<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OJG</journal-id><journal-title-group><journal-title>Open Journal of Geology</journal-title></journal-title-group><issn pub-type="epub">2161-7570</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojg.2023.1312055</article-id><article-id pub-id-type="publisher-id">OJG-129730</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Earth&amp;Environmental Sciences</subject></subj-group></article-categories><title-group><article-title>
 
 
  Tracing the Origin of Metasedimentary Rocks in the Tortiya Diamond Region (Northern C&#244;te d’Ivoire)
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Tessia</surname><given-names>Miryam</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Adingra</surname><given-names>Martial Pohn Koffi</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Koffi</surname><given-names>Yao Augustin</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Houssou</surname><given-names>Nestor</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Allialy</surname><given-names>Marc Ephrem</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kouassi</surname><given-names>Brice Roland</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Félix Houphou&amp;amp;#235;t-Boigny University of Abidjan, Abidjan, C&amp;amp;#244;te d’Ivoire</addr-line></aff><aff id="aff2"><addr-line>Peleforo Gon Coulibaly University of Korhogo, Korhogo, C&amp;amp;#244;te d’Ivoire</addr-line></aff><pub-date pub-type="epub"><day>05</day><month>12</month><year>2023</year></pub-date><volume>13</volume><issue>12</issue><fpage>1271</fpage><lpage>1290</lpage><history><date date-type="received"><day>7,</day>	<month>November</month>	<year>2023</year></date><date date-type="rev-recd"><day>9,</day>	<month>December</month>	<year>2023</year>	</date><date date-type="accepted"><day>12,</day>	<month>December</month>	<year>2023</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  Metasedimentary rocks from the Tortiya diamondiferous region (northern C
  &amp;#244;te d’Ivoire), located in the Ivorian Paleoproterozoic domain, were analyzed with the aim of identifying their different petrographic facies, constraining their provenance and tectonic environment, and assessing the effects of sedimentary processes and weathering on the signature of their source rocks. These analyses were carried out with a view to helping trace the origin of Tortiya diamonds, which are generally hosted in these metasediments. Major and trace element geochemical data reveal that these samples are characterized by negative Eu anomaly values, low to moderate weathering index values and a high compositional variation index (ICV). These results led to the definition of these metasediments as immature sediments potentially originating from rapid erosion and sediment deposition from local sources. Chemical alteration index (CIA) values and Al
  <sub>2</sub>O
  <sub>3</sub>-(CaO* + Na
  <sub>2</sub>O)-K
  <sub>2</sub>O composition space suggest low to medium degrees of meteoric alteration of the parent rock. These rocks therefore show poorly differentiated compositions from the parent rock and poor sediment sorting. Geochemical data and ratios of immobile elements, e.g. Al
  <sub>2</sub>O
  <sub>3</sub>/TiO
  <sub>2</sub>, Cr/Th, Eu/Eu* and (La/Yb)n, indicate that the clastic materials derive mainly from felsic to intermediate sources. Sedimentary tectonic discrimination diagrams demonstrate that most of the samples from the Tortiya diamond-bearing region were deposited on an active continental margin or in a continental arc-island environment. Although this region has a long history of diamond mining, its petrogenesis remains unresolved, and this petrogeochemical work is a step towards initiating scientific research in the area.
 
</p></abstract><kwd-group><kwd>Petrography</kwd><kwd> Geochemistry</kwd><kwd> Metasediments</kwd><kwd> Tortiya</kwd><kwd> Ivory Coast</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Paleoproterozoic domain that forms the northern and eastern parts of the Man-L&#233;o Shield, which occupies the southern segment of the West African craton, consists of belts of metavolcanic and metasedimentary rocks intruded by different generations of granitoids, at the boundaries of which large tonalite batholiths, trondhjemites and granodiorites (TTG) [<xref ref-type="bibr" rid="scirp.129730-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref2">2</xref>] are encountered. Geochronological studies on Birimian rocks suggest that they were formed between 2.3 and 2.0 billion (Ga) [<xref ref-type="bibr" rid="scirp.129730-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref5">5</xref>] . They were deposited on deformed and metamorphosed basement rocks no older than 50 million (ma) [<xref ref-type="bibr" rid="scirp.129730-ref1">1</xref>] . They exposed Birimian age, accreted around 2.1 Ma during the Eburnean orogeny [<xref ref-type="bibr" rid="scirp.129730-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref7">7</xref>] . Tectonically, they were affected by medium-grade tectonometamorphism evolving from greenschist to amphibolite facies although granulite-facies rocks are also found in some very localized areas. Our study area lies in the north-western extension of the NNE-SSW-trending Ferkess&#233;dougou belt (northern C&#244;te d’Ivoire). This furrow consists mainly of shales, sandstones and conglomerates affected by epizonal metamorphism.</p><p>Geochemical studies of the metavolcanic rocks of Birimian greenstone belts are numerous [<xref ref-type="bibr" rid="scirp.129730-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref8">8</xref>] and varied, whereas Birimian sedimentary rocks in comparison have received very little attention [<xref ref-type="bibr" rid="scirp.129730-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref10">10</xref>] , despite representing a reliable source of information on the provenance and evolution of the Earth’s crust [<xref ref-type="bibr" rid="scirp.129730-ref11">11</xref>] . While it is true that petrographic study, through the description of a rock’s mineralogical assemblages, enables us to define part of its geological history, this step remains insufficient when it comes to examining metasediments. Geochemical examination, and more specifically rare earth element (REE) analysis, could be used effectively to assess the nature and evolution of the provenance of sedimentary history.