Andean-type active continental margin arc formed during the Early Paleozoic by the southward subduction of the Paleo-Asian Ocean beneath the NCC (<xref ref-type="bibr" rid="B13">Gu et al., 2012</xref>; <xref ref-type="bibr" rid="B87">Zhang et al., 2013</xref>; <xref ref-type="bibr" rid="B71">Wu et al., 2016</xref>; <xref ref-type="bibr" rid="B38">Ma et al., 2020</xref>). Recently, many researchers have proposed the existence of the South Bainaimiao Ocean between the Bainaimiao arc and the NCC prior to the late Silurian. Following the subduction of the South Bainaimiao Ocean, the Bainaimiao arc, as an allochthonous terrane, collided with and amalgamated into the NCC during the Late Silurian period (<xref ref-type="bibr" rid="B31">Li et al., 2012</xref>; <xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>; <xref ref-type="bibr" rid="B30">Li et al., 2015</xref>; <xref ref-type="bibr" rid="B66">Wang et al., 2016</xref>; <xref ref-type="bibr" rid="B81">Zhang et al., 2018</xref>; <xref ref-type="bibr" rid="B92">Zhou, H. et al., 2018</xref>; <xref ref-type="bibr" rid="B37">Ma et al., 2019</xref>; <xref ref-type="bibr" rid="B7">Chen et al., 2020</xref>; <xref ref-type="bibr" rid="B16">Hou et al., 2020</xref>; <xref ref-type="bibr" rid="B35">Liu et al., 2020</xref>; <xref ref-type="bibr" rid="B38">Ma et al., 2020</xref>; <xref ref-type="bibr" rid="B1">Alexis N&#x2019;dri et al., 2021</xref>; <xref ref-type="bibr" rid="B44">Meng et al., 2021</xref>; <xref ref-type="bibr" rid="B61">Tang et al., 2021</xref>; <xref ref-type="bibr" rid="B93">Zhou et al., 2021</xref>; <xref ref-type="bibr" rid="B26">Li et al., 2023</xref>; <xref ref-type="bibr" rid="B26">Li et al., 2023</xref>; <xref ref-type="bibr" rid="B26">Li et al., 2023</xref>; <xref ref-type="bibr" rid="B63">Tian et al., 2023</xref>). Many studies have proposed the existence of the South Bainaimiao Ocean, but they differ its subduction polarity. Some argue that it subducted northward beneath the Bainaimiao arc, while the northern margin of the NCC remained in a passive continental margin stage (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>; <xref ref-type="bibr" rid="B44">Meng et al., 2021</xref>; <xref ref-type="bibr" rid="B26">Li et al., 2023</xref>; <xref ref-type="bibr" rid="B79">Zeng et al., 2023</xref>; <xref ref-type="bibr" rid="B82">Zhang et al., 2024</xref>); others propose that the Paleozoic Bainaimiao Ocean subducted southward beneath the northern margin of the NCC, influencing the Bainaimiao arc due to the southward subduction of the Paleo-Asian Ocean (<xref ref-type="bibr" rid="B6">Chen et al., 2018</xref>; <xref ref-type="bibr" rid="B54">Shi et al., 2024</xref>).</p>
<p>The Early Paleozoic ophiolitic m&#xe9;langes of Chegendalai are situated between the Bainaimiao arc and the northern margin of the NCC. To the north, there is extensive development of early Paleozoic arc-related island arc magmatic rocks (<xref ref-type="fig" rid="F2">Figure 2</xref>), making this area ideal for studying the evolution of the South Bainaimiao Ocean and the arc-continent collision (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>). This study conducted petrological, geochronological, and geochemical methods to analyze the formation ages and tectonic settings of the Chegendalai ophiolite m&#xe9;lange belt and the magmatic rocks in the northern part of Damaoqi. It also aimed to elucidate the subduction mechanism and closure time of the South Bainaimiao Ocean in the Early Paleozoic.</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>Geological map of the study area (modified after 1:25,000 Mandula and Bayan Obo sheets).</p>
</caption>
<graphic xlink:href="feart-12-1487090-g002.tif"/>
</fig>
</sec>
<sec id="s2">
<title>2 Geological setting</title>
<p>The Xingmeng Orogenic Belt is located in the southeastern part of the Central Asian Orogenic Belt, within Chinese territory, which is subdivided from north to south into the Uliastai continental margin, Hegenshan ophiolitic m&#xe9;langes, the Northern Orogenic Belt, the Solonker Suture Zone, and the Southern Orogenic Belt (<xref ref-type="fig" rid="F1">Figure 1B</xref>). The Southern Orogenic Belt comprises, from north to south, the Ondor Sum subduction accretion complex and the Bainaimiao arc (<xref ref-type="bibr" rid="B73">Xiao et al., 2003</xref>; <xref ref-type="bibr" rid="B86">Zhang and Jian, 2008</xref>; <xref ref-type="bibr" rid="B74">Xu et al., 2013</xref>; <xref ref-type="bibr" rid="B81">Zhang et al., 2018</xref>; <xref ref-type="bibr" rid="B77">Yang et al., 2019</xref>).</p>
<p>The Ondor Sum subduction accretion complex extends southward to the Bainaimiao arc, bounded by the Xar Moron Fault (<xref ref-type="fig" rid="F1">Figure 1B</xref>) (<xref ref-type="bibr" rid="B73">Xiao et al., 2003</xref>). The Early Paleozoic Ondor Sum subduction accretion complex, formed by the southward subduction of the Paleo-Asian Ocean, consists primarily of greenschists, carbonate lens bodies, muscovite-quartz schists, quartzites, and interbedded marble layers. This subduction accretion complex is overlain unconformably by Carboniferous and Permian volcanic and sedimentary rocks (<xref ref-type="bibr" rid="B92">Zhou et al., 2018</xref>). Scholars have reported mylonite ages indicating subduction-related high-pressure metamorphic events at 453&#x2013;449 Ma and subduction-type ophiolites at 490&#x2013;450 Ma in this area (Jong et al., 2006; Xiao et al., 2015; <xref ref-type="bibr" rid="B74">Xu et al., 2013</xref>; <xref ref-type="bibr" rid="B86">Zhang and Jian, 2008</xref>).</p>
<p>The Bainaimiao arc is situated between the Ondor Sum subduction accretion complex and the North China Craton (NCC), delineated by the Bayan Obo-Chifeng fault (<xref ref-type="fig" rid="F1">Figure 1B</xref>) (<xref ref-type="bibr" rid="B73">Xiao et al., 2003</xref>). The Bainaimiao arc displays abundant Early Paleozoic intrusive rocks including tonalite, quartz diorite, granodiorite, and granite, indicative of subduction or collision-related settings. It also features magmatic rocks such as basalt and andesite (<xref ref-type="bibr" rid="B86">Zhang and Jian, 2008</xref>; <xref ref-type="bibr" rid="B34">Liu et al., 2013</xref>; <xref ref-type="bibr" rid="B87">Zhang et al., 2013</xref>; <xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>; <xref ref-type="bibr" rid="B92">Zhou et al., 2018</xref>; <xref ref-type="bibr" rid="B7">Chen et al., 2020</xref>; <xref ref-type="bibr" rid="B17">Hu et al., 2022</xref>; <xref ref-type="bibr" rid="B26">Li et al., 2023</xref>). Zircon U-Pb dating of dacite in the western segment of the Bainaimiao arc yields an age of 447 Ma (<xref ref-type="bibr" rid="B17">Hu et al., 2022</xref>). SHRIMP zircon U-Pb dating indicates intrusion ages of 452 &#xb1; 3 Ma, 446 &#xb1; 2 Ma, and 440 &#xb1; 2 Ma for gabbro, quartz diorite, and granodiorite respectively in the Damaoqi area. The age of 417 &#xb1; 2 Ma for tonalite is interpreted as magmatic activity related to arc-continent collision at the northern margin of the NCC (<xref ref-type="bibr" rid="B86">Zhang and Jian, 2008</xref>). Zircon U-Pb ages and geochemical characteristics indicate that activity in the Bainaimiao arc spanned from 520 to 420 million years ago (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>). Gabbro ages of 453&#x2013;431 Ma, granite ages of 441&#x2013;436 Ma, and sedimentary rock ages of 441 Ma have been reported in this area (<xref ref-type="bibr" rid="B7">Chen et al., 2020</xref>). Hence, the Early Paleozoic magmatic rocks of the Bainaimiao arc are predominantly concentrated in the Ordovician to Silurian periods. The Middle-Late Silurian Xuniwusu Formation and the Late Silurian-Early Devonian Xibiehe Formation unconformably overlie the island arc magmatic rocks. The Xuniwusu Formation comprises Middle-Late Silurian turbidite sediments predominantly composed of sandstone, siltstone, and mudstone. The Xibiehe Formation, on the other hand, consists of Late Silurian-Early Devonian molasse sediments, interpreted as products of arc-continent collision termination (<xref ref-type="bibr" rid="B86">Zhang and Jian, 2008</xref>; <xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>).</p>
