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  <front>
    <journal-meta><journal-id journal-id-type="publisher">SE</journal-id><journal-title-group>
    <journal-title>Solid Earth</journal-title>
    <abbrev-journal-title abbrev-type="publisher">SE</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Solid Earth</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1869-9529</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/se-17-1035-2026</article-id><title-group><article-title>Silurian syn- and post-collision granitic magmatism in the western section of the North Qinling Orogen: implications for collisional orogenic processes</article-title><alt-title>Silurian syn- and post-collision granitic magmatism</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Lin</surname><given-names>Hao</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Li</surname><given-names>Zuochen</given-names></name>
          <email>lizuochen@chd.edu.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Pei</surname><given-names>Xianzhi</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Zhao</surname><given-names>Shaowei</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Wang</surname><given-names>Meng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Zhou</surname><given-names>Hai</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Gao</surname><given-names>Feng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Wang</surname><given-names>Mao</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Qin</surname><given-names>Li</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>School of Earth Science and Resources, Chang'an University, Xi'an 710054, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Xi'an Key Laboratory for Mineralization and Efficient Utilization of Critical Metals, Xi'an 710054, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Geophysical Exploration Academy of China Metallurgical Geology Bureau, Baoding 071051, China</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>School of Geology and Mining Engineering, Xinjiang University, Urumqi 830046, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Zuochen Li (lizuochen@chd.edu.cn)</corresp></author-notes><pub-date><day>9</day><month>September</month><year>2026</year></pub-date>
      
      <volume>17</volume>
      <issue>9</issue>
      <fpage>1035</fpage><lpage>1062</lpage>
      <history>
        <date date-type="received"><day>7</day><month>July</month><year>2024</year></date>
           <date date-type="rev-request"><day>21</day><month>October</month><year>2024</year></date>
           <date date-type="rev-recd"><day>27</day><month>July</month><year>2026</year></date>
           <date date-type="accepted"><day>31</day><month>August</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Hao Lin et al.</copyright-statement>
        <copyright-year>2026</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026.html">This article is available from https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026.html</self-uri><self-uri xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026.pdf">The full text article is available as a PDF file from https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e178">The Liqiao and Xianping plutons can provide crucial evidence for the collision-orogeny process of the Proto-Tethys Ocean in the western section of the North Qinling Orogen. In this study, we present petrological, zircon U-Pb geochronological, geochemical, and zircon Lu-Hf isotopic data for these plutons. Both the Liqiao and Xianping plutons are characterized as high-K, calc-alkaline, metaluminous to weakly peraluminous granites, with ages of 429   and 421 Ma, respectively. The Liqiao pluton was classified as I-type granite, displaying positive <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values ranging from <inline-formula><mml:math id="M2" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.1 to <inline-formula><mml:math id="M3" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>3.4, and high Mg<sup><italic>#</italic></sup> values from 37.86 to 48.25. We interpret this to indicate that it was generated by the partial melting of juvenile felsic lower crust, with a contribution from mantle-derived material. In contrast, the Xianping pluton exhibits lower Mg<sup><italic>#</italic></sup> values (20.40 to 35.11) and negative <inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values (<inline-formula><mml:math id="M7" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>18.0 to <inline-formula><mml:math id="M8" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13.9), consistent with the geochemical characteristics of highly fractionated I-type granite. This suggests that the Xianping pluton formed through the partial melting of ancient felsic crust and followed by extensive fractional crystallization. We propose that the Liqiao pluton originated in a syn-collisional setting, while the Xianping pluton formed in a post-collisional environment. Both plutons are products of the collisional orogeny between the Yangtze Block and the North Qinling Orogen, which were associated with the closure of the Wushan-Shangdan Ocean, the northern of the Proto-Tethys Ocean.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>41872235</award-id>
<award-id>42172236</award-id>
<award-id>41872234</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Fundamental Research Funds for the Central Universities</funding-source>
<award-id>300102270202</award-id>
<award-id>300103183081</award-id>
<award-id>300104282717</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d2e271">It is generally believed that the Proto-Tethys Ocean was a giant ocean, which was located between the northern Laurasia continent and the southern Gondwana continent (Stampfli and Borel, 2002; Li et al., 2016a; Wu et al., 2020). The Central China Orogenic Belt (CCOB) is one of the most developed areas of the Proto-Tethys tectonic domain, it includes the West Kunlun Orogen, East Kunlun Orogen, Altyn Orogen, North Qaidam Orogen, Qilian Orogen and Qinling-Dabie Orogen, which preserved abundant information on the process of orogeny of various blocks in the North China, South China, Qaidam, Tarim, and Qiangtang regions from the Paleozoic-Early Mesozoic (Dong et al., 2021, 2022a, 2022b). The Qinling Orogen is an important component of the CCOB, which was located between the Yangtze Block (YB) and the North China Block (NCB), it consists of two sutures (the Wushan-Shangdan Suture and the Mianlue Suture) and three blocks (the North Qinling Orogen, the South Qinling micro-block, and the northern margin of the YB) (Zhang et al., 2001; Wang et al., 2015; Wang and Wu, 2013; Dong et al., 2021, 2022a, b; Fig. 1a). Previous scholars have conducted extensive studies on the Qinling Orogen (Zhang et al., 2001, 2019; Pei et al., 2004, 2009; Wu et al., 2006; Wang et al., 2006, 2007; Xu et al., 2008; Dong et al., 2011a, 2011b, 2011c, 2021), the Early Paleozoic was the main ocean-continent transformation stage of the Qinling Orogen (Xia et al., 1998; Dong et al., 2008; Wang et al., 2015; Ren et al., 2019; Dong et al., 2021). As an important part of the Qinling Orogen, the North Qinling Orogen has complex tectonic evolution and large-scale magmatism. It is a key for exploring the collision of the YB and the North Qinling Orogen. Also, it is an important window for studying the structural evolution of the Proto-Tethys Ocean.</p>
      <p id="d2e274">Existing studies indicate that the Wushan-Shangdan Suture was formed during the Caledonian period., which is the result of the collision orogeny between the YB and the NCB (Ren et al., 2019). However, there is still considerable controversy over the duration of the subduction-collision orogeny process of the northern branch of the Proto-Tethys Ocean represented by the Wushan-Shangdan Ocean. There are two main views: some scholars believe that the main orogenic stage of the North Qinling Orogen was the late Neoproterozoic to the Mid-Late Triassic, the Wushan-Shangdan Ocean was subducted into the NCB during the Early Paleozoic, by the Middle-Late Devonian, this process transitioned into a continent-continent collision between the YB with the NCB, culminating in the closure along the Wushan-Shangdan Suture (Zhang et al., 2001, 2019; Dong et al., 2011a, c). Another scholar believes that the Wushan-Shangdan Ocean was formed in the North Qinling Orogen during the Late Cambrian, the ocean subduction and the development of ancient island arc occurred in the Ordovician, until to the Silurian-Late Devonian periods, there were continent-continent or continent-arc collision orogeny (Pei et al., 2009; Wang et al., 2009; Ren et al., 2019).</p>
      <p id="d2e277">In the western section of the North Qinling Orogen, there are lots of Caledonian basic-intermediate pluton and granite distributed in the Liushuigou-Shuangchangxia and Baihua-Liqiao areas (Pei et al., 2007a; Fig. 1b). These are primarily magmatic rocks related to subduction-collision (Dong et al., 2011a; Li et al., 2018a; Ren et al., 2018, 2021; Yang et al., 2018a). Research on the Paleozoic magmatic rocks of different ages and origins in the western section of the North Qinling Orogen can provide important evidence for the subduction-collision-post-collision orogeny process of the Wushan-Shangdan Ocean in the western section of the North Qinling Orogen in the Early Paleozoic, there by constraining the process and timing of Early Paleozoic orogeny in eastern of the Proto-Tethys Ocean. For a clearer understanding of the tectonic evolution of the western section of North Qinling Orogen, we focus on the Liqiao pluton (LP) and Xianping pluton (XP) in the western section of the North Qinling Orogen (Figs. 1, 2). We conduct studies on petrology, geochemistry, zircon U-Pb geochronology, and zircon Lu-Hf isotope to determine the petrogenesis and age of the rocks, trace the magma source and tectonic background, establish a sequence of tectonic and magmatic evolution events, and explore the relationship between the Caledonian orogeny in the North Qinling Orogen and the tectonic evolution of the Proto-Tethys Ocean.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e283"><bold>(a)</bold> Simplified geological map of the division of tectonic units in Qinling Orogen (Mao et al., 2017; Dong et al., 2022b). <bold>(b)</bold> Simplified geological map of the conjunction zone between the North Qinling Orogen and the North Qilian Orogen showing the distribution of Early Paleozoic plutons (Pei et al., 2004a; Xu et al., 2012).</p></caption>
        <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f01.jpg"/>

      </fig>

</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Geological Setting</title>
      <p id="d2e305">The western section of the North Qinling Orogen is limited in the Tethys tectonic domain, the Paleo-Asian Ocean tectonic domain, and the Pacific tectonic domain (Pei et al., 2009). It is located in the middle section of the CCOB (Zhang et al., 2001; Dong et al., 2022a; Fig. 1a). It is bounded by the North Qilian Orogen and NCB to the north, and the South Qinling tectonic belt to the south (Fig. 1b), which has developed an active continental margin trench-arc-basin system in the Early Paleozoic (Pei et al., 2009; Dong et al., 2011a; Zhang et al., 2011; Dong and Santosh, 2016). The exposed strata in this area range from the Paleoproterozoic to the Early Paleozoic (Pei et al., 2009). The Precambrian crystalline basement is composed by Paleoproterozoic Qinling Group, which was composed by felsic gneisses, aluminous gneiss and marble-calc-silicate (Pei et al., 2009; Diwu et al., 2014). Previous zircon U-Pb dating indicate that it was formed in 2298 to 1867 Ma (Zhang et al., 2001). The high-pressure and ultra-high-pressure (HP-UHP) metamorphic rock are exposed in the Qinling Group, which are the products of exhumation of continental crust experienced subduction to deep-subduction during the Early Paleozoic (Gong et al., 2016; Liu et al., 2020). The previous studies of the Kuanping Group have mainly focused on the central and eastern parts of the North Qinling Orogen, and have reported Meso-Neoproterozoic ages from 1974 to 813 Ma for the meta-volcanic rocks which with normal-type mid-ocean ridge basalt (N-MORB) affinities, and it was considered to represent oceanic crust (Xue et al., 1996; Zhang et al., 2001; He et al., 2007; Pei et al., 2009; Diwu et al., 2010; Gao et al., 2015; Dong et al., 2014, 2015, 2021; Zeng et al., 2023). The ophiolite with Late Cambrian N-MORB type basic volcanic rocks developed in the Guanzizhen area, which extends eastward to the Liqiao area and westward to the Wushan-Yuanyangzhen area, representing the material record of ancient oceanic crust (Pei et al., 2004b, 2007a; Dong et al., 2008). In the Late Cambrian-Early Ordovician, the Wushan-Shangdan Ocean (represented by the Guanzizhen-Wushan ophiolite) was subducted from south to north, and formed the island arc-forearc basin represented by the Liziyuan Group metamorphic sedimentary-volcanic rocks (Pei et al., 2006; Yang et al., 2018b). The Paleozoic Liziyuan Group are composed by metamorphic clastic rocks and carbonates sedimentary facies and metamorphic basalt, metamorphic basalt andesites, and metamorphic andesites volcanic facies (Pei et al., 2006). With the continued subduction of the Wushan-Shangdan Ocean, the metavolcanic rocks of the Caotangou Group and the corresponding volcaniclastic and shallowly metamorphosed clastic rocks, which are typical of island arc, were formed in the Middle-Late Ordovician (Yan et al., 2007; Zhu et al., 2008; Pei et al., 2009; Xu et al., 2014; Xie et al., 2020). The Ordovician Caotangou Group was composed by metamorphic volcanic-sediment, and it was divided into the lower Honghuapu Formation, the middle Zhangjiazhuang Formation, and the upper Longwanggou Formation (Song et al., 1991; Sun and Dong, 1995; Pei et al., 2009; Chen et al., 2019). Concurrently, intermediate-basic igneous complex of Liushuigou and Baihua were formed (Pei et al., 2007b; Gao et al., 2012), as well as subduction-type pluton such as Tangzang quartz diorite, Honghuapu tonalite, Yangjiazhuang quartz diorite, and Sanchahe quartz diorite (Chen et al., 2002, 2008; Wang et al., 2006; Ren et al., 2018; Qin et al., 2022). The tectonic background began to transition to the continental-continental or arc-continental collision orogeny after the subduction of the ancient oceanic crust and developed Caledonian collision-type pluton such as Dangchuan granite, and entered into an extension environment until the end of the orogeny in the Late Silurian-Early Devonian (Wang et al., 2008; Wang, 2013; Ren et al., 2018, 2021; Qin et al., 2022; Xin and Huang, 2023).</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e310">Geological map showing the LP and XP in the western section of North Qinling Orogen (Pei et al., 2004a; Xu et al., 2012).</p></caption>
        <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f02.png"/>

