<?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.2021.116011</article-id><article-id pub-id-type="publisher-id">OJG-109781</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>
 
 
  Energy Dispersive X-Ray Spectroscopy of the Sohnari Member of Laki Formation from Southern Indus Basin of Pakistan
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Muhammad</surname><given-names>Asif Noonari</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>Surih</surname><given-names>Sibaghatullah Jagirani</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Huafeng</surname><given-names>Tang</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>Asghar</surname><given-names>A. A. D. Hakro</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Ali</surname><given-names>Ghulam Sahito</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kaleemullah</surname><given-names>Jagirani</given-names></name><xref ref-type="aff" rid="aff4"><sup>4</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Shahid</surname><given-names>Ali Shaikh</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Muhammad</surname><given-names>Dodo Jagirani</given-names></name><xref ref-type="aff" rid="aff5"><sup>5</sup></xref></contrib></contrib-group><aff id="aff3"><addr-line>Centre for Pure and Applied Geology University of Sindh, Jamshoro, Pakistan</addr-line></aff><aff id="aff4"><addr-line>Oil and Gas Development Company Limited, Islamabad, Pakistan</addr-line></aff><aff id="aff5"><addr-line>Department of Geography University of Sindh, Jamshoro, Pakistan</addr-line></aff><aff id="aff2"><addr-line>Institute of Tibetan Plateau Research, Chinese Academy of Science, Beijing, China</addr-line></aff><aff id="aff1"><addr-line>College of Earth Science, Jilin University, Changchun, China</addr-line></aff><pub-date pub-type="epub"><day>08</day><month>06</month><year>2021</year></pub-date><volume>11</volume><issue>06</issue><fpage>183</fpage><lpage>196</lpage><history><date date-type="received"><day>8,</day>	<month>April</month>	<year>2021</year></date><date date-type="rev-recd"><day>7,</day>	<month>June</month>	<year>2021</year>	</date><date date-type="accepted"><day>10,</day>	<month>June</month>	<year>2021</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>
 
 
  This study determines the geochemical and depositional environment analysis of the sediments of the Sohnari Member of the Laki Formation, Northern Kirthar Fold Belt of Pakistan. The Energy-Dispersive-X-Ray Spectroscopy (EDS) technique is used for the detection of major elements and the effects of shifting depositional climatic conditions of six representative samples which were acquired from the Sohnari Member of the Laki Formation at Lakhra area, Sindh, Pakistan. The sedimentological studies clarify that the sediments the Sonahri Member are relatively immature and most migrated in clastic mode. The availability of Silica shows that the Member was formed due to biochemical precipitation and detrital mode and was deposited at a fast rate of sediment deposition under the fluvio-deltaic depositional system. This is also deduced that the rapid rate of sediment deposition might be created a reducing atmosphere and allowing for the mineralization of sulphur.