<p>Between the Bainaimiao arc and the NCC lie the Wude ophiolitic m&#xe9;lange belt and the Chegenda ophiolitic m&#xe9;lange belt (<xref ref-type="fig" rid="F2">Figure 2</xref>). The Wude ophiolitic m&#xe9;lange belt comprises ultrabasic rocks, gabbro, and Ordovician arc-related magmatic rocks (<xref ref-type="bibr" rid="B20">Jia et al., 2003</xref>; <xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>). However, the controversy surrounding this Ordovician ophiolitic m&#xe9;lange belt is beyond the scope of this paper. The Chegenda ophiolitic m&#xe9;lange includes Ordovician-Silurian gabbro, basalt, peridotite, diabase, and schist (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>; <xref ref-type="bibr" rid="B44">Meng et al., 2021</xref>). Both the Wude and Chegenda ophiolitic m&#xe9;lange belts have been intruded by Late Paleozoic granitic plutons and overlain by Late Paleozoic to Cenozoic strata.</p>
<p>The northern margin of the North China Craton comprises a Precambrian crystalline basement and sedimentary cover ranging from the Paleozoic to Mesozoic Eras. The basement primarily comprises Archean to Paleoproterozoic magmatic and metamorphic rocks. Over the Precambrian basement, the sequence comprises the Mesoproterozoic to Neoproterozoic (&#x223c;1600-850 Ma) Bayan Obo Group and Late Paleozoic magmatic rocks (<xref ref-type="bibr" rid="B80">Zhang et al., 2017</xref>; <xref ref-type="bibr" rid="B94">Zhou et al., 2018a</xref>). Late Paleozoic magmatic rocks primarily occur in the Carboniferous and Permian periods and include rhyolite, andesite, and volcanic breccia. (<xref ref-type="bibr" rid="B61">Tang et al., 2021</xref>).</p>
<p>The Chegendalai ophiolitic m&#xe9;lange belt extends approximately 15 km predominantly southeastward. Its margins display well-developed fractures, contacting the overlying Mesoproterozoic Baiyinbaolage Formation quartzite and muscovite quartz schist along fault planes oriented at 160&#xb0; strike and 35&#xb0; dip. The m&#xe9;lange comprises both blocks and a matrix. The blocks vary in size and mainly consist of peridotite, pyroxenite, gabbro, basalt, and limestone. The matrix is predominantly schist, and both blocks and matrix display faulted structural contacts (<xref ref-type="fig" rid="F3">Figures 3</xref>, <xref ref-type="fig" rid="F4">4</xref>).</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Simplified map of the study area and sampling locations.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g003.tif"/>
</fig>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>Profile of the Chegendalai ophiolitic m&#xe9;lange. The AB is the end point and the starting point of the profile, respectively, and the specific location is reflected in <xref ref-type="fig" rid="F3">Figure 3</xref>.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g004.tif"/>
</fig>
<p>Ultrabasic rock blocks in the m&#xe9;lange zone are extensively fractured by tectonic activity. Weathered surfaces are gray-white to gray-black, with fresh surfaces showing a light yellow-green color often in lens-shaped forms (<xref ref-type="fig" rid="F5">Figures 5A, C, E</xref>). Gabbro blocks in the m&#xe9;lange zone are predominantly lens-shaped. Some gabbro blocks have undergone late-stage regional metamorphism and ductile shear deformation, forming mylonitized gabbro (<xref ref-type="fig" rid="F5">Figure 5D</xref>). The gabbro rock is gray-green, with zoisite being the predominant alteration mineral. Diabase porphyrite in the m&#xe9;lange zone occurs in blocky and lens-shaped forms, undergoing weaker structural deformation and metamorphism compared to ultrabasic rocks and gabbros, and is in structural contact with surrounding rocks. The rock shows a weathered surface in grayish-green, with the fresh surface appearing light grayish-green, displaying a diabasic porphyritic texture. Internally, there is slight chloritization and actinolitization (<xref ref-type="fig" rid="F5">Figure 5B</xref>). The plagioclase actinolite schist matrix is in fault contact with rock blocks, with the exposed weathered surface appearing gray-black, and the fresh surface gray-black to gray-green. The rock is relatively fragmented with well-developed foliation (<xref ref-type="fig" rid="F5">Figures 5A, C</xref>).</p>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>Sampling points for ultrabasic rocks <bold>(A, C, E)</bold>, gabbros <bold>(D)</bold>, plagioclase actinolite schist <bold>(A, C)</bold> and diabase porphyrite <bold>(B)</bold>.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g005.tif"/>
</fig>
<p>The Arigong and Xilahada areas in the northern part of Chegendalai are characterized by extensive distribution of arc magmatic rocks, consisting mainly of quartz diorite, tonalite, and granodiorite (<xref ref-type="fig" rid="F3">Figure 3</xref>). Quartz diorite has a weathered surface that is gray-black, with its fresh surface appearing gray-green, displaying a blotchy structure and blocky texture (<xref ref-type="fig" rid="F6">Figures 6A, B</xref>). Granodiorite has a weathered surface that is gray-white to gray-black, with its fresh surface appearing gray-white, displaying a medium to fine-grained granitic structure with a blocky texture (<xref ref-type="fig" rid="F6">Figures 6C&#x2013;E, G</xref>). Tonalite has a weathered surface that is gray-black, with its fresh surface appearing gray-white, showing a medium to fine-grained granitic structure with a blocky texture. In the field, occurrences of granodiorite intruded by tonalite are observed (<xref ref-type="fig" rid="F6">Figure 6F</xref>).</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>Sampling points of quartz diorite <bold>(A, B)</bold>, tonalite <bold>(F)</bold>, and granodiorite <bold>(C&#x2013;E, G)</bold>.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g006.tif"/>
</fig>
</sec>
<sec id="s3">
<title>3 Sampling and methods</title>
<p>A total of 37 samples were collected for this study, with their locations illustrated in (<xref ref-type="fig" rid="F3">Figures 3</xref>, <xref ref-type="fig" rid="F4">4</xref>). These samples include nine ultrabasic rock samples (DME<sub>5</sub>-TW<sub>1</sub>, DME<sub>5</sub>-YQ<sub>1-5</sub>, DME<sub>7</sub>-YQ<sub>1-3</sub>), two gabbro samples (DME<sub>6</sub>-YQ<sub>1-2</sub>), and one diabase porphyrite sample (DMX). One schist sample was collected, specifically plagioclase actinolite schist (DME<sub>10</sub>-TW<sub>1</sub>). A total of 24 samples of intermediate-acid magmatic rocks were collected, consisting of tonalite (XLHD<sub>1</sub>-TW<sub>1</sub>, XLHD1-YQ<sub>1-3</sub>), quartz diorite (ARG<sub>2</sub>-YQ<sub>1-3</sub>, ARG<sub>4</sub>-YQ<sub>1-3</sub>), and granodiorite (XLHD<sub>2</sub>-TW<sub>1</sub>, XLHD<sub>2</sub>-YQ<sub>1-3</sub>, XHDT<sub>1</sub>-TW<sub>1</sub>, XHDT<sub>1</sub>-YQ<sub>1-3</sub>, TLMM<sub>1</sub>-YQ<sub>1-3</sub>, XWLH<sub>1</sub>-YQ<sub>1-3</sub>). Sample Form <xref ref-type="sec" rid="s12">Supplementary Table S1</xref>.</p>