      </fig>

</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Petrography and samples</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Liqiao pluton</title>
      <p id="d2e334">The LP is located in the Xiongshangou-Shaping-Yujiaping-Liqiao area of the western section of the North Qinling Orogen (Figs. 1b,   2), and the pluton is distributed in the NWW direction, which is consistent with the regional tectonic line. In spatial distribution, it intruded into the Paleoproterozoic complex (e.g. Qinling Group), the Early Silurian Baihua intermediate-basic igneous complex, the Ordovician metasedimentary clastic strata (e.g. the Honghuapu Formation of the Caotangou Group). The LP is in fault contact with the Baihua Complex. In addition, there is a large number of diorite xenolith of Baihua Complex in the LP. The LP consists of monzogranite and minor syenogranite (Fig. 3a–b). The red monzogranite shows medium- to coarse-grained, some with pseudoporphyritic granite, and massive structure (Fig. 3a). Samples from the monzogranite are composed by K-feldspar (35 vol %–45 vol %), plagioclase (35 vol %–45 vol %), quartz (20 vol %–25 vol %), biotite (<inline-formula><mml:math id="M9" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 5 vol %). The accessory minerals are mainly apatite, sphene, ilmenite, monazite. It shows distinct myrmekitic structure (Fig. 3c). K-feldspar is euhedral, with development of gridiron twinning, ranging from 1.0 to 5.0 mm in size. Plagioclase is generally euhedral or subhedral, with development of polysynthetic twin and carlsbad—albite compound twin, ranging from 2.0 to 3.0 mm in size. The plagioclase crystals are commonly euhedral to subhedral laths. Quartz is allotriomorphic granular structure with undulatory extinction. Biotite is yellow-brown, block-like structure with significant pleochroism, local chloritization. To contrast with the monzogranite, the syenogranite (Fig. 3b) has higher K-feldspar (45 vol %–55 vol %), lower plagioclase (20 vol %–25 vol %), similar quartz (20 vol %–30 vol %), biotite (<inline-formula><mml:math id="M10" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 5 vol %), and a small amount of hornblende (Fig. 3d).</p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e353">Representative field photographs and photomicrographs of the LP <bold>(a–d)</bold> and XP <bold>(e–h)</bold> in the western section of North Qinling Orogen. Kfs <inline-formula><mml:math id="M11" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> K-feldspar, Pl <inline-formula><mml:math id="M12" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> Plagioclase, Bt <inline-formula><mml:math id="M13" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> biotite, Qz <inline-formula><mml:math id="M14" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> Quartz, Hbl <inline-formula><mml:math id="M15" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> Hornblende, Spn <inline-formula><mml:math id="M16" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> Sphene.</p></caption>
          <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f03.jpg"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Xianping pluton</title>
      <p id="d2e419">The XP locates in the east-north of the LP (Fig. 2). It also contacted with Baihua Complex by faults. The pluton intruded into the Meso-Neoproterozoic metamorphic volcanic-sediment (e.g. Kuanping Group), the Early Silurian Baihua intermediate-basic igneous complex. It is bounded by the Qinlingdabao granite to the north, which is in contact with a fault. The original structures observed in XP are believed to have been formed during magmatic crystallisation process. During the process of magmatic crystallisation, the magma at the edge of the XP remains thermoplastic due to the influence of its melt. The upwelling magma, along with the pressure of surrounding rocks, results in the formation of local shear, leading to mylonitization of surrounding rocks, the minerals are flattened and elongated. This causes the minerals to become flattened and elongated, and it also leads to the formation of augen structures and banded structures. The XP is mainly syenogranite, which shows medium-coarse-grained and massive structure (Fig. 3e–f). There was a distinct coarse-medium-grained transition zone can be seen in the pluton (Fig. 3e). The syenogranites are comprising K-feldspar (45 vol %–60 vol %), plagioclase (10 vol %–20 vol %), quartz (25 vol %–30 vol %), biotite (<inline-formula><mml:math id="M17" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 5 vol %), and minor accessory minerals include zircon, apatite, sphene, monazite, hornblende (Fig. 3g–h). K-feldspar is ranging from 2.0 to 4.0 mm. Plagioclase is ranging from 2.0 to 5.0 mm. Quartz is subhedral and allotriomorphic granular structure with undulatory extinction, it fills in the spaces between other minerals in a granular form. Biotite is gray-brown, block-like structure, form with significant pleochroism, local chloritization.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Samples</title>
      <p id="d2e437">Two zircon U-Pb dating samples were collected from the LP, including a monzogranite (TS19001-3) and a syenogranite (TS19007-2). The locations of the two samples are 34°14<sup>′</sup>04.05<sup>′′</sup> N, 106°25<sup>′</sup>09.71<sup>′′</sup> E, and 34°13<sup>′</sup>22.92<sup>′′</sup> N, 106°24<sup>′</sup>27.68<sup>′′</sup> E in the Liqiao-Yanghe-Wuhe area. Two zircon U-Pb dating samples were collected from the XP, including two syenogranite (TS19014-1 and TS19014-3). The sampling location is in the Xianpinggou-Shangxianping-Nianziping area, which located in 34°16<sup>′</sup>28.15<sup>′′</sup> N, 106°24<sup>′</sup>26.88<sup>′′</sup> E, and 34°16<sup>′</sup>28.21<sup>′′</sup> N, 106°24<sup>′</sup>26.95<sup>′′</sup> E, respectively. We also collected 15 whole-rock geochemical samples (including two zircon U-Pb dating samples) from the LP and 12 samples (including two zircon U-Pb dating samples) from the XP. All samples were fresh and free of corrosion, and the sampling locations are shown in Fig. 2.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Analytical methods</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Zircon U-Pb age</title>
      <p id="d2e626">The samples used for geochronological research were crushed and zircon separated by Xi'an Ruishi Geological Technology Co., Ltd. Zirconium target and cathodoluminescence (CL) imaging were completed by Beijing Zircon Nian Linghang Technology Co., Ltd. Zircon U-Pb isotope testing was conducted on the German Jena PQMS ICP-MS instrument using the laser ablation system NWR193. The 91500 standard sample and GJ-1 control sample were used in this analysis. Data processing was done using the ICPMSDataCal program (Liu et al., 2010). Weighted mean age calculations and concordia diagrams were produced using the Isoplot program (Ludwig, 2012). For a detailed description of the analysis methods and instrument parameters, refer to Li et al.  (2009).</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Whole-rock major and trace elements</title>
      <p id="d2e637">The testing of major, rare earth, and trace elements in whole-rock samples was conducted in the Key Laboratory of Western China's Mineral Resources and Geological Engineering, Ministry of Education, Chang'an University. The analysis of major elements was performed using X-ray fluorescence spectroscopy (XRF) method. The XRF fusion method was carried out in accordance with the national standard GB/T 14506.28-1993, with an analysis precision better than 2 % to 3 %. The samples were weighed after being heated at 1000 °C for 90 min in an oven to determine the loss on ignition (LOI). Rare earth and trace elements were analyzed using a Thermo-X7 Inductively Coupled Plasma Mass Spectrometer (ICP-MS).</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Zircon Lu-Hf isotope</title>
      <p id="d2e648">The zircon Lu-Hf isotope dating was carried out at Langfang Fengzeyuan Rock Mine Detection Technology Co., Ltd. The selected Zircon Lu-Hf isotope analysis point was located in the in-situ region of the zircon U-Pb dating site, and the zircon was ablated by the Resolution SE 193 nm excimer laser ablation system of ASI (Applied Spectra Inc.), and the spot beam diameter of laser ablation was generally 38 <inline-formula><mml:math id="M34" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, the energy density was 7–8 J cm<sup>−2</sup>, and the frequency was 10 Hz. The analytical system used is the multi-collector inductively coupled plasma mass spectrometer (Neptune Plus) from the American company Thermo Fisher, with laser ablation material introduced into the Neptune Plus (MC-ICPMS) using high-purity He as carrier gas. The temperature requirement for the detection environment is 18–22 °C, with a relative humidity of less than 65 %. For detailed experimental principles, analytical techniques, and experimental procedures, refer to Wu et al. (2007) and Geng et al. (2011).</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Results of analyses</title>
      <p id="d2e681">The data for zircon U-Pb ages, zircon trace elements, whole-rock major and trace elements, and zircon Lu-Hf isotopes are shown in Supplement Tables S1, S2, S3 and S4, respectively.</p>
<sec id="Ch1.S5.SS1">
  <label>5.1</label><title>Zircon U-Pb age</title>
      <p id="d2e691">The zircon CL image and concordant U-Pb diagrams are shown in Fig. 4. Zircons (TS19001-3) from the Liqiao monzogranite have length of 80 to 180 <inline-formula><mml:math id="M36" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, with respect ratios from <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, most grains display developed oscillatory zoning (Fig. 4a). Except for 4 discordant spots, the remaining 21 concordant spots have U <inline-formula><mml:math id="M39" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1020 to 2806 <inline-formula><mml:math id="M40" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>, Th <inline-formula><mml:math id="M42" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 875 to 4928 <inline-formula><mml:math id="M43" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>, with variable <inline-formula><mml:math id="M45" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Th</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">U</mml:mi></mml:mrow></mml:math></inline-formula> ratios of 0.48 to 1.98, consistent with the characteristics of typical magmatic zircons (Fig. 5). They have <sup>206</sup>Pb <inline-formula><mml:math id="M47" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <sup>238</sup>U ages of 417 to 435 Ma (Fig. 4a) and yielding a weighted mean age of 429.9 <inline-formula><mml:math id="M49" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.6 Ma (MSWD <inline-formula><mml:math id="M50" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.77, <inline-formula><mml:math id="M51" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M52" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 21).</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e849">CL image of zircons and the U-Pb zircon concordia diagrams from the LP and XP in the western section of North Qinling Orogen.</p></caption>
          <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f04.png"/>