</p><p>The main objective of this study is to determine the sources and tectonic setting of the metasedimentary rocks of the Tortiya diamond field. We focus on immobile elements such as rare earths and high field strength elements (HFSE) [<xref ref-type="bibr" rid="scirp.129730-ref5">5</xref>] as these elements are generally transferred quantitatively and unfractionated during sedimentary processes that may reflect the source rock signature [<xref ref-type="bibr" rid="scirp.129730-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref13">13</xref>] , unlike elements such as Si, Na, K, Ca, Mg, Rb and Sr [<xref ref-type="bibr" rid="scirp.129730-ref1">1</xref>] which are generally affected by even low-grade metamorphism or alteration.</p></sec><sec id="s2"><title>2. Geological Settings</title><p>The study area is located in the Paleoproterozoic domain of C&#244;te d’Ivoire (<xref ref-type="fig" rid="fig1">Figure 1</xref>) and consists mainly of ortho- and paraderivative magmatic and metamorphic rocks [<xref ref-type="bibr" rid="scirp.129730-ref14">14</xref>] . The magmatic rocks consist of granitoids and dioritoids.</p><p>Granitoids are essentially non-oriented biotite bearing granites and biotite-hornblende metagranodiorites with a general NNE-SSW direction. Dioritoids consist mainly of gabbros. Metamorphic rocks include schists, metagabbros, metadolerites, amphibolo-pyroxenites and biotite and/or hornblende bearing metagranodiorites. Schists form a diverse direction N22˚ band across our study area, consisting of alternating greywacke schists and arkosic schists. These latter are crosscutted by with lenses of conglomeratic schist [<xref ref-type="bibr" rid="scirp.129730-ref15">15</xref>] (<xref ref-type="fig" rid="fig2">Figure 2</xref>). The tectonics are represented by global trending ESE-WNW faults and strike-slip that generally affect the shales.</p></sec><sec id="s3"><title>3. Sample Description</title><p>Four samples (sample TOR 04, sample TOR 50, sample TOR 78, sample TOR C) collected in the field were subjected to geochemical analysis. To the naked eye, they are mainly characterized by a distinctive dark-gray color, considerable hardness, and massive structure (<xref ref-type="fig" rid="fig3">Figure 3</xref>). They consist of subangular to subrounded, moderately to poorly sorted grains. On the microscopic scale, the mineralogy of greywacke consists of quartz (20% - 35%) sometimes showing rolling extinction, alkali feldspars (15% - 25%) presented in dusty-looking clasts, lithic clasts (20% - 25%), sericite-included plagioclase (approx. 15%) and a small amount of sericite and a few chlorite-altered biotites (&lt;5%). Interpenetration of the edges of the quartz grains is certainly due to compaction and distribution of phyllite minerals (muscovite) around certain quartz and feldspar clasts mark a clear schistosity. Two samples (TOR 61 and TOR 17) are meta-arenites with a whitish color at outcrop. Microscopically, they are composed of quartz with a mosaic structure and large rolling extinction crystals representing around 75% of the rock. Muscovites show a preferential orientation and occupy the interstices like a filling. Feldspars account for around 15% of the rock. The rock has undergone slight stretching and alignment of quartz and feldspars.</p></sec><sec id="s4"><title>4. Methodology</title><p>Six (06) rock samples were selected and sent to the Bureau Veritas C&#244;te d’Ivoire mineral analysis laboratory to determine their major and trace element compositions by atomic emission spectrometry (ICP-AES) and mass spectrometry (ICP-MS).</p><p>The samples were successively jaw crushed and then roller crushed. The powders are divided by quartering using an equiproportional separator. Their particle size is reduced to 70 - 80 &#181;m. Chemical analyses are carried out on 10 grams of rock powder and fifty-six chemical elements are assayed.</p><p>These are:</p><p>- Major elements (12): SiO<sub>2</sub>, Al<sub>2</sub>O<sub>3</sub>, Fe<sub>2</sub>O<sub>3</sub>, CaO, MgO, Na<sub>2</sub>O, K<sub>2</sub>O, TiO<sub>2</sub>, MnO, P<sub>2</sub> O<sub>5</sub>, Cr<sub>2</sub>O<sub>3</sub> and loss on ignition (LOI). 11 elements were analyzed by atomic emission spectrometry (ICP AES), while Cr<sub>2</sub>O<sub>3</sub> was quantified by mass spectrometry (ICP MS);</p><p>- Base metals (8): Ag, Co, Cu, Mo, Ni, Pb, Zn and Cd obtained by an etching (AQ 200). This procedure is followed by atomic emission spectrometry emission spectrometry (ICP AES) for determining the content;</p><p>- Volatile elements (6): As, Bi, Hg, Sb, Se and Be were first digested by Aqua Regia (AQ 200) and then quantified by plasma torch mass spectrometry mass spectrometry (ICP-MS);</p><p>- Trace elements and rare earth elements REE (30 elements): Ba, Ce, Cs, Dy, Er, Eu, Ga, Gd, Hf, Ho, La, Lu, Nb, Nd, Pr, Rb, Sm, Sn, Sr, Ta, Tb, Th, Tl, Tm, U, V, W, Y, Yb and Zr first undergo lithium-boron melting before dissolving dissolution. Finally, plasma torch mass spectrometry (ICP MS) was used to quantify them.</p></sec><sec id="s5"><title>5. Results</title><sec id="s5_1"><title>5.1. Major Elements</title><p>Samples analyzed showed high SiO<sub>2</sub> contents ranging from 67.11% to 94.97%. TiO<sub>2</sub> compositions ranged from 0.04 to 0.66 and MgO from 0.08% to 2.27%. CaO and Al<sub>2</sub>O<sub>3</sub> contents range from 0.02% - 3.62% and 2.34% - 13.81% respectively, and Fe<sub>2</sub>O<sub>3</sub> contents from 1.06% to 6.13%. SiO<sub>2</sub>/Al<sub>2</sub>O<sub>3</sub> ratios ranged from 4.24 to 40.58 and Na<sub>2</sub>O/K<sub>2</sub>O ratios from 0.01 to 11.33 (<xref ref-type="table" rid="table1">Table 1</xref>). As a result, most of samples fall into greywackes field and 2 samples fall into sub-arenites field in diagram Log (Na<sub>2</sub>O/K<sub>2</sub>O) vs Log (SiO<sub>2</sub>/Al<sub>2</sub>O<sub>3</sub>) by [<xref ref-type="bibr" rid="scirp.129730-ref16">16</xref>] (<xref ref-type="fig" rid="fig4">Figure 4</xref>). Diagram Log (SiO<sub>2</sub>/Al<sub>2</sub>O<sub>3</sub>) vs Log (Fe<sub>2</sub>O<sub>3</sub>/K<sub>2</sub>O) by [<xref ref-type="bibr" rid="scirp.129730-ref17">17</xref>] (<xref ref-type="fig" rid="fig5">Figure 5</xref>) presents most samples as wackes except for 2 samples described as sublitharenites as does diagram Al<sub>2</sub>O<sub>3</sub>/CaO + Na<sub>2</sub>O + K<sub>2</sub>O by [<xref ref-type="bibr" rid="scirp.129730-ref18">18</xref>] except for TOR 61 identified as a sub-arkose by this diagram. However, diagram (<xref ref-type="fig" rid="fig6">Figure 6</xref>) by [<xref ref-type="bibr" rid="scirp.129730-ref19">19</xref>] specifies that these samples are all sedimentary origin.