<p>The OLYMPUS-BX53 detection equipment was used under environmental conditions of 21&#xb0;C&#x2013;25&#xb0;C temperature and 50%&#x2013;70% relative humidity. The selected zircon samples were sent to Beijing Zhongke Mining Research and Testing Technology Co., Ltd. Zircon grains intended for analysis were mounted in resin and imaged using scanning electron microscopy for cathodoluminescence (<xref ref-type="fig" rid="F9">Figure 9</xref>). The zircon selection, target fabrication, and cathodoluminescence imaging of the diabase porphyrite (DMX) samples were conducted at the Beijing National Geological Testing Center (<xref ref-type="fig" rid="F9">Figure 9F</xref>). Zircon targets were sent to the Institute of Geomechanics, Chinese Academy of Geological Sciences for LA-ICP-MS zircon U-Pb dating analysis. The analysis was conducted using the GeoLas Hd 193 nm ArF excimer laser ablation system and an Agilent 7,900 quadrupole inductively coupled plasma mass spectrometer at the Key Laboratory of Paleomagnetism and Paleotectonic Reconstruction, Ministry of Natural Resources. Standard zircon 91,500, with a spot size of 32 &#x3bc;m, was used as the external standard (<xref ref-type="bibr" rid="B67">Wang et al., 2022</xref>). Zircon U-Pb isotope dating of diabase porphyrite samples was conducted using LA-ICP-MS at the North China Mineral Resources Supervision and Testing Center, Tianjin Institute of Geological Survey, China Geological Survey. Concordia diagrams and detrital zircon age frequency distribution plots were analyzed with Isoplot (<xref ref-type="bibr" rid="B36">Ludwig, 2003</xref>). Age distribution comparison histograms were created with DensityPlotter 7.2 (<xref ref-type="bibr" rid="B64">Vermeesch, 2012</xref>). Zircons older than 1,000 Ma were dated using <sup>207</sup>Pb-<sup>206</sup>Pb ages, and those younger than 1,000 Ma were dated using <sup>206</sup>Pb-<sup>238</sup>U ages.</p>
<p>Whole rock geochemical analysis samples undergo initial screening. Fresh, uncontaminated samples are then crushed to 200 mesh size at the Hebei Regional Geological Survey Institute laboratory before being sent to the Beijing National Geological Testing Center for analysis of major elements, trace elements, and rare earth elements content. Major elements were analyzed using X-ray fluorescence spectrometry (PW4400), following methods specified in national standard GB/T 14,506.28&#x2013;2010. Trace elements and rare earth elements were analyzed using inductively coupled plasma mass spectrometry (PE300Q), following methods strictly adhering to national standard GB/T 14,506.30&#x2013;2010. FeO, H2O<sup>&#x2b;</sup>, Cr, and LOI were tested according to national standards GB/T 14,506.14&#x2013;2010, GB/T 14,506.2&#x2013;2010, Q/GD 001&#x2013;2002, and GB/T 14,506.34&#x2013;2019, respectively.</p>
</sec>
<sec sec-type="results" id="s4">
<title>4 Results</title>
<sec id="s4-1">
<title>4.1 Petrography</title>
<p>The ultrabasic rocks within the m&#xe9;lange belt exhibit metasomatic structures and have undergone extensive serpentinization. Most minerals in these rocks have transformed into fibrous serpentine, with no residual minerals remaining (<xref ref-type="fig" rid="F7">Figures 7A, B, D</xref>).</p>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>Under the microscope characteristics of ultrabasic rock <bold>(A, B, D)</bold>, gabbros <bold>(C)</bold>, diabase porphyrite <bold>(F)</bold>, and Plagioclase actinolite schist <bold>(E)</bold> samples (Qtz, quartz; Pl, plagioclase; Srp, serpentine; Px, pyroxene; Act, actinolite; Hb, hornblende; Zo, zoisite).</p>
</caption>
<graphic xlink:href="feart-12-1487090-g007.tif"/>
</fig>
<p>Most of the gabbro rocks have altered to zoisite. Locally, some original features persist, including plate-like plagioclase and granular pyroxene, which are indicative of a typical gabbro structure. Microscopic examination reveals that the gabbro consists predominantly of actinolite (60%) and analcime (37%&#x2013;40%), with minor albite present. No residual crystals are preserved elsewhere (<xref ref-type="fig" rid="F7">Figure 7C</xref>).</p>
<p>The diabase porphyrite shows slight chloritization and actinolization. Porphyroblasts in the rock mainly consist of granular and columnar hornblende (5%). The matrix is predominantly composed of granular plagioclase (45%), columnar pyroxene (35%), and a small amount of granular hornblende (10%) (<xref ref-type="fig" rid="F7">Figure 7F</xref>).</p>
<p>The plagioclase amphibole schist consists of light green columnar actinolite (40%) arranged in a banded top-line pattern, forming a sheet-like structure. Interspersed among these minerals are granular quartz (20%) and plagioclase (35%), forming a lenticular and banded structure between the columnar actinolites. Some plagioclase grains exhibit slight sericitization and actinolization. Additionally, a small amount of biotite (5%) occurs in flake and scaly orientations (<xref ref-type="fig" rid="F7">Figure 7E</xref>).</p>
<p>The quartz diorite exhibits a porphyritic and massive structure. It consists of plagioclase (45%), hornblende (30%), quartz (15%), and a small amount of biotite (10%). The minerals are irregularly distributed. The plagioclase shows sericitization, while the amphibole locally contains tin-bearing minerals and has been metasomatized by biotite schistosity (<xref ref-type="fig" rid="F8">Figure 8A</xref>).</p>
<fig id="F8" position="float">
<label>FIGURE 8</label>
<caption>
<p>Microscopic features of intermediate to acidic magmatic rocks: Quartze diorite <bold>(A)</bold>, Granodiorite <bold>(B, D&#x2013;F)</bold>and Tonalite <bold>(C)</bold> (Qtz, quartz; Pl, plagioclase; Ms, muscovite; Bt, biotite; Hb, hornblende; Afs, alkali feldspar).</p>
</caption>
<graphic xlink:href="feart-12-1487090-g008.tif"/>
</fig>
<p>The granodiorite exhibits a medium to fine-grained granite structure with a massive appearance. The rock consists primarily of plagioclase (40%&#x2013;55%), quartz (25%), potassium feldspar (10%&#x2013;25%), with minor amounts of biotite and muscovite (10%&#x2013;15%), exhibiting irregular mineral distribution. The plagioclase grains exhibit zirconization and contain biotite along with minor metasomatic plagioclase. Biotite and muscovite occur as scattered flakes, with some biotite showing chloritization and muscovitization (<xref ref-type="fig" rid="F8">Figures 8B, D&#x2013;F</xref>).</p>
<p>The tonalite exhibits a medium to fine-grained granite structure with a blocky appearance. The rock is primarily composed of plagioclase (65%), quartz (20%&#x2013;25%), and biotite (10%&#x2013;15%), with minerals irregularly distributed. Some plagioclase exhibits potassium feldspar, and flake biotite ranges in color from light yellowish brown to brown (<xref ref-type="fig" rid="F8">Figure 8C</xref>).</p>
