<?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.2024.146028</article-id><article-id pub-id-type="publisher-id">OJG-133848</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>
 
 
  Petrology and Structural Characterization of Post-Neoproterozoic Dolerites from the Kimberlite Fields in the K&#233;ni&#233;ba Region (Western Mali)
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Gbele</surname><given-names>Ouattara</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>Baco</surname><given-names>Traore</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>Ziandj&amp;#234;d&amp;#233;</surname><given-names>Herv&amp;#233; Siagn&amp;#233;</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>Aboubacar</surname><given-names>Denon</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>Souleymane</surname><given-names>Sangare</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Marc</surname><given-names>Ephrem Allialy</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref></contrib></contrib-group><aff id="aff3"><addr-line>Unit&amp;amp;#233; de Formation et de Recherche des Sciences de la Terre et des Ressources Mini&amp;amp;#232;res (UFR-STRM), University of Cocody, Abidjan, C&amp;amp;#244;te d&amp;amp;#8217;Ivoire</addr-line></aff><aff id="aff1"><addr-line>Laboratoire des Sciences G&amp;amp;#233;ographiques, du G&amp;amp;#233;nie Civil et des G&amp;amp;#233;osciences, Institut National Polytechnique F&amp;amp;#233;lix HOUPHOU&amp;amp;#203;T-BOIGNY (INP-HB), Yamoussoukro, C&amp;amp;#244;te d&amp;amp;#8217;Ivoire</addr-line></aff><aff id="aff2"><addr-line>EUREKAGEO Sarl Consulting Mining Company, Bamako, Republic of Mali</addr-line></aff><pub-date pub-type="epub"><day>18</day><month>06</month><year>2024</year></pub-date><volume>14</volume><issue>06</issue><fpage>655</fpage><lpage>670</lpage><history><date date-type="received"><day>8,</day>	<month>May</month>	<year>2024</year></date><date date-type="rev-recd"><day>15,</day>	<month>June</month>	<year>2024</year>	</date><date date-type="accepted"><day>18,</day>	<month>June</month>	<year>2024</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-NonCommercial International License (CC BY-NC).http://creativecommons.org/licenses/by-nc/4.0/</license-p></license></permissions><abstract><p>
 
 
  Post-Neoproterozoic dolerites from the K&#233;ni&#233;ba region (Western Mali) are often associated with kimberlites. The rarity of kimberlite outcrops led to the study of doleritic rocks, spatially associated with them. The petrographic and lithogeochemical study showed that the dolerites of the K&#233;ni&#233;ba kimberlitic fields are of tholeiitic nature and of the E-MORB (Enriched-Mid Ocean Ridge Basalt) type. This reflects an enrichment over time, compared to the Birimian dolerites of the volcano-sedimentary greenstone belt of Toumodi, in central C?te d’Ivoire. Furthermore, these dolerites are enriched in SiO
  <sub>2</sub>, TiO
  <sub>2</sub>, Zr and poor in Fe
  <sub>2</sub>O
  <sub>3</sub>, MgO. These dolerites would have formed in a late to post-orogenic intracontinental context during the breakup of Gondwana. Structurally, K&#233;ni&#233;ba dolerites are often associated with kimberlite pipes, fractures and large deep structures identified using aeromagnetic images. Taking into account the fact that kimberlites do not outcrop in the K&#233;ni&#233;ba region, the geochemical study coupled with the interpretation of aeromagnetic data proved to be very useful for the search for pipes.
 
</p></abstract><kwd-group><kwd>Dolerites</kwd><kwd> Kimberlitic Fields</kwd><kwd> Petrology</kwd><kwd> Structures</kwd><kwd> K&#233;ni&#233;ba</kwd><kwd> Mali</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The kimberlite fields of the K&#233;ni&#233;ba region are located in western Mali where the first kimberlite was discovered between 1955 and 1957 by the DFGM. Numerous exploration works carried out by mining companies followed this discovery. Around thirty pipes and kimberlitic dikes have been revealed within the Birimian formations, mainly composed of metasediments and intrusions of granitoids covered by neoproterozoic sandstones formations. All of these formations are crossed by occurrences of doleritic to gabbroic nature which were established during magmatic activities, approximately 180 My ago [<xref ref-type="bibr" rid="scirp.133848-ref1">1</xref>] , following which the Gondwana was dislocated. The kimberlite occurrences of K&#233;ni&#233;ba are often located along certain structures controlling the dolerites, some of which are of Turonian age (92 My), [<xref ref-type="bibr" rid="scirp.133848-ref2">2</xref>] .</p><p>Several generations of dolerite intrusions are present in the K&#233;ni&#233;ba sector, of which eight (8) have been the subject of this study. These basic intrusions penetrate fractures and/or faults to form dikes which extend over large areas. The occurrences of dolerites correspond to the last phase of basic volcanism, and generally precede the kimberlite occurrences which appear in the form of explosions.</p><p>In the region, the kimberlites appear in the form of clusters forming groups of three (3) to five (5) kimberlite pipes and which are aligned on fractures oriented along the WNW-ESE direction (125˚ to 127˚) which intersect the NE-SW directions (15˚ to 20˚) which form a very tight network of dikes [<xref ref-type="bibr" rid="scirp.133848-ref3">3</xref>] .</p><p>The structural data clearly show control of kimberlite clusters by structures associated with dolerites which are distributed in two systems of different directions: latitudinal and sub-meridian. Many diamonds have been discovered at K&#233;ni&#233;ba, in areas relatively close to the dolerite dikes. However, the petrographic and structural characteristics associated with the emplacement of these dolerites, as well as their relationships with the kimberlites, are not yet clearly established.</p><p>This work aims to establish the petrological and structural characteristics of these post-Neoproterozoic dolerites from the kimberlitic fields of the K&#233;ni&#233;ba region, compared to certain Birimian dolerites from the West African craton.