</p></sec><sec id="s5_2"><title>5.2. Trace-Element</title><p>Composition of large-ion lithophile elements (LILE) such as Rb (14 - 63.3 ppm), Sr (65.3 - 796.6 ppm) and Ba (90 - 533 ppm) shows varying degrees of variation. The average Sr content (381.6) far exceeds that of the Post-Archean Australian Shale (PAAS), which is 200 ppm according to [<xref ref-type="bibr" rid="scirp.129730-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref20">20</xref>] and the Upper Continental Crust (UCC), which is 320 ppm according to [<xref ref-type="bibr" rid="scirp.129730-ref21">21</xref>] and considered as references. Average Ba concentration (357.7) is much lower than that of the PAAS (650 ppm) and the UCC (628 ppm). The HFSE content such as Nb (0.4 - 7.2; average grade: 4.4); Ta (0.1 - 0.4; average grade: 0.31) and Hf (1 - 4.4; average grade: 3.4) varies little and their average grades are roughly like those of PAAS and UCC (<xref ref-type="table" rid="table1">Table 1</xref>).</p><p>Average Zr content (35.5 - 170, average grade: 125.9) is much lower than that of PAAS (210 ppm) and UCC (193 ppm). Transition elements such as Co (0.6 - 15.8; mean grade: 9.6), Ni (0.9 - 32.6; mean grade: 21.6) and V (18 - 87; mean grade: 58.7) show wide variations, and mean grades are lower than those reported by PAAS and UCC (<xref ref-type="table" rid="table1">Table 1</xref>).</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Major elements (wt%) and trace elements (ppm) of the metasedimentary rocks from the Tortiya Formation in comparison to other sediments from references</title></caption><table><tbody><thead><tr><th align="center" valign="middle"  rowspan="2"  >Samples</th><th align="center" valign="middle"  colspan="4"  >Grauwacke</th><th align="center" valign="middle"  colspan="2"  >Arenite</th><th align="center" valign="middle" >PAAS</th><th align="center" valign="middle" >UCC</th></tr></thead><tr><td align="center" valign="middle" >TOR 04</td><td align="center" valign="middle" >CONG-SAINT</td><td align="center" valign="middle" >TOR 50</td><td align="center" valign="middle" >TOR 78</td><td align="center" valign="middle" >TOR 17</td><td align="center" valign="middle" >TOR 61</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Major elements (%Wt)</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >SiO<sub>2</sub></td><td align="center" valign="middle" >71.54</td><td align="center" valign="middle" >70.96</td><td align="center" valign="middle" >71.72</td><td align="center" valign="middle" >67.11</td><td align="center" valign="middle" >87.66</td><td align="center" valign="middle" >94.97</td><td align="center" valign="middle" >62.80</td><td align="center" valign="middle" >66.60</td></tr><tr><td align="center" valign="middle" >Al<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >13.81</td><td align="center" valign="middle" >13.67</td><td align="center" valign="middle" >14.26</td><td align="center" valign="middle" >15.82</td><td align="center" valign="middle" >5.55</td><td align="center" valign="middle" >2.34</td><td align="center" valign="middle" >18.9</td><td align="center" valign="middle" >15.40</td></tr><tr><td align="center" valign="middle" >Fe<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >4.18</td><td align="center" valign="middle" >5.16</td><td align="center" valign="middle" >4.82</td><td align="center" valign="middle" >6.13</td><td align="center" valign="middle" >2.88</td><td align="center" valign="middle" >1.06</td><td align="center" valign="middle" >6.50</td><td align="center" valign="middle" >5.04</td></tr><tr><td align="center" valign="middle" >MnO</td><td align="center" valign="middle" >0.09</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.08</td><td align="center" valign="middle" >0.07</td><td align="center" valign="middle" >0.04</td><td align="center" valign="middle" >0.02</td><td align="center" valign="middle" >0.10</td><td align="center" valign="middle" >0.11</td></tr><tr><td align="center" valign="middle" >MgO</td><td align="center" valign="middle" >1.09</td><td align="center" valign="middle" >1.67</td><td align="center" valign="middle" >1.27</td><td align="center" valign="middle" >2.27</td><td align="center" valign="middle" >0.19</td><td align="center" valign="middle" >0.08</td><td align="center" valign="middle" >2.20</td><td align="center" valign="middle" >2.48</td></tr><tr><td align="center" valign="middle" >CaO</td><td align="center" valign="middle" >3.62</td><td align="center" valign="middle" >2.48</td><td align="center" valign="middle" >3.59</td><td align="center" valign="middle" >1.31</td><td align="center" valign="middle" >0.46</td><td align="center" valign="middle" >0.02</td><td align="center" valign="middle" >1.30</td><td align="center" valign="middle" >9.59</td></tr><tr><td align="center" valign="middle" >Na<sub>2</sub>O</td><td align="center" valign="middle" >4.42</td><td align="center" valign="middle" >3.67</td><td align="center" valign="middle" >3.76</td><td align="center" valign="middle" >3.17</td><td align="center" valign="middle" >1.52</td><td align="center" valign="middle" >0.01</td><td align="center" valign="middle" >1.20</td><td align="center" valign="middle" >3.27</td></tr><tr><td align="center" valign="middle" >K<sub>2</sub>O</td><td align="center" valign="middle" >0.39</td><td align="center" valign="middle" >1.37</td><td align="center" valign="middle" >0.49</td><td align="center" valign="middle" >2.11</td><td align="center" valign="middle" >1.52</td><td align="center" valign="middle" >0.7</td><td align="center" valign="middle" >3.70</td><td align="center" valign="middle" >2.80</td></tr><tr><td align="center" valign="middle" >TiO<sub>2</sub></td><td align="center" valign="middle" >0.46</td><td align="center" valign="middle" >0.56</td><td align="center" valign="middle" >0.58</td><td align="center" valign="middle" >0.66</td><td align="center" valign="middle" >0.23</td><td align="center" valign="middle" >0.04</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" >0.64</td></tr><tr><td align="center" valign="middle" >P<sub>2</sub>O<sub>5</sub></td><td align="center" valign="middle" >0.09</td><td align="center" valign="middle" >0.14</td><td align="center" valign="middle" >0.13</td><td align="center" valign="middle" >0.15</td><td align="center" valign="middle" >0.04</td><td align="center" valign="middle" >0.04</td><td align="center" valign="middle" >0.16</td><td align="center" valign="middle" >0.15</td></tr><tr><td align="center" valign="middle" >PF</td><td align="center" valign="middle" >0.64</td><td