</sec>
<sec id="s4-2">
<title>4.2 Zircon U-Pb dating</title>
<p>This study conducted age dating on ultrabasic rocks (DME<sub>5</sub>-TW<sub>1</sub>), plagioclase actinolite schist (DME<sub>10</sub>-TW<sub>1</sub>), and island arc intermediate-acid magmatic rocks (XHDT<sub>1</sub>-TW<sub>1</sub>, XLHD<sub>1</sub>-TW<sub>1</sub>, XLHD<sub>2</sub>-TW<sub>1</sub>). The LA-ICP-MS zircon U-Pb dating results are presented in <xref ref-type="sec" rid="s12">Supplementary Tables S2, S3</xref>.</p>
<p>Twenty-seven zircon grains were selected for dating from the ultrabasic rock sample DME<sub>5</sub>-TW<sub>1</sub>. The zircons are mainly tabular, with some being granular, having grain sizes ranging approximately from 40 to 100 &#x3bc;m, and generally exhibiting poor crystal shapes. Zircon exhibits oscillatory zoning, with Th/U ratios ranging from 0.05 to 2.5, averaging 0.65, indicative of a magmatic origin (<xref ref-type="fig" rid="F9">Figure 9A</xref>). Twenty data points with high concordance were selected to construct a concordia diagram. The weighted mean age of four zircons using <sup>206</sup>Pb-<sup>238</sup>U dating is 424 &#xb1; 15 Ma (MSWD &#x3d; 4.5) (<xref ref-type="fig" rid="F10">Figure 10A</xref>). The older zircon age may represent the inherited zircon age. The rock was modified by the late Permian magma and mixed with young zircons (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>).</p>
<fig id="F9" position="float">
<label>FIGURE 9</label>
<caption>
<p>Cathodoluminescence (CL) image of representative zircons: ultrabasic rock <bold>(A)</bold>, Plagioclase actinolite schist <bold>(B)</bold>, Granodiorite <bold>(C, E)</bold>, Tonalite <bold>(D)</bold> and diabase porphyrite <bold>(F)</bold>.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g009.tif"/>
</fig>
<fig id="F10" position="float">
<label>FIGURE 10</label>
<caption>
<p>Concordia diagram and detrital zircon age spectrum: <bold>(A)</bold> Serpentinized ultrabasic rock, sample DME5-TW1; <bold>(B)</bold> Tonalite, sample XLHD1-TW1; <bold>(C)</bold> Granodiorite, sample XLHD2-TW1; <bold>(D)</bold> Granodiorite, sample XHDT1-TW1; <bold>(E)</bold> Diabase porphyrite, sample DMX1-TW1; <bold>(F)</bold> Plagioclase actinolite schist, sample DME10-TW1.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g010.tif"/>
</fig>
<p>One hundred detrital zircon grains were selected for dating from the Plagioclase actinolite schist sample DME<sub>10</sub>-TW<sub>1</sub>. The zircon grains have diameters ranging approximately from 20 to 130 &#x3bc;m, exhibit clear oscillatory zoning, and have Th/U ratios ranging from 0.08 to 3.26 with an average of 0.71, typical of magmatic zircons, and are relatively fractured (<xref ref-type="fig" rid="F9">Figure 9B</xref>). Ninety-seven zircon grains with relatively high concordance were selected to construct a concordia diagram and detrital zircon age spectrum. The detrital zircons show predominant age peaks at 430 Ma and 1800 Ma (<xref ref-type="fig" rid="F11">Figure 11</xref>). After excluding younger zircon ages influenced by later events (273 &#xb1; 4 Ma and 395 &#xb1; 3 Ma), the remaining young detrital zircon ages concentrate around 432.9 &#xb1; 3.5 Ma, with the youngest age being 421 &#xb1; 4 Ma, interpreted as the protolith age of the schist (<xref ref-type="fig" rid="F10">Figure 10F</xref>).</p>
<fig id="F11" position="float">
<label>FIGURE 11</label>
<caption>
<p>Detrital zircon age frequency distribution diagram of Plagioclase actinolite schist.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g011.tif"/>
</fig>
<p>Thirty zircon grains were selected for dating from the diabase porphyrite sample DMX<sub>1</sub>-TW<sub>1</sub>. The zircon grains have diameters ranging from 50 to 120 &#x3bc;m, with a length-to-width ratio generally around 1:1 or 2:1. Most zircon grains exhibit clear oscillatory zoning, and Th/U ratios are concentrated between 0.41 and 0.99, displaying typical characteristics of magmatic zircons (<xref ref-type="fig" rid="F9">Figure 9F</xref>). Six zircon grains with relatively clustered ages were used for weighted mean age calculation, resulting in an age of 431.9 &#xb1; 3.7 Ma (MSWD &#x3d; 0.87) (<xref ref-type="fig" rid="F10">Figure 10E</xref>). This is interpreted as the crystallization age of the diabase porphyrite. The older zircon grains likely represent inherited zircons captured during diagenesis.</p>
<p>Zircon dating was conducted on twenty-five grains each from the diorite samples XHDT<sub>1</sub>-TW<sub>1</sub>, XLHD<sub>1</sub>-TW<sub>1</sub>, and XLHD<sub>2</sub>-TW<sub>1</sub>. The zircon grains in the samples are relatively large, approximately 100&#x2013;240 &#x3bc;m in size, mostly elongated and short prismatic shapes. The Th/U ratios average 0.53, 0.32, and 0.47 respectively, with clear growth zoning, displaying typical characteristics of magmatic zircons (<xref ref-type="fig" rid="F9">Figures 9C&#x2013;E</xref>). The age data of 25 zircons measured by tonalite samples XLHD<sub>1</sub>-TW<sub>1</sub> are relatively concentrated. The weighted average age of <sup>206</sup>Pb-<sup>238</sup>U is 425.7 &#xb1; 3.2 Ma (MSWD &#x3d; 3.1) (<xref ref-type="fig" rid="F10">Figure 10B</xref>). In the granodiorite sample XLHD<sub>2</sub>-TW<sub>1</sub>, after excluding seven zircon grains with low concordance, a weighted mean <sup>206</sup>Pb-<sup>238</sup>U age of 433.2 &#xb1; 4.4 Ma was obtained from the remaining 18 zircon grains (MSWD &#x3d; 2.6) (<xref ref-type="fig" rid="F10">Figure 10C</xref>). In the granodiorite samples XHDT<sub>1</sub>-TW<sub>1</sub>, the dating results have a low degree of concordance, with only six data points showing high concordance and reliability. Four concentrated <sup>206</sup>Pb-<sup>238</sup>U ages are used for weighted average calculation. The crystallization age of the magma is 431 &#xb1; 11 Ma (MSWD &#x3d; 3.9) (<xref ref-type="fig" rid="F10">Figure 10D</xref>).</p>
</sec>
<sec id="s4-3">
<title>4.3 Whole-rock geochemistry</title>
<sec id="s4-3-1">
<title>4.3.1 Major elements</title>
<p>
<xref ref-type="sec" rid="s12">Supplementary Table S4</xref> presents the results of major and trace element analyses for 28 samples.</p>
<p>Ultrabasic rocks have very low levels of K<sub>2</sub>O (0.01 wt%), Na<sub>2</sub>O (&#x3c;0.01 wt%), and P<sub>2</sub>O<sub>5</sub> (&#x3c;0.01 wt%); relatively low levels of SiO<sub>2</sub> (38.96&#x2013;41.69 wt%), Al<sub>2</sub>O<sub>3</sub> (0.57&#x2013;1.42 wt%), and CaO (0.09&#x2013;4.18 wt%); low levels of TiO<sub>2</sub> (0.02&#x2013;0.04 wt%) and MnO (0.07&#x2013;0.14 wt%); and high levels of TFe<sub>2</sub>O<sub>3</sub> (6.49&#x2013;8.5 wt%), FeO (3.14&#x2013;3.72 wt%), and MgO (33.04&#x2013;35.31 wt%). Before mapping, loss on ignition is eliminated, and the rock&#x2019;s major elements are recalculated on a dry basis. In <xref ref-type="fig" rid="F12">Figure 12A</xref>, ultrabasic rocks are concentrated mainly in the Olivine gabbro field, and they are shown as part of the tholeiitic series in <xref ref-type="fig" rid="F12">Figure 12B</xref>.</p>
<fig id="F12" position="float">
<label>FIGURE 12</label>
<caption>