</p></sec><sec id="s2"><title>2. Location and Geological Setting of the Study Area</title><p>The K&#233;ni&#233;ba region is located in the west of Mali, on the border with Senegal (<xref ref-type="fig" rid="fig1">Figure 1</xref>). The study area is geologically associated with the K&#233;dougou-K&#233;ni&#233;ba Inlier (KKI) which is underlain by volcanic, volcano-sedimentary formations and granitoid intrusions [<xref ref-type="bibr" rid="scirp.133848-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.133848-ref5">5</xref>] .</p><p>Knowledge of the geology of the Malian part of the KKI has been greatly improved as part of a cooperation program between the government of the Republic of Mali and the BRGM/Geosystem Maps consortium, which led to the production of the geological map at 1/200,000 [<xref ref-type="bibr" rid="scirp.133848-ref3">3</xref>] . The establishment of the formations of the K&#233;ni&#233;ba region are associated with the Eburnean orogeny dated approximately between 2030 and 1830 My [<xref ref-type="bibr" rid="scirp.133848-ref6">6</xref>] . These formations are represented by metamorphic rocks of the greenschist facies, namely, metagrauwackes as well as granitoid intrusions [<xref ref-type="bibr" rid="scirp.133848-ref7">7</xref>] . They are limited to the east by the vast sedimentary cover of the Neoproterozoic domain.</p></sec><sec id="s3"><title>3. Materials and Methods</title><p>The material includes field data (samples), laboratory data and aeromagnetic images. The first phase consisted of the collection of field data, through sampling of dolerites (generally in the form of dikes), both in the Birimian formations and in the Neoproterozoic formations. The preparation of twelve (12) thin sections at the Basement Geology Laboratory of the F&#233;lix Houphou&#235;t-Boigny University of Abidjan (C&#244;te d’Ivoire) made it possible to determine the petrographic characteristics of dolerites and surrounding rocks.</p><p>Geochemical analyzes (done at the Mineral Laboratories, Bureau Veritas Commodities, Vancouver, Canada) also made it possible to clarify the petrographic nature, lineages and environments of the establishment of these dolerites. A comparison of the lithogeochemical data of the dolerites of K&#233;ni&#233;ba with those of other regions made it possible to better characterize them.</p><p>Structural data were collected in the immediate environment of these dolerites. An interpretation of aeromagnetic imagery made it possible to identify major geological structures.</p></sec><sec id="s4"><title>4. Results</title><sec id="s4_1"><title>4.1. Petrographic Characteristics of Dolerites</title><p>In the field, dolerites appear in the form of dikes and sometimes associated with microgabbros. The coloring oscillates between dark gray and black. These are micro-grained rocks reflecting their semi-depth origin. In thin sections, the mineralogy consists essentially of entangled plagioclase rods, pyroxenes (orthopyroxenes and clinopyroxenes), amphiboles and a few fine quartz crystals (<xref ref-type="fig" rid="fig2">Figure 2</xref>). These rocks present intergranular, microgabbro and subophitic textures.</p></sec><sec id="s4_2"><title>4.2. Lithogeochemical Characteristics of Dolerites</title><p>The major element data (<xref ref-type="table" rid="table1">Table 1</xref>) show an average composition of SiO<sub>2</sub> (49.94% - 52.35%), MgO (5.94% - 8.62%), Fe<sub>2</sub>O<sub>3</sub> (9.01% - 12.47%), Al<sub>2</sub>O<sub>3</sub> (14.01% - 15.33%), Na<sub>2</sub>O + K<sub>2</sub>O (2.26% - 4.05%) and Na<sub>2</sub>O/K<sub>2</sub>O (0.5 - 3.71) and relatively low values of TiO<sub>2</sub> (0.76% - 1.3%) (<xref ref-type="table" rid="table1">Table 1</xref>).</p><p>A study of the chemical composition of basic rock dikes located in the fields of Bilali (Bilali south), S&#233;konomata and Kobato showed a slight increase in TiO<sub>2</sub></p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Chemical composition in major elements (% by weight) of representative samples of dolerites across the K&#233;ni&#233;ba kimberlite province</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >DOL-1A %</th><th align="center" valign="middle" >DOL-1B %</th><th align="center" valign="middle" >DOL-1C %</th><th align="center" valign="middle" >DOL-1D %</th><th align="center" valign="middle" >DOL-2 %</th><th align="center" valign="middle" >DOL-3B %</th><th align="center" valign="middle" >DOL-4 %</th><th align="center" valign="middle" >DOL-5 %</th></tr></thead><tr><td align="center" valign="middle" >SiO<sub>2</sub></td><td align="center" valign="middle" >51.99</td><td align="center" valign="middle" >49.94</td><td align="center" valign="middle" >52.23</td><td align="center" valign="middle" >51.92</td><td align="center" valign="middle" >52.08</td><td align="center" valign="middle" >51.29</td><td align="center" valign="middle" >49.95</td><td align="center" valign="middle" >52.35</td></tr><tr><td align="center" valign="middle" >Al<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >14.05</td><td align="center" valign="middle" >15.33</td><td align="center" valign="middle" >14.02</td><td align="center" valign="middle" >14.55</td><td align="center" valign="middle" >14.2</td><td align="center" valign="middle" >15.1</td><td align="center" valign="middle" >14.93</td><td align="center" valign="middle" >14.01</td></tr><tr><td align="center" valign="middle" >Fe<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >11.53</td><td align="center" valign="middle" >12.47</td><td align="center" valign="middle" >11.83</td><td align="center" valign="middle" >11.87</td><td align="center" valign="middle" >11.47</td><td align="center" valign="middle" >9.01</td><td align="center" valign="middle" >12.35</td><td align="center" valign="middle" >11.84</td></tr><tr><td align="center" valign="middle" >MgO</td><td align="center" valign="middle" >6.82</td><td align="center" valign="middle" >6.04</td><td