 
</p></abstract><kwd-group><kwd>Energy Dispersive X-Ray Spectroscopy</kwd><kwd> Geochemistry</kwd><kwd> Sohnari Member the Laki Formation</kwd><kwd> Northern Kirthar Fold Belt of Pakistan</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Sohnari member is the basal part of the Laki Formation which overlies the Ranikot group and the Lakhra Formation of the Lakhra area [<xref ref-type="bibr" rid="scirp.109781-ref1">1</xref>] and [<xref ref-type="bibr" rid="scirp.109781-ref2">2</xref>]. Its basal contact is with Ranikot Group and got is unconformable obvious and its upper contact is with chat member of Laki Formation [<xref ref-type="bibr" rid="scirp.109781-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.109781-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.109781-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.109781-ref6">6</xref>]. Our study is focused on a geochemical investigation of the Sohnari member of the Laki Formation to interpret its origin and climate (<xref ref-type="fig" rid="fig1">Figure 1</xref>). SM of the Laki Formation is also thought to be a distinct origin from the Lakhra Formation and the overlying Chat member. Due to different characters the Sonhari member (<xref ref-type="fig" rid="fig3">Figure 3</xref>). It is worth including the position from the Laki formation SM is a section of clastic sedimentary rock transported beginning the east also placed among the Chat member and the Lakhra Formation. The SM is known as basal Laki laterite and represents the very slight regression possibly a reduction in the rate of the sinking of the continental shelf in the Indian Shield of Indian Plate and the peat is accumulated very close to the sea level.</p><sec id="s1_1"><title>1.1. General Geology of the Study Area</title><p>Rocks exposed in the studied area are mainly composed of detrital and non-detrital sediment. The rocks exposed in the study area belongs to the Ranikot, [<xref ref-type="bibr" rid="scirp.109781-ref7">7</xref>] and [<xref ref-type="bibr" rid="scirp.109781-ref8">8</xref>], which is primarily made up of the Bara Formation (Middle Paleocene)</p><p>Lakhra Formation (Late Paleocene), Sohnari, and Chat members of the Laki Formation (Early Eocene), Manchar Formation (Pliocene). These components contain shallow seas and floating sediments. Projected area is the Sohnari member that is chiefly composed of sandstone, nodular limestone, and lateritic clay, and gypsiferous shale of variegated colors including yellow, orange, red, maroon, rusty brown, and gray. Sandstone sometimes occurs in lenticular beds of variegated colors (<xref ref-type="fig" rid="fig2">Figure 2</xref>). Sandstone is soft and friable, lenticular beds of limonite</p><p>ochre, white clay, (fire clay), and lignite coal seams.</p></sec><sec id="s1_2"><title>1.2. Stratigraphy of the Area</title><p>The general stratigraphy of the study area is very much interesting in the research. The oldest stratigraphic unit is Bara Formation (Middle Paleocene age), [<xref ref-type="bibr" rid="scirp.109781-ref9">9</xref>]. The second oldest unit is Lakhra Formation (Late Paleocene). And the third one is the Laki Formation of the Eocene age. The fourth youngest stratigraphic unit is the Siwalik group i.e. Manchar Formation of (Mio-Pliocene age). General stratigraphy of the studied area is presented in (<xref ref-type="table" rid="table1"><xref ref-type="table" rid="table">Table </xref>1</xref>).</p><p>The second oldest stratigraphic unit of this area is the Lakhra Formation of (late Paleocene) age [<xref ref-type="bibr" rid="scirp.109781-ref2">2</xref>], Lakhra Formation was also proposed as a name for the “Upper Ranikot (limestone)” and “Upper Ranikot” of later workers, after Lakhra, Laki range [<xref ref-type="bibr" rid="scirp.109781-ref10">10</xref>]. The Formation is predominantly grey limestone with yellowish staining and weathering brown and buff, with some orange-brown and pinkish-brown patches. The lower section is made up of sandstone., with sand interbeds. In the upper section, there are sandstone and shale interbeds. The Bara Formation is uniformly overlain by the Formation. It is uncomfortably overlain by the Laki formation in the Kirthar province [<xref ref-type="bibr" rid="scirp.109781-ref2">2</xref>].