<p>Geochemical classification diagrams: TAS diagram <bold>(A)</bold> (<xref ref-type="bibr" rid="B45">Middlemost, 1994</xref>) and AFM diagram <bold>(B)</bold> (<xref ref-type="bibr" rid="B19">Irvine and Baragar, 1971</xref>). 1 - Olivine gabbro; 2a - Alkaline gabbro; 2b - Subalkaline gabbro; 3 - Gabbro diorite; 4 - Diorite; 5 - Granodiorite; 6 - Granite; 7 - Silicon quartzite; 8 - Monzogabbro; 9 -Monzodiorite; 10 - Monzonite; 11 - Quartz Monzonite; 12 Syenite; 13 - Foid Gabbro; 14 - Foid Monzodiorite; 15 - Foid Monzosyenite; 16 - Foid Syenite; 17 -Foidolite; 18 - Sodalite/nepheline rock/pure leucite. Data for the early Paleozoic magmatic rocks from other locations of the Bainaimiao arc system are from <xref ref-type="bibr" rid="B85">Zhang et al. (2014)</xref>, <xref ref-type="bibr" rid="B7">Chen et al. (2020)</xref>, <xref ref-type="bibr" rid="B44">Meng et al. (2021)</xref>, <xref ref-type="bibr" rid="B14">Hao et al. (2022)</xref>.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g012.tif"/>
</fig>
<p>Gabbros have relatively low levels of SiO<sub>2</sub> (43.77&#x2013;45.98 wt%), K<sub>2</sub>O (0.15&#x2013;0.28 wt%), TiO<sub>2</sub> (0.51&#x2013;0.63 wt%), and P<sub>2</sub>O<sub>5</sub> (0.01 wt%); and high levels of CaO (12.38&#x2013;16.89 wt%), MgO (8.65&#x2013;9.21 wt%), Al<sub>2</sub>O<sub>3</sub> (15.28&#x2013;18.32 wt%), TFe<sub>2</sub>O<sub>3</sub> (8.8&#x2013;12 wt%), and FeO (4.98&#x2013;8.86 wt%). Before mapping, loss on ignition is eliminated, and the rock&#x2019;s major elements are recalculated on a dry basis. In <xref ref-type="fig" rid="F12">Figure 12A</xref>, gabbros are concentrated mainly in the Olivine gabbro field, and they are shown as part of the tholeiitic series in <xref ref-type="fig" rid="F12">Figure 12B</xref>.</p>
<p>Diorites have low levels of TFe<sub>2</sub>O<sub>3</sub> (2.68&#x2013;3.05 wt%), P<sub>2</sub>O<sub>5</sub> (0.13&#x2013;0.14 wt%), TiO<sub>2</sub> (0.09&#x2013;0.36 wt%), and MgO (1.11&#x2013;1.26 wt%); and high levels of SiO<sub>2</sub> (64.5&#x2013;65.53 wt%), Al<sub>2</sub>O<sub>3</sub> (18.29&#x2013;18.43 wt%), K<sub>2</sub>O (2.73&#x2013;3.46 wt%), and Na<sub>2</sub>O (4.77&#x2013;5.25 wt%). Granodiorites exhibit high levels of SiO<sub>2</sub> (66.77&#x2013;74.01 wt%), Al<sub>2</sub>O<sub>3</sub> (14.35&#x2013;17.49 wt%), K<sub>2</sub>O (1.88&#x2013;4.63 wt%), and Na<sub>2</sub>O (3.35&#x2013;4.83 wt%); and low levels of TFe<sub>2</sub>O<sub>3</sub> (0.99&#x2013;2.79 wt%), P<sub>2</sub>O<sub>5</sub> (0.02&#x2013;0.11 wt%), TiO<sub>2</sub> (0.09&#x2013;0.36 wt%), and MgO (0.28&#x2013;1.01 wt%). Quartz diorites exhibit high levels of SiO<sub>2</sub> (58.36&#x2013;73.78 wt%), Al<sub>2</sub>O<sub>3</sub> (14.49&#x2013;16.5 wt%), K<sub>2</sub>O (1.96&#x2013;4.12 wt%), and Na<sub>2</sub>O (3.71&#x2013;4.3 wt%); and low levels of TFe<sub>2</sub>O<sub>3</sub> (0.88&#x2013;5.8 wt%), P<sub>2</sub>O<sub>5</sub> (0.05&#x2013;0.2 wt%), TiO<sub>2</sub> (0.02&#x2013;0.6 wt%), and MgO (0.09&#x2013;4.75 wt%). Before mapping, loss on ignition is eliminated, and the rock&#x2019;s major elements are recalculated on a dry basis. In <xref ref-type="fig" rid="F12">Figure 12A</xref>, intermediate-acid magmatic rocks are primarily concentrated in the diorite-granite region, depicted as part of the calc-alkaline series in <xref ref-type="fig" rid="F12">Figure 12B</xref>.</p>
</sec>
<sec id="s4-3-2">
<title>4.3.2 Trace elements</title>
<p>The chondrite-normalized rare earth element spidergrams of gabbroic nodules exhibit low total rare earth element content, depleted LREEs, flat HREEs, resembling E-MORB characteristics, and significant positive Eu anomalies (&#x3b4;Eu&#x3d;1.30&#x2013;2.46) (<xref ref-type="fig" rid="F13">Figure 13C</xref>). The primitive mantle-normalized spidergrams show enrichment of LILEs (e.g., Rb, Ba, K, Pb, Sr) and significant depletion of HFSEs (e.g., Nb, Zr, Hf) (<xref ref-type="fig" rid="F13">Figure 13D</xref>).</p>
<fig id="F13" position="float">
<label>FIGURE 13</label>
<caption>
<p>Chondrite-normalized rare earth element <bold>(A, C)</bold> and primitive mantle-normalized spidergrams <bold>(B, D)</bold>. Normalization data from <xref ref-type="bibr" rid="B60">Sun and McDonough (1989)</xref>.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g013.tif"/>
</fig>
<p>The chondrite-normalized rare earth element spidergrams of ultrabasic rock show a slightly low total rare earth element content, with a slight trend of LREE enrichment and HREE depletion to slight enrichment, and positive (&#x3b4;Eu&#x3d;1.03&#x2013;1.99) or negative (&#x3b4;Eu&#x3d;0.62&#x2013;0.69) Eu anomalies (<xref ref-type="fig" rid="F13">Figure 13C</xref>). The primitive mantle-normalized spidergrams show enrichment of LILEs (e.g., U, Pb, Sr) and depletion of HFSEs (e.g., Nb, Zr, Hf) (<xref ref-type="fig" rid="F13">Figure 13D</xref>).</p>
<p>The chondrite-normalized rare earth element spidergrams of intermediate-acid magmatic rocks show enrichment of LREEs and depletion of HREEs. Quartz diorites exhibit a prominent negative Eu anomaly (&#x3b4;Eu&#x3d;0.56&#x2013;0.93), while the other samples do not show significant Eu anomalies (<xref ref-type="fig" rid="F13">Figure 13A</xref>). The primitive mantle-normalized spidergrams for most samples show lower contents of HFSEs (e.g., Nb, Ta, <italic>p</italic>, and Ti) and higher contents of LILEs (e.g., Ba, K, Pb, and Sr) (<xref ref-type="fig" rid="F13">Figure 13B</xref>).</p>
</sec>
</sec>
</sec>
<sec sec-type="discussion" id="s5">
<title>5 Discussion</title>
<sec id="s5-1">
<title>5.1 Formation ages</title>
<p>Previous studies in the Chegendalai area dated gabbro blocks to be 448&#x2013;450 Ma using LA-ICP-MS zircon U-Pb geochronology (<xref ref-type="bibr" rid="B44">Meng et al., 2021</xref>). This study indicates that the formation age of the rock mass in the ophiolite is Middle-Late Silurian (431.9&#x2013;424 Ma). The ophiolite in the ophiolitic m&#xe9;lange zone thus represents the lower limit of oceanic crust existence around 424 Ma, indicating ocean closure occurred after 424 Ma. Therefore, the formation age of the ophiolite spans from Late Ordovician to Late Silurian (450&#x2013;424 Ma), indicating the South Bainaimiao Ocean it represents existed from at least 450 Ma to around 424 Ma. The plagioclase actinolite schist age of the matrix in the Chegendalai ophiolitic m&#xe9;lange is 421 Ma, representing the mixing age of the ophiolitic m&#xe9;lange, indicating mixing occurred by the Late Silurian. The South Bainaimiao Ocean closed during the Late Silurian, just before 421 Ma. Ophiolite emplacement occurred within 10 million years after the formation of the oceanic lithosphere it represents (<xref ref-type="bibr" rid="B56">Smith and Rassios, 2003</xref>). In summary, the formation period of this ophiolite is Late Ordovician to Late Silurian. Emplacement occurred slightly after the youngest block age (424 Ma), and mixing occurred before 421 Ma, forming the ophiolitic m&#xe9;lange.</p>
