<?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">JEP</journal-id><journal-title-group><journal-title>Journal of Environmental Protection</journal-title></journal-title-group><issn pub-type="epub">2152-2197</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jep.2015.611115</article-id><article-id pub-id-type="publisher-id">JEP-61581</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>
 
 
  Characterization of Clay of the Benin Used in Ruminale Feeding. Complete Determination of the Smectites Contained in These Clays
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>tienne</surname><given-names>Sagbo</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>Marielle</surname><given-names>Agbahoungbata</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>Wilfried</surname><given-names>Kangbode</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>Arthur</surname><given-names>Cakpo</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>Jacques</surname><given-names>Kinlehoume</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>Jean-Baptise</surname><given-names>Mensah</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>Yves</surname><given-names>Noack</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Laboratoire de Chimie Théoriqueet de Spectroscopie Moléculaire (LACTHESMO), Faculté des Sciences et 
Techniques (FAST), Universitéd’ Abomey-Calavi, Cotonou, Bénin</addr-line></aff><aff id="aff3"><addr-line>Centre Européen de Rechercheetd’ Enseignementen Géosciences de L’Environnement (CEREGE), 
Universitéd’Aix Marseille, AIX en Provence, France</addr-line></aff><aff id="aff1"><addr-line>Laboratoire de ChimieInorganiqueet de l’Environnement (LaCIE), Faculté des Sciences et Techniques (FAST), Universitéd’ Abomey-Calavi, Cotonou, Bénin</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>esagbo@yahoo.fr(TS)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>12</day><month>11</month><year>2015</year></pub-date><volume>06</volume><issue>11</issue><fpage>1322</fpage><lpage>1336</lpage><history><date date-type="received"><day>31</day>	<month>August</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>27</month>	<year>November</year>	</date><date date-type="accepted"><day>30</day>	<month>November</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>
 
 
  In this work, by the use of several physico-chemical complementary methods for the characterization of soil (diffraction of x-rays, chemical analysis, density, cationic exchange capacity, specific sur faces, m?ssbauer, granulometry, etc.), the smectite of the three clayey localities of Benin (Gb&#233;dji-Kotovi, Massi-S&#232;hou&#232; and Zogbodomey) was notably studied. Thus, these three sites principally contain principally smectite, kaolinite and quartz in variable proportion. This smectite is a beidellite. Its chemical formula is proposed. The specific surfaces and the cationic exchange capacity of the samples are determined. For these samples, the fraction lower than 2 μm is practically beidellitic for Gb&#233;dji-Kotovi and Massi-S&#232;hou&#232; (more than 82% of beidellite) and practically kaolinitic (70% of kaolinite) for Zogbodomey. So, used as additive food to ruminant, the clay of Gb&#233;dji-Kotovi and Massi-S&#232;hou&#232; will induce an enteric reduction of methane more than clay of Zogbodomey. 
 
</p></abstract><kwd-group><kwd>Clay</kwd><kwd> Characterization</kwd><kwd> Beidellite</kwd><kwd> Formula</kwd><kwd> B&#233;nin</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In order to optimize digestion of ruminants and reduce the emission of the enteric methane which constitutes a loss of energy for the animal and an economic loss for the cattle breeders [<xref ref-type="bibr" rid="scirp.61581-ref1">1</xref>] , it is incorporated in the B&#233;nin clay in ruminale feeding. Indeed, clay is well known for its specific surface, its capacity of cationic exchange and its richness in necessary cations for ruminale feeding [<xref ref-type="bibr" rid="scirp.61581-ref2">2</xref>] .