</p></sec><sec id="s1_3"><title>1.3. Sohnari Member</title><p>The thickness of the Sonhari member is about 25 feet [<xref ref-type="bibr" rid="scirp.109781-ref11">11</xref>]. SM is very well developed in the meeting Jhimpir area of Thatta district. The SM sometimes there are thin beds of sandy yellow limestone with assilina granulose. The thickness of the SM is varying from place to place (10 to 25 feet). SM is well developed in onger, mettign and Jampir areas. It is Lanticular, thickness varies from 1 to 20 meters. In the Lakhra area, the thickness ranges from 0 to 8 meters. The SM is missing in drill no L-25 and L-27 of the Lakhra area. Lenticular beds of limonite, ochre white clay (fire clay) and lignite coal seams of varying thickness or characteristic unit for the member and have also the commercial importance and The Ranikot and the Laki have interacted. There is a layer of ferogeneous claystone and siltstone that ranges from 17 to 19 feet thick and is known as laterite. It’s a concrete color with sporadic white spots, and it’s moderately strong (<xref ref-type="fig" rid="fig3">Figure 3</xref>). These lateritic beds are on the contact of the Formation are present in the Lakhra area [<xref ref-type="bibr" rid="scirp.109781-ref12">12</xref>]. The surface exposure of the Sohnari member consists of the highly ferruginous claystone and the sandstone of the variegated colors varies from yellowish-brown, rusty brown, dark yellowish, brown, white, cheery red, and</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1"><xref ref-type="table" rid="table">Table </xref>1</xref></label><caption><title> Shows the Stratigraphy of the study area</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >S. No</th><th align="center" valign="middle" >Formation</th><th align="center" valign="middle" >Age</th><th align="center" valign="middle" >Lithology</th></tr></thead><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >Siwalik group</td><td align="center" valign="middle" >Mio-Pliocene</td><td align="center" valign="middle" >Conglomerate, Sandstone and Clay</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >Laki Formation</td><td align="center" valign="middle" >Eocene</td><td align="center" valign="middle" >Limestone, shale and sandstone</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >Lakhra Formation</td><td align="center" valign="middle" >Late Paleocene</td><td align="center" valign="middle" >Limestone, shale and sandstone</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >Bara Formation</td><td align="center" valign="middle" >Middle Paleocene</td><td align="center" valign="middle" >Sandstone, Shale and shale</td></tr></tbody></table></table-wrap><p>purple color. The Sandstone is fine to medium-grained [<xref ref-type="bibr" rid="scirp.109781-ref13">13</xref>]. Poorly sorted loose friable and the lansoide and ferruginous sandstone with white calcareous sandstone are common in this member. Sometimes sandstone occurs in lenticular beds of variegated colors. Vary colored lateritic clay, shale of variegated color including, yellow-orange, maroon, rusty brown, arenaceous limestone, packed limestone of ochre lignited. There are no fossils present in the Sohnari Member of the Laki Formation, which dates from the early Eocene.</p><p>The SM is the basal part of the Laki Formation which overlies the Ranikot group and the Lakhra Formation of the Lakhra area [<xref ref-type="bibr" rid="scirp.109781-ref14">14</xref>]. It has an uncomfortably marked basal contact with the Ranikot group and an upper contact with the Chat member of the Laki Formation. The Sohnari member of the Laki Formation is also thought to be distinct from the underlying Lakhra Formation and the overlying Chat member (<xref ref-type="fig" rid="fig3">Figure 3</xref>).</p></sec></sec><sec id="s2"><title>2. Material &amp; Methods</title><p>The detailed geological fieldwork was carried out and rock samples were collected for the study, one section of Sohnari member was measured from the eastern flank of the Lakhra anticline. The elemental analysis of the sample was accomplished by (SEM &amp; EDS), a total of fifteen samples was collected according to the bedding of the Formation.