align="center" valign="middle" >6.14</td><td align="center" valign="middle" >6.26</td><td align="center" valign="middle" >6.62</td><td align="center" valign="middle" >8.62</td><td align="center" valign="middle" >5.94</td><td align="center" valign="middle" >6.13</td></tr><tr><td align="center" valign="middle" >CaO</td><td align="center" valign="middle" >10.34</td><td align="center" valign="middle" >9.47</td><td align="center" valign="middle" >9.86</td><td align="center" valign="middle" >9.99</td><td align="center" valign="middle" >10.22</td><td align="center" valign="middle" >12.11</td><td align="center" valign="middle" >8.41</td><td align="center" valign="middle" >9.8</td></tr><tr><td align="center" valign="middle" >Na<sub>2</sub>O</td><td align="center" valign="middle" >2.07</td><td align="center" valign="middle" >1.97</td><td align="center" valign="middle" >2.19</td><td align="center" valign="middle" >2.13</td><td align="center" valign="middle" >2.07</td><td align="center" valign="middle" >1.78</td><td align="center" valign="middle" >1.35</td><td align="center" valign="middle" >2.17</td></tr><tr><td align="center" valign="middle" >K<sub>2</sub>O</td><td align="center" valign="middle" >0.94</td><td align="center" valign="middle" >0.97</td><td align="center" valign="middle" >0.98</td><td align="center" valign="middle" >0.93</td><td align="center" valign="middle" >0.82</td><td align="center" valign="middle" >0.48</td><td align="center" valign="middle" >2.7</td><td align="center" valign="middle" >1.18</td></tr><tr><td align="center" valign="middle" >TiO<sub>2</sub></td><td align="center" valign="middle" >1.22</td><td align="center" valign="middle" >1.28</td><td align="center" valign="middle" >1.29</td><td align="center" valign="middle" >1.27</td><td align="center" valign="middle" >1.3</td><td align="center" valign="middle" >0.76</td><td align="center" valign="middle" >1.26</td><td align="center" valign="middle" >1.26</td></tr><tr><td align="center" valign="middle" >P<sub>2</sub>O<sub>5</sub></td><td align="center" valign="middle" >0.16</td><td align="center" valign="middle" >0.17</td><td align="center" valign="middle" >0.17</td><td align="center" valign="middle" >0.17</td><td align="center" valign="middle" >0.19</td><td align="center" valign="middle" >0.1</td><td align="center" valign="middle" >0.17</td><td align="center" valign="middle" >0.16</td></tr><tr><td align="center" valign="middle" >MnO</td><td align="center" valign="middle" >0.18</td><td align="center" valign="middle" >0.17</td><td align="center" valign="middle" >0.18</td><td align="center" valign="middle" >0.18</td><td align="center" valign="middle" >0.17</td><td align="center" valign="middle" >0.15</td><td align="center" valign="middle" >0.22</td><td align="center" valign="middle" >0.17</td></tr><tr><td align="center" valign="middle" >Cr<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >0.023</td><td align="center" valign="middle" >0.019</td><td align="center" valign="middle" >0.011</td><td align="center" valign="middle" >0.015</td><td align="center" valign="middle" >0.037</td><td align="center" valign="middle" >0.079</td><td align="center" valign="middle" >0.018</td><td align="center" valign="middle" >0.014</td></tr><tr><td align="center" valign="middle" >LOI</td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >0.9</td><td align="center" valign="middle" >0.9</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >0.4</td><td align="center" valign="middle" >2.5</td><td align="center" valign="middle" >0.7</td></tr><tr><td align="center" valign="middle" >Sum</td><td align="center" valign="middle" >99.91</td><td align="center" valign="middle" >99.92</td><td align="center" valign="middle" >99.91</td><td align="center" valign="middle" >99.92</td><td align="center" valign="middle" >99.92</td><td align="center" valign="middle" >99.94</td><td align="center" valign="middle" >99.9</td><td align="center" valign="middle" >99.91</td></tr></tbody></table></table-wrap><p>inside and in the immediate vicinity of the kimberlites as well as the heavy rare earths like Hf, Y and Nd (<xref ref-type="table" rid="table1">Table 1</xref> and <xref ref-type="table" rid="table2">Table 2</xref>). A dike located outside the kimberlite field shows a TiO<sub>2</sub> content of less than 1% (DOL-3B), which seems to correspond to normal levels in the K&#233;ni&#233;ba dolerites.</p><p>The Batifara dolerite dike (DOL-2) located at 1.2 km from the kimberlite intrusion of the same name gives a content of 1.3% while the TiO<sub>2</sub> content in the Kassama dike (DOL-3B) located approximately 2.7 km to the East is 0.76%. For dikes located between 300 and 10 m from the kimberlite intrusion (in the field of influence), the grade reaches between 1.22% and 1.28%. It can be noted that chemical analyzes show that the composition of the dolerites is substantially identical in the K&#233;ni&#233;ba area. Only the contents of samples DOL-4 and DOL-5 which come from the immediate environment of the kimberlites show relatively high K<sub>2</sub>O contents compared to the other samples.</p><p>In the SiO<sub>2</sub> vs Na<sub>2</sub>O + K<sub>2</sub>O diagram (<xref ref-type="fig" rid="fig3">Figure 3</xref>(a)), the K&#233;ni&#233;ba dolerites are located in tholeiitic rocks. Comparatively, the Birimian dolerites of the Toumodi region (in C&#244;te d’Ivoire [<xref ref-type="bibr" rid="scirp.133848-ref8">8</xref>] ) are less alkaline and less siliceous than those of K&#233;ni&#233;ba (more siliceous). This tholeiitic trend of dolerites is confirmed by the AFM diagrams of Irvine and Baragar ( [<xref ref-type="bibr" rid="scirp.133848-ref9">9</xref>] <xref ref-type="fig" rid="fig3">Figure 3</xref>(b)) and SiO<sub>2</sub> vs FeO<sub>t</sub>/MgO (<xref ref-type="fig" rid="fig3">Figure 3</xref>(c)). The K&#233;ni&#233;ba dolerites are more titaniferous (<xref ref-type="fig" rid="fig3">Figure 3</xref>(d) and <xref ref-type="fig" rid="fig3">Figure 3</xref>(e)), less chromiferous (<xref ref-type="fig" rid="fig3">Figure 3</xref>(f)) and richer in zirconium (<xref ref-type="fig" rid="fig3">Figure 3</xref>(g)) than those of Toumodi region. Furthermore, the dolerites of K&#233;ni&#233;ba are more depleted in titanium than those of Nakyn in Siberia (2.17% - 4.69% [<xref ref-type="bibr" rid="scirp.133848-ref10">10</xref>] ) and those of Vilyui Middle Paleozoic paleorift of the east of the Siberian Platform, in Russia (2.48% - 2.6% [<xref ref-type="bibr" rid="scirp.133848-ref11">11</xref>] ). The K&#233;ni&#233;ba dolerites have an affinity for sub-alkaline basalts (<xref ref-type="fig" rid="fig3">Figure 3</xref>(h)).