</p><p>The clayey samples which are used are taken in the south of the B&#233;nin.The characteristics of these clays previously were the object of some rare chemical analyses and studies with x-rays [<xref ref-type="bibr" rid="scirp.61581-ref3">3</xref>]. Thereafter, it was given some characteristics of total fractions of these clays [<xref ref-type="bibr" rid="scirp.61581-ref4">4</xref>]. Then, the good knowledge of the characteristics (compositions and properties) of the argillaceous fractions used, and especially of the smectites contained in these samples will make possible to improve the hoped outputs. It is accordingly that, this study is accomplished by combining several methods (diffraction of x-rays, the chemical analysis, the density, the cationic capacity of exchange, the exchangeable bases, specific surfaces granulometry and M&#246;ssbauer, etc.). This work will make possible to select clays which are likely to involve a clear reduction of enteric methane and to fatten animals.</p></sec><sec id="s2"><title>2. Materials and Methods</title><sec id="s2_1"><title>2.1. Materials</title><p>Located in the south-west of the Benin between meridians 1˚40'E and 2˚45'E and parallels 6˚15'N and 7˚30'N, the basin where the samples were took belongs to the basins of the Gulf of Guinea (<xref ref-type="fig" rid="fig1">Figure 1</xref>) The pluviometric annual average is there of 1200 mm. Temperature varies around 29˚C and the vegetation is presented in the form of arboreous savanna. On the geomorphological level, this basin includes two zones (<xref ref-type="fig" rid="fig2">Figure 2</xref>): A zone of 7 platetaux limited by the valleys of the main rivers (Ou&#233;m&#233;, S&#244;, Couffo and Mono) and the depression of Lama. They are the plateaux of Aplahou&#233;, of Abomey, of Zagnanado and of K&#233;tou and those of Com&#233;, of Allada and of Saket&#233; and a zone of low plain constituting a margino-coastal domain occupied by marshy depressions, lagoons (lagoon of Porto Novo, coastal lagoon), sand cords and lakes (lake Ah&#233;m&#233;, lake Nokou&#233;). On geological level, this basin is of cretaceous age to pr&#233;sent. Il contain gritty, sandy, argillaceous and calcareous formations [<xref ref-type="bibr" rid="scirp.61581-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.61581-ref6">6</xref>] .</p><p>The studied materials come from deposits of Gbedji-Kotovi (GK), of Massi-S&#232;hou&#232; (MS), and of Zogbodomey (ZY).These sites are represented on the <xref ref-type="fig" rid="fig2">Figure 2</xref>. The 1st site (GK) prospected is between longitude 2˚00'E and 2˚02E, and between latitude 6˚40'N and 6˚42'N. The relief is there slightly undulating there .The studied deposit (during dry season) is in the bed of the river Couffo. Ten wells of 1m of diameter and of 5 m of maximum depth are dug there in the stitch of 100 m (<xref ref-type="table" rid="table1">Table 1</xref>). Globally the clay, of black grey colour with by place of tasks rusts, is very plastic. The 2nd site (MS) is between 2˚13'E and 2˚16'E, between 6˚57'N and 6˚59'N in the depression of Lama. The relief, here, is generally flat. 10 wells in the stitch of 100m and of maximum depth 5 m mostly and sometimes 7 m are explored here (<xref ref-type="table" rid="table1">Table 1</xref>). The clay is plastic and in general of Belgian grey colour. When to 3rd site (ZY) it also presents, with a light slope towards the east, a flat and monotonous relief between 2˚06'E and 2˚08'E and between 7˚04'N and 7˚06'N. This zone is to the bottom of the plate of Abomey; 6 wells in bulk, of maximum depth 7 m are exploited there (<xref ref-type="table" rid="table1">Table 1</xref>).</p><p>In general, clay appears only after one lateritic layer of 2 to 3 m. It is initially white with red passages (zone of transition), then white with yellow passages and of the red tasks. The precise geographical co-ordinates of wells were raised with the aid of a positioning system by portable satellite of type G.P.S (Global Positioning System) and regrouped in <xref ref-type="table" rid="table1">Table 1</xref>.</p><p>According to later results (KANGBODE), the major crystalline phases contained in all the total samples are the following minerals: kaolinite (K): Al<sub>2</sub>Si<sub>2</sub>O<sub>5</sub>(OH)<sub>4</sub> (7.14 &#197;; 3.56 &#197;), quartz (Q): 1.81 &#197;; 4.26 &#197;.) [<xref ref-type="bibr" rid="scirp.61581-ref7">7</xref>] , smectite (S): (Ca, Mg)(Al, Fe)<sub>2</sub>(Si, Al)O<sub>10</sub>(OH)<sub>2</sub> (14 - 15 &#197;) [<xref ref-type="bibr" rid="scirp.61581-ref8">8</xref>] and like phase trace the anatase (A): TiO<sub>2</sub> (3.52 &#197;; 1.89 &#197;). There are also feldspar traces (Na, K, Ca) (Al, Fe, Si)<sub>4</sub>O<sub>8</sub> (3.18 - 3.33 &#197;; 4.02 - 4.25 &#197;) for the samples of Gbedji-Kotovi and particularly for GSO<sub>1/2</sub> and goethite (G) α-FeOOH (4.18 &#197;; 2.49 &#197;) for the samples of Zogbodomey.