</p><sec id="s2_1"><title>2.1. Geological Fieldwork</title><p>The section of Sohnari Member of Laki Formation was measured, latitude 25˚40'00&quot;N and longitude Long; 68˚5'00&quot;E). Geological hammer, Brunton compass, measuring tape, sample bags, permanent marker, hand lenses were used during field at Sohnari Member of Laki Formation. During geological fieldwork, we have observed primary sedimentary structures i.e. (cross-bedding, lamination, and ripples) and massive beds of outcrops, and Photographed.</p></sec><sec id="s2_2"><title>2.2. Sampling</title><p>These samples enclosed sandstone, nodular limestone and lateritic clay, and gypsiferous shale of variegated colors including yellow, orange, red, maroon, rusty brown, and gray. Sandstones of Sohnari Member of Laki Formation vary in Brown (dark brown to light brown) yellowish, light yellow, white, pinkish, and purple colors. These sandstones are loose and consolidated. Clay of Sohnari Member of Laki Formation varies in radish brown and dark brown colors. Sampling was done according to the bedding in Sohnari Member of Laki Formation. The loose and unconsolidated sandstones of the studied stratigraphic unit are selected for Lab analysis.</p></sec></sec><sec id="s3"><title>3. Result</title><p>Six rock samples from the Sohnari member were collected, prepared, and analyzed by the Advance Research Laboratory of the Centre for Pure and Applied Geology, University of Sindh, Jamshoro. Energy-dispersive x-ray spectroscopy (EDS) is a technique for analyzing elements and determining the chemical properties of a sample form of XRF [<xref ref-type="bibr" rid="scirp.109781-ref15">15</xref>] and [<xref ref-type="bibr" rid="scirp.109781-ref16">16</xref>]. It is a form of spectroscopy that involves analyzing a sample by interactions between electromagnetic radiation and matter, such as detecting X-rays imitated by matter in response to being struck with charged particles [<xref ref-type="bibr" rid="scirp.109781-ref17">17</xref>]. Its classification abilities are due in large part to the general premise that each element has a unique atomic structure, which enables X-rays that are products of an element’s atomic structure to be differentiated from one another is centered into the sample being analyzed to induce the release of distinctive X-rays (<xref ref-type="fig" rid="fig4">Figure 4</xref>). When an atom in a sample is at rest, it includes ground state (or unexcited) electrons in distinct energy ranges or electron shells, which are expelled from the shell, leaving an electron-hole in its place. An electron released from an exterior, higher-energy shell, and a lower-energy shell in the shape of a specimen can be quantified with an energy dispersive spectrometer.</p><p>The elemental composition of the specimen can be measured since x-ray radiation is a result of the temperature differential between the two shells as well as the atomic structure of the elements from which it was emitted.</p></sec><sec id="s4"><title>4. Discussion</title><p>Silicon (SiO<sub>2</sub>):</p><p>The silicon dioxide content of the sediments analyses ranges from 19.25% to</p><p>32.83%, with an average of 24.54%, in (n = 6) samples (TableS1). Si/Al ratios are used by sedimentary geochemists to determine the presence of various forms of silica in sedimentary rocks [<xref ref-type="bibr" rid="scirp.109781-ref18">18</xref>]. Couture made use of the Si/Al scale in sedimentary rocks for the measurement of bigamous Silica, indicated that a higher Si/Al value indicates the A higher Si/Al value indicates the presence of bigamous silica, while a lower Si/Al value indicates the presence of terrigenous material. The Si/Al amount of the surveyed sediments varies from (0.59) to (1.94), with an average of (1.27), as seen in the graph (TableS2). The presence of biogenically precipitated Silica and detrital Silica is indicated by the highest and lowest values in the observed sediments, respectively.