</p><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Chemical composition of dolerites in trace elements of dolerites from certain kimberlite fields of K&#233;ni&#233;ba</title></caption><table><tbody><thead><tr><th align="center" valign="middle" ></th><th align="center" valign="middle" >DOL-1A ppm</th><th align="center" valign="middle" >DOL-1B ppm</th><th align="center" valign="middle" >DOL-1C ppm</th><th align="center" valign="middle" >DOL-1D ppm</th><th align="center" valign="middle" >DOL-2 ppm</th><th align="center" valign="middle" >DOL-3B ppm</th><th align="center" valign="middle" >DOL-4 ppm</th><th align="center" valign="middle" >DOL-5 ppm</th></tr></thead><tr><td align="center" valign="middle" >Ba</td><td align="center" valign="middle" >198</td><td align="center" valign="middle" >205</td><td align="center" valign="middle" >200</td><td align="center" valign="middle" >213</td><td align="center" valign="middle" >258</td><td align="center" valign="middle" >142</td><td align="center" valign="middle" >346</td><td align="center" valign="middle" >220</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" >&lt;1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >2</td></tr><tr><td align="center" valign="middle" >Co</td><td align="center" valign="middle" >42.6</td><td align="center" valign="middle" >46.8</td><td align="center" valign="middle" >43.9</td><td align="center" valign="middle" >42.8</td><td align="center" valign="middle" >41.9</td><td align="center" valign="middle" >41.5</td><td align="center" valign="middle" >60.6</td><td align="center" valign="middle" >43.5</td></tr><tr><td align="center" valign="middle" >Cs</td><td align="center" valign="middle" >1.0</td><td align="center" valign="middle" >1.3</td><td align="center" valign="middle" >1.1</td><td align="center" valign="middle" >1.0</td><td align="center" valign="middle" >1.0</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >0.9</td><td align="center" valign="middle" >1.6</td></tr><tr><td align="center" valign="middle" >Ga</td><td align="center" valign="middle" >15.2</td><td align="center" valign="middle" >16.6</td><td align="center" valign="middle" >16.3</td><td align="center" valign="middle" >15.5</td><td align="center" valign="middle" >15.3</td><td align="center" valign="middle" >13.0</td><td align="center" valign="middle" >16.6</td><td align="center" valign="middle" >15.4</td></tr><tr><td align="center" valign="middle" >Hf</td><td align="center" valign="middle" >3.0</td><td align="center" valign="middle" >2.9</td><td align="center" valign="middle" >3.0</td><td align="center" valign="middle" >3.2</td><td align="center" valign="middle" >3.2</td><td align="center" valign="middle" >1.7</td><td align="center" valign="middle" >3.1</td><td align="center" valign="middle" >3.2</td></tr><tr><td align="center" valign="middle" >Nb</td><td align="center" valign="middle" >8.4</td><td align="center" valign="middle" >8.8</td><td align="center" valign="middle" >9.0</td><td align="center" valign="middle" >8.4</td><td align="center" valign="middle" >9.5</td><td align="center" valign="middle" >5.2</td><td align="center" valign="middle" >8.7</td><td align="center" valign="middle" >8.6</td></tr><tr><td align="center" valign="middle" >Rb</td><td align="center" valign="middle" >31.7</td><td align="center" valign="middle" >36.3</td><td align="center" valign="middle" >32.9</td><td align="center" valign="middle" >32.3</td><td align="center" valign="middle" >22.4</td><td align="center" valign="middle" >14.8</td><td align="center" valign="middle" >58.7</td><td align="center" valign="middle" >40.0</td></tr><tr><td align="center" valign="middle" >Sn</td><td align="center" valign="middle" >&lt;1</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >&lt;1</td><td align="center" valign="middle" >&lt;1</td><td align="center" valign="middle" >&lt;1</td><td align="center" valign="middle" >&lt;1</td><td align="center" valign="middle" >&lt;1</td><td align="center" valign="middle" >&lt;1</td></tr><tr><td align="center" valign="middle" >Sr</td><td align="center" valign="middle" >187.5</td><td align="center" valign="middle" >173.7</td><td align="center" valign="middle" >197.3</td><td align="center" valign="middle" >183.2</td><td align="center" valign="middle" >220.6</td><td align="center" valign="middle" >176.3</td><td align="center" valign="middle" >195.5</td><td align="center" valign="middle" >199.8</td></tr><tr><td align="center" valign="middle" >Ta</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle" >0.4</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >0.5</td></tr><tr><td align="center" valign="middle" >Th</td><td align="center" valign="middle" >2.9</td><td align="center" valign="middle" >2.9</td><td align="center" valign="middle" >2.8</td><td align="center" valign="middle" >2.9</td><td align="center" valign="middle" >2.5</td><td align="center" valign="middle" >1.6</td><td align="center" valign="middle" >2.9</td><td align="center" valign="middle" >2.9</td></tr><tr><td align="center" valign="middle" >U</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >0.8</td><td align="center" valign="middle" >0.6</td><td align="center" valign="middle" >0.7</td><td align="center" valign="middle" >0.4</td><td align="center" valign="middle" >0.3</td><td align="center" valign="middle" >0.7</td><td align="center" valign="middle" >0.7</td></tr><tr><td align="center" valign="middle" >V</td><td align="center" valign="middle" >263</td><td align="center" valign="middle" >280</td><td align="center" valign="middle" >283</td><td