align="center" valign="middle" >0.9</td><td align="center" valign="middle" >0.49</td><td align="center" valign="middle" >1.66</td><td align="center" valign="middle" >−0.13</td><td align="center" valign="middle" >0.26</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Total</td><td align="center" valign="middle" >100.33</td><td align="center" valign="middle" >100.68</td><td align="center" valign="middle" >101.19</td><td align="center" valign="middle" >100.46</td><td align="center" valign="middle" >99.96</td><td align="center" valign="middle" >99.54</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Na<sub>2</sub>O/K<sub>2</sub>O</td><td align="center" valign="middle" >11.33</td><td align="center" valign="middle" >2.68</td><td align="center" valign="middle" >7.67</td><td align="center" valign="middle" >1.50</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" >0.01</td><td align="center" valign="middle" >3.08</td><td align="center" valign="middle" >0.86</td></tr><tr><td align="center" valign="middle" >K<sub>2</sub>O/Na<sub>2</sub>O</td><td align="center" valign="middle" >0.09</td><td align="center" valign="middle" >0.37</td><td align="center" valign="middle" >0.13</td><td align="center" valign="middle" >0.67</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" >70.00</td><td align="center" valign="middle" >3.08</td><td align="center" valign="middle" >0.85</td></tr><tr><td align="center" valign="middle" >SiO<sub>2</sub>/Al<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >5.18</td><td align="center" valign="middle" >5.19</td><td align="center" valign="middle" >5.03</td><td align="center" valign="middle" >4.24</td><td align="center" valign="middle" >15.79</td><td align="center" valign="middle" >40.59</td><td align="center" valign="middle" >3.32</td><td align="center" valign="middle" >4.32</td></tr><tr><td align="center" valign="middle" >Al<sub>2</sub>O<sub>3</sub>/TiO<sub>2</sub></td><td align="center" valign="middle" >30.02</td><td align="center" valign="middle" >24.41</td><td align="center" valign="middle" >24.59</td><td align="center" valign="middle" >23.97</td><td align="center" valign="middle" >24.13</td><td align="center" valign="middle" >58.50</td><td align="center" valign="middle" >18.90</td><td align="center" valign="middle" >24.06</td></tr><tr><td align="center" valign="middle" >CIA</td><td align="center" valign="middle" >42.03</td><td align="center" valign="middle" >55.47</td><td align="center" valign="middle" >50.84</td><td align="center" valign="middle" >64.03</td><td align="center" valign="middle" >57.56</td><td align="center" valign="middle" >75.54</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >ICV</td><td align="center" valign="middle" >1.32</td><td align="center" valign="middle" >1.10</td><td align="center" valign="middle" >1.02</td><td align="center" valign="middle" >0.99</td><td align="center" valign="middle" >1.23</td><td align="center" valign="middle" >0.82</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >PIA</td><td align="center" valign="middle" >38.77</td><td align="center" valign="middle" >56.23</td><td align="center" valign="middle" >50.88</td><td align="center" valign="middle" >67.20</td><td align="center" valign="middle" >61.41</td><td align="center" valign="middle" >100.00</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Trace (ppm)</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >As</td><td align="center" valign="middle" >1.1</td><td align="center" valign="middle" >0.9</td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle" >0.7</td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Ba</td><td align="center" valign="middle" >90</td><td align="center" valign="middle" >533</td><td align="center" valign="middle" >95</td><td align="center" valign="middle" >507</td><td align="center" valign="middle" >387</td><td align="center" valign="middle" >530</td><td align="center" valign="middle" >650</td><td align="center" valign="middle" >628</td></tr><tr><td align="center" valign="middle" >Be</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Bi</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Cd</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Ce</td><td align="center" valign="middle" >44.6</td><td align="center" valign="middle" >65.1</td><td align="center" valign="middle" >53.2</td><td align="center" valign="middle" >48.3</td><td align="center" valign="middle" >29.9</td><td align="center" valign="middle" >46.3</td><td align="center" valign="middle" >79.6</td><td align="center" valign="middle" >63.0</td></tr><tr><td align="center" valign="middle" >Co</td><td align="center" valign="middle" >9.6</td><td align="center" valign="middle" >15.8</td><td align="center" valign="middle" >12.1</td><td align="center" valign="middle" >15.8</td><td align="center" valign="middle" >4.2</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Cs</td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle" >1.3</td><td align="center" valign="middle" >1.4</td><td align="center" valign="middle" >1.2</td><td align="center" valign="middle" >1.2</td><td align="center" valign="middle" >0.3</td><td align="center" valign="middle" >15</td><td align="center" valign="middle" >4.9</td></tr><tr><td align="center" valign="middle" >Cu</td><td align="center" valign="middle" >11.9</td><td align="center" valign="middle" >26.3</td><td align="center" valign="middle" >12.2</td><td align="center" valign="middle" >33.4</td><td align="center" valign="middle" >2.3</td><td align="center" valign="middle" >3.8</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >28</td></tr><tr><td align="center" valign="middle" >Dy</td><td align="center" valign="middle" >2.38</td><td align="center" valign="middle" >3.3</td><td align="center" valign="middle" >2.62</td><td align="center" valign="middle" >2.41</td><td align="center" valign="middle" >1.45</td><td align="center" valign="middle" >3.1</td><td align="center" valign="middle" >4.48</td><td align="center" valign="middle" >3.90</td></tr><tr><td align="center" valign="middle" >Er</td><td align="center" valign="middle" >1.27</td><td align="center" valign="middle" >2.03</td><td align="center" valign="middle" >1.36</td><td align="center" valign="middle" >1.71</td><td align="center" valign="middle" >0.81</td><td align="center" valign="middle" >0.71</td><td align="center" valign="middle" >2.85</td><td align="center" valign="middle" >2.30</td></tr><tr><td align="center" valign="middle" >Eu</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1.29</td><td