</p><p>Titanium (TiO<sub>2</sub>):</p><p>The titanium dioxide content of the analyzed (N = 6) samples ranges from 1.25% to 3.10%, with an average of 8.37%. The majority of Ti/Al ratios in the studied samples indicate that the Sohnari member of the Laki Formation is made up of sandstone, confirming previous research. Furthermore, [<xref ref-type="bibr" rid="scirp.109781-ref19">19</xref>] used the (Ti/Al) ratio to complete the Transition in Temperature during Deposition, and the interpretation of the (Ti/Al) ratio indicates that the Sample region witnessed shifting Climatic conditions during Sediment Deposition.</p><p>Aluminum (Al<sub>2</sub>O<sub>3</sub>):</p><p>The Aluminum trioxide of Sohnari member of Laki Formation Sediments (N = 6) varies (TableS1), from (11.12%) to (32.25%) with an average of (21.28%). Kaolinite and illite hold high concentrations [<xref ref-type="bibr" rid="scirp.109781-ref20">20</xref>]. Kaolinite, chlorite, illite, and Montmorillonite Clay minerals are present in Sohnari members of the Laki Formation. The maturity index of the analyses rock samples was determined using the Al<sub>2</sub>O<sub>3</sub>/Na<sub>2</sub>O<sub>3</sub> ratio, as suggested by [<xref ref-type="bibr" rid="scirp.109781-ref21">21</xref>] and [<xref ref-type="bibr" rid="scirp.109781-ref22">22</xref>]. The Al<sub>2</sub>O<sub>3</sub>/Na<sub>2</sub>O ratios (6.62 to 20.80) mean that the sediments analyzed are younger and are shipped as detrital particles. The Al<sub>2</sub>O<sub>3</sub>/SiO<sub>2</sub> ratio of the analyzed rock samples, suggests that sediments of Sohnari member of the Laki Formation do not contain a substantial amount of minerals found in clay (TableS2).</p><p>Iron (Fe<sub>2</sub>O<sub>3</sub>):</p><p>The iron concentration in Sohnari member samples studied (N = 6) ranges from 2.75% to 37.54%, with an average of 2.75% to 16.17%). To determine the relationship between iron and clay minerals, the Fe<sub>2</sub>O<sub>3</sub>/Al<sub>2</sub>O<sub>3</sub> ratio is used [<xref ref-type="bibr" rid="scirp.109781-ref23">23</xref>] and [<xref ref-type="bibr" rid="scirp.109781-ref24">24</xref>]. The Fe<sub>2</sub>O<sub>3</sub>/Al<sub>2</sub>O<sub>3</sub> ratios of the samples analyzed show a poor association with clay minerals (TableS2). The Mn/Fe ratio has been used to classify depositional conditions in sedimentary rocks [<xref ref-type="bibr" rid="scirp.109781-ref25">25</xref>] and [<xref ref-type="bibr" rid="scirp.109781-ref26">26</xref>]. The observed Mn/Fe ratios indicate that the Sohnari member of the Laki Formation was deposited nearshore to offshore. The Low Mn/Fe ratio is a consequence of this leaching process. Strong chemical weathering can cause a high concentration of Fe<sub>2</sub>O<sub>3</sub> to develop [<xref ref-type="bibr" rid="scirp.109781-ref27">27</xref>].</p><p>Magnesium (MgO):</p><p>The mg/Al<sub>2</sub>O<sub>3</sub> ratio measured from the MgO distribution in the analyzed (N = 6) samples ranges from 0.92% to 1.65%, (TableS1), with mean values of (1.05%). [<xref ref-type="bibr" rid="scirp.109781-ref23">23</xref>] for the presence of Montmorillonite and Clay minerals, and the mg/Al<sub>2</sub>O<sub>3</sub> ratio calculated according to [<xref ref-type="bibr" rid="scirp.109781-ref24">24</xref>] for the presence of Montmorillonite and Clay minerals, and the mg/Al<sub>2</sub>O<sub>3</sub> (TableS2). The occurrence of MgO in montmorillonite lattices is suggested by its weak positive correlation with iron.</p><p>Sodium (Na<sub>2</sub>O):</p><p>The concentration of (Na<sub>2</sub>O) in the Sohnari member of the Laki Formation ranges from 1.79% to 7.85%, with a mean of 3.61% (n = 51) samples (TableS1). In contrast to other cations including Ca<sup>2+</sup> and Mg<sup>2+</sup>, the montmorillonite (smectite) produces fewer Na+ in the inter-layered position [<xref ref-type="bibr" rid="scirp.109781-ref20">20</xref>] and [<xref ref-type="bibr" rid="scirp.109781-ref25">25</xref>] used the Na/K ratio to calculate the sediment deposition rate. These Na/K ratios suggest a medium to high rate of sediment deposition in the samples analyzed.