align="center" valign="middle" >264</td><td align="center" valign="middle" >257</td><td align="center" valign="middle" >211</td><td align="center" valign="middle" >273</td><td align="center" valign="middle" >277</td></tr><tr><td align="center" valign="middle" >W</td><td align="center" valign="middle" >&lt;0.5</td><td align="center" valign="middle" >&lt;0.5</td><td align="center" valign="middle" >&lt;0.5</td><td align="center" valign="middle" >&lt;0.5</td><td align="center" valign="middle" >&lt;0.5</td><td align="center" valign="middle" >&lt;0.5</td><td align="center" valign="middle" >&lt;0.5</td><td align="center" valign="middle" >0.5</td></tr><tr><td align="center" valign="middle" >Zr</td><td align="center" valign="middle" >106.0</td><td align="center" valign="middle" >112.9</td><td align="center" valign="middle" >115.6</td><td align="center" valign="middle" >113.3</td><td align="center" valign="middle" >113.6</td><td align="center" valign="middle" >61.9</td><td align="center" valign="middle" >111.7</td><td align="center" valign="middle" >112.8</td></tr><tr><td align="center" valign="middle" >Y</td><td align="center" valign="middle" >22.4</td><td align="center" valign="middle" >22.5</td><td align="center" valign="middle" >23.4</td><td align="center" valign="middle" >23.5</td><td align="center" valign="middle" >23.3</td><td align="center" valign="middle" >15.6</td><td align="center" valign="middle" >22.3</td><td align="center" valign="middle" >24.1</td></tr><tr><td align="center" valign="middle" >La</td><td align="center" valign="middle" >13.1</td><td align="center" valign="middle" >2.12</td><td align="center" valign="middle" >13.9</td><td align="center" valign="middle" >13.8</td><td align="center" valign="middle" >14.0</td><td align="center" valign="middle" >8.4</td><td align="center" valign="middle" >15.0</td><td align="center" valign="middle" >14.1</td></tr><tr><td align="center" valign="middle" >Ce</td><td align="center" valign="middle" >28.0</td><td align="center" valign="middle" >0.36</td><td align="center" valign="middle" >30.1</td><td align="center" valign="middle" >28.8</td><td align="center" valign="middle" >31.1</td><td align="center" valign="middle" >16.9</td><td align="center" valign="middle" >34.0</td><td align="center" valign="middle" >29.4</td></tr><tr><td align="center" valign="middle" >Pr</td><td align="center" valign="middle" >3.50</td><td align="center" valign="middle" >2.47</td><td align="center" valign="middle" >3.72</td><td align="center" valign="middle" >3.68</td><td align="center" valign="middle" >3.88</td><td align="center" valign="middle" >2.16</td><td align="center" valign="middle" >3.66</td><td align="center" valign="middle" >3.76</td></tr><tr><td align="center" valign="middle" >Nd</td><td align="center" valign="middle" >15.2</td><td align="center" valign="middle" >0.85</td><td align="center" valign="middle" >15.6</td><td align="center" valign="middle" >16.0</td><td align="center" valign="middle" >17.1</td><td align="center" valign="middle" >9.5</td><td align="center" valign="middle" >15.1</td><td align="center" valign="middle" >16.0</td></tr><tr><td align="center" valign="middle" >Sm</td><td align="center" valign="middle" >3.46</td><td align="center" valign="middle" >4.22</td><td align="center" valign="middle" >3.96</td><td align="center" valign="middle" >3.74</td><td align="center" valign="middle" >3.79</td><td align="center" valign="middle" >2.26</td><td align="center" valign="middle" >3.75</td><td align="center" valign="middle" >3.80</td></tr><tr><td align="center" valign="middle" >Eu</td><td align="center" valign="middle" >1.19</td><td align="center" valign="middle" >0.65</td><td align="center" valign="middle" >1.17</td><td align="center" valign="middle" >1.22</td><td align="center" valign="middle" >1.22</td><td align="center" valign="middle" >0.76</td><td align="center" valign="middle" >1.16</td><td align="center" valign="middle" >1.23</td></tr><tr><td align="center" valign="middle" >Gd</td><td align="center" valign="middle" >4.13</td><td align="center" valign="middle" >4.09</td><td align="center" valign="middle" >4.38</td><td align="center" valign="middle" >4.24</td><td align="center" valign="middle" >4.28</td><td align="center" valign="middle" >2.63</td><td align="center" valign="middle" >4.23</td><td align="center" valign="middle" >4.27</td></tr><tr><td align="center" valign="middle" >Tb</td><td align="center" valign="middle" >0.67</td><td align="center" valign="middle" >1.13</td><td align="center" valign="middle" >0.73</td><td align="center" valign="middle" >0.71</td><td align="center" valign="middle" >0.70</td><td align="center" valign="middle" >0.44</td><td align="center" valign="middle" >0.67</td><td align="center" valign="middle" >0.73</td></tr><tr><td align="center" valign="middle" >Dy</td><td align="center" valign="middle" >4.42</td><td align="center" valign="middle" >3.44</td><td align="center" valign="middle" >4.39</td><td align="center" valign="middle" >4.36</td><td align="center" valign="middle" >4.33</td><td align="center" valign="middle" >2.90</td><td align="center" valign="middle" >4.19</td><td align="center" valign="middle" >4.41</td></tr><tr><td align="center" valign="middle" >Ho</td><td align="center" valign="middle" >0.87</td><td align="center" valign="middle" >15.0</td><td align="center" valign="middle" >0.94</td><td align="center" valign="middle" >0.96</td><td align="center" valign="middle" >0.85</td><td align="center" valign="middle" >0.56</td><td align="center" valign="middle" >0.86</td><td align="center" valign="middle" >0.94</td></tr><tr><td align="center" valign="middle" >Er</td><td align="center" valign="middle" >2.49</td><td align="center" valign="middle" >3.48</td><td align="center" valign="middle" >2.74</td><td align="center" valign="middle" >2.64</td><td align="center" valign="middle" >2.50</td><td align="center" valign="middle" >1.76</td><td align="center" valign="middle" >2.45</td><td align="center" valign="middle" >2.59</td></tr><tr><td align="center" valign="middle" >Tm</td><td