align="center" valign="middle" >1.16</td><td align="center" valign="middle" >1.03</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >1.82</td><td align="center" valign="middle" >1.08</td><td align="center" valign="middle" >1.00</td></tr><tr><td align="center" valign="middle" >Ga</td><td align="center" valign="middle" >9.9</td><td align="center" valign="middle" >15.4</td><td align="center" valign="middle" >11.3</td><td align="center" valign="middle" >14.2</td><td align="center" valign="middle" >3.7</td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >17.5</td></tr><tr><td align="center" valign="middle" >Gd</td><td align="center" valign="middle" >2.87</td><td align="center" valign="middle" >4.23</td><td align="center" valign="middle" >3.13</td><td align="center" valign="middle" >3.15</td><td align="center" valign="middle" >2.11</td><td align="center" valign="middle" >5.38</td><td align="center" valign="middle" >4.66</td><td align="center" valign="middle" >4.00</td></tr><tr><td align="center" valign="middle" >Hf</td><td align="center" valign="middle" >4.3</td><td align="center" valign="middle" >4.4</td><td align="center" valign="middle" >3.7</td><td align="center" valign="middle" >3.9</td><td align="center" valign="middle" >3.1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >5.00</td><td align="center" valign="middle" >5.30</td></tr><tr><td align="center" valign="middle" >Ho</td><td align="center" valign="middle" >0.45</td><td align="center" valign="middle" >0.69</td><td align="center" valign="middle" >0.49</td><td align="center" valign="middle" >0.47</td><td align="center" valign="middle" >0.31</td><td align="center" valign="middle" >0.37</td><td align="center" valign="middle" >0.99</td><td align="center" valign="middle" >0.83</td></tr><tr><td align="center" valign="middle" >La</td><td align="center" valign="middle" >26.4</td><td align="center" valign="middle" >34.3</td><td align="center" valign="middle" >26</td><td align="center" valign="middle" >22.3</td><td align="center" valign="middle" >17.7</td><td align="center" valign="middle" >37.1</td><td align="center" valign="middle" >38.0</td><td align="center" valign="middle" >31.0</td></tr><tr><td align="center" valign="middle" >Lu</td><td align="center" valign="middle" >0.18</td><td align="center" valign="middle" >0.29</td><td align="center" valign="middle" >0.2</td><td align="center" valign="middle" >0.24</td><td align="center" valign="middle" >0.14</td><td align="center" valign="middle" >0.05</td><td align="center" valign="middle" >0.43</td><td align="center" valign="middle" >0.31</td></tr><tr><td align="center" valign="middle" >Mo</td><td align="center" valign="middle" >0.2</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.3</td><td align="center" valign="middle" >0.2</td><td align="center" valign="middle" >0.4</td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Nb</td><td align="center" valign="middle" >5.3</td><td align="center" valign="middle" >7.2</td><td align="center" valign="middle" >5.2</td><td align="center" valign="middle" >5.9</td><td align="center" valign="middle" >2.8</td><td align="center" valign="middle" >0.4</td><td align="center" valign="middle" >19.0</td><td align="center" valign="middle" >12.0</td></tr><tr><td align="center" valign="middle" >Nd</td><td align="center" valign="middle" >22.6</td><td align="center" valign="middle" >27.9</td><td align="center" valign="middle" >23.1</td><td align="center" valign="middle" >22.5</td><td align="center" valign="middle" >16</td><td align="center" valign="middle" >36</td><td align="center" valign="middle" >33.9</td><td align="center" valign="middle" >27.0</td></tr><tr><td align="center" valign="middle" >Ni</td><td align="center" valign="middle" >23.8</td><td align="center" valign="middle" >32.6</td><td align="center" valign="middle" >31.7</td><td align="center" valign="middle" >31.3</td><td align="center" valign="middle" >10.6</td><td align="center" valign="middle" >0.9</td><td align="center" valign="middle" >55.0</td><td align="center" valign="middle" >47.0</td></tr><tr><td align="center" valign="middle" >Pb</td><td align="center" valign="middle" >3.6</td><td align="center" valign="middle" >2.7</td><td align="center" valign="middle" >1.8</td><td align="center" valign="middle" >1.9</td><td align="center" valign="middle" >2.9</td><td align="center" valign="middle" >1.7</td><td align="center" valign="middle" >20.0</td><td align="center" valign="middle" >17.0</td></tr><tr><td align="center" valign="middle" >Pr</td><td align="center" valign="middle" >5.72</td><td align="center" valign="middle" >7.54</td><td align="center" valign="middle" >5.91</td><td align="center" valign="middle" >5.85</td><td align="center" valign="middle" >4.07</td><td align="center" valign="middle" >8.63</td><td align="center" valign="middle" >8.83</td><td align="center" valign="middle" >7.10</td></tr><tr><td align="center" valign="middle" >Rb</td><td align="center" valign="middle" >14</td><td align="center" valign="middle" >63.3</td><td align="center" valign="middle" >27.5</td><td align="center" valign="middle" >66.5</td><td align="center" valign="middle" >34.6</td><td align="center" valign="middle" >14.7</td><td align="center" valign="middle" >160</td><td align="center" valign="middle" >82</td></tr><tr><td align="center" valign="middle" >Sb</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Sm</td><td align="center" valign="middle" >3.73</td><td align="center" valign="middle" >5.08</td><td align="center" valign="middle" >4.01</td><td align="center" valign="middle" >4.08</td><td align="center" valign="middle" >2.69</td><td align="center" valign="middle" >6.77</td><td align="center" valign="middle" >5.55</td><td align="center" valign="middle" >4.70</td></tr><tr><td align="center" valign="middle" >Sn</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Sr</td><td align="center" valign="middle" >796.6</td><td align="center" valign="middle" >470.3</td><td align="center" valign="middle" >543.5</td><td align="center" valign="middle" >288.6</td><td align="center" valign="middle" >125.4</td><td align="center" valign="middle" >65.3</td><td align="center" valign="middle" >200</td><td align="center" valign="middle" >320</td></tr><tr><td align="center" valign="middle" >Ta</td><td align="center" valign="middle" >0.4</td><td align="center" valign="middle" >0.4</td><td align="center" valign="middle" >0.4</td><td align="center" valign="middle" >0.4</td><td align="center" valign="middle" >0.2</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >1.28</td><td