</p><p>Potassium (K<sub>2</sub>O):</p><p>The Sohnari member of the Laki Formation (K<sub>2</sub>O) concentration ranges from 0.51% to 0.80%, with a mean value of 0.51% and 0.21%. As compared to other cations (calcium and magnesium), the lattices of montmorillonite often contain small amounts of potassium and sodium oxides [<xref ref-type="bibr" rid="scirp.109781-ref20">20</xref>], and [<xref ref-type="bibr" rid="scirp.109781-ref28">28</xref>] used the Na/K ratio to calculate the rate of sediment deposition and the crystallinity of Illite. The presence of depleted illite and a low to high rate of sediment deposition was demonstrated by the Na/K ratios of the examined samples. The K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> ratio is used to determine the amount of sand in a sediment sample [<xref ref-type="bibr" rid="scirp.109781-ref24">24</xref>], the density of sand in sediments, and the fast rate of sediment deposition was suggested by the K<sub>2</sub>O/Al<sub>2</sub>O<sub>3</sub> ratio of the samples analyzed.</p><p>Sulphur (S):</p><p>The sulphur concentrations range from 0.72% to 0.52%, with an average value of 0.52% and 0.37% (TableS1). Sulfur content of shales is on average below 1%. (0.25%), the average concentration of European Paleozoic shales is 0.32% [<xref ref-type="bibr" rid="scirp.109781-ref29">29</xref>] and [<xref ref-type="bibr" rid="scirp.109781-ref30">30</xref>]. The Sohnari member of the Laki Formation Sulphur in the samples indicates the presence of metabolizable organic matter, sulfate-reducing bacteria, and dissolved sulphide in the depositional conditions. [<xref ref-type="bibr" rid="scirp.109781-ref31">31</xref>] knows that the presence of sulphides in some Pacific Ocean trenches is due to a heavy content of organic matter and a high rate of sediment deposition. The Sohnari member of the Laki Formation sediments’ rapid deposition rate may have resulted in reducing conditions during deposition, which may explain the presence of sulphur in the studied samples.</p></sec><sec id="s5"><title>5. Conclusions</title><p>The Sohnari Laki Formation member is mostly quartz (low), with biogenically precipitated or detrital silica as the source of the silica. The Ti/Al ratio indicates that during the deposition of the Sohnari member of the Laki Formation sediments, the study region was subjected to shifting climatic conditions. The sediments under examination are younger and are shipped as detrital particles. The deposition rate is medium to high, and there is degraded illite in the samples. A sand abundance of sediments implies a high rate of deposition. Sulfur means that there is enough metabolizable organic matter available, reducing the depositional condition.</p><p>The Sohnari Laki Formation member was deposited under the fluvio-deltaic depositional scheme, based on its dominant quartz mineral composition, material ratios, and lower maturity. In the light of geochemical results, the sediments of Sohnari members composed of detrital Silica deposited in changing climatic conditions and medium to high rate of deposition, less mature, sufficient availability of metabolized of origin matter. It is concluded here these sediments are deposited under fluviotile conditions/origin.</p></sec><sec id="s6"><title>Acknowledgements</title><p>This study was financially supported by the National Nature Science Foundation of China Grant, Prof. Dr. Huafeng Tang, and the Chinese Scholarship Council to Muhammad Asif Noonari to pursue the Master’s Degree at College of Earth Science Jilin University of China. Furthermore, the auothers are thankful to Ex-Director of Centre Pure and Applied Geology University of Sindh Jamshoro Sindh, Prof. Dr. Sarfarz Hussain Solangi for providing the transport facility and moral support to carry out this study.</p></sec><sec id="s7"><title>Conflicts of Interest</title><p>The authors declare no conflicts of interest regarding the publication of this paper.