        </fig>

      <p id="d2e858">Zircons (TS19007-2) from the Liqiao syenogranite have length of 60 to 170 <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, with respect ratios of <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, most grains display developed oscillatory zoning (Fig. 4b). 23 out of 25 spots have U <inline-formula><mml:math id="M56" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 341 to 2939 <inline-formula><mml:math id="M57" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>, Th <inline-formula><mml:math id="M59" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 290 to 3153 <inline-formula><mml:math id="M60" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>, with <inline-formula><mml:math id="M62" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Th</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">U</mml:mi></mml:mrow></mml:math></inline-formula> ratios of 0.21 to 1.63, consistent with the characteristics of typical magmatic zircons (Fig. 5). One spot (#21) has <sup>206</sup>Pb <inline-formula><mml:math id="M64" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <sup>238</sup>U age of 489 <inline-formula><mml:math id="M66" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 6.39 Ma, suggesting inherited origin. The remaining 22 spots have <sup>206</sup>Pb <inline-formula><mml:math id="M68" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <sup>238</sup>U ages of 421 to 432 Ma (Fig. 4b) and yield a weighted mean age of 429.4 <inline-formula><mml:math id="M70" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.4 Ma (MSWD <inline-formula><mml:math id="M71" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.22, <inline-formula><mml:math id="M72" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M73" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 22).</p>
      <p id="d2e1048">Zircons (TS19014-1) from the Xianping syenogranite have length of 50 to 130 <inline-formula><mml:math id="M74" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, with respect ratios of <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, most grains display developed oscillatory zoning (Fig. 4b). Except for one disconcordant spots, the remaining 24 spot have high U and Th contents (U <inline-formula><mml:math id="M77" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 692 to 9684 <inline-formula><mml:math id="M78" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>, Th <inline-formula><mml:math id="M80" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 342 to 3117 <inline-formula><mml:math id="M81" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>, with variable <inline-formula><mml:math id="M83" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Th</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">U</mml:mi></mml:mrow></mml:math></inline-formula> ratios of 0.22 to 0.70). They are consistent with the characteristics of typical magmatic zircons (Fig. 5). These 24 spots have <sup>206</sup>Pb <inline-formula><mml:math id="M85" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <sup>238</sup>U ages of 409 to 432 Ma (Fig. 4b), yield a weighted mean age of 421.8 <inline-formula><mml:math id="M87" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.2 Ma (MSWD <inline-formula><mml:math id="M88" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.00, <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">24</mml:mn></mml:mrow></mml:math></inline-formula>).</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e1204">Zircons U-Pb age-<inline-formula><mml:math id="M90" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Th</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">U</mml:mi></mml:mrow></mml:math></inline-formula> <bold>(a)</bold> and Chondrite-normalized REE patterns <bold>(b)</bold> diagram of the LP and XP in the western section of North Qinling Orogen. The chondrite and Primitive Mantle values are from Sun and McDonough (1989).</p></caption>
          <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f05.png"/>

        </fig>

      <p id="d2e1231">Zircons (TS19014-3) from the Xianping syenogranite have length of 40 to 170 <inline-formula><mml:math id="M91" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m, with respect ratios of <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, most grains display developed oscillatory zoning (Fig. 4c). In the 25 analysis spots, 18 spots display concordant U-Pb ages. They have high U and Th contents (U <inline-formula><mml:math id="M94" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1244 to 12052 <inline-formula><mml:math id="M95" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>, Th <inline-formula><mml:math id="M97" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 714 to 2351 <inline-formula><mml:math id="M98" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>, with variable <inline-formula><mml:math id="M100" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Th</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">U</mml:mi></mml:mrow></mml:math></inline-formula> ratios of 0.15 to 0.59), consistent with the characteristics of typical magmatic zircons (Fig. 5). These 18 spots have <sup>206</sup>Pb <inline-formula><mml:math id="M102" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <sup>238</sup>U ages of 408 to 428 Ma (Fig. 4d), yield a weighted mean age of 421.5 <inline-formula><mml:math id="M104" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.5 Ma (MSWD <inline-formula><mml:math id="M105" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.04, <inline-formula><mml:math id="M106" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M107" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 18).</p>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><title>Whole-rock major and trace element geochemistry</title>
<sec id="Ch1.S5.SS2.SSS1">
  <label>5.2.1</label><title>Liqiao pluton</title>
      <p id="d2e1402">Liqiao monzogranite and syenogranite have similar geochemistry characteristics. The LP display high SiO<sub>2</sub> (71.09 wt % to 76.45 wt %) contents, Al<sub>2</sub>O<sub>3</sub> <inline-formula><mml:math id="M111" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 12.15 wt % to 15.26wt%, as shown in the Q-A-P diagram (Fig. 6a), these sample plotted in the field of monzogranite and syenogranite. They have low Fe<sub>2</sub>O<inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mi>T</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> (0.90 wt % to 1.77 wt %) contents, MgO (0.30 wt % to 0.55 wt %) contents and Mg<sup><italic>#</italic></sup> (37.86 to 48.25) values, high differentiation index (DI <inline-formula><mml:math id="M115" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 89.21 to 93.24) values, high K<sub>2</sub>O (4.02 wt % to 5.76 wt %) contents, high total alkali (K<sub>2</sub>O <inline-formula><mml:math id="M118" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Na<sub>2</sub>O <inline-formula><mml:math id="M120" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 8.02 wt % to 9.83 wt %) contents and low Na<sub>2</sub>O <inline-formula><mml:math id="M122" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> K<sub>2</sub>O (0.68 to 1.00) ratios. In the TAS diagram (Fig. 6b), they plotted in the subalkaline granite field. They have low rittmann index(<inline-formula><mml:math id="M124" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) values of 1.94 to 3.43. As shown in the SiO<sub>2</sub> versus K<sub>2</sub>O diagram (Fig. 6c), most samples display high-K calc-alkaline series. All the samples have moderate <inline-formula><mml:math id="M127" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">A</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">CNK</mml:mi></mml:mrow></mml:math></inline-formula> values of 0.95 to 1.05 (Fig. 6d).</p>
      <p id="d2e1582">All samples have high total REE contents of 180.35 to 412.32 ppm. They show variable enrichment in LREE with (<inline-formula><mml:math id="M128" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> ratios <inline-formula><mml:math id="M130" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 27.46 to 51.51, (<inline-formula><mml:math id="M131" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sm</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> ratios <inline-formula><mml:math id="M133" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 6.94 to 12.72, (<inline-formula><mml:math id="M134" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Gd</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> ratios <inline-formula><mml:math id="M136" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2.49 to 3.48, and display insignificant Eu anomalies with <inline-formula><mml:math id="M137" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Eu</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Eu</mml:mi></mml:mrow></mml:math></inline-formula><sup>*</sup> <inline-formula><mml:math id="M139" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.54 to 1.03, <inline-formula><mml:math id="M140" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ce</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Ce</mml:mi></mml:mrow></mml:math></inline-formula><sup>*</sup> <inline-formula><mml:math id="M142" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.90 to 0.98 (Fig. 7a). On the primitive mantle normalized trace element spider diagram (Fig. 7b), all these samples show enrichment in Rb, Th, K and Pb, and significantly negative Nb, Ta, Zr, Sr, P, Ce and Ti anomalies, with high Sr (229 to 336 ppm), Ba (688 to 1877 ppm) and Rb (202 to 267 ppm) contents, characterizing crust-derived melts.</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e1727">Geochemical plots for rocks of the LP and XP of the western section of North Qinling Orogen: <bold>(a)</bold> Q-A-P diagram (Streckeisen, 1976); <bold>(b)</bold> TAS classification diagram (Middlemost, 1994); <bold>(c)</bold> K<sub>2</sub>O versus SiO<sub>2</sub> diagram (Peccerillo and Taylor, 1976); <bold>(d)</bold> <inline-formula><mml:math id="M145" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">A</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">CNK</mml:mi></mml:mrow></mml:math></inline-formula> (molar Al<sub>2</sub>O<sub>3</sub> <inline-formula><mml:math id="M148" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> [CaO <inline-formula><mml:math id="M149" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Na<sub>2</sub>O <inline-formula><mml:math id="M151" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> K<sub>2</sub>O]) versus <inline-formula><mml:math id="M153" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">A</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">NK</mml:mi></mml:mrow></mml:math></inline-formula> (molar Al<sub>2</sub>O<sub>3</sub> <inline-formula><mml:math id="M156" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> [Na<sub>2</sub>O <inline-formula><mml:math id="M158" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> K<sub>2</sub>O]) diagram (Maniar and Piccoli, 1989). </p></caption>
            <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f06.png"/>

