<?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.2015.510061</article-id><article-id pub-id-type="publisher-id">OJG-60581</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>
 
 
  Dolomitization in Campanian Oil Shale Rocks from South-Western Jordan
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ani</surname><given-names>M. Alnawafleh</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>Khalid</surname><given-names>E. Tarawneh</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>Hani</surname><given-names>N. Khoury</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>Nafeth</surname><given-names>A. Abdelhadi</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>Osama</surname><given-names>Y. Shakkoury</given-names></name><xref ref-type="aff" rid="aff5"><sup>5</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Reyad</surname><given-names>A. Dwairi</given-names></name><xref ref-type="aff" rid="aff6"><sup>6</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Mazen</surname><given-names>N. Amaireh</given-names></name><xref ref-type="aff" rid="aff6"><sup>6</sup></xref></contrib></contrib-group><aff id="aff3"><addr-line>Department of Geology, The University of Jordan, Amman, Jordan</addr-line></aff><aff id="aff2"><addr-line>Faculty of Engineering, Isra University, Amman, Jordan</addr-line></aff><aff id="aff4"><addr-line>Faculty of Engineering Technology, Al Balqa Applied University, Salt, Jordan</addr-line></aff><aff id="aff6"><addr-line>Faculty of Engineering, Tafila Technical University, Tafila, Jordan</addr-line></aff><aff id="aff5"><addr-line>Natural Resources Authority, Amman, Jordan</addr-line></aff><aff id="aff1"><addr-line>Faculty of Engineering, Al-Hussein Bin Talal University, Ma’an, Jordan</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>hanialnawafleh@ahu.edu.jo(AMA)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>14</day><month>10</month><year>2015</year></pub-date><volume>05</volume><issue>10</issue><fpage>689</fpage><lpage>700</lpage><history><date date-type="received"><day>23</day>	<month>August</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>23</month>	<year>October</year>	</date><date date-type="accepted"><day>26</day>	<month>October</month>	<year>2015</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 work represents the first detailed study of an oil shale (OS) section from the Upper Campanian Amman Silicified Limestone (ASL) Formation in south-western part of Jordan. More than five meters of oil shale have been recorded. Using the petrography and geochemistry, this study aims to focus on such non-conventional types of oil shale rocks in Jordan and to shed some light on their composition and formational environment. Unlike oil shale from Maastrichtian to early Tertiary, this type of oil shale is highly dolomitized. The dolomite is diagenetic in origin. This oil shale type contains considerable amount of OM and remarkably enriched in some trace elements and shows quite low sulfur content. Results suggest that the formation of dolomite appears to be limited by the rate of organic matter oxidation.
 
</p></abstract><kwd-group><kwd>Jordan</kwd><kwd> Oil Shale</kwd><kwd> Dolomitization</kwd><kwd> Campanian</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Jordan has huge oil shale (OS) resource and considered one of the world leading countries in its OS potential deposits. More than 24 deposits are recorded [<xref ref-type="bibr" rid="scirp.60581-ref1">1</xref>] . The well-known Jordanian OS belongs to the upper cretaceous and lower tertiary formations [<xref ref-type="bibr" rid="scirp.60581-ref2">2</xref>] . The Jordanian OS is generally not exposed. Previous work conducted on Jordanian OS is based mainly upon shallow boreholes and limited OS outcrops. Previous work and OS exploration in Jordan have focused on Upper Cretaceous OS from Muwaqqar Chalk Marl formation (MCM) (e.g. [<xref ref-type="bibr" rid="scirp.60581-ref3">3</xref>] - [<xref ref-type="bibr" rid="scirp.60581-ref8">8</xref>] ). The OS from MCM formation is bituminous limestone [<xref ref-type="bibr" rid="scirp.60581-ref8">8</xref>] . At Wadi Al-Bustan, south-western corner of Jordan (<xref ref-type="fig" rid="fig1">Figure 1</xref> and <xref ref-type="fig" rid="fig2">Figure 2</xref>), the OS is found in two stratigraphical levels. The upper (younger) level is that of MCM formation (<xref ref-type="fig" rid="fig2">Figure 2</xref>(a)) from Maastrchtian-Paleocene [<xref ref-type="bibr" rid="scirp.60581-ref2">2</xref>] . Full Petrographic and geochemical characterization of this OS type is found in Alnawafleh [<xref ref-type="bibr" rid="scirp.60581-ref8">8</xref>] and later papers by the same author (e.g. [<xref ref-type="bibr" rid="scirp.60581-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref10">10</xref>] ). The lower level (older) (<xref ref-type="fig" rid="fig2">Figure 2</xref>(b)), which is bituminous dolomitic limestone, is a part of upper Campanian Amman Silicified Limestone (ASL) Formation [<xref ref-type="bibr" rid="scirp.60581-ref2">2</xref>] .