align="center" valign="middle" >0.34</td><td align="center" valign="middle" >28.7</td><td align="center" valign="middle" >0.39</td><td align="center" valign="middle" >0.38</td><td align="center" valign="middle" >0.37</td><td align="center" valign="middle" >0.24</td><td align="center" valign="middle" >0.37</td><td align="center" valign="middle" >0.37</td></tr><tr><td align="center" valign="middle" >Yb</td><td align="center" valign="middle" >2.23</td><td align="center" valign="middle" >13.1</td><td align="center" valign="middle" >2.31</td><td align="center" valign="middle" >2.34</td><td align="center" valign="middle" >2.21</td><td align="center" valign="middle" >1.45</td><td align="center" valign="middle" >2.16</td><td align="center" valign="middle" >2.39</td></tr></tbody></table></table-wrap><p>In the diagrams normalized to the MORB (Mid Ocean Ridge Basalt) [<xref ref-type="bibr" rid="scirp.133848-ref14">14</xref>] , the K&#233;ni&#233;ba dolerites are distinguished from the Birimian dolerites by a strong enrichment in light rare earths (<xref ref-type="table" rid="table3">Table 3</xref>). Compared to the primitive mantle and poorly mobile elements [<xref ref-type="bibr" rid="scirp.133848-ref15">15</xref>] , the K&#233;ni&#233;ba dolerites are forty times more enriched in light rare earths than those of the Toumodi Birimian dolerites (<xref ref-type="fig" rid="fig4">Figure 4</xref>(a)). In the diagram of Anders and Grevesse [<xref ref-type="bibr" rid="scirp.133848-ref16">16</xref>] , the K&#233;ni&#233;ba dolerites</p><table-wrap id="table3" ><label><xref ref-type="table" rid="table3">Table 3</xref></label><caption><title> Pearson correlation matrix (n) of the major elements of the K&#233;ni&#233;ba dolerites</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Variables</th><th align="center" valign="middle" >SiO<sub>2</sub></th><th align="center" valign="middle" >Al<sub>2</sub>O<sub>3</sub></th><th align="center" valign="middle" >Fe<sub>2</sub>O<sub>3</sub></th><th align="center" valign="middle" >MgO</th><th align="center" valign="middle" >CaO</th><th align="center" valign="middle" >Na<sub>2</sub>O</th><th align="center" valign="middle" >K<sub>2</sub>O</th><th align="center" valign="middle" >TiO<sub>2</sub></th><th align="center" valign="middle" >P<sub>2</sub>O<sub>5</sub></th><th align="center" valign="middle" >MnO</th><th align="center" valign="middle" >Cr<sub>2</sub>O<sub>3</sub></th></tr></thead><tr><td align="center" valign="middle" >SiO<sub>2</sub></td><td align="center" valign="middle" >1</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><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Al<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >−0.870</td><td align="center" valign="middle" >1</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><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Fe<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >−0.215</td><td align="center" valign="middle" >−0.159</td><td align="center" valign="middle" >1</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" >MgO</td><td align="center" valign="middle" >0.116</td><td align="center" valign="middle" >0.243</td><td align="center" valign="middle" >−0.983</td><td align="center" valign="middle" >1</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" >CaO</td><td align="center" valign="middle" >0.400</td><td align="center" valign="middle" >0.022</td><td align="center" valign="middle" >−0.924</td><td align="center" valign="middle" >0.920</td><td align="center" valign="middle" >1</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" >Na<sub>2</sub>O</td><td align="center" valign="middle" >0.770</td><td align="center" valign="middle" >−0.619</td><td align="center" valign="middle" >0.069</td><td align="center" valign="middle" >−0.116</td><td align="center" valign="middle" >0.280</td><td align="center" valign="middle" >1</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" >K<sub>2</sub>O</td><td align="center" valign="middle" >−0.535</td><td align="center" valign="middle" >0.148</td><td align="center" valign="middle" >0.534</td><td align="center" valign="middle" >−0.535</td><td align="center" valign="middle" >−0.809</td><td align="center" valign="middle" >−0.727</td><td align="center" valign="middle" >1</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" >TiO<sub>2</sub></td><td align="center" valign="middle" >0.071</td><td align="center" valign="middle" >−0.414</td><td align="center" valign="middle" >0.942</td><td align="center" valign="middle" >−0.948</td><td align="center" valign="middle" >−0.810</td><td align="center" valign="middle" >0.284</td><td align="center" valign="middle" >0.364</td><td align="center" valign="middle" >1</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" >P<sub>2</sub>O<sub>5</sub></td><td align="center" valign="middle" >0.058</td><td align="center" valign="middle" >−0.374</td><td align="center" valign="middle" >0.865</td><td align="center" valign="middle" >−0.863</td><td align="center" valign="middle" >−0.748</td><td align="center" valign="middle" >0.231</td><td align="center" valign="middle" >0.327</td><td align="center" valign="middle" >0.964</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" >MnO</td><td align="center" valign="middle" >−0.400</td><td align="center" valign="middle" >−0.010</td><td align="center" valign="middle" >0.644</td><td align="center" valign="middle" >−0.635</td><td align="center" valign="middle" >−0.846</td><td align="center" valign="middle" >−0.568</td><td align="center" valign="middle" >0.934</td><td align="center" valign="middle" >0.528</td><td align="center" valign="middle" >0.498</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >Cr<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >−0.054</td><td align="center" valign="middle" >0.392</td><td align="center" valign="middle" >−0.936</td><td align="center" valign="middle" >0.956</td><td align="center" valign="middle" >0.825</td><td align="center" valign="middle" >−0.265</td><td align="center" valign="middle" >−0.428</td><td align="center" valign="middle" >−0.918</td><td align="center" valign="middle" >−0.787</td><td align="center" valign="middle" >−0.581</td><td align="center" valign="middle" >1</td></tr></tbody></table></table-wrap><p>are sixty (60) times more enriched in light rare earths than the chondrites, while the Birimian dolerites show a weak fractionation of rare earths, with a slight positive anomaly in Europium (<xref ref-type="fig" rid="fig4">Figure 4</xref>(b)).