align="center" valign="middle" >0.90</td></tr><tr><td align="center" valign="middle" >Tb</td><td align="center" valign="middle" >0.38</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >0.44</td><td align="center" valign="middle" >0.43</td><td align="center" valign="middle" >0.27</td><td align="center" valign="middle" >0.66</td><td align="center" valign="middle" >0.77</td><td align="center" valign="middle" >0.70</td></tr><tr><td align="center" valign="middle" >Th</td><td align="center" valign="middle" >7</td><td align="center" valign="middle" >6.7</td><td align="center" valign="middle" >4.8</td><td align="center" valign="middle" >5.3</td><td align="center" valign="middle" >3.7</td><td align="center" valign="middle" >1.2</td><td align="center" valign="middle" >14.6</td><td align="center" valign="middle" >10.5</td></tr><tr><td align="center" valign="middle" >Tm</td><td align="center" valign="middle" >0.18</td><td align="center" valign="middle" >0.28</td><td align="center" valign="middle" >0.2</td><td align="center" valign="middle" >0.22</td><td align="center" valign="middle" >0.12</td><td align="center" valign="middle" >0.07</td><td align="center" valign="middle" >0.41</td><td align="center" valign="middle" >0.30</td></tr><tr><td align="center" valign="middle" >U</td><td align="center" valign="middle" >1.4</td><td align="center" valign="middle" >1.2</td><td align="center" valign="middle" >0.9</td><td align="center" valign="middle" >1.5</td><td align="center" valign="middle" >0.8</td><td align="center" valign="middle" >0.3</td><td align="center" valign="middle" >3.10</td><td align="center" valign="middle" >2.70</td></tr><tr><td align="center" valign="middle" >V</td><td align="center" valign="middle" >51</td><td align="center" valign="middle" >87</td><td align="center" valign="middle" >69</td><td align="center" valign="middle" >84</td><td align="center" valign="middle" >42</td><td align="center" valign="middle" >18</td><td align="center" valign="middle" >150</td><td align="center" valign="middle" >97.0</td></tr><tr><td align="center" valign="middle" >W</td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle" >0.7</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >1.5</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Y</td><td align="center" valign="middle" >12.1</td><td align="center" valign="middle" >19.4</td><td align="center" valign="middle" >12.4</td><td align="center" valign="middle" >13.4</td><td align="center" valign="middle" >8.2</td><td align="center" valign="middle" >6.9</td><td align="center" valign="middle" >27.0</td><td align="center" valign="middle" >35.0</td></tr><tr><td align="center" valign="middle" >Yb</td><td align="center" valign="middle" >1.18</td><td align="center" valign="middle" >1.95</td><td align="center" valign="middle" >1.43</td><td align="center" valign="middle" >1.57</td><td align="center" valign="middle" >0.85</td><td align="center" valign="middle" >0.4</td><td align="center" valign="middle" >2.82</td><td align="center" valign="middle" >2.00</td></tr><tr><td align="center" valign="middle" >Zn</td><td align="center" valign="middle" >42</td><td align="center" valign="middle" >51</td><td align="center" valign="middle" >42</td><td align="center" valign="middle" >68</td><td align="center" valign="middle" >14</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >67.0</td></tr><tr><td align="center" valign="middle" >Zr</td><td align="center" valign="middle" >160.4</td><td align="center" valign="middle" >170</td><td align="center" valign="middle" >135.8</td><td align="center" valign="middle" >137.7</td><td align="center" valign="middle" >116.4</td><td align="center" valign="middle" >35.5</td><td align="center" valign="middle" >210</td><td align="center" valign="middle" >193</td></tr><tr><td align="center" valign="middle" >Eu/Eu*</td><td align="center" valign="middle" >0.93</td><td align="center" valign="middle" >0.85</td><td align="center" valign="middle" >1.00</td><td align="center" valign="middle" >0.88</td><td align="center" valign="middle" >0.77</td><td align="center" valign="middle" >0.92</td><td align="center" valign="middle" >0.66</td><td align="center" valign="middle" >0.72</td></tr><tr><td align="center" valign="middle" >(La/Yb)N</td><td align="center" valign="middle" >15.08</td><td align="center" valign="middle" >11.86</td><td align="center" valign="middle" >12.26</td><td align="center" valign="middle" >9.58</td><td align="center" valign="middle" >14.04</td><td align="center" valign="middle" >62.53</td><td align="center" valign="middle" >9.20</td><td align="center" valign="middle" >10.53</td></tr><tr><td align="center" valign="middle" >(La/Sm)N</td><td align="center" valign="middle" >4.45</td><td align="center" valign="middle" >4.25</td><td align="center" valign="middle" >4.08</td><td align="center" valign="middle" >3.44</td><td align="center" valign="middle" >4.14</td><td align="center" valign="middle" >3.45</td><td align="center" valign="middle" >4.30</td><td align="center" valign="middle" >4.12</td></tr><tr><td align="center" valign="middle" >∑REE</td><td align="center" valign="middle" >112.94</td><td align="center" valign="middle" >154.58</td><td align="center" valign="middle" >123.25</td><td align="center" valign="middle" >114.26</td><td align="center" valign="middle" >77.02</td><td align="center" valign="middle" >147.36</td><td align="center" valign="middle" >184.4</td><td align="center" valign="middle" >148.1</td></tr></tbody></table></table-wrap></sec></sec><sec id="s6"><title>6. Discussion</title><sec id="s6_1"><title>6.1. Element Mobility</title><p>Tortiya metasedimentary samples have not undergone significant secondary alteration, as evidenced by their low loss on ignition (LOI), ranging from −0.13 to 1.66 (all samples have LOI values below 2). As they have undergone low metamorphism, mobility of major and trace elements and on isotopic compositions needs to be assessed.</p></sec><sec id="s6_2"><title>6.2. Alteration of Metasediments</title><p>Alteration in source zones can lead to relative depletion of alkaline elements and LILEs and enrichment in TiO<sub>2</sub> and Al<sub>2</sub>O<sub>3</sub> in clastic sedimentary rocks [<xref ref-type="bibr" rid="scirp.129730-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref23">23</xref>] . Chemical Index of Alteration (CIA) [<xref ref-type="bibr" rid="scirp.129730-ref24">24</xref>] , the Plagioclase Alteration Index (PIA) [<xref ref-type="bibr" rid="scirp.129730-ref25">25</xref>] and Compositional Variation Index (ICV) [<xref ref-type="bibr" rid="scirp.129730-ref26">26</xref>] can be used to quantitatively assess the degree of rock alteration (<xref ref-type="table" rid="table1">Table 1</xref>). CIA index measures the extent to which feldspars have been transformed into Ca-, Na- and K-depleted aluminous clays relative to the unweathered source and is defined as follows:</p><p>CIA = [Al<sub>2</sub>O<sub>3</sub>/(Al<sub>2</sub>O<sub>3</sub> + CaO* + Na<sub>2</sub>O + K<sub>2</sub>O)] &#215; 100 (molar proportions),</p><p>where CaO* represents the CaO content of the silicate fraction.