</p><p>The ASL formation is related to the Late Cretaceous Belqa Group. Jordan was flooded during the Late Cretaceous and the shallow marine sediments of the Belqa Group were deposited [<xref ref-type="bibr" rid="scirp.60581-ref11">11</xref>] . The age of the ASL Formation is latest Cretaceous (Campanian-early Maastrichtian) [<xref ref-type="bibr" rid="scirp.60581-ref12">12</xref>] . Its thickness varies from 30 to 100 m [<xref ref-type="bibr" rid="scirp.60581-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref14">14</xref>] . The base of this formation is defined below the first massive thick-bedded chert and above the marly chalks or silts/sands of the Wadi Umm Ghudran/Fassua Formation [<xref ref-type="bibr" rid="scirp.60581-ref15">15</xref>] .</p><p>Dolomite is generally associated with sedimentary limestone. As a mineral, dolomite is common in ancient marine and terrestrial deposits [<xref ref-type="bibr" rid="scirp.60581-ref16">16</xref>] . Dolomite is found in wide range of formational setting [<xref ref-type="bibr" rid="scirp.60581-ref17">17</xref>] . Theories re-</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Location of Wadi Al-Bustan (study area)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1210399x5.png"/></fig><fig-group id="fig2"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Oil shale surface exposures in Wadi Al-Bustan, S-W of Jordan. (a) Oil shale (bituminous rocks) exposure from Muwaqqar Chalk Marl Formation; (b) Close view of oil shale from Amman Silicified Limestone Formation.</title></caption><fig id ="fig2_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1210399x6.png"/></fig></fig-group><p>lated to dolomite formation are continued to evolve and many modes of dolomite origins are proposed. Based on their mode of formation, dolomites can be broadly divided into primary and secondary dolomites [<xref ref-type="bibr" rid="scirp.60581-ref18">18</xref>] . In Jordan, dolomite can be found in the Burj Dolomite-Shale Formation of Cambrian age and in upper cretaceous Naur, Hummar and Wadi Es-sir formations [<xref ref-type="bibr" rid="scirp.60581-ref19">19</xref>] .</p><p>Literature deals with dolomitization in OS are quite limited. It is the purpose of this paper to understand the geologic characteristics and the genesis of dolomitized OS rocks from Jordan. The geochemical parameters discussed here are based on the various analyses results on OS surface outcrop samples from the bituminous dolomitic limestone section of the upper Campanian ASL Formation.</p></sec><sec id="s2"><title>2. Geologic Setting</title><p>Jordan’s OS from Campanian age is rarely referred to in literature. More attention has been given to that OS of the Muwaqqar Chalk Marl Formation. The OS from Campanian age is related to Amman Silicified Limestone Formation (ASL). These OS beds can easily be traced in the field as they are exposed in some wadis like Wadi Al-Bustan in Ash-Shoubak area. Amman Silicified Limestone Formation is easily traced across the country. This formation is characterized by cliff forming, massive chert beds overlaying the Wadi Umm Ghudran/Fassua Formation [<xref ref-type="bibr" rid="scirp.60581-ref15">15</xref>] . In South and Southeast Jordan, the deposition took place under marginal marine conditions with increased content of siliciclastic deposits [<xref ref-type="bibr" rid="scirp.60581-ref15">15</xref>] . Shallow near-shore environment for chert beds of this formation was concluded by Abed and Kraishan [<xref ref-type="bibr" rid="scirp.60581-ref20">20</xref>] . More information about the genesis of this formation is found in Abu Jaber et al. [<xref ref-type="bibr" rid="scirp.60581-ref13">13</xref>] . They reported that the ASL Formation was deposited on a shallow carbonate platform along the fringes of the Tethyan seaway. The stratigraphic column of ASL Formation within the studied area is shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>.