<p>Previous studies extensively investigated the timing of formation of the Bainaimiao Island Arc Belt. Accurate SHRIMP zircon U-Pb ages from the Damaoqi area indicate intrusion ages of 452 &#xb1; 3 Ma for diorite, 446 &#xb1; 2 Ma for quartz diorite, and 440 &#xb1; 2 Ma for granodiorite (<xref ref-type="bibr" rid="B86">Zhang and Jian, 2008</xref>). The age of 417 &#xb1; 2 Ma for the tonalite indicates magmatic activity associated with the collision between the island arc and the northern margin of the NCC (<xref ref-type="bibr" rid="B86">Zhang and Jian, 2008</xref>). Combining regional zircon U-Pb ages and geochemical characteristics suggests that Bainaimiao arc activity occurred during the interval 0.52&#x2013;0.42 Ga (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>). Gabbro ages ranging from 453 to 431 Ma, granite ages from 441 to 436 Ma, and sedimentary rock ages of 441 Ma have all been reported in this region (<xref ref-type="bibr" rid="B7">Chen et al., 2020</xref>). Sedimentary ages of the Bainaimiao Group in the middle segment of the island arc belt range from 500 to 443 Ma (<xref ref-type="bibr" rid="B13">Gu et al., 2012</xref>; <xref ref-type="bibr" rid="B32">Liu et al., 2014</xref>; <xref ref-type="bibr" rid="B80">Zhang, J.F. et al., 2017</xref>; <xref ref-type="bibr" rid="B90">Zhang et al., 2020</xref>). In conclusion, the formation period of Bainaimiao Island arc magmatic rocks spans approximately from the Cambrian to the Silurian. The results of this study indicate zircon U-Pb ages of 425.7 Ma for the tonalite sample XLHD<sub>1</sub>-TW<sub>1</sub>, 431 Ma and 433.2 M for the granite diorite samples XHDT<sub>1</sub>-TW<sub>1</sub> and XLHD<sub>2</sub>-TW<sub>1</sub>. Therefore, the formation period of the intermediate-acid magmatic rocks in the northern Damaoqi area is determined to be during the Middle Silurian.</p>
</sec>
<sec id="s5-2">
<title>5.2 Genesis of magmatic rocks</title>
<p>In this study, the arc magmatic rocks and ophiolitic m&#xe9;lange exhibit geochemical similarities to the early Paleozoic magmatic rocks of the Bainaimiao arc. The ophiolitic m&#xe9;lange is predominantly found in the olivine diabase and sub-alkaline diabase ranges, while the arc magmatic rocks are concentrated in the intermediate to acidic diorite-granite ranges (<xref ref-type="fig" rid="F12">Figure 12</xref>). The trace element characteristics of both the ophiolitic m&#xe9;lange and arc magmatic rocks align with the results of earlier studies from the Bainaimiao region (<xref ref-type="fig" rid="F13">Figures 13</xref>, <xref ref-type="fig" rid="F14">14</xref>). Consequently, the island arc belt examined in this study represents the western extension of the Bainaimiao arc.</p>
<fig id="F14" position="float">
<label>FIGURE 14</label>
<caption>
<p>Primitive mantle-normalized spidergrams. Normalization data from <xref ref-type="bibr" rid="B60">Sun and McDonough (1989)</xref>. Data for the early Paleozoic magmatic rocks from other locations of the Bainaimiao arc system are from <xref ref-type="bibr" rid="B85">Zhang et al. (2014)</xref>, <xref ref-type="bibr" rid="B7">Chen et al. (2020)</xref>, <xref ref-type="bibr" rid="B44">Meng et al. (2021)</xref>, <xref ref-type="bibr" rid="B14">Hao et al. (2022)</xref>.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g014.tif"/>
</fig>
<p>The Nb/La ratios ranging from 0.08 to 0.6 for gabbros and ultrabasic rocks indicate that the origin was from the lithospheric mantle (<xref ref-type="bibr" rid="B57">Smith et al., 1999</xref>). Geochemical signatures show that (Th/Nb)<sub>N</sub> &#x3e; 1 and (Nb/La)<sub>N</sub> &#x3c; 1 reliably indicate crustal contamination (<xref ref-type="bibr" rid="B52">Saunders et al., 1992</xref>; <xref ref-type="bibr" rid="B22">Kieffer et al., 2004</xref>). The (Th/Nb)<sub>N</sub> ratios range from 9.32 to 37.28 and (Nb/La)<sub>N</sub> ratios range from 0.07 to 0.58 for gabbros and ultrabasic rocks indicative of significant crustal assimilation. On the chondrite-normalized rare earth element spidergrams, gabbros have LREE depletion and slightly enriched HREEs. The distribution pattern is similar to N-MORB, and positive Eu anomalies (&#x3b4;Eu &#x3d; 1.30&#x2013;2.46), indicating plagioclase accumulation in the rock (<xref ref-type="bibr" rid="B18">Huang and Frey, 2003</xref>). Ultrabasic rocks have slight LREEs enrichment and slight HREEs depletion. The rare earth element distribution pattern is E-MORB and positive (&#x3b4;Eu &#x3d; 1.03&#x2013;1.99) or negative (&#x3b4;Eu &#x3d; 0.62&#x2013;0.69) Eu anomalies. On the primitive mantle-normalized spidergrams, gabbros are enriched in LILEs (e.g., Rb, Ba, K) and significantly depletion in HFSEs (e.g., Nb, Zr, Hf), indicating subduction-related characteristics (<xref ref-type="bibr" rid="B48">Pearce and Robinson, 2010</xref>; <xref ref-type="bibr" rid="B40">Ma et al., 2021</xref>). Ultrabasic rocks are enriched in LILEs (e.g., Sr, U, Pb) and depletion in HFSEs (e.g., Nb, Zr, Hf), indicating crustal characteristics (<xref ref-type="bibr" rid="B15">Hofmann, 1988</xref>). Therefore, gabbros and ultrabasic rocks likely originate from the lithospheric mantle of oceanic arcs or mid-ocean ridges and have undergone crustal assimilation.</p>
<p>Early Paleozoic magmatic rocks in the Bainaimiao island arc comprise diorite, tonalite, quartz diorite, and granodiorite compositions. Their geochemical characteristics indicate formation in an arc environment associated with subduction-related magmatism (<xref ref-type="bibr" rid="B41">Maniar and Piccoli, 1989</xref>; <xref ref-type="bibr" rid="B4">Barbarin, 1999</xref>; <xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>). Within the medium to acidic magmatic rocks, chondrite-normalized rare earth element spidergrams show enrichment of LREEs and depletion of HREEs, with most lacking significant Eu anomalies. The primitive mantle-normalized spidergrams reveal enrichment of LILEs (e.g., Rb, Ba, K, Pb) and depletion of HFSEs (e.g., Nb, Ta, Ti). The geochemical characteristics of the arc magmatic rocks and ophiolitic m&#xe9;lange display similarities, with identical element distribution patterns in the primitive mantle normalization diagrams (<xref ref-type="fig" rid="F14">Figure 14</xref>). These trace element characteristics originate from fluids, melts, and supercritical fluids formed by dehydration melting of subducted slabs (<xref ref-type="bibr" rid="B37">Ma et al., 2019</xref>). Adakites are medium to acidic special island arc magmatic rocks composed of andesite, dacite, and rhyolite. The rocks are different with typical island arc magmatic rocks by lacking basalt and being characterized geochemically by high Sr, low Yb and Y contents, and a high Sr/Y ratio (<xref ref-type="bibr" rid="B10">Defant and Drummond, 1990</xref>; <xref ref-type="bibr" rid="B43">Martin, 1999</xref>). In this study, the northern Damaoqi medium-acidic island arc magmatic rocks exhibit high contents of Al<sub>2</sub>O<sub>3</sub>, Sr, Ba, and a high Sr/Y ratio, showing geochemical characteristics similar to adakites (<xref ref-type="bibr" rid="B3">Atherton and Petford, 1993</xref>; <xref ref-type="bibr" rid="B59">Stern and Kilian, 1996</xref>). Island arc magmatic rocks are positioned in the adakite field on (La/Yb)<sub>N</sub>-Yb<sub>N</sub> and Sr/Y-Y diagrams (<xref ref-type="fig" rid="F15">Figure 15</xref>). Granodiorite, tonalite, and quartz diorite as early Paleozoic magmatic rocks in the Bainaimiao island arc may have formed due to partial melting of subducted slabs and interaction with the crust and mantle wedge (<xref ref-type="bibr" rid="B76">Xu et al., 2003</xref>; <xref ref-type="bibr" rid="B62">Tao et al., 2005</xref>).</p>
<fig id="F15" position="float">
<label>FIGURE 15</label>
<caption>