</p><p>Research into the geotectonic environment of the K&#233;ni&#233;ba dolerites, through different diagrams, shows that the K&#233;ni&#233;ba dolerites belong to the late to post-orogenic intracontinental domain in a compressive to distensive context of the volcanic arc type on the edge of the continent [<xref ref-type="bibr" rid="scirp.133848-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.133848-ref18">18</xref>] (<xref ref-type="fig" rid="fig5">Figure 5</xref>(a)) and correspond to within-plate basalts ( [<xref ref-type="bibr" rid="scirp.133848-ref19">19</xref>] <xref ref-type="fig" rid="fig5">Figure 5</xref>(b)).</p><p>The statistical analysis of the relationships between chemical elements in dolerites required the use of principal components analysis or PCA [<xref ref-type="bibr" rid="scirp.133848-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.133848-ref21">21</xref>] . Regarding the major elements, the data matrix consists of eleven variables: SiO<sub>2</sub>, Al<sub>2</sub>O<sub>3</sub>, Fe<sub>2</sub>O<sub>3</sub>, MgO, CaO, Na<sub>2</sub>O, K<sub>2</sub>O, TiO<sub>2</sub>, P<sub>2</sub>O<sub>5</sub>, MnO, Cr<sub>2</sub>O<sub>3</sub>. The principal components were calculated from a correlation matrix. In the case of correlations, the most significant are displayed in bold (<xref ref-type="table" rid="table3">Table 3</xref>). The correlation matrix</p><p>gives a first idea of the existing associations between the different variables. Thus, we note the following correlations (<xref ref-type="table" rid="table3">Table 3</xref>).</p><p>- Strong positives correlations (0.9) between: Fe<sub>2</sub>O<sub>3</sub> and TiO<sub>2</sub>, P<sub>2</sub>O<sub>5</sub>; MgO and Cao, Cr<sub>2</sub>O<sub>3</sub>; K<sub>2</sub>O and MnO; TiO<sub>2</sub> and P<sub>2</sub>O<sub>5</sub>;</p><p>- Strong negatives correlations (&lt;−0.9) between: Fe<sub>2</sub>O<sub>3</sub> and MgO, CaO, Cr<sub>2</sub>O<sub>3</sub>; MgO and TiO<sub>2</sub>; TiO<sub>2</sub> and Cr<sub>2</sub>O<sub>3</sub>.</p><p>The correlation matrix indicates a strong correlation between: TiO<sub>2</sub> and P<sub>2</sub>O<sub>5</sub>; Na<sub>2</sub>O and SiO<sub>2</sub>; MgO and Cr<sub>2</sub>O<sub>3</sub>; MnO and K<sub>2</sub>O; TiO<sub>2</sub> and Cr<sub>2</sub>O<sub>3</sub> (<xref ref-type="fig" rid="fig6">Figure 6</xref>).</p></sec><sec id="s4_3"><title>4.3. Structural Characterization of the Doleritic Dikes of K&#233;ni&#233;ba</title><p>The establishment of West African dolerite dikes can be associated with the opening (rifting) of the Atlantic Ocean, on the one hand, and on the other hand, with late to post-Eburnean distensions [<xref ref-type="bibr" rid="scirp.133848-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.133848-ref23">23</xref>] . From the aeromagnetic image of K&#233;ni&#233;ba, dolerites appear in the form of a network of lineaments affecting Birimian units, as well as intrusions and sedimentary covers (Neoproterozoic), (<xref ref-type="fig" rid="fig7">Figure 7</xref>).</p><p>The color contrast on the magnetic map draws a boundary between the two domains, and highlights the numerous dikes of basic rocks (grouped under the generic name of dolerites) in the form of lineaments.</p><p>A combination of airborne photo-geological and geophysical images (magnetic, electromagnetic, and radiometric) made it possible to trace major tectonic structures [<xref ref-type="bibr" rid="scirp.133848-ref24">24</xref>] . The interpretation of the map sheets shows an orientation of the major faults following a NW-SE direction with its different branches which are N-S, NE-SW, and E-W along which the dikes of a basic nature are set up. And it must be remembered that the kimberlites are arranged in a WNW-ESE orientation.</p><p>Three main directions frequently appear WNW-ESE, E-W, NE-SW for doleritic dikes which coincide with major fractures. The last two directions are the majority among which the almost E-W orientations are intersected by those of submeridian direction; which suggests different tectonic episodes [<xref ref-type="bibr" rid="scirp.133848-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.133848-ref24">24</xref>] [<xref ref-type="bibr" rid="scirp.133848-ref25">25</xref>] [<xref ref-type="bibr" rid="scirp.133848-ref26">26</xref>] .</p><p>The general interpretation of the different structural features of the aeromagnetic map made it possible to develop a synthetic structural model (<xref ref-type="fig" rid="fig8">Figure 8</xref> [<xref ref-type="bibr" rid="scirp.133848-ref24">24</xref>] ). This model, whose major axis in the shape of a horse’s tail is oriented NE-SW, defines a set of dextral and sinistral faults. The correlative analysis of the spatial distribution of diamondiferous and non-diamondiferous dolerite and kimberlite samples collected in the study area, with the interpreted structures (<xref ref-type="fig" rid="fig8">Figure 8</xref>), shows that they are mainly located in fault zones.