</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Lithologic column of Amman Silicified Limestone Formation in the study area. Modified from Barjous [<xref ref-type="bibr" rid="scirp.60581-ref36">36</xref>] </title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1210399x7.png"/></fig><p>The formational framework of the Jordanian OS has been investigated by many researchers over the last four decades (e.g. [<xref ref-type="bibr" rid="scirp.60581-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref21">21</xref>] - [<xref ref-type="bibr" rid="scirp.60581-ref26">26</xref>] ).There are several scenarios about the formation of Jordanian oil shales. These scenarios are combination of paleoclimatic, paleogeographic and paleotectonic factors. Recent biostratigraphic and petrographic studies on Upper Cretaceous-Eocene OS from Jordan have reached to similar results on the formational and controlling factors that have been reported and discussed previously by Alnawafleh [<xref ref-type="bibr" rid="scirp.60581-ref8">8</xref>] (e.g. [<xref ref-type="bibr" rid="scirp.60581-ref27">27</xref>] - [<xref ref-type="bibr" rid="scirp.60581-ref31">31</xref>] ). In central Jordan, oil shale deposited in synclinal basins [<xref ref-type="bibr" rid="scirp.60581-ref3">3</xref>] . During the late Cretaceous period, the eastern Mediterranean formed part of the southern broad shallow epeiric shelf of the Tethys Ocean [<xref ref-type="bibr" rid="scirp.60581-ref15">15</xref>] . The sea-floor of the eastern Mediterranean was not topographically smooth but consisted of basins and swells [<xref ref-type="bibr" rid="scirp.60581-ref12">12</xref>] . These structures are believed to be resulted from the late cretaceous major tectonic pulse of the Syrian Arc fold belt [<xref ref-type="bibr" rid="scirp.60581-ref32">32</xref>] . With the areas covered by the Syrian Arc, the basins and swells are folded whereas in Jordan such structures are not folded [<xref ref-type="bibr" rid="scirp.60581-ref33">33</xref>] indicates the importance of the sea-floor bathymetry as a controlling factor of the upper cretaceous sedimentation in the region including Jordan’s OS. Regional sea-level fluctuations of Late Cretaceous have played a major role in the deposition of OS in Jordan [<xref ref-type="bibr" rid="scirp.60581-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref29">29</xref>] . The high productivity due to upwelling currents along the shelf edge and the anoxic bottom water conditions are major controlling factors in OS formation [<xref ref-type="bibr" rid="scirp.60581-ref4">4</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref34">34</xref>] . It is important to mention that some parts of OS in central Jordan have been pyrometamorphosed to marble [<xref ref-type="bibr" rid="scirp.60581-ref35">35</xref>] .</p></sec><sec id="s3"><title>3. Field Work and Sampling</title><p>Twelve samples were collected from the OS section that exposed at the base of Wadi Al-Bustan north of Ash-Shoubak area in south-western part of Jordan (<xref ref-type="fig" rid="fig1">Figure 1</xref>). The field observations show that this OS section is made of irregular rhythmic repetition of pale and dark bands of fine-grained mudstone. Nearly 5.5 meters were recorded and sampled. Oil shale section varies in hardness and occasionally fractured. The lower part is almost rich in shell fragments and fossil debris and biogenic material and contains some coarse concretion particles (biogenic debris or dolomitic lumps) and reveals sugary texture. Some bands in this section have distinguished bituminous smell. The OS in this section is overlain by marl and chert bands and underlain by phosphorite beds at the bottom.</p></sec><sec id="s4"><title>4. Experimental Work and Methodology</title><p>Each sample was divided into three parts. One is saved as archive sample. The second was cut to prepare thin section for microscopic inspection. Twelve oil shale thin sections were prepared at the laboratories of Natural Resources Authority (NRA), Jordan. Half of each thin section was stained using staining test solution (Alizarin Red S) and then studied using the polarizing microscope. Photomicrographs of each OS type were taken using digital camera type Canon Power Shot S70. The third part of each sample was crushed by a crushing machine then further reduced down to monomineralic particles by vibrating agate ball mills. All samples were analyzed by carbon determinator (thermal conductivity detector) to indirectly estimate the quantity of organic matter in each sample. Total sulfur content (S wt%) in four selected samples was determined using the multi EA&#174;200 element analyzer available at NRA. Those samples have been tested for their oil shale retorting properties via Fischer Assay apparatus available at the NRA that determines oil, water, spent shale and gas loss in OS samples according to ISO 647 by thermal cracking method. Quantitative analysis of major oxides and trace elements was performed using X-Ray Fluorescence Spectrometer (XRF).