<p>Discrimination diagrams for medium-acidic magmatic rocks in northern Damaoqi: <bold>(A)</bold> (La/Yb)N-YbN (<xref ref-type="bibr" rid="B42">Martin, 1986</xref>), and <bold>(B)</bold> Sr/Y-Y (<xref ref-type="bibr" rid="B10">Defant and Drummond, 1990</xref>; <xref ref-type="bibr" rid="B12">Drummond and Defant, 1990</xref>; <xref ref-type="bibr" rid="B43">Martin, 1999</xref>).</p>
</caption>
<graphic xlink:href="feart-12-1487090-g015.tif"/>
</fig>
<p>On the Th/Yb-Ta/Yb diagram (<xref ref-type="bibr" rid="B46">Pearce, 1982</xref>) and the Th-Hf-Nb discrimination diagram (<xref ref-type="bibr" rid="B70">Wood, 1980</xref>), gabbro is situated within the VAB (<xref ref-type="fig" rid="F16">Figure 16</xref>). On the Th/Yb-Ta/Yb diagram, ultrabasic rocks are situated within the WPB or MORB field. The Th-Hf-Nb discrimination diagram indicates the tectonic setting of VAB (<xref ref-type="fig" rid="F16">Figure 16</xref>). On the Th/Yb-Ta/Yb discrimination diagram and the Th-Hf-Nb discrimination diagram, tonalite and quartz diorite situated in the VAB field (<xref ref-type="fig" rid="F15">Figure 15</xref>). Granodiorite is classified as I-type granite in the Nb-SiO<sub>2</sub> and Zr-SiO<sub>2</sub> discrimination diagrams, and as VAG or syn-COLG in the Nb-Y diagram, and VAG in the Rb-(Yb&#x2b;Ta) discrimination diagram (<xref ref-type="fig" rid="F17">Figure 17</xref>). In summary, gabbro and ultrabasic rocks likely originate from the tectonic environments of volcanic arc basalt or mid-ocean ridges. The magmatic rocks in northern Damao Banner suggest a volcanic island arc setting.</p>
<fig id="F16" position="float">
<label>FIGURE 16</label>
<caption>
<p>Tectonic discrimination diagrams: <bold>(A)</bold> Th/Yb-Ta/Yb diagram (<xref ref-type="bibr" rid="B46">Pearce, 1982</xref>): VAB - Volcanic Arc Basalt (IAT - Island Arc Tholeiite Basalt, CAB - Calc-Alkaline Basalt, SHO - shoshonitic), MORB - Mid-Ocean Ridge Tholeiite Basalt, WPB - Within Plate Basalt (TH - Tholeiitic, TR - Transitional, ALK - Alkaline); <bold>(B)</bold> Th-Hf-Nb diagram (<xref ref-type="bibr" rid="B70">Wood, 1980</xref>): A - N-type MORB, B - E-type MORB and Intraplate Tholeiite Basalt, C - Alkaline Intraplate Basalt, D - Volcanic Arc Basalt.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g016.tif"/>
</fig>
<fig id="F17" position="float">
<label>FIGURE 17</label>
<caption>
<p>Discrimination diagrams for A-type and I-type granites and their tectonic environments: <bold>(A)</bold> Nb-SiO2 discrimination diagram (<xref ref-type="bibr" rid="B9">Collins et al., 1982</xref>); <bold>(B)</bold> Zr-SiO2 discrimination diagram (<xref ref-type="bibr" rid="B9">Collins et al., 1982</xref>); <bold>(C)</bold> Nb-Y discrimination diagram (<xref ref-type="bibr" rid="B47">Pearce et al., 1984</xref>) <bold>(D)</bold> Rb-(Y&#x2b;Ta) discrimination diagram (<xref ref-type="bibr" rid="B47">Pearce et al., 1984</xref>). I - I-type granite, A - A-type granite; WPG - Within Plate Granite, ORG - Ocean Ridge Granite, VAG - Volcanic Arc Granite, syn-COLG - Syn-Collision Granite.</p>
</caption>
<graphic xlink:href="feart-12-1487090-g017.tif"/>
</fig>
</sec>
<sec id="s5-3">
<title>5.3 Early paleozoic evolution of the south bainaimiao ocean</title>
<sec id="s5-3-1">
<title>5.3.1 Subduction polarity</title>
<p>Recently, scholars have proposed the existence of the South Bainaimiao Ocean (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>), a viewpoint widely accepted by other researchers. However, considerable controversy exists regarding the subduction polarity of the South Bainaimiao Ocean (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>; <xref ref-type="bibr" rid="B7">Chen et al., 2020</xref>; <xref ref-type="bibr" rid="B44">Meng et al., 2021</xref>; <xref ref-type="bibr" rid="B26">Li et al., 2023</xref>; <xref ref-type="bibr" rid="B79">Zeng et al., 2023</xref>; <xref ref-type="bibr" rid="B54">Shi et al., 2024</xref>; <xref ref-type="bibr" rid="B82">Zhang et al., 2024</xref>). Previous studies indicate that during the early Paleozoic, the northern margin of the NCC was a passive continental margin (<xref ref-type="bibr" rid="B75">Xu and Chen, 1997</xref>; <xref ref-type="bibr" rid="B27">Li et al., 2009</xref>). Arc-related diorites and ultrabasic rocks have been reported in the Chegendalai serpentinite m&#xe9;lange (<xref ref-type="bibr" rid="B44">Meng et al., 2021</xref>). This study suggests that the Middle Silurian intrusive rocks in northern Damaoqi may have formed through partial melting of subducting plates interacting with mantle wedges, showing geochemical characteristics similar to adakites. Therefore, the South Bainaimiao Ocean should have subducted northward, with the NCC acting as a passive continental margin during this time.</p>
</sec>
<sec id="s5-3-2">
<title>5.3.2 Closure time of the south bainaimiao ocean</title>
<p>Previous studies have extensively investigated the timing of the South Bainaimiao Ocean closure. The tonalite in the Damaoqi area, dated at 417 Ma, is interpreted as a result of arc-continent collision subsequent to the closure of oceanic crust (<xref ref-type="bibr" rid="B86">Zhang and Jian, 2008</xref>). Scholars suggest the closure of the South Bainaimiao Ocean occurred around 420 Ma, based on the ages and geochemical characteristics of island-arc magmatic rocks in the Bayan Obo area (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>). Rhyolites from the southern part of the island arc, dated at 412 &#xb1; 1 Ma, exhibit Hf isotopic characteristics similar to those of the NCC (<xref ref-type="bibr" rid="B49">Qian et al., 2017</xref>). Middle to acidic rocks from the Late Silurian period and reverse thrust structures resulting from subduction collision in the Bainaimiao area indicate significant tectonic activity (<xref ref-type="bibr" rid="B30">Li et al., 2015</xref>; <xref ref-type="bibr" rid="B95">Zhou et al., 2018b</xref>). The development of quartz veins dated at 422.4 Ma further suggests a tectonic transition during mountain building in the Bainaimiao arc (<xref ref-type="bibr" rid="B96">Zhou et al., 2017</xref>). The unconformable overlay of the Late Silurian to early Devonian Xibiehe Formation over early Paleozoic ophiolites and arc-related magmatic rocks indicates the termination of the orogenic event (<xref ref-type="bibr" rid="B89">Zhang et al., 2004</xref>). During the Devonian period, the northern margin of the NCC developed a post-collisional extensional environment characterized by an alkaline rock belt (<xref ref-type="bibr" rid="B55">Shi et al., 2010</xref>; <xref ref-type="bibr" rid="B88">Zhang et al., 2010</xref>). Paleomagnetic data indicate that the southeastern part of the Central Asian Orogenic Belt amalgamated before the late Devonian period (<xref ref-type="bibr" rid="B91">Zhao et al., 2013</xref>). In this study, plagioclase actinolite schist as the matrix of ophiolitic m&#xe9;lange displays two distinct age peaks (<xref ref-type="fig" rid="F11">Figure 11</xref>). The younger age peak corresponds to the age of island-arc magmatic rocks, whereas the older age exhibits similarities to the NCC (<xref ref-type="fig" rid="F18">Figure 18</xref>), suggesting that the plagioclase actinolite schist at this time accumulated sedimentary material from both the Bainaimiao arc and the northern margin of the NCC. The closure of the South Bainaimiao Ocean took place prior to the metamorphic age of 421 Ma for the plagioclase actinolite schist. In summary, the closure of the South Bainaimiao Ocean occurred during the Late Silurian. During this period, the Bainaimiao arc and the northern margin of the NCC underwent arc-continent collision, which continued until the conclusion of the early Devonian collisional orogeny.</p>