</p></sec><sec id="s8"><title>Cite this paper</title><p>Noonari, M.A., Jagirani, S.S., Tang, H.F., Hakro, A.A.A.D., Sahito, A.G., Jagirani, K., Shaikh, S.A. and Jagirani, M.D. (2021) Energy Dispersive X-Ray Spectroscopy of the Sohnari Member of Laki Formation from Southern Indus Basin of Pakistan. Open Journal of Geology, 11, 183-196. https://doi.org/10.4236/ojg.2021.116011</p></sec><sec id="s9"><title>Appendix Tables</title><table-wrap id="table2" ><label><xref ref-type="table" rid="table">Table </xref>S1</label><caption><title> Major elements of study area</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Sample</th><th align="center" valign="middle" >Sio<sub>2</sub></th><th align="center" valign="middle" >TiO</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" >Ca<sub>2</sub></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" >SO<sub>3</sub></th><th align="center" valign="middle" >Total</th></tr></thead><tr><td align="center" valign="middle" >1Ra</td><td align="center" valign="middle" >19.25</td><td align="center" valign="middle" >1.55</td><td align="center" valign="middle" >32.25</td><td align="center" valign="middle" >37.54</td><td align="center" valign="middle" >1.65</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >0.51</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >92.75</td></tr><tr><td align="center" valign="middle" >3Ra</td><td align="center" valign="middle" >21.86</td><td align="center" valign="middle" >1.68</td><td align="center" valign="middle" >24.01</td><td align="center" valign="middle" >28.36</td><td align="center" valign="middle" >1.47</td><td align="center" valign="middle" >2.44</td><td align="center" valign="middle" >5.13</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >0.72</td><td align="center" valign="middle" >85.67</td></tr><tr><td align="center" valign="middle" >5Ra</td><td align="center" valign="middle" >29.22</td><td align="center" valign="middle" >2.03</td><td align="center" valign="middle" >19.63</td><td align="center" valign="middle" >7.14</td><td align="center" valign="middle" >0.96</td><td align="center" valign="middle" >5.19</td><td align="center" valign="middle" >7.85</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >72.02</td></tr><tr><td align="center" valign="middle" >6Ra</td><td align="center" valign="middle" >21.62</td><td align="center" valign="middle" >1.35</td><td align="center" valign="middle" >11.12</td><td align="center" valign="middle" >8.39</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.42</td><td align="center" valign="middle" >1.79</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >45.69</td></tr><tr><td align="center" valign="middle" >10Ra</td><td align="center" valign="middle" >22.48</td><td align="center" valign="middle" >1.25</td><td align="center" valign="middle" >19.83</td><td align="center" valign="middle" >2.75</td><td align="center" valign="middle" >0.92</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >4.97</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.52</td><td align="center" valign="middle" >53.72</td></tr><tr><td align="center" valign="middle" >11Ra</td><td align="center" valign="middle" >32.83</td><td align="center" valign="middle" >3.10</td><td align="center" valign="middle" >20.55</td><td align="center" valign="middle" >12.86</td><td align="center" valign="middle" >1.32</td><td align="center" valign="middle" >3.00</td><td align="center" valign="middle" >1.94</td><td align="center" valign="middle" >0.80</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >76.4</td></tr><tr><td align="center" valign="middle" >Minimum</td><td align="center" valign="middle" >19.25</td><td align="center" valign="middle" >1.25</td><td align="center" valign="middle" >11.12</td><td align="center" valign="middle" >2.75</td><td align="center" valign="middle" >0.92</td><td align="center" valign="middle" >1.42</td><td align="center" valign="middle" >1.79</td><td align="center" valign="middle" >0.51</td><td align="center" valign="middle" >0.72</td><td align="center" valign="middle" >-</td></tr><tr><td align="center" valign="middle" >Maximum</td><td align="center" valign="middle" >32.83</td><td align="center" valign="middle" >3.10</td><td align="center" valign="middle" >32.25</td><td align="center" valign="middle" >37.54</td><td align="center" valign="middle" >1.65</td><td align="center" valign="middle" >5.19</td><td align="center" valign="middle" >7.85</td><td