</p></sec><sec id="s5"><title>5. Results and Discussion</title><sec id="s5_1"><title>5.1. Organic Matter Distribution</title><p>Organic matter distribution is indicated from the distribution of total organic carbon (TOC) in the studied section. The TOC &#215; 1.22 is commonly equated to total organic matter (TOM). The resulting TOM is approximate because the 1.22 factor assumes certain amounts of oxygen, nitrogen, and sulfur is present [<xref ref-type="bibr" rid="scirp.60581-ref37">37</xref>] . The TOC in the studied oil shale section ranges from 3.62 % to 20.57 %, therefore, the approximate TOM ranges from 4.42% to 25.10% respectively. The OS in some bands is of good quality as indicated from quite high values of TOM. <xref ref-type="fig" rid="fig4">Figure 4</xref> shows a rapid transition from organic-rich to organic-depleted and inverse relationship between TOC and total inorganic carbon (TIC). The approximate TOM in this type of OS is within the range of Maastrichtian OS type reported from Jordan and adjacent areas (e.g. [<xref ref-type="bibr" rid="scirp.60581-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref38">38</xref>] ).</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Depth profiles illustrate TOC distribution in the studied oil shale section</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1210399x8.png"/></fig></sec><sec id="s5_2"><title>5.2. Mineralogical and Textural Change</title><p><xref ref-type="fig" rid="fig5">Figure 5</xref> illustrates the prepared OS thin sections in relation to their TOC content. Generally, dark samples are TOC-rich and pale samples are TOC-depleted.</p><p>Under transmitted white light microscope, the TOC-depleted samples (<xref ref-type="fig" rid="fig6">Figure 6</xref>) have coarse crystalline dolomite mosaic texture. Dolomite grains are euhedral rhombs and idiomorphic. Samples show cross-cut relic microfabrics of the original carbonate with coarse replacement dolomite, carbonate overgrowth and intercrystalline porosity. The TOC-rich bands (<xref ref-type="fig" rid="fig6">Figure 6</xref>) are more laminated, composed of productivity derived and authigenic components. Samples show carbonate shell dissolution. This type contains more phosphatic particles and detrital grains. Such textural changes from TOC-rich bands to TOC-depleted bands suggest complex diagenetic history and indicate that the diagenetic processes have played a major role in the formation of this type of OS. The diagenesis is widely reported as a major factor controlled the formation of Upper Cretaceous rocks in region ( [<xref ref-type="bibr" rid="scirp.60581-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref39">39</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref40">40</xref>] , among many others).</p><p>The XRD analysis results for selected OS samples relative to their TOC content is shown in <xref ref-type="fig" rid="fig7">Figure 7</xref>. Based on relative XRD high peak data, OS samples shows major dolomite mineral phase. It is very obvious in TOC- depleted samples. The dolomatic content in high-TOC OS sample is lower than those of low-TOC samples. In addition to calcite, the highest TOC sample has minor quantities of quartz and traces of phosphate as fluorapatite, hematite, smectite and kaolinite. The later clay fraction is found only in TOC-rich samples. This suggests contribution terrigenous input. Combination the results of OS petrography with that of OS mineralogy and TOC content distribution, all suggest that there is a link between the OM content and dolomite formation. In other words, the formation of dolomite could be limited by OM content as the dolomite content decreases with increase of OM content. Dolomite decrease is associated with increase of calcite and productivity derived materials.