<fig id="F18" position="float">
<label>FIGURE 18</label>
<caption>
<p>Comparison of zircon age histograms: <bold>(A)</bold> Plagioclase actinolite schist; <bold>(B)</bold> Bainaimiao arc (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>; <xref ref-type="bibr" rid="B7">Chen et al., 2020</xref>; <xref ref-type="bibr" rid="B93">Zhou et al., 2021</xref>); <bold>(C)</bold> North China Craton (<xref ref-type="bibr" rid="B50">Rojas-Agramonte et al., 2011</xref>; <xref ref-type="bibr" rid="B65">Wang et al., 2015</xref>; <xref ref-type="bibr" rid="B33">Liu et al., 2017</xref>; <xref ref-type="bibr" rid="B93">Zhou et al., 2021</xref>).</p>
</caption>
<graphic xlink:href="feart-12-1487090-g018.tif"/>
</fig>
</sec>
<sec id="s5-3-3">
<title>5.3.3 Evolutionary process</title>
<p>Scholars have conducted extensive research on Early Paleozoic evolution in various regions of the Bainaimiao Arc within the South Bainaimiao Ocean and proposed several evolutionary models (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>; <xref ref-type="bibr" rid="B7">Chen et al., 2020</xref>; <xref ref-type="bibr" rid="B54">Shi et al., 2024</xref>). This study categorizes the Early Paleozoic evolution in the South Bainaimiao Ocean into three distinct stages based on the findings. The oldest rock fragments in the Chagendalai serpentinite m&#xe9;lange date back to 448&#x2013;450 Ma (<xref ref-type="bibr" rid="B44">Meng et al., 2021</xref>), suggesting that the South Bainaimiao Ocean had formed. During this period, the Bainaimiao arc separated the South Bainaimiao Ocean from the Paleo-Asian Ocean, with the former serving as a branch ocean basin (<xref ref-type="fig" rid="F19">Figure 19A</xref>). Ages of ophiolite blocks suggest that the South Bainaimiao Ocean persisted into the Late Middle to Late Silurian. From 450 to 424 Ma, ongoing northward subduction of the South Bainaimiao Ocean resulted in significant Bainaimiao arc-related magmatism (<xref ref-type="fig" rid="F19">Figure 19B</xref>). The closure of the South Bainaimiao Ocean is dated to the Late Silurian based on ages of the matrix and the youngest blocks within the ophiolite. During this period, the ophiolite matrix accumulated sediment from both Bainaimiao arc magmatism and materials of the northern margin of the NCC. The Bainaimiao arc collided with the NCC, leading to arc-continent collision (<xref ref-type="fig" rid="F19">Figure 19C</xref>). Following the arc-continent collision in the Late Silurian, a composite the NCC and the Bainaimiao arc emerged south of the Solon Suture Zone. Hence, arc-continent collision in the CAOB was pivotal in its formation and the growth of continental crust (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>). Subsequently, the NCC and the Bainaimiao arc remained a passive continental margin until the Late Carboniferous to Middle Permian, when southward subduction of Paleozoic South Asia transformed it into an Andean-type active continental margin (<xref ref-type="bibr" rid="B58">Song et al., 2021</xref>; <xref ref-type="bibr" rid="B26">Li et al., 2023</xref>; <xref ref-type="bibr" rid="B26">Li et al., 2023</xref>).</p>
<fig id="F19" position="float">
<label>FIGURE 19</label>
<caption>
<p>Early Paleozoic evolution of the South Bainaimiao Ocean (<xref ref-type="bibr" rid="B85">Zhang et al., 2014</xref>; <xref ref-type="bibr" rid="B54">Shi et al., 2024</xref>).</p>
</caption>
<graphic xlink:href="feart-12-1487090-g019.tif"/>
</fig>
</sec>
</sec>
</sec>
<sec sec-type="conclusion" id="s6">
<title>6 Conclusion</title>
<p>
<list list-type="simple">
<list-item>
<p>(1) This study determined the following ages: Plagioclase actinolite schist, which forms the matrix of the ophiolitic m&#xe9;lange, is dated at 421 Ma; ultrabasic rock blocks are dated at 424 Ma; diabase porphyrite blocks have an age of 431.9 Ma; tonalite has a zircon U-Pb age of 425.7 Ma; and granodiorite has zircon U-Pb ages of 431 Ma and 433.2 Ma.</p>
</list-item>
<list-item>
<p>(2) Gabbros and ultrabasic rocks derived from the lithospheric mantle and undergo assimilation and mixing with the crust. Tonalite, quartz diorite, and granodiorite are island arc magmatic rocks formed by the interaction of subducted slabs, melting, the mantle wedge, and the crust, and exhibit geochemical characteristics similar to adakites. The gabbro and ultrabasic rocks in this study may be associated with tectonic environments such as volcanic arc basalt or mid-ocean ridges. The magmatic rocks in the northern part of Damaoqi are associated with a volcanic island arc tectonic environment.</p>
</list-item>
<list-item>
<p>(3) The evolution of the South Bainaimiao Ocean is divided into three stages: First stage (&#x223c;450 Ma): The Bainaimiao arc separated the South Bainaimiao Ocean from the Paleo-Asian Ocean, with the former acting as a branch basin of the latter. Second stage (450&#x2013;424 Ma): The South Bainaimiao Ocean subducted northward. The subducted slab partially melted and interacted with the crust-mantle wedge, producing subduction-related island arc magmatic rocks. Third stage (424&#x2013;421 Ma): The South Bainaimiao Ocean closed, leading to an arc-continent collision between the Bainaimiao arc and the northern margin of the North China Craton.</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 sec-type="author-contributions" id="s8">
<title>Author contributions</title>
<p>Chenfei Feng: Data curation, Investigation, Methodology, Visualization, Writing&#x2013;original draft. GW: Conceptualization, Funding acquisition, Investigation, Project administration, Resources, Writing&#x2013;review and editing. ZZ: Conceptualization, Funding acquisition, Investigation, Project administration, Resources, Writing&#x2013;review and editing. SG: Writing&#x2013;review and editing. JC: Investigation, Writing&#x2013;review and editing. HH: Investigation, Writing&#x2013;review and editing.</p>
</sec>
<sec sec-type="funding-information" id="s9">
<title>Funding</title>
<p>The author(s) declare that financial support was received for the research, authorship, and/or publication of this article. This research was financially supported by the National Science Foudation of China: Early Paleozoic tectonic framework and evolution in the southern margin of western Xing-Meng Orogenic Belt (42272239) and The spatial-temporal relationships and its tectonic significance of the newly discovered tectonic m&#x00E9;lange within the Xingmeng Orogenic Belt (41872232).</p>
</sec>
<sec sec-type="COI-statement" id="s10">
<title>Conflict of interest</title>
<p>The reviewer JW declared a shared affiliation with the authors to the handling editor at the time of review.</p>
<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.2024.1487090/full#supplementary-material">https://www.frontiersin.org/articles/10.3389/feart.2024.1487090/full&#x23;supplementary-material</ext-link>
</p>
<supplementary-material xlink:href="Table1.xlsx" id="SM1" mimetype="application/xlsx" xmlns:xlink="http://www.w3.org/1999/xlink"/>
</sec>
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