</p></sec></sec><sec id="s5"><title>5. Discussion</title><p>The study of doleritic rocks in the K&#233;ni&#233;ba region was carried out in two stages during which we carried out an analysis of lithogeochemical (petrography and</p><p>petrology) and structural data. The results of the analysis during this study show similar values for dolerites located in the field of influence of kimberlites. Only one sample taken outside the field of influence of the kimberlites (DOL-3B) presents relatively low contents of major elements and certain rare earths compared to the others. Thus, we can retain the idea of partial mantle fusion at relatively high pressures. The kimberlites appear in the form of explosions in the dolerites which supposes that the dolerite dikes were already in place at the time of the intrusion of these kimberlites. The ascent of kimberlite magma enriched in certain major elements (TiO<sub>2</sub>, Fe<sub>2</sub>O<sub>3</sub>, CaO and Zr) creates metasomatism in contact with dolerite with enrichment of these major elements at the level within the limits of the zones of influence of the kimberlites; as noted in Russia [<xref ref-type="bibr" rid="scirp.133848-ref11">11</xref>] . We do not notice any significant difference between the major elements in the dolerites located in the field of influence of the kimberlites unlike those located outside the field of influence. These dolerites are chemically enriched than those of the Birimian of Toumodi in C&#244;te d’Ivoire [<xref ref-type="bibr" rid="scirp.133848-ref8">8</xref>] and those of Burkina Faso [<xref ref-type="bibr" rid="scirp.133848-ref27">27</xref>] . Therefore dolerites enriched in TiO<sub>2</sub>, Fe<sub>2</sub>O<sub>3</sub>, CaO and Zr can be used in the K&#233;ni&#233;ba area as a search criterion for kimberlite.</p><p>The reinterpretation of the aeromagnetic data highlighted three types of structures according to their direction, filled by dolerite dikes. Several generations of dolerites are each represented by a privileged direction. Among the three types of direction, we generally have East-West, NE-SW, WNW-ESE. This last direction corresponds to those that can be observed for the dolerite dikes in the southwest of C&#244;te d’Ivoire [<xref ref-type="bibr" rid="scirp.133848-ref28">28</xref>] and those of Birimian in the north of Burkina Faso [<xref ref-type="bibr" rid="scirp.133848-ref27">27</xref>] .</p><p>The age of doleritiques intrusions is associated with tectono-magmatic events that appeared on the African plate at the time of the dislocation of Gondwana. Among these events, we note that which occurred in the Jurassic which saw the establishment of large swarms of dolerites oriented following NE-SW which appear on maps of the region [<xref ref-type="bibr" rid="scirp.133848-ref23">23</xref>] [<xref ref-type="bibr" rid="scirp.133848-ref29">29</xref>] [<xref ref-type="bibr" rid="scirp.133848-ref30">30</xref>] [<xref ref-type="bibr" rid="scirp.133848-ref31">31</xref>] [<xref ref-type="bibr" rid="scirp.133848-ref32">32</xref>] . The lineaments constitute networks of dikes following the WNW-ESE direction which are Cretaceous and which control the K&#233;ni&#233;ba kimberlites. Elsewhere in the country, dolerites dating from the Carboniferous appear like those of the Taoud&#233;ni basin represented by E-W directions.</p><p>It is accepted that the kimberlites in this area are younger than the doleritic dikes they cross. However, the dating work of kimberlites using the Rb/Sr method on phlogopite showed an age of 1070 Ma for the S&#233;konomata pipe [<xref ref-type="bibr" rid="scirp.133848-ref33">33</xref>] ; which seems improbable when referring to the position of the kimberlites which intrude the dolerites. The significance of such an age could probably lie in contamination [<xref ref-type="bibr" rid="scirp.133848-ref34">34</xref>] .</p><p>Furthermore, we do not have recent dating concerning the kimberlites, however, elements of information could be provided by a more precise knowledge of the positions respective kimberlites and dolerites [<xref ref-type="bibr" rid="scirp.133848-ref35">35</xref>] . Kobato’s pipe, located on the Neoproterozoic plateau, is crossed by a dolerite dyke. It is the same for that of Bilali North in the Birimian plain. It’s necessary therefore admit, that at least these pipes predate the doleritic intrusions, at least to those of supposed age Middle or upper Cretaceous.</p></sec><sec id="s6"><title>6. Conclusion</title><p>Post-Neoproterozoic dolerites from the K&#233;ni&#233;ba region (Western Mali) are often associated with kimberlite pipes. They are tholeiitic in nature, of the E-MORB type and are more enriched in titanium than the Birimian dolerites of Toumodi, in central C&#244;te d’Ivoire. These dolerites would have formed in a late to post-orogenic intracontinental context during the dislocation of Gondwana, according to the pre-rifting period of the Atlantic Ocean. Structurally, K&#233;ni&#233;ba dolerites are often associated with kimberlite pipes, fractures and large deep structures identified using aeromagnetic images. Given the fact that the K&#233;ni&#233;ba kimberlites are difficult to observe in the field, the study of certain dolerites can be a helping tool and an indicator in the search for kimberlites in the region.</p></sec><sec id="s7"><title>Acknowledgements</title><p>This study was initiated as part of the thesis of Mr. Traore Baco at the Polytechnic Doctoral School of INP-HB in Yamoussoukro, C&#244;te d’Ivoire.</p></sec><sec id="s8"><title>Funding</title><p>Thanks to funding (for the field works) from the Eureka GEO Consulting Company of Bamako (Republic of Mali).</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>Ouattara, G., Traore, B., Siagn&#233;, Z.H., Denon, A., Sangare, S. and Allialy, M.E. (2024) Petrology and Structural Characterization of Post-Neopro- terozoic Dolerites from the Kimberlite Fields in the K&#233;ni&#233;ba Region (Western Mali). Open Journal of Geology, 14, 655-670. https://doi.org/10.4236/ojg.2024.146028</p></sec></body><back><ref-list><title>References</title><ref id="scirp.133848-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Dalrymphe, G.B., Gromme, C.S. and White, R.W. (1975) Potassium-Argon Age and Paleomagnetism of Diabase Dikes in Liberia: Initiation of Central Atlantic Rifting. &lt;i&gt;GSA Bulletin&lt;/i&gt;, 86, 399-411. &lt;br&gt;https://doi.org/10.1130/0016-7606(1975)86&lt;399:PAAPOD&gt;2.0.CO;2</mixed-citation></ref><ref id="scirp.133848-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Bardet, M.G. (1974) G&amp;#233;ologie du Diamant, Deuxi&amp;#232;me Partie: Gisements de Diamant d&amp;#8217;Afrique. 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