</p></sec><sec id="s5_3"><title>5.3. Oil Shale Geochemistry</title><p>The chemistry of OS section relative to the TOC content is illustrated in <xref ref-type="fig" rid="fig8">Figure 8</xref> and <xref ref-type="fig" rid="fig9">Figure 9</xref> respectively. Detail on origin, productivity, bottom water conditions and even climate can be inferred from the distribution of major elements oxides in addition to that of minor elements. Carbonate profiles (<xref ref-type="fig" rid="fig8">Figure 8</xref>) show negative trend</p><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> The studied oil shale samples (thin sections) in relation to their TOC content</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1210399x9.png"/></fig><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Texture of all studied oil shale samples under TWLM</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1210399x10.png"/></fig><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> A series of XRD diffractograms for the studied oil shale samples in relation to their TOC content</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1210399x11.png"/></fig><fig id="fig8"  position="float"><label><xref ref-type="fig" rid="fig8">Figure 8</xref></label><caption><title> Depth profiles illustrate the distribution of major elements oxides</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1210399x12.png"/></fig><fig id="fig9"  position="float"><label><xref ref-type="fig" rid="fig9">Figure 9</xref></label><caption><title> Depth profiles illustrate the distribution of minor elements</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1210399x13.png"/></fig><p>with that of TOC. Based on petrography results; calcite is mainly found as biogenic carbonate and Mg is mainly from dolomite. Productivity indicators (e.g. P<sub>2</sub>O<sub>5</sub>) in addition to that of sulfur (<xref ref-type="fig" rid="fig1">Figure 1</xref>0) show positive distribution with that of TOC. P<sub>2</sub>O<sub>5</sub> is reported to increase with increasing productivity ( [<xref ref-type="bibr" rid="scirp.60581-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref41">41</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref42">42</xref>] ). The good correlation between the sulfur distribution and TOC distribution indicates that the majority of sulfur in this section is related to OM and therefore the sulfur is organic in origin and not diagenetic. Similar results have been reported for some OS from the region (e.g. [<xref ref-type="bibr" rid="scirp.60581-ref43">43</xref>] ). Clay and clastic input indicators profiles (e.g. Al<sub>2</sub>O<sub>3</sub>) reveal positive distribution with that of TOC. Such trend in these profiles is important in discussing the OS genesis. These indicators reported to be increase with clay input increase (e.g. [<xref ref-type="bibr" rid="scirp.60581-ref44">44</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref45">45</xref>] ).</p><p>With exception of Mn, almost all minor elements show quite similar distribution to that of TOC. Mn is considered as a redox sensitive. Low Mn indicates reduced bottom water. Mn content increases with the O<sub>2</sub> increase in bottom water [<xref ref-type="bibr" rid="scirp.60581-ref44">44</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref46">46</xref>] . Barium (Ba) and Chromium (Cr) increase with increase OM and productivity and oxygen depletion (e.g. [<xref ref-type="bibr" rid="scirp.60581-ref45">45</xref>] [<xref ref-type="bibr" rid="scirp.60581-ref47">47</xref>] ). Strontium (Sr) is associated with carbonate and used as continental weathering indicator (e.g. [<xref ref-type="bibr" rid="scirp.60581-ref48">48</xref>] ). Vanadium (V) is mainly associated with OM (e.g. [<xref ref-type="bibr" rid="scirp.60581-ref49">49</xref>] ). Copper (Cu) and Zinc (Zn) are related to sulfides and OM and they increase with increased primary productivity (e.g. [<xref ref-type="bibr" rid="scirp.60581-ref45">45</xref>] ). Overall, this section is quite rich in certain trace elements. The enrichment of Belqa Group sediments with trace elements has been attributed to direct precipitation from sea water (chemical precipitation and biogenic activity), especially sea water enriched with an exogenic metal flux leached from the Troodos and Baer Bassit ophiolites [<xref ref-type="bibr" rid="scirp.60581-ref50">50</xref>] .