          </fig>

</sec>
<sec id="Ch1.S5.SS2.SSS2">
  <label>5.2.2</label><title>Xianping pluton</title>
      <p id="d2e1908">Xianping syenogranite have SiO<sub>2</sub> <inline-formula><mml:math id="M161" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 73.92 wt % to 78.28 wt %, Al<sub>2</sub>O<sub>3</sub> <inline-formula><mml:math id="M164" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 11.27 wt % to 14.14 wt %, Fe<sub>2</sub>O<inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mi>T</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M167" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.56 wt % to 1.91 wt %, MgO <inline-formula><mml:math id="M168" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.13 wt % to 0.26 wt % and Mg<sup><italic>#</italic></sup> <inline-formula><mml:math id="M170" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 20.40 to 35.11, differentiation index (DI) <inline-formula><mml:math id="M171" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 91.69 to 94.47. Samples from the XP plot into the syenogranite field on the Q-A-P diagram (Fig. 6a). In the TAS diagram (Fig. 6b), all the samples plotted in the subalkaline granite field. They are rich in K<sub>2</sub>O (K<sub>2</sub>O <inline-formula><mml:math id="M174" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 3.57 to 5.34 wt %, Na<sub>2</sub>O <inline-formula><mml:math id="M176" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> K<sub>2</sub>O <inline-formula><mml:math id="M178" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.71 to 0.91) and have total alkali (K<sub>2</sub>O <inline-formula><mml:math id="M180" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Na<sub>2</sub>O) contents of 6.83 wt % to 9.37 wt %. They have low rittmann index(<inline-formula><mml:math id="M182" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) values of 1.32 to 2.81. The Xianping syenogranite show calc-alkaline affinity. As shown in the SiO<sub>2</sub> versus K<sub>2</sub>O diagram (Fig. 6c), most samples display high-K calc-alkaline series. Xianping syenogranite are metaluminous-weakly peraluminous with <inline-formula><mml:math id="M185" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">A</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">CNK</mml:mi></mml:mrow></mml:math></inline-formula> ratios of 0.98 to 1.04 (Fig. 6d).</p>
      <p id="d2e2133">These samples have REE contents of 81.26 to 205.05 ppm and show fractionated REE patterns expressed by LREE enrichment and HREE depletion with (<inline-formula><mml:math id="M186" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>N</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.46</mml:mn></mml:mrow></mml:math></inline-formula> to 8.99, (<inline-formula><mml:math id="M188" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sm</mml:mi></mml:mrow></mml:math></inline-formula>)<inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>N</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.43</mml:mn></mml:mrow></mml:math></inline-formula> to 4.66, (<inline-formula><mml:math id="M190" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Gd</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>N</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.55</mml:mn></mml:mrow></mml:math></inline-formula> to 1.39. They show significant negative Eu anomalies with <inline-formula><mml:math id="M192" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Eu</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Eu</mml:mi></mml:mrow></mml:math></inline-formula><sup>*</sup> <inline-formula><mml:math id="M194" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.18 to 0.33 (Fig. 7c). On the spider diagram (Fig. 7d), they are enriched in Rb, K, Pb, Th, and U and depleted in Nb, Ta, Ti, P, Zr, Ce and Ba, with low Sr (39 to 74 ppm), Ba (159 to 271 ppm) and Rb (189 to 477 ppm) contents.</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e2244">Chondrite-normalized REE patterns <bold>(a, c)</bold> and primitive mantle normalized trace element spider diagrams <bold>(b, d)</bold> of the LP and XP in the western section of North Qinling Orogen. The chondrite and Primitive Mantle values are from Sun and McDonough (1989). Syn-Collision granites from the western section of North Qinling Orogen after Wang et al.  (2008), Ren et al.  (2021), Qin et al. (2022), Xin and Huang (2023). Post-Collision granites from the western section of North Qinling Orogen after Ren et al. (2021).</p></caption>
            <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f07.png"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S5.SS3">
  <label>5.3</label><title>Zircon Lu-Hf isotope</title>
      <p id="d2e2268">Fifteen Lu-Hf spots from the Liqiao monzogranite (TS19001-3, 429 Ma) have positive <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values of <inline-formula><mml:math id="M196" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.5 to <inline-formula><mml:math id="M197" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>3.4, corresponding two-stage model ages of 1197 to 1383 Ma. Sixteen zircon Lu-Hf analysis spots from the Liqiao syenogranite (TS19007-2, 429 Ma) have variable Lu-Hf isotopic compositions, 14 spots display positive <inline-formula><mml:math id="M198" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values of <inline-formula><mml:math id="M199" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.6 to <inline-formula><mml:math id="M200" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>3.3, corresponding two-stage model ages of 1202 to 1374 Ma, only one spot (#1) has negative <inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> value of <inline-formula><mml:math id="M202" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.1 with corresponding two-stage model ages of 1411 Ma. And one inherited origin spot (#21) has positive <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values of <inline-formula><mml:math id="M204" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.3, corresponding two-stage model ages of 1269 Ma.</p>
      <p id="d2e2382">Fifteen Lu-Hf spots from the Xianping syenogranite (TS19014-1, 421 Ma) have negative <inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values of <inline-formula><mml:math id="M206" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>18.0 to <inline-formula><mml:math id="M207" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13.9, corresponding two-stage model ages of 2276 to 2530 Ma. Fifteen Lu-Hf spots from the Xianping syenogranite (TS19014-3, 421 Ma) have negative <inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values of <inline-formula><mml:math id="M209" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>18.5 to <inline-formula><mml:math id="M210" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13.6 with corresponding two-stage model ages of 2259 to 2560 Ma.</p>
</sec>
</sec>
<sec id="Ch1.S6">
  <label>6</label><title>Discussion</title>
<sec id="Ch1.S6.SS1">
  <label>6.1</label><title>Types of rock genesis</title>
      <p id="d2e2465">Currently, the most widely used classification scheme for granite types is the MISA classification, with M-type granite derived from mantle magmas being rare, and I-type, S-type, and A-type granite being predominant (Chappell and White, 1974, 2001; Coleman and Peterman, 1975; Whalen et al., 1987; Amri et al., 1996; Wu et al., 2007). Hornblende, cordierite and alkaline dark minerals are considered to be the most important and effective markers for the identification of I-type, S-type, and A-type granite, respectively (Miller, 1985). Fractionated granite is commonly characterized by the presence of the following minerals: beryl, tantalum-niobium ores, elbaite, lepidolite, or lithium muscovite (Zhu et al., 2002; Chudík et al., 2008; Merino et al., 2013; Wu et al., 2017).</p>
      <p id="d2e2468">Not only do the LP exhibit low concentrations of Zr (143 to 253 ppm), Ce (83.8 to 201.3 ppm), Zr <inline-formula><mml:math id="M211" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Nb <inline-formula><mml:math id="M212" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Ce <inline-formula><mml:math id="M213" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Y (258.2 to 507.68 ppm), and FeO<sup><italic>T</italic></sup> <inline-formula><mml:math id="M215" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> MgO ratios (2.25 to 3.44), but the XP also display low levels of Zr (85.3 to 187.2 ppm), Ce (26.7 to 90.5 ppm), Zr <inline-formula><mml:math id="M216" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Nb <inline-formula><mml:math id="M217" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Ce <inline-formula><mml:math id="M218" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Y (201.99 to 345.07 ppm), and FeO<sup><italic>T</italic></sup> <inline-formula><mml:math id="M220" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> MgO ratios (3.88 to 8.18). Both are distinct from typical A-type granites (Zr <inline-formula><mml:math id="M221" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 250 ppm, Zr <inline-formula><mml:math id="M222" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Nb <inline-formula><mml:math id="M223" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Ce <inline-formula><mml:math id="M224" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Y <inline-formula><mml:math id="M225" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 350 ppm, Ce <inline-formula><mml:math id="M226" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 100 ppm, FeO<sup><italic>T</italic></sup> <inline-formula><mml:math id="M228" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> MgO <inline-formula><mml:math id="M229" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 16; Whalen et al., 1987). Furthermore, the zircon saturation temperatures calculated using the empirical Watson and Harrison (1983) model show that the LP (<inline-formula><mml:math id="M230" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">Zm</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>: 770 to 825 °C) and XP (<inline-formula><mml:math id="M231" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">Zm</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>: 729 to 807 °C) are notably lower than those of typical A-type granites (<inline-formula><mml:math id="M232" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 850 °C, Watson and Harrison, 1983; Eby, 1990, 1992; Siégel et al., 2018). In addition, all compositions of the XP fall in the region of FG, while the LP plotted into the OGT in the discrimination diagrams (Fig. 8a–b). Consequently, the LP and XP cannot be classified as A-type granites. The LP exhibits lower Rb contents (159 to 267 ppm, mean 201 ppm) compared to highly fractionated granites (Rb <inline-formula><mml:math id="M233" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 270 ppm, King et al., 1997). In contrast, the XP displays high Rb contents (189 to 477 ppm, mean 307 ppm), indicating that the XP is a highly fractionated granite (Fig. 8c), whereas the LP is not. The 10 000<inline-formula><mml:math id="M234" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ga</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> ratio is elevated in late-crystallizing granite when I- and S-type granites undergo highly fractional crystallization of plagioclase (Dahlquist et al., 2014). Meanwhile, samples will be positioned within the A-type granite field in the 10 000<inline-formula><mml:math id="M235" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ga</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> discriminant diagrams (Whalen et al., 1987). The LP exhibits low 10 000<inline-formula><mml:math id="M236" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ga</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> ratios (2.14 to 2.78), while the XP displays high 10 000<inline-formula><mml:math id="M237" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ga</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> ratios (2.46 to 3.29). It is consistent with the observation that the samples are categorized as I &amp; S-type granite and A-type granite, respectively (Fig. 8d–e). The LP is characterized by a low <inline-formula><mml:math id="M238" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">A</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">CNK</mml:mi></mml:mrow></mml:math></inline-formula> ratio (0.95 to 1.05, less than 1.1), low P<sub>2</sub>O<sub>5</sub> content (0.07 wt % to 0.14 wt %, less than 0.20 wt %), and high Na<sub>2</sub>O content (3.27 wt % to 4.22 wt %, greater than 3.26 wt %). Similarly, the XP exhibits low P<sub>2</sub>O<sub>5</sub> contents (less than 0.20 wt %) and high Na<sub>2</sub>O contents (greater than 3.26 wt %), and these characteristics differ from those of S-type granites (Chappell and White, 1974; Chappell, 1999). Moreover, all samples are positioned in the I-type granite field in the Zr versus TiO2 discrimination diagrams (Fig. 8f). The presence of potential I-type granite indicators, such as hornblende (Fig. 3d and g, Miller, 1985), suggests that the LP should be classified as I-type granite and the XP as highly fractionated I-type granite.</p>

      <fig id="F8" specific-use="star"><label>Figure 8</label><caption><p id="d2e2767">Pluton type discrimination diagram of the LP and XP in the western section of North Qinling Orogen: <bold>(a)</bold> FeO<sup><italic>T</italic></sup> <inline-formula><mml:math id="M246" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> MgO versus (Zr <inline-formula><mml:math id="M247" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Nb <inline-formula><mml:math id="M248" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Ce <inline-formula><mml:math id="M249" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Y) (Whalen et al., 1987); <bold>(b)</bold> (K<sub>2</sub>O <inline-formula><mml:math id="M251" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Na<sub>2</sub>O) <inline-formula><mml:math id="M253" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> CaO versus (Zr+Nb+Ce+Y) (Whalen et al., 1987); <bold>(c)</bold> 100 <inline-formula><mml:math id="M254" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> (MgO <inline-formula><mml:math id="M255" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> FeO<sup><italic>T</italic></sup> <inline-formula><mml:math id="M257" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> TiO<sub>2</sub>) <inline-formula><mml:math id="M259" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> SiO<sub>2</sub> versus (Al<sub>2</sub>O<sub>3</sub> <inline-formula><mml:math id="M263" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> CaO) <inline-formula><mml:math id="M264" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> (FeO<sup><italic>T</italic></sup> <inline-formula><mml:math id="M266" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Na<sub>2</sub>O+K<sub>2</sub>O) (Sylvester, 1989); <bold>(d)</bold> 10 000<inline-formula><mml:math id="M269" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ga</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> versus Zn (Whalen et al., 1987); <bold>(e)</bold> 10 000<inline-formula><mml:math id="M270" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ga</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula> versus Zr (Whalen et al., 1987); <bold>(f)</bold> Zr versus TiO<sub>2</sub>.</p></caption>
          <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f08.png"/>