align="center" valign="middle" >0.80</td><td align="center" valign="middle" >1.52</td><td align="center" valign="middle" >-</td></tr><tr><td align="center" valign="middle" >Average</td><td align="center" valign="middle" >24.54</td><td align="center" valign="middle" >1.82</td><td align="center" valign="middle" >21.23</td><td align="center" valign="middle" >16.17</td><td align="center" valign="middle" >1.05</td><td align="center" valign="middle" >2.00</td><td align="center" valign="middle" >3.61</td><td align="center" valign="middle" >0.21</td><td align="center" valign="middle" >0.37</td><td align="center" valign="middle" >-</td></tr></tbody></table></table-wrap><table-wrap id="table3" ><label><xref ref-type="table" rid="table">Table </xref>S2</label><caption><title> Ratios of elements of samples from Sohnari member of Laki formation</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Sample</th><th align="center" valign="middle" >Al<sub>2</sub>O<sub>3</sub>/ SiO<sub>2</sub></th><th align="center" valign="middle" >Al<sub>2</sub>O<sub>3</sub>/ Na<sub>2</sub>O</th><th align="center" valign="middle" >Fe<sub>2</sub>O<sub>3</sub>/ Al<sub>2</sub>O<sub>3</sub></th><th align="center" valign="middle" >K<sub>2</sub>O/ Al<sub>2</sub>O<sub>3</sub></th><th align="center" valign="middle" >MgO/ Al<sub>2</sub>O<sub>3</sub></th><th align="center" valign="middle" >SiO<sub>2</sub>/ Al<sub>2</sub>O<sub>3</sub></th><th align="center" valign="middle" >Na<sub>2</sub>O/ K<sub>2</sub>O</th><th align="center" valign="middle" >TiO<sub>2</sub>/ Al<sub>2</sub>O<sub>3</sub></th></tr></thead><tr><td align="center" valign="middle" >1Ra</td><td align="center" valign="middle" >0.59</td><td align="center" valign="middle" >32.25</td><td align="center" valign="middle" >1.16</td><td align="center" valign="middle" >0.01</td><td align="center" valign="middle" >0.05</td><td align="center" valign="middle" >0.59</td><td align="center" valign="middle" >0.51</td><td align="center" valign="middle" >0.04</td></tr><tr><td align="center" valign="middle" >3Ra</td><td align="center" valign="middle" >0.91</td><td align="center" valign="middle" >4.68</td><td align="center" valign="middle" >1.18</td><td align="center" valign="middle" >24.01</td><td align="center" valign="middle" >0.06</td><td align="center" valign="middle" >0.91</td><td align="center" valign="middle" >5.13</td><td align="center" valign="middle" >0.06</td></tr><tr><td align="center" valign="middle" >5Ra</td><td align="center" valign="middle" >1.48</td><td align="center" valign="middle" >2.50</td><td align="center" valign="middle" >0.36</td><td align="center" valign="middle" >19.63</td><td align="center" valign="middle" >0.04</td><td align="center" valign="middle" >1.48</td><td align="center" valign="middle" >7.85</td><td align="center" valign="middle" >0.10</td></tr><tr><td align="center" valign="middle" >6Ra</td><td align="center" valign="middle" >1.94</td><td align="center" valign="middle" >6.21</td><td align="center" valign="middle" >0.75</td><td align="center" valign="middle" >11.12</td><td align="center" valign="middle" >11.12</td><td align="center" valign="middle" >1.94</td><td align="center" valign="middle" >1.79</td><td align="center" valign="middle" >0.12</td></tr><tr><td align="center" valign="middle" >10Ra</td><td align="center" valign="middle" >1.13</td><td align="center" valign="middle" >3.98</td><td align="center" valign="middle" >0.13</td><td align="center" valign="middle" >19.83</td><td align="center" valign="middle" >0.04</td><td align="center" valign="middle" >1.13</td><td align="center" valign="middle" >4.97</td><td align="center" valign="middle" >0.06</td></tr><tr><td align="center" valign="middle" >11Ra</td><td align="center" valign="middle" >1.59</td><td align="center" valign="middle" >10.59</td><td align="center" valign="middle" >0.62</td><td align="center" valign="middle" >20.55</td><td align="center" valign="middle" >0.06</td><td align="center" valign="middle" >1.59</td><td align="center" valign="middle" >2.42</td><td align="center" valign="middle" >0.15</td></tr><tr><td align="center" valign="middle" >Average</td><td 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