</p></sec><sec id="s5_4"><title>5.4. Oil Shale Quality</title><p>The quality of the OS within this horizon can be inferred from results of fisher assay analysis (<xref ref-type="fig" rid="fig1">Figure 1</xref>1), in addition to that of total S% determination that was performed on selected samples of different TOC contents (<xref ref-type="fig" rid="fig1">Figure 1</xref>0). This section show different oil yielding capacities. As the OM content increases the oil yield increase. The moisture content is relatively low. The sulfur content is related to organic matter as discussed above. One positive point for this type of OS is that the total sulfur content in OS of this section is quite low compared with sulfur content of Maastrichtian OS types. The sulfur content in the Maastrichtian OS types is quite high and reaches nearly 5% wt [<xref ref-type="bibr" rid="scirp.60581-ref1">1</xref>] . Therefore, the OS of this type is considered as potential for future utilization.</p><fig id="fig10"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>0</label><caption><title> Depth profiles illustrate the distribution of S% in four selected samples</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1210399x14.png"/></fig><fig id="fig11"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>1</label><caption><title> Fisher assay analysis results for selected OS samples</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-1210399x15.png"/></fig></sec><sec id="s5_5"><title>5.5. Oil Shale Genesis</title><p>The lamination in TOC-rich bands may indicate low oxygen concentrations. This supported with the reduced concentration of Mn which has been used by Minster et al. [<xref ref-type="bibr" rid="scirp.60581-ref46">46</xref>] as redox sensitive indicator. Combination the results of petrography, mineralogy, and geochemistry discussed previously; data suggest that the OS has been formed during period of high productivity with increase of clastic input from the continental part. Bottom water conditions have fluctuated. Periods of reduced productivity with increase of bottom water oxygenation and OM oxidation might be existed. Dolomite in TOC-depleted bands was formed by replacement of calcite under variety of conditions. Dolomitization might take place in shallow, warm, restricted Mg-rich environment within the continental shelf of Tethys Ocean under favourable pH, Eh, salinity, and temperature conditions. For the formation of dolomite, Mg might be supplied from overlying seawater, while calcium was supplied by the dissolution of calcium carbonate. The carbon was seemed to be supplied from carbonate dissolution and organic carbon oxidation. It can be suggested that under such conditions and with the availability of source materials; the dolomite has started to be originated. The rate of dolomite formation appears to be limited by the rate of calcium carbonate dissolution and organic matter oxidation.</p></sec></sec><sec id="s6"><title>6. Conclusion</title><p>Unlike oil shale from Maastrichtian to early Tertiary, this OS horizon is highly dolomitized. This OS type contains considerable content of OM. One economic potential for this types of OS is that the sulfur content is quite low compared with that of Maastrichtian OS types. This type of OS shows textural variations in both TOC-rich and TOC-depleted bands. The major rock component is dolomite with variable amounts of OM, calcite, quartz, and other minor minerals. Productivity indicators are positively distributed with OM. There is a negative correlation of organic matter content with carbonate content. The dolomite is diagenetic in origin and reveals complex diagenetic history and illustrates the importance of diagenetic alteration in the formation of this type of OS. The results of this study suggest that the formation of dolomite in this OS type appears to be limited by the rate of organic matter oxidation.</p></sec><sec id="s7"><title>Acknowledgements</title><p>The authors are thankful for the NRA staff for their assistance during the lab work.</p></sec><sec id="s8"><title>Cite this paper</title><p>Hani M.Alnawafleh,Khalid E.Tarawneh,Hani N.Khoury,Nafeth A.Abdelhadi,Osama Y.Shakkoury,Reyad A.Dwairi,Mazen N.Amaireh, (2015) Dolomitization in Campanian Oil Shale Rocks from South-Western Jordan. Open Journal of Geology,05,689-700. doi: 10.4236/ojg.2015.510061</p></sec></body><back><ref-list><title>References</title><ref id="scirp.60581-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Alali, J. and Sawaqed, S. 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