        </fig>

</sec>
<sec id="Ch1.S6.SS2">
  <label>6.2</label><title>Petrogenesis of the late Silurian intrusions</title>
      <p id="d2e3030">It is generally believed that there are three main origins of granite: (1) fractional crystallization of primary basaltic magma (Cawthorn and Brown, 1976; Wyborn et al., 1987; Turner et al., 1992; Mushkin et al., 2003), (2) partial melting of crustal material and followed by fractional crystallization (Barbarin, 1988; Skjerlie and Johnston, 1992; Turpin et al., 1990; Patiño Douce, 1997; Chappell et al., 2012), (3) The mixing of mantle- and crustal-derived materials (Petford and Atherton, 1996; Chappell, 1999; Harris et al., 1999; Yang et al., 2006).</p>
      <p id="d2e3033">The LP and XP consist of K-feldspar, plagioclase, quartz, biotite and a few accessory minerals. They differ in the following details: (1) the LP has higher Al<sub>2</sub>O<sub>3</sub> (12.15 wt % to 15.26 wt %), K<sub>2</sub>O (4.02 to 5.76 wt %) and Na<sub>2</sub>O <inline-formula><mml:math id="M276" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> K<sub>2</sub>O values (0.68 to 1.00) than the XP (11.27 wt % to 14.14 wt %, 3.57 wt % to 5.34 wt % and 0.71 to 0.91, respectively); (2) the LP has higher Sr (276 to 575 ppm) and Ba (688 to 1877 ppm) contents and <inline-formula><mml:math id="M278" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Sr</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Y</mml:mi></mml:mrow></mml:math></inline-formula> ratios (15.67 to 53.85), and lower Y contents (8.12 to 19.49 ppm) and <inline-formula><mml:math id="M279" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Rb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sr</mml:mi></mml:mrow></mml:math></inline-formula> ratios (0.35 to 0.85) than the XP (Sr <inline-formula><mml:math id="M280" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 39 to 74 ppm; Ba <inline-formula><mml:math id="M281" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 159 to 271 ppm; <inline-formula><mml:math id="M282" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Sr</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Y</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M283" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.97 to 2.62; Y <inline-formula><mml:math id="M284" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 20.43 to 42.41 ppm; <inline-formula><mml:math id="M285" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Rb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sr</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M286" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2.57 to 11.64); (3) the LP has higher La contents (44.80 to 108.25 ppm), lower Yb contents (1.89 to 19.35 ppm), and more fractional REEs ((<inline-formula><mml:math id="M287" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> <inline-formula><mml:math id="M289" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 27.5 to 51.5; LREE/HREE <inline-formula><mml:math id="M290" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 18.9 to 30.0) than the XP (La <inline-formula><mml:math id="M291" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 12.17 to 44.17 ppm; Yb <inline-formula><mml:math id="M292" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2.53 to 5.99 ppm; (<inline-formula><mml:math id="M293" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> <inline-formula><mml:math id="M295" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.5 to 9.0; LREE <inline-formula><mml:math id="M296" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HREE <inline-formula><mml:math id="M297" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2.3 to 8.9), and the Eu anomalies are slightly negative (<inline-formula><mml:math id="M298" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Eu</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Eu</mml:mi></mml:mrow></mml:math></inline-formula><sup>*</sup> <inline-formula><mml:math id="M300" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.54 to 1.03) and significant negative (<inline-formula><mml:math id="M301" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Eu</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Eu</mml:mi></mml:mrow></mml:math></inline-formula><sup>*</sup> <inline-formula><mml:math id="M303" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.18 to 0.33), respectively; and (4) LP has positive <inline-formula><mml:math id="M304" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values of <inline-formula><mml:math id="M305" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.1 to <inline-formula><mml:math id="M306" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>3.4 and XP has negative <inline-formula><mml:math id="M307" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values of <inline-formula><mml:math id="M308" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>18.5 to <inline-formula><mml:math id="M309" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13.6. These differences indicate that the LP and XP formed by different process.</p>

      <fig id="F9" specific-use="star"><label>Figure 9</label><caption><p id="d2e3386">Age versus <inline-formula><mml:math id="M310" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> diagram <bold>(a)</bold> and Age versus <sup>176</sup>Hf <inline-formula><mml:math id="M312" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <sup>177</sup>Hf diagram <bold>(b)</bold> of the LP and XP in the western section of North Qinling Orogen.</p></caption>
          <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f09.png"/>

        </fig>

<sec id="Ch1.S6.SS2.SSS1">
  <label>6.2.1</label><title>Liqiao pluton</title>
      <p id="d2e3452">On the one hand, LP has low Na<sub>2</sub>O <inline-formula><mml:math id="M315" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> K<sub>2</sub>O (0.68 to 1.00) and middle <inline-formula><mml:math id="M317" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">A</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">CNK</mml:mi></mml:mrow></mml:math></inline-formula> (0.95 to 1.05) ratios, indicating that it is formed by biotite dehydration melting (Patiño Douce and Beard, 1995). In general, a positive value of <inline-formula><mml:math id="M318" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> can be interpreted as the source rock being from the juvenile crust or depleted mantle, whereas a negative value of <inline-formula><mml:math id="M319" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> indicates that the source rock is ancient crustal components (Taylor and McLennan, 1985; Wu et al., 2007). The <inline-formula><mml:math id="M320" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values of the LP range from <inline-formula><mml:math id="M321" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.1 to <inline-formula><mml:math id="M322" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>3.4 (Fig. 9), which indicating that the source rock is juvenile crustal components. On the other hand, LP has high Sr (276 to 575) and La (44.8 to 108.3) contents, low Y (8.12 to 19.49) and Yb (0.88 to 1.89) contents indicated that the LP might be partial melting of thickened crust. The negative Eu anomalies (<inline-formula><mml:math id="M323" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Eu</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Eu</mml:mi></mml:mrow></mml:math></inline-formula><sup>*</sup> <inline-formula><mml:math id="M325" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.54 to 1.03) indicate that plagioclase is the predominant residue phase in the melting process (Patiño Douce and Beard, 1995). The <inline-formula><mml:math id="M326" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Nb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Ta</mml:mi></mml:mrow></mml:math></inline-formula> ratios (mean 14.28) and <inline-formula><mml:math id="M327" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Zr</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Hf</mml:mi></mml:mrow></mml:math></inline-formula> ratios (mean 37.42) of the LP are close to the continental crust (<inline-formula><mml:math id="M328" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Nb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Ta</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M329" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 13.4, <inline-formula><mml:math id="M330" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Zr</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Hf</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M331" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 35.7), significantly lower than melted magmas from the mantle source (<inline-formula><mml:math id="M332" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Nb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Ta</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M333" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 17.5) (McDonough and Sun, 1995; Rudnick, 1995; Weyer et al., 2003). The <inline-formula><mml:math id="M334" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Rb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sr</mml:mi></mml:mrow></mml:math></inline-formula> ratios of the crust-derived magmas are generally greater than 0.5, while the <inline-formula><mml:math id="M335" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ti</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Zr</mml:mi></mml:mrow></mml:math></inline-formula> ratios are usually less than 20 and the Cr contents of the primitive basaltic magma are 500 to 600 <inline-formula><mml:math id="M336" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup> (Wilson, 1989). LP has low Cr content (2.89 to 7.27 <inline-formula><mml:math id="M338" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 500 <inline-formula><mml:math id="M339" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>), <inline-formula><mml:math id="M341" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ti</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Zr</mml:mi></mml:mrow></mml:math></inline-formula> ratios (6.12 to 7.85 <inline-formula><mml:math id="M342" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 20) and high <inline-formula><mml:math id="M343" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Rb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sr</mml:mi></mml:mrow></mml:math></inline-formula> ratios (0.35 to 0.85 <inline-formula><mml:math id="M344" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.5), which indicates the LP is fundamentally different from mantle source magma and similar to crust-derived magma. Also, In the LP, no mafic intrusions have been found, and it has high SiO<sub>2</sub> contents (71.09 wt % to 76.45 wt %), which indicates that the fractional crystallization of mantle source magma model is impossible (Defant and Drummond, 1990).</p>

      <fig id="F10" specific-use="star"><label>Figure 10</label><caption><p id="d2e3790">The source region diagrams of the LP and XP in the western section of North Qinling Orogen: <bold>(a)</bold> molar K<sub>2</sub>O <inline-formula><mml:math id="M347" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Na<sub>2</sub>O versus molar CaO <inline-formula><mml:math id="M349" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> (MgO <inline-formula><mml:math id="M350" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> FeO<sup><italic>T</italic></sup>) (Altherr and Siebel, 2002); <bold>(b)</bold> Nb/Y versus Th/Y (Boztuğ et al., 2007); <bold>(c)</bold> CaO versus Sr (He et al., 2011); <bold>(d)</bold> (La/Yb)<sub><italic>N</italic></sub> versus Sr/Y (He et al., 2011).</p></caption>
            <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f10.png"/>

          </fig>

      <p id="d2e3869">As shown in the K<sub>2</sub>O <inline-formula><mml:math id="M354" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Na<sub>2</sub>O versus CaO <inline-formula><mml:math id="M356" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> (MgO <inline-formula><mml:math id="M357" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> FeO<sup><italic>T</italic></sup>) diagram (Fig. 10a), the samples plot in the field of metaandesites and metabasalts. In the <inline-formula><mml:math id="M359" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Nb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Y</mml:mi></mml:mrow></mml:math></inline-formula> versus <inline-formula><mml:math id="M360" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Th</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Y</mml:mi></mml:mrow></mml:math></inline-formula> diagram (Fig. 10b), they plot in middle-lower crust field. In the CaO versus Sr and (<inline-formula><mml:math id="M361" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> versus <inline-formula><mml:math id="M363" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Sr</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Y</mml:mi></mml:mrow></mml:math></inline-formula> diagrams (Fig. 10c–d), they plot in crust field. The positive correlations of La and <inline-formula><mml:math id="M364" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sm</mml:mi></mml:mrow></mml:math></inline-formula>, Zr and <inline-formula><mml:math id="M365" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Zr</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sm</mml:mi></mml:mrow></mml:math></inline-formula> suggest that the LP exhibits partial melting trend (Fig. 11a–b). The Mg<sup><italic>#</italic></sup> value can serve as a basis for determining whether mantle-derived material has been added to crustal source magma (Frost et al., 2001). Melt produced by crustal melting shows Mg<sup><italic>#</italic></sup> <inline-formula><mml:math id="M368" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 40, and Mg<sup><italic>#</italic></sup> does not change with the degree of partial melting, and it only displays Mg<sup><italic>#</italic></sup> <inline-formula><mml:math id="M371" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 40 when mantle-derived material is added (Frey et al., 1978; Rapp and Watson, 1995; Hawkes and Kemp, 2006). The Mg<sup><italic>#</italic></sup> values of LP range from 37.86 to 48.25 (mean 41.81 <inline-formula><mml:math id="M373" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 40), indicating the involvement of mantle-derived material in the magmatic source area. In summary, we propose that the LP was formed by partial melting of juvenile felsic crust with the involvement of mantle-derived material.</p>

      <fig id="F11" specific-use="star"><label>Figure 11</label><caption><p id="d2e4073">The evolution and fractional diagrams of the LP and XP in the western section of North Qinling Orogen: <bold>(a)</bold> La versus <inline-formula><mml:math id="M374" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sm</mml:mi></mml:mrow></mml:math></inline-formula> <bold>(b)</bold> Zr versus <inline-formula><mml:math id="M375" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Zr</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sm</mml:mi></mml:mrow></mml:math></inline-formula> <bold>(c)</bold> Sr versus Ba (Rudnick, 1995) <bold>(d)</bold> La versus (<inline-formula><mml:math id="M376" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> (Rudnick, 1995). Pl: Plagioclase; Kfs: K-feldspar; Amp: Amphibole; Bt: biotite; Zr: Zircon; Spn-Sphene; Ap: Apatite; Mon: Monazite; Allan-Allanite.</p></caption>
            <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f11.png"/>