</p><p>On a scale of 40 to 100, unweathered igneous rocks have CIA values of 45 to 55, while moderately weathered shales have CIA values of 70 to 75. Intense alteration of the feldspars in a rock result in high concentrations of residual clays (kaolinite and/or gibbsite) and produces CIA values close to 100.</p><p>CIA values for metasediments in the Tortiya area range from 42.03 to 75.53 with an average value of 57.57 higher than those for fresh UCC [<xref ref-type="bibr" rid="scirp.129730-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref21">21</xref>] but lower than those for PAAS (70 - 75) [<xref ref-type="bibr" rid="scirp.129730-ref22">22</xref>] , implying a low to moderate degree of alteration of the source rocks (<xref ref-type="fig" rid="fig6">Figure 6</xref>). The low CIA values and negative Eu anomalies (for TOR 61 and TOR 17 arenites) are properties of juvenile crustal material from local sources and suggest high erosion rates, low transport, poor sorting, and rapid sediment deposition [<xref ref-type="bibr" rid="scirp.129730-ref27">27</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref28">28</xref>] .</p><p>PIA (PIA = [Al<sub>2</sub>O<sub>3</sub> K<sub>2</sub>O]/[Al<sub>2</sub>O<sub>3</sub> + CaO* + Na<sub>2</sub>O − K<sub>2</sub>O] &#215; 100) is like the CIA but is not influenced by K redistribution and is commonly used to describe plagioclase alteration [<xref ref-type="bibr" rid="scirp.129730-ref25">25</xref>] . For fresh rocks, the PIA is 50, while for clay minerals such as kaolinite, illite and smectite, PIA is around 100 [<xref ref-type="bibr" rid="scirp.129730-ref25">25</xref>] . PIA values for metasedimentary rocks in the Tortiya area range from 60 to 83 and have an average value of 71, and these values suggest that the source of the metasedimentary rocks had a relatively low to moderate degree of alteration. Furthermore, the high CIA content of TOR 61 suggests that this sample is geochemically and texturally mature.</p><p>ICV (ICV = [Fe<sub>2</sub>O<sub>3</sub> + K<sub>2</sub>O + Na<sub>2</sub>O + CaO + MgO + TiO<sub>2</sub>]/Al<sub>2</sub>O<sub>3</sub>) was proposed by [<xref ref-type="bibr" rid="scirp.129730-ref26">26</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref29">29</xref>] and represents another important chemical index for measuring the abundance of alumina relative to other major cations, indicating the compositional maturity of a rock. Non-clay minerals have higher ICV values than clay minerals; consequently, ICV values decrease with increasing degree of alteration and/or rock maturity. ICV values for metasedimentary rocks in the Tortiya formation range from 0.82 to 1.32, with an average value of 1.08, suggesting moderate weathering and/or maturity of the source.</p></sec><sec id="s6_3"><title>6.3. Origin</title><p>Since the source of the metasedimentary rocks studied are not highly altered (CIA &lt; 80) and they are chemically immature (SiO<sub>2</sub>/Al<sub>2</sub>O<sub>3</sub> &lt; 6). Apart from the TOR 17 and TOR 61 arenites, the geochemical composition of the metasedimentary rocks studied may better reflect the properties and characteristics of the provenance.</p><sec id="s6_3_1"><title>6.3.1. Evidences of Major Elements</title><p>Previous researchers have asserted that the Al<sub>2</sub>O<sub>3</sub>/TiO<sub>2</sub> ratio is one of the most functional provenance indicators for sedimentary rocks [<xref ref-type="bibr" rid="scirp.129730-ref30">30</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref31">31</xref>] . Al<sub>2</sub>O<sub>3</sub>/TiO<sub>2</sub> ratios of sandstones are basically identical to those of their source rocks [<xref ref-type="bibr" rid="scirp.129730-ref32">32</xref>] . Consequently, the Al<sub>2</sub>O<sub>3</sub>/TiO<sub>2</sub> ratio represents a good indicator of source rocks, particularly for igneous source rocks. [<xref ref-type="bibr" rid="scirp.129730-ref33">33</xref>] reported that sediments from mafic rocks show Al<sub>2</sub>O<sub>3</sub>/TiO<sub>2</sub> &lt; 14 ratios and sediments from felsic rocks show Al<sub>2</sub>O<sub>3</sub>/TiO<sub>2</sub> ratios between 19 and 28. Al<sub>2</sub>O<sub>3</sub>/TiO<sub>2</sub> ratios of the metasedimentary rocks of the Tortiya Formation range from 23.96 to 58.5 (mean = 30.96) (<xref ref-type="table" rid="table1">Table 1</xref>), indicating that the source materials are mainly from felsic to intermediate igneous sources.</p><p>Alteration trend of Tortiya samples in the Al<sub>2</sub>O<sub>3</sub>-(CaO* + Na<sub>2</sub>O)-K<sub>2</sub>O (A-CN-K) diagram [<xref ref-type="bibr" rid="scirp.129730-ref34">34</xref>] is broadly parallel to the A-CN line, suggesting K<sub>2</sub>O loss and plagioclase abundance in the grauwacke’s mineralogical composition TOR 04, 50, define their source rock as a gabbro. The intersection of the alteration trend with the feldspar line establishes the source rock of greywacke TOR C as a basalt and that of grauwacke TOR 78 as an andesite. Finally, according to the diagram, the TOR 17 and 61 arenites are derived from granite (<xref ref-type="fig" rid="fig7">Figure 7</xref>). According to the plot of Tortiya samples on the discriminant diagram of [<xref ref-type="bibr" rid="scirp.129730-ref18">18</xref>] , the sediments studied derived from mafic igneous sources and intermediate provenance. Grauwackes TOR 04, 50 and TOR C have an intermediate provenance, while TOR 78 has a mafic provenance and arenites TOR 17 and 61 have a sedimentary provenance (<xref ref-type="fig" rid="fig8">Figure 8</xref>).