          </fig>

</sec>
<sec id="Ch1.S6.SS2.SSS2">
  <label>6.2.2</label><title>Xianping pluton</title>
      <p id="d2e4148">There are two main sources of highly fractionated I-type granite: (1) Formation of highly fractionated I-type granite as a result of partial melting of crustal material due to magmatic underplating of the fractionated mantle source (Wu et al., 2003; Wang et al., 2014). (2) The fractionated basic magma from mantle source underplated the lower crust and mixed with crust-derived felsic magma. They formed shallow-source hybrid magma chambers and undergo fractional crystallization to form highly fractionated I-type granite in later stage (Qiu et al., 2008). The high SiO<sub>2</sub> contents (73.92 wt % to 78.28 wt %) of the XP suggests that it was not derived from mantle-derived magmas (Defant and Drummond, 1990). The XP shows evolved zircon Hf isotopic compositions (<inline-formula><mml:math id="M379" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">18.5</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M380" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13.6), with corresponding two-stage model ages of 2259 to 2560 Ma (Fig. 9), these features clearly differ from the LP, suggesting a matured continental source region (Taylor and McLennan, 1985; Wu et al., 2007). It has higher K<sub>2</sub>O contents (3.57 wt % to 5.34 wt %), low <inline-formula><mml:math id="M382" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Nb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Ta</mml:mi></mml:mrow></mml:math></inline-formula> ratios (mean 11.61) and <inline-formula><mml:math id="M383" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Zr</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Hf</mml:mi></mml:mrow></mml:math></inline-formula> ratios (mean 27.93), similar to crustal source magmas (<inline-formula><mml:math id="M384" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Nb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Ta</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M385" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 13.4, <inline-formula><mml:math id="M386" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Zr</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Hf</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M387" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 35.7), different from mantle source magmas (<inline-formula><mml:math id="M388" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Nb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Ta</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M389" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 17.5) (McDonough and Sun, 1995; Rudnick, 1995; Weyer et al., 2003). It also has low Cr content (1.42 to 5.36 <inline-formula><mml:math id="M390" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 500 <inline-formula><mml:math id="M391" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>), <inline-formula><mml:math id="M393" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ti</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Zr</mml:mi></mml:mrow></mml:math></inline-formula> ratio (2.63 to 5.73 <inline-formula><mml:math id="M394" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 20) and high <inline-formula><mml:math id="M395" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Rb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sr</mml:mi></mml:mrow></mml:math></inline-formula> ratio (2.57 to 11.64 <inline-formula><mml:math id="M396" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.5), suggesting that the XP was crustal source origin (Wilson, 1989). As shown in the K<sub>2</sub>O <inline-formula><mml:math id="M398" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Na<sub>2</sub>O versus CaO <inline-formula><mml:math id="M400" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> (MgO <inline-formula><mml:math id="M401" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> FeO<sup><italic>T</italic></sup>) diagram (Fig. 10a), the samples plot in the field of metaandesites and metabasalts. In the <inline-formula><mml:math id="M403" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Nb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Y</mml:mi></mml:mrow></mml:math></inline-formula> versus <inline-formula><mml:math id="M404" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Th</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Y</mml:mi></mml:mrow></mml:math></inline-formula> diagram (Fig. 10b), they plotted in middle-upper crust field. In the CaO versus Sr and (<inline-formula><mml:math id="M405" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> versus <inline-formula><mml:math id="M407" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Sr</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Y</mml:mi></mml:mrow></mml:math></inline-formula> diagrams (Fig. 10c–d), they plot in crust field. The Mg<sup><italic>#</italic></sup> values of XP range from 20.40 to 35.11 (<inline-formula><mml:math id="M409" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 40), indicating the absence of mantle-derived material in the magmatic source area (Frey et al., 1978; Rapp and Watson, 1995; Hawkes and Kemp, 2006). Characterization of partial melting in La versus <inline-formula><mml:math id="M410" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sm</mml:mi></mml:mrow></mml:math></inline-formula> and Zr versus <inline-formula><mml:math id="M411" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Zr</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Sm</mml:mi></mml:mrow></mml:math></inline-formula> diagrams (Fig. 11a–b). The XP is characterized by a high differentiation index (91.69–94.47, average 93.22) as well as significant depleting in HFSEs (i.e., Nb, Ta, P, Ti), suggesting that its source magma underwent significant fractional crystallization. Negative anomalies of Eu (<inline-formula><mml:math id="M412" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Eu</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Eu</mml:mi></mml:mrow></mml:math></inline-formula><sup>*</sup> <inline-formula><mml:math id="M414" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.18 to 0.33) and depleted in Sr and Ba in the samples are also indicative the fractional crystallization of plagioclase and K-feldspar (Rudnick, 1995; Patiño Douce and Beard, 1995). The Sr versus Ba diagram (Fig. 11c) reflects fractional crystallization of K-feldspar and plagioclase with a predominance of K-feldspar, which is consistent with the occurrence of K-feldspar and plagioclase phenocrysts in the samples. The depletions in P and Ti, Nb, and Ta are due to fractional crystallization of apatite and Ti-rich minerals, respectively, and as shown in the La versus (<inline-formula><mml:math id="M415" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> diagram (Fig. 11d), also reflect fractional crystallization of apatite and sphene. In summary, XP may have been formed through the partial melting of the ancient felsic crust, followed by extensive fractional crystallization.</p>
</sec>
</sec>
<sec id="Ch1.S6.SS3">
  <label>6.3</label><title>Tectonic background</title>
      <p id="d2e4553">The orogeny is typically used to describe a range of geological processes, including the magmatism of island and continental arcs, oceanic subduction and closure, continents collision and subduction, slab rollback during the syn-collision, delamination and orogenic collapse during the post-collision (Song et al., 2015; Xu et al., 2021; Zhang and Hou, 2015; Zheng et al., 2015, 2022; Zhu et al., 2022). The initiation of continental collision occurs when two continents converge and the oceanic crust between them is fully subducted, and the demise of this oceanic crust can be inferred from the ages of the high-pressure (HP) metamorphic rocks, arc volcanic rocks, and youngest ophiolites (Song et al., 2015). The syn-collision is characterized by a continental collision and subduction process. Despite the ocean having closed, subduction is not terminated, this is because it requires a significant amount of time for one continent to be subducted beneath another and achieve ultra-high-pressure (UHP) metamorphic conditions. During the process of continental collision and subduction, both the previously subducted oceanic crust and the continental crust undergo decompression melting as they are exhumed and the crust thickens, and accompanied by partial melting of crustal material to produce tonalites and peraluminous granites, without input of mantle materials (Chen et al., 2013; Liu et al., 2014; Song et al., 2014). Additionally, crustal melts derived from the deep subducted continental crust during exhumation could metasomatize the overlying lithospheric mantle, leading to the formation of mafic magmas (Zhao et al., 2012). The post-collisional is used to describe magmatism that occurs after the major collisional event, which typically marks the end of orogeny. It occured in the relaxation phase following the main orogeny, characterized by the large-scale horizontal movement of plate boundaries in the early phase and, in the late phase, by the delamination and collapse of orogeny, extension of the lithosphere, and crust-mantle interactions, such as the post-collisional magmas in the North Qaidam UHP metamorphic belt (Wu et al., 2014; Wang et al., 2014).</p>

      <fig id="F12" specific-use="star"><label>Figure 12</label><caption><p id="d2e4558">The tectonic setting diagrams of the LP and XP in the western section of North Qinling Orogen: <bold>(a)</bold> Zr versus (<inline-formula><mml:math id="M417" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Nb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Zr</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> (Batchelor and Bowden, 1985); <bold>(b)</bold> SiO<sub>2</sub> versus FeO<sup><italic>T</italic></sup> <inline-formula><mml:math id="M421" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> (FeO<sup><italic>T</italic></sup> <inline-formula><mml:math id="M423" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> MgO) (Maniar and Piccoli, 1989); <bold>(c)</bold> Y versus Nb (Pearce et al. 1984); <bold>(d)</bold> Yb versus Ta (Pearce et al., 1984); <bold>(e)</bold> (Y+Nb) versus Rb (Pearce et al., 1984); <bold>(f)</bold> R1 versus R2 (Batchelor and Bowden, 1985). Syn-Collision plutons from the western section of North Qinling Orogen after Wang et al., 2008; Ren et al., 2021; Qin et al., 2022; Xin and Huang, 2023. Post-Collision pluton from the western section of North Qinling Orogen after Ren et al. (2021).</p></caption>
          <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f12.png"/>

        </fig>

      <p id="d2e4649">According to the variations in chronology and geochemical features in the western section of the North Qinling Orogen, Ren et al. (2021) proposed that three magmatic pulses indicate a tectonic switch from slab rollback (ca. 441–434 Ma), slab break-off (ca. 430–423 Ma), to post-collision (ca. 415–409 Ma) from 441 to 409 Ma. In contrast, Qin et al. (2022) identified three main Paleozoic magmatic pulses from <inline-formula><mml:math id="M424" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 500 to 410 Ma, which correspond to oceanic subduction (ca. 500 to 450 Ma), slab rollback and break-off (ca. 440 to 430 Ma), and extension in a post-collision setting (ca. 420 to 410 Ma), respectively. The Qinling Complex in the western section of the North Qinling Orogen underwent late Silurian (433–424 Ma) granulite-facies metamorphism with a clockwise <inline-formula><mml:math id="M425" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M426" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> path, and followed by 411–402 Ma amphibolite-facies or retrograde overprinting metamorphism, suggesting that the granulite-facies rocks may have been formed by the continent-continent collisional orogeny in the Paleozoic (Guo et al., 2022; Mao et al., 2017, 2018). In contrast, the ages of granulite-facies metamorphism in the Qinling Complex, located in the eastern part of the North Qinling Orogen is mainly concentrated between 430 and 450 Ma (Liu et al., 2013; Xiang et al., 2014; Zhang et al., 2009, 2011). The zircon U-Pb age of the LP is 429 Ma, coinciding with the timeframe of magmatism during the second pulse, specifically the slab break-off (Ren et al., 2021; Qin et al., 2022). This aligns with the granulite-facies metamorphism period at 433–424 Ma (Mao et al., 2017, 2018), suggesting that the LP was likely formed during the intermediate stage of slab break-off in the syn-collisional process. Pay attention, the collision of YB and North Qinling Orogen along the Wushan-Shangdan Ocean margin might not terminate subduction (Li et al., 2018b, c; Allen et al., 2023). The zircon U-Pb age of the XP is 421 Ma, coinciding with the post-collisional orogenic process within the error range (420–409 Ma; Ren et al., 2021; Qin et al., 2022). It is also close to the timeframe limit of the amphibolite-facies or retrograde overprinting metamorphism from 411 to 402 Ma, suggesting that the XP was formed during the early stage of the post-collisional phase. Therefore, both of the LP and XP represent periods of collisional orogeny (Pei et al., 2009; Wang, 2013; Liu, 2013; Xie et al., 2020).</p>
      <p id="d2e4674">In the Zr versus (<inline-formula><mml:math id="M427" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Nb</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Zr</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> diagram (Fig. 12a), LP and XP plotted into the region of the collision related environment, indicating that they were formed in the collision-related setting, and the XP should be later than LP. In the SiO<sub>2</sub> versus FeO<sup><italic>T</italic></sup> <inline-formula><mml:math id="M431" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> (FeO<sup><italic>T</italic></sup> <inline-formula><mml:math id="M433" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> MgO) diagram (Fig. 12b), most samples from the LP plotted into the IAG-CAG-CCG region, while the XP fell into the POG region. In the Y versus Nb and Yb versus Ta diagrams (Fig. 12c–d), the LP mostly fell into the syn-collision field. In the (Y+Nb) versus Rb diagram (Fig. 12e), the XP mainly fell into the post-collision field. The LP shows syn-collision-related features, while the XP shows late-orogenic-related features (Fig. 12f). Combining with previous research on syn-collision and post-collision granite in the western section of the North Qinling Orogen (Wang et al., 2008; Ren et al., 2021; Qin et al., 2022; Xin and Huang, 2023), chondrite-normalized REE patterns and primitive mantle normalized trace element spider diagrams of the LP (Fig. 7a–b) was similar to the syn-collision granite, while the XP (Fig. 7c–d) was similar to the post-collisional granite, and there was a very clear linear evolutionary relationship from the LP to the XP, namely the trend from syn-collision to post-collision (Fig. 12). It can be inferred that the LP formed in syn-collision stage, as well as the XP formed in a post-collision stage. Both were products of the collisional orogeny between the northern margin of the YB and the North Qinling Orogen. The genesis of the LP and XP suggests that the heat required for partial melting of the lower-middle crust is likely to have originated from upwelling of the asthenosphere and the underplating of basaltic magma within an extension setting (Turnbull et al., 2016), and ridge subduction, slab rollback, slab break-off, and lower crustal delamination are the main deep geodynamic mechanisms that trigger extensional activity. Slab windows can provide enhanced heat flux during ridge subduction and form a large number of high-temperature granites (e.g., charnockite and alkali-feldspar granite; Geng et al., 2009). However, the North Qinling Orogen does not expose any high-temperature granites from the Ordovician and Silurian periods. The K-rich High-Ba-Sr intrusions (439–438 Ma) formed in a slab subduction setting, and the Na-rich intrusion (429–425 Ma) was associated with slab break-off (Ren et al., 2018). Moreover, the LP has a similar age to the Na-rich high-Ba-Sr intrusion.</p>
      <p id="d2e4740">Therefore, we suggest that the slab break-off following continental collision is the most likely cause of the magmatism that formed the LP (Fig. 13a). Since delamination of a thickened lower crust generally occurs in post-collisional setting (Song et al., 2015), it may therefore be the main mechanism for the formation of the magmatism of the XP (Fig. 13b).</p>

      <fig id="F13" specific-use="star"><label>Figure 13</label><caption><p id="d2e4745">Schematics geodynamic and petrogenetic model illustrating the evolution of the western section of the North Qinling Orogen at ca. 429 and 421 Ma, and the generation of the LP <bold>(a)</bold> and XP <bold>(b)</bold> during Late Silurian.</p></caption>
          <graphic xlink:href="https://se.copernicus.org/articles/17/1035/2026/se-17-1035-2026-f13.png"/>

        </fig>

</sec>
<sec id="Ch1.S6.SS4">
  <label>6.4</label><title>Tectonic significance</title>
      <p id="d2e4768">The rock types and geochemical characteristics of the intermediate-acid intrusive are closely related to the composition of the crustal and mantle (Chen et al., 2014). Furthermore, different tectonic setting can form the same type of granitic rocks, whereas the same tectonic environment can also give rise to different types of granitic rocks (Li et al., 2013; Wang et al., 2014). Therefore, any discussion on the magmatism and formation mechanism of orogeny must be based on the tectonic framework. The Proto-Tethys Ocean was a giant ocean developed during Neoproterozoic to Early Paleozoic, which was located between the northern Laurasia and the southern Gondwana, and it generated by the breakup of the Rodinia Supercontinent (Mattern and Schneider, 2000; Stampfli and Borel, 2002; Raumer and Stampfli, 2008; Li et al., 2016b, 2018b; Yang et al., 2018a; Wu et al., 2020). The northern boundary of the Qinling-Qilian Orogen in the CCOB is regarded as the northern boundary of the Early Paleozoic Proto-Tethys Ocean closure (Li et al., 2016b, 2017). The North Qinling Orogen preserves abundant Early Paleozoic records, revealing the tectonic evolution of the northern Proto-Tethys Ocean on the periphery of the northern margin of eastern Gondwana (Dong et al., 2021; Allen et al., 2023). The Wushan-Shangdan Suture is considered to represent an oceanic suture zone formed by closure of the Wushan-Shangdan Ocean, which formed the northern part of the Proto-Tethys Ocean along the northern margin of the eastern Gondwana during the Early Paleozoic (Zhang et al., 2001; Pei et al., 2009; Chen et al., 2024). The Wushan-Shangdan Suture is the most important tectonic zone separating the NCB from the YB (Zhang et al., 2001; Yang et al., 2002; Xu et al., 2006; Pei et al., 2009). The mate-basic volcanic rocks within Guanzizhen and Wushan ophiolite exhibit features of N-MORB and E-MORB, respectivelt, and yield zircon U-Pb ages of 534 to 489 Ma, which were both represented the remnants of the Wushan-Shangdan Ocean lithosphere (Hou et al., 2006; Li et al., 2007; Li, 2008; Pei et al., 2004, 2007a, 2009; Dong et al., 2008, 2011a). The northward subduction of the Wushan-Shangdan Ocean in the western section of the North Qinling Orogen in the Ediacaran-Ordovician resulted in the collision of the YB and the North Qinling Orogen in the southern part of the NCB, which reflected the relationship between the Caledonian orogeny in the North Qinling Orogen and the tectonic evolution of the Proto-Tethys Ocean (Pei et al., 2005, 2009). In combination with the results of previous research, the tectonic evolution of the western section of the North Qinling Orogen can be divided into three stages as follows.</p>
      <p id="d2e4771">Stage 1 from 472 to 438 Ma. Northward subduction of the Wushan-Shangdan Ocean.</p>
      <p id="d2e4774">With the northward subduction of the North Qinling Orogen, the Liziyuan Group represented by the metamorphic-volcanic-sedimentary rock system of the island arc-forearc basin during 472 to 451 Ma, and the Caotangou Group represented by the island-arc-type volcano-sedimentary rock system was formed in the fore-arc basin, which located between the island arc and the subduction zone at the southern margin of the North Qinling Orogen (Pei et al., 2006; He et al., 2007; Yan et al., 2007; Yang et al., 2018a). The Liushuigou gabbro, located north of the Guanzizhen ophiolite, has a zircon U-Pb age of 471 Ma, which was formed in island-arc tectonic setting (Pei et al., 2005, 2009; Yang et al., 2006). Additionally, the Baihua intermediate-basic igneous complex (449.7 Ma) in the western section of the North Qinling Orogen, the Hualingou meta-gabbro (440 Ma) and the Yuanyangzhen meta-gabbroic amphibolite (456 Ma) in the Wushan area were formed in an island-arc tectonic setting (Pei et al., 2007b; Li, 2008). The intermediate-basic volcanic (456.4 Ma, e.g. the Zhangjiazhuang Formation) and the acidic tuffs (457.4 Ma, e.g. the Longwanggou Formation) showed arc magmatism characterize, which recorded the subduction of Wushan-Shangdan Ocean in the Early Paleozoic (Wang et al., 2007; Chen et al., 2019; Zhu et al., 2008; Xu et al., 2014). There were Honghuapu tonalite (450.5 Ma), Tangzang quartz diorite (454.7 Ma), and the Sanchahe quartz diorite (459 Ma) in the Fengxian area (Wang et al., 2006, Chen et al., 2008, Qin et al., 2022), as well as the Yangjiazhuang and Honghuapu K-rich, high-Ba-Sr granitoids (439–438 Ma, Ren et al., 2018), were formed in subduction-related setting. In this stage, the slab roll-back of the Wushan-Shangdan Ocean initiated asthenosphere decompression melting in the mantle wedge and generated corresponding magmatic activities. Subsequently, asthenosphere convection induced partial melting of enriched mantle that had interacted with slab-derived fluids and produced basaltic magma that evolved into the Early Ordovician-Early Silurian gabbro, diorite and quartz diorite by fractional crystallization. Slab roll-back and its consequences strongly increased the geothermal gradient of the lower crust, which formed the early Silurian granites. These arc-related and subduction-related magmatic rocks define the age for the northward subduction of the Wushan-Shangdan Ocean from 472 to 438 Ma.</p>
      <p id="d2e4777">Stage 2 from 438 to 423 Ma. Initial continental collision of the YB with the North Qinling Orogen.</p>
      <p id="d2e4781">Previous studies have shown that slab break-off usually occurs very soon after continental collision (Duretz et al., 2011; van de Zedde and Wortel, 2001). Continuous subduction ultimately gave rise to the consumption of the Wushan-Shangdan Ocean oceanic crust and final collision between the YB and the North Qinling Orogen in the Early Silurian which resulted in the significantly thickened the crust, and there was no typical sedimentary state exposed in the area during this stage, but the intrusion activities of collisional-related magmas was voluminous with extensive development of Caledonian pluton (Pei et al., 2009). Due to buoyancy differences, slab break-off might have taken place, followed by subsequent asthenosphere upwelling, as well as the asthenosphere mantle-derived magma supplied both heat and mantle material, which underplated the lower part of the accretionary prism and triggered partial melting of juvenile crustal material accompanied by crust-mantle interaction (Davies and von Blanckenburg, 1995). The Dangchuan granite was formed by the partial melting of the thickened lower crust, with a U-Pb age from 438 to 432 Ma (Wang et al., 2008; Qin et al., 2022; Xin and Huang, 2023), as well as the Xiongshangou syn-collision granite (named LP of this paper) formed at 438 Ma (Wang, 2013), and the Jiguanya syn-collision granite at 435 Ma (Xu et al., 2018). The Tangzang Na-rich high-Ba-Sr granite, Zhangjiazhuang two-mica granite and muscovite granite formed during the slab break-off from 430 to 423 Ma (Ren et al., 2018, 2021). The formation of the LP (429 Ma) studied in this paper was attributed to partial melting of lower crust dominated by accreted Wushan-Shangdan Ocean oceanic crust and sediments, accompanied by local magma mixing with the mantle-derived magma. The presence of these intrusive rocks suggested that the Wushan-Shangdan Ocean closed before 438 Ma, and that the northern margin of the YB and the North Qinling Orogen underwent continent-continent collision from 438 to 423 Ma. During the Late Silurian (433 to 424 Ma), the western section of the North Qinling Orogen experienced granulite-facies metamorphism and anatexis (Mao et al., 2017), which may have occurred in a thickened lower crustal setting during the early stage of collision orogeny (Yu et al., 2013; Peng et al., 2021). This reflects the existence of an Early Paleozoic crustal thickening in the western section of the North Qinling Orogen, which comprehensively indicates that the northern margin of the YB and the North Qinling Orogen were in a docking and collision stage during the period of 438 to 423 Ma.</p>
      <p id="d2e4784">Stage 3 from 421 to 409 Ma. Post-collision extension phase.</p>
      <p id="d2e4787">Given that slab break-off occurred before 423 Ma in the western section of the North Qinling Orogen (Ren et al., 2021), delamination of thickened crust might have caused extension during the Late Silurian-Early Devonian. Continued continental compression from 438 to 423 Ma would cause shortening and thickening of the continental crust and underlying lithospheric mantle to produce a high-density lithospheric root (eclogitic root) that protruded into the asthenosphere (Houseman and Molnar, 1997). The delamination was characterized by the sinking of eclogitic root and subsequent upwelling of extensive hot asthenosphere, accompanied by crustal extension (Deng et al., 2015; Ma et al., 2015). Huoyanshan granite was formed by high-temperature melting of the heterogeneous continental crust under extensional environment, with a zircon U-Pb age of 415 Ma (Qin et al., 2022). Leijayuan quartz diorite (415 Ma), Beixinggou black mica granite (412 Ma) and Yanwan dolomite granite (409 to 414 Ma) were formed in a post-collision tectonic setting (Wang et al., 2009; Ren et al., 2021). They record the tectonic evolution of the post-collision phase of the North Qinling Orogen. The XP (421 Ma) in this paper was product of the post-collision orogeny stage of extension between the northern margin of the YB and the North Qinling Orogen. The upwelling of hot asthenosphere underplated the ancient crust and supplied heat, not only caused the crust to thin and decompress, but also resulted in widespread partial melting of the ancient intermediate-basic lower crust. Later, under the control of mineral separation crystallization processes such as K-feldspar, plagioclase, and apatite, it underwent highly fractional crystallization to form the Xianping highly fractionated I-type granite. Reflecting the information on the differentiated evolution of crustal materials during the Late Caledonian post-collision in the western section of the North Qinling Orogen, it provides further evidence to reveal the subduction-collision timeframe of the Wushan-Shangdan Ocean in the North Qinling Orogen during the Early Paleozoic.</p>
      <p id="d2e4790">When the continental crust was disconnected from the subducting oceanic crust, the continental crust stopped subducting, and UHP metamorphic rocks began to emerge due to the buoyancy (Davies and von Blanckenburg, 1995). The continental subduction channel model posits that deep-subducted crustal rocks may be detached at mantle depth and subsequently rollback to crustal levels or even to the surface, driven by buoyancy and corner flow (Zheng et al., 2013). This process can be observed in the <inline-formula><mml:math id="M434" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M435" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> paths of UHP metamorphic rocks (Li et al., 2014). The <inline-formula><mml:math id="M436" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M437" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> paths of high-grade metamorphic rocks are typically closely related to the tectonic background in which they occur. Clockwise <inline-formula><mml:math id="M438" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M439" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> paths are predominantly associated with tectonic contexts involving subduction, arc-continent collision, and continent-continent collision at convergent margins (Brown, 1995; England and Thompson, 1984; Thompson and England, 1984). In contrast, anticlockwise <inline-formula><mml:math id="M440" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>–<inline-formula><mml:math id="M441" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> paths are usually associated with island-arc, back-arc, continental rift or mantle plume tectonic environment (Sandiford and Powell, 1986; Bohlen, 1987). Furthermore, the geochronological sequence of Caledonian igneous and metamorphic rocks in the North Qinling Orogen offers significant insights into the temporal framework of the YB with NCB. The Qinling Complex in the eastern part of the North Qinling Orogen has been identified as containing HP-UHP metamorphic rocks between 507  and 485 Ma (Chen et al., 2004; Chen and Liu, 2011; Liu et al., 2013; Su et al., 2004; Wang and Wu, 2013; Yang et al., 2002; Zhang et al., 2011), medium- to low-pressure granulite-facies metamorphic rocks between 430  and 450 Ma (Liu et al., 2013; Xiang et al., 2014; Zhai et al., 1998; Zhang et al., 2009, 2011), and the amphibolite-facies metamorphic rocks overprinting between 420  and 426 Ma (Liu et al., 2013; Zhang et al., 2009, 2011). Significant anatexis associated with granulite-amphibolite facies metamorphism is also identified (Liu et al., 2014; Xiang et al., 2014). However, there are still controversies about the genesis of the medium- to low-pressure granulite-facies metamorphic rocks as follows: (1) related to the northward subduction of the Shangdan Ocean (Wang et al., 2011, 2013; Wu and Zheng, 2013; Xiang et al., 2014); (2) related to the collisional orogeny of the Early Paleozoic (Liu et al., 2016; Zhai et al., 1998; Zhang et al., 2011, 2013). The garnet amphibolite probably experienced eclogite-facies metamorphism at 497 Ma and two stages retrograde overprint at 452  and 423 Ma in the western section of the North Qinling Orogen, which are basically consistent with the continental-type HP-UHP rocks of the eastern section of North Qinling Orogen, suggesting that both western and eastern section of North Qinling Orogen experienced similar continental deep subduction and exhumation processes (Tang et al., 2022). Combined with regional geological data, this suggests that the granulite-facies metamorphic rocks in the western section of the North Qinling Orogen may be the result of the Early Paleozoic continent-continent collision orogenic process.</p>
      <p id="d2e4850">In the global context, the Proto-Tethys Ocean was located between the North American Laurentia-Tarim-North China and Gondwana continent, formed by the breakup of the Rodinia supercontinent (Stampfli and Borel, 2002; Wu et al., 2020; Dong et al., 2022b). The Rodinia supercontinent underwent a breakup during the Neoproterozoic, and the Laurentia and Baltic continent separated to form the Iapetus Oceans in the Late Proterozoic, which face west towards the continent of West Gondwana in the Southern Hemisphere (van Staal et al., 2012). In the Late Ordovician, the Avalonia Terrane drifted northwards to form the Rheic Ocean in the active continental margin of the western Gondwana, which continued to expand and shrink the Iapetus Ocean, while the collision of the Avalonia Terrane with the Baltic continent caused the disappearance of the Tornquist Ocean and the formation of the Thor Suture (Torsvik and Rehnstrom, 2003). Subsequently, the collision of the Avalonia Terrane-Baltic continent with the Laurentia continent formed the Appalachian-Caledonian orogen in southern North America-Britain-Norway, which resulted in the disappearance of the Iapetus Ocean between the Laurentia and Baltic continents, it means the closure of the Proto-Tethys Ocean (McKerrow et al., 2000; Dewey et al., 2015; Torsvik, 2019). In the northern part of the British Caledonian Belt, between the Baltic and Greenland continent, the famous Norwegian HP-UHP metamorphic rocks were formed due to the subduction of the Baltic under the Laurentia continent, which indicated that the Proto-Tethys Ocean had disappeared at ca. 435 Ma (Wu et al., 2020).</p>
      <p id="d2e4853">The CCOB is one of the most developed locations in the Proto-Tethys tectonic domain. Through long-term research on this area, it has been found that the ages of ophiolites in the North Altyn-North Qilian-Kuanping Suture, South Altyn-North Qaidam-Shandan Suture, and Kudi-Kunzhong Suture were mainly concentrated between 520 to 490 Ma (Xiao et al., 2003; Zhang et al., 2004, 2015; Song et al., 2019). The Kangxiwar-A'nyemaqen-Mianlue Suture zone developed a large number of Early Paleozoic ophiolites of 530 to 480 Ma and Late Paleozoic ophiolites. A small amount of Proto-Tethys ophiolites also developed in the Longmuco-Shuanghu-Changning-Menglian belt (Pan et al., 2020; Wang et al., 2021). These ophiolites reflected the formation of the Proto-Tethys Ocean in China, while the formation of the European Iapetus Ocean is basically consistent with or slightly earlier than this (Xu et al., 2010a, b; Song et al., 2013, 2019; Wu et al., 2020; Li et al., 2022). The North Qinling Orogen marks the northernmost boundary of the Proto-Tethys Ocean in the eastern part of the CCOB (Li et al., 2016a), as well as the Wushan-Shangdan Ocean is located in the northern part of the Proto-Tethys Ocean (Zhang et al., 2001). The closure of the Wushan-Shangdan Ocean resulted in the collision of the northern margin of the YB with the North Qinling Orogen in the Silurian, which ultimately merged with the eastern part of the Gondwana continent, and were closely related to the evolution of the Proto-Tethys Ocean (Zhao et al., 2018; Li et al., 2018b).</p>
</sec>
</sec>
<sec id="Ch1.S7" sec-type="conclusions">
  <label>7</label><title>Conclusions</title>
      <p id="d2e4865"><list list-type="order">
          <list-item>