</p></sec><sec id="s6_3_2"><title>6.3.2. Trace Element Evidences</title><p>Multi-element diagrams normalized to the upper crust according to the values of [<xref ref-type="bibr" rid="scirp.129730-ref12">12</xref>] (<xref ref-type="fig" rid="fig9">Figure 9</xref>) show quite different profiles, grouped together by similarity of appearance. The multi-element spectra of TOR 61 and TOR 17 arenites show positive anomalies in Ba, K, Ta, La and Nd and negative anomalies in Nb, Sr and P. TOR 61 also shows negative anomalies in Ti and Sr and positive anomalies in Sm and Y. TOR C and 78 show negative anomalies in Nb, Zr, Tb and Th and positive anomalies in Ta, Ba, K, Ce, Nd and Sm. Finally, grauwackes 04 and 50 show negative anomalies in Ta, Ba, K, Ce and P and positive anomalies in Nb, Th, Sr and Ti. REEs are insoluble trace elements with very low mobility during lower-gradient metamorphism, weathering, hydrothermal alteration, and diagenesis [<xref ref-type="bibr" rid="scirp.129730-ref20">20</xref>] . As a result, they are reliable in determining the provenance of metasedimentary rocks. In general, volcanic-mafic rocks range from light rare-earth depletion (tholeiitic) to heavy rare-earth enrichment (calc-alkaline), while felsic rocks show light rare-earth enrichment. The sum of rare earth contents (∑REE) in Tortiya metasediments ranges from 77.02 to 154.58 ppm (<xref ref-type="table" rid="table1">Table 1</xref>). <xref ref-type="fig" rid="fig1">Figure 1</xref>0 shows that the spectra of TOR samples C, 04, 50, 17 and 78 evolve in a similar way and present identical parallel alleles in them with an enrichment in light rare earths (LREE) such as La, Ce, Pr, Nd, Pm, Sm, Eu and Gd. Beyond gadolinium, heavy rare earths (Tb, Dy, Ho, Er, Tm, Yb, Lu) show a slight concavity (TOR 17), sometimes spreading out into flat profiles (TOR C, 04, 78). However, the TOR 61 spectrum is depleted in heavy rare earths. Chondrite-normalized La to Yb ratios (La/Yb)N range from 9.58 to 62.53 (<xref ref-type="table" rid="table1">Table 1</xref>) for the metasediment samples. The TOR 61 arenite has the highest (La/Yb)N ratio. Its spectrum shows a well-marked negative Ce anomaly. Grauwackes samples TOR 04 and TOR 78 show a slight negative Europium (Eu) anomaly, with Eu/Eu* ratios ranging from 0.77 to 1.00 (<xref ref-type="table" rid="table1">Table 1</xref>) and an average of 0.88 close to UCC (Eu/Eu* = 0.72). Except for the arenite TOR 61, all other samples are exempt from Ce anomalies. Furthermore, the rocks studied show intense fractionation between light and heavy rare earths, indicating that mafic igneous rocks are not a significant source.</p><p>Transition elements (Cr, Sc, Ni, Co and V) are preferentially concentrated in mafic minerals such as pyroxenes and olivines. This is why sedimentary rocks derived from their erosion are characterized by high concentrations of these elements [<xref ref-type="bibr" rid="scirp.129730-ref35">35</xref>] . The Tortiya metasediments show only low levels of these compatible elements (<xref ref-type="table" rid="table1">Table 1</xref>), which therefore rules out the exposure of significant mafic rocks in origin of these metasediments. Also, as shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>1 by [<xref ref-type="bibr" rid="scirp.129730-ref36">36</xref>] illustrating Rb vs. K2O diagram discriminating sedimentary rock provenance, the metasediments studied fall within the intermediate to acidic rock field once again.</p></sec></sec><sec id="s6_4"><title>6.4. Tectonic Setting</title><p>It has been shown that the geochemical compositions of sediments can be linked to plate tectonic processes, making geochemistry a powerful tool for the recognition of ancient tectonic settings [<xref ref-type="bibr" rid="scirp.129730-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref12">12</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref37">37</xref>] - [<xref ref-type="bibr" rid="scirp.129730-ref42">42</xref>] . Some major element discrimination diagrams (K<sub>2</sub>O/Na<sub>2</sub>O versus SiO<sub>2</sub> and SiO<sub>2</sub>/Al<sub>2</sub>O<sub>3</sub> versus K<sub>2</sub>O/Na<sub>2</sub>O) (<xref ref-type="fig" rid="fig1">Figure 1</xref>2) have been used to distinguish different tectonic settings [<xref ref-type="bibr" rid="scirp.129730-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.129730-ref41">41</xref>] .</p><p>In these two (2) diagrams, samples TOR C, 50 and 78 are in the oceanic island-arc margin field, while sample TOR 04 is in the active continental margin field and sample TOR 61 in the passive margin field. In addition, samples TOR C, 17 and 78 exhibit evolved arc properties with felsic plutonic detritus, while sample TOR 50 displays arc tectonic properties with basaltic and andesitic detritus. Geochemical studies carried out on metasediments from the SASCA domain [<xref ref-type="bibr" rid="scirp.129730-ref43">43</xref>] in southwestern C&#244;te d’Ivoire and the southeastern Como&#233; basin [<xref ref-type="bibr" rid="scirp.129730-ref44">44</xref>] suggest that they also belong to the oceanic island arc and active continental margin domains.</p></sec></sec><sec id="s7"><title>7. Conclusions</title><p>The low CIA PIA and ICV values and negative Eu anomalies suggest that these metasediments are derived from locally sourced juvenile crustal material that has undergone poor weathering, erosion, transport and rapid sediment deposition.</p><p>Based on geochemical analyses of metasediments from Tortiya area, the following conclusions have been drawn:</p><p>1) Tortiya metasediment samples identified as wackes and sub-arkoses probably originate from felsic to intermediate (granite-andesite) sources.</p><p>2) They would have been emplaced in a geodynamic environment of active to passive continental margin and/or evolved island-arc ocean margin.</p><p>To complete this analysis, we suggest electron microprobe analyses of the heavy minerals in the sediments, in order to search for any link with ultrabasics. It would also be advisable to combine these results with geophysical and structural analyses to elucidate the origins of the diamonds contained in the Tortiya metasediments.</p></sec><sec id="s8"><title>Acknowledgements</title><p>We would like to thank the management and staff of the exploration department of the “Soci&#233;t&#233; pour le D&#233;veloppement des Mines en C&#244;te d’Ivoire” for their technical support and the accessibility of their property for field work. This research was funded by the Agate project and the UEMOA excellence grant.</p></sec><sec id="s9"><title>Conflicts of Interest</title><p>The authors declare no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s10"><title>Cite this paper</title><p>Miryam, T., Koffi, A.M.P., Augustin, K.Y., Nestor, H., Ephrem, A.M. and Roland, K.B. (2023) Tracing the Origin of Metasedimentary Rocks in the Tortiya Diamond Region (Northern C&#244;te d’Ivoire). 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