      <p id="d2e4870">LP and XP are both high-K calc-alkaline metaluminous-weakly peraluminous granite series. They show high K<sub>2</sub>O, low Na<sub>2</sub>O, Fe<sub>2</sub>O<inline-formula><mml:math id="M445" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mi>T</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, with distinct enrichment in LFSE (e.g. Rb, K, and Pb), and depletion in HFSE (e.g. Nb, Ta, Ti, Zr, and Ce). The LP has higher REE contents (180.35 to 412.32 <inline-formula><mml:math id="M446" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>) and more fractionated REEs ((<inline-formula><mml:math id="M448" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> <inline-formula><mml:math id="M450" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 27.5 to 51.5; <inline-formula><mml:math id="M451" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">LREE</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">HREE</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M452" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 18.9 to 30.0) than the XP (REE <inline-formula><mml:math id="M453" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 81.26 to 205.05 <inline-formula><mml:math id="M454" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g g<sup>−1</sup>, (<inline-formula><mml:math id="M456" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">La</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Yb</mml:mi></mml:mrow></mml:math></inline-formula>)<sub><italic>N</italic></sub> <inline-formula><mml:math id="M458" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula>  1.5 to 9.0, <inline-formula><mml:math id="M459" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">LREE</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">HREE</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M460" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2.3 to 8.9). In addition, LP shows slightly negative (<inline-formula><mml:math id="M461" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Eu</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Eu</mml:mi></mml:mrow></mml:math></inline-formula><sup>*</sup> <inline-formula><mml:math id="M463" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.54 to 1.03), whereas XP exhibits strongly negative (<inline-formula><mml:math id="M464" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Eu</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Eu</mml:mi></mml:mrow></mml:math></inline-formula><sup>*</sup> <inline-formula><mml:math id="M466" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.18 to 0.33), respectively;</p>
          </list-item>
          <list-item>

      <p id="d2e5114">The zircon U-Pb age of the LP and XP are 429  and 421 Ma, respectively. The LP is I-type granite with positive <inline-formula><mml:math id="M467" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> values of <inline-formula><mml:math id="M468" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.1 to <inline-formula><mml:math id="M469" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>3.4, and was formed by partial melting of the intermediate-basic juvenile lower crust, accompanied by magma mixing with mantle material. The Xianping highly fractionated I-type granite (<inline-formula><mml:math id="M470" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi mathvariant="normal">Hf</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M471" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M472" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>18.5 to <inline-formula><mml:math id="M473" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13.6) is interpreted to have been formed by partial melting of mature lower crust, followed by extensive fractional crystallization in extensional setting.</p>
          </list-item>
          <list-item>

      <p id="d2e5190">The LP was formed by slab break-off during the syn-collisional setting, whereas the XP was formed by delamination during the post-collisional setting. The evolution from the Liqiao I-type granite to the Xianping highly fractionated I-type granite reflects the transition from the syn-collisional to post-collisional stage between the YB and the North Qinling Orogen. They were closely related to the evolution of the Wushan-Shangdan Ocean, northern of the Proto-Tethys Ocean.</p>
          </list-item>
        </list></p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d2e5200">The data are presented in the Supplement below.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e5203">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/se-17-1035-2026-supplement" xlink:title="zip">https://doi.org/10.5194/se-17-1035-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e5212">HL: Conceptualization, Formal analysis, Investigation, Methodology, Visualization, Writing – original draft. ZCL: Conceptualization, Formal analysis, Investigation, Methodology, Visualization, Funding acquisition. XZP: Investigation, Methodology, Funding acquisition. MW (Meng Wang): Investigation. SWZ: Formal analysis, Methodology. HZ: Formal analysis, Methodology. FG: Investigation. MW (Mao Wang): Writing – review and editing, Methodology. LQ: Investigation, Methodology.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e5218">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e5224">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e5231">We thanks are extended to the chief editor and the two anonymous reviewers for their constructive reviews which have greatly improved our manuscript. We wish to acknowledge Yifeng Wang and others for their help during the fieldwork and sample preparations. We also extremely thankful to Dr. Yinchuan Wang and Dr. Xiao Wang provided valuable comments on the language of this paper.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e5236">This research has been supported by the National Natural Science Foundation of China (grant nos. 41872235, 42172236, and 41872234), the Fundamental Research Funds for the Central Universities (grant nos. 300102270202, 300103183081, and 300104282717), and  the Youth Innovation Team of Shaanxi Universities.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e5242">This paper was edited by Andrea Di Muro and reviewed by Mark Allen and Massimo Coltorti.</p>
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