</p><p>The samples coming from the same site present the same ores showing of this fact the homogeneity of each site. What enabled us to choose there after a representative sample by locality for certain analyses with GNE1 (G), its fraction fine or normal GNEIN (GN) and saturated with glycol GNEIG for GBEDJI-KOTOVI (GK), and with respectively MNO1 (M), MNOIN (MN) and MNOIG for Sehoue-Massi (MS) and ZTII2 (Z), ZTI2N (ZN) and ZTI2G for Zogbodomey (ZY).</p></sec><sec id="s2_2"><title>2.2. Methods</title><p>The argillaceous fraction lower than 2 μm of diameter is obtained by purification and sedimentation. This fine</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Card of g&#233;ographical situation of Benin (IHETA et al., 1983)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x7.png"/></fig><p>fraction, dried and finely crushed allowed to prepare oriented pastes on natural trial and having undergone specific treatments (Ethylene glycol, Hydrazine, heating during 4 hours at 490˚C). These oriented pastes were subjected to diffraction x-rays on powder. The diffractograms were recorded using a Philips diffractometer equipped with a generator PW 1800 with graphite monochromator, using the radiation of cobalt and functioning under 40 Kv, 40 mA. They were acquired by data APD and were treated by the software X’ PERT &amp; IDENTIFY and X’ PERT High Score Plus. The results obtained by DRX are supplemented by the elementary chemical analyses. It is about an atomic spectrophotometer of emission by coupling of inductive plasma (I.C P./AES) Jobin Yvon of the mark Ultima C V5 which makes it possible to proportion the chemical elements constitutive of argillaceous material. The granulometric analysis was carried out on the fine grounds of diameter D lower than 500 μm using a laser particle-measurement instrument MALVERN of the type MATERSIZER. Specific surfaces were given from the analysis of the isotherm of adsorption of a gas by the solid by using the method of Brunauer,</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Geomorphological card of the coastal basin of the Benin (Slansky, 1962)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x8.png"/></fig><p>Emmett and Teller (B.E.T.). The measurement of the CEC by the method of Aubert [<xref ref-type="bibr" rid="scirp.61581-ref9">9</xref>] , was done on the total rock. For the infrared spectroscopy, after a mixture (2% in mass approximately) with of KBr (average IR) or polyethylene (remote IR), the samples, (fine fraction &lt; 2 &#181;m) are put in pastilles of diameter of 13 mm and of thickness of about 0.4 mm. Measurements were carried out in the field of the average infra-red between 400 cm<sup>−1</sup> and 4000 cm<sup>−1</sup> using a spectrometer with Fourier transform of the type PERKIN ELMER (model 1760X), provided with a software of automatic processing data. In the remote infra-red (between 50 cm<sup>−1</sup> and 400 cm<sup>−1</sup>), the spectra IR were recorded with a spectrometer BONEM D.A.8 with Fourier transform Moreover for M&#246;ssbauer our samples were analyzed in transmission using a standard Spectrometer EG &amp; G assembly equipped with a 57Co source (Rh). The rate of travel was gauged by reference to the sextuplet recorded starting from a pure sheet of Fe. The values of displacement are referred compared to the center of the spectrum, for a zero value of acceleration. The absorbing material was prepared with crushed clay 1.5 g approximately, inserted in a support surrounded by lead. The spectra, by using the Lorentzian, were calculated with the program ISO [<xref ref-type="bibr" rid="scirp.61581-ref10">10</xref>] . Isometric displacements are given compared to metal iron. The refinements were controlled by the test χ<sup>2</sup>.</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Localization of the samples</title></caption><table><tbody><thead><tr><th align="center" valign="middle"  colspan="4"  >Clays of Gbedji-Kotovi</th><th align="center" valign="middle"  colspan="3"  >Clays of Zogbodomey</th><th align="center" valign="middle"  colspan="3"  >Clays of Sehoue-Massi</th></tr></thead><tr><td align="center" valign="middle" >Number of Wells</td><td align="center" valign="middle" >Coordinates by GPS</td><td align="center" valign="middle" >Samples</td><td align="center" valign="middle" >Depth (m)</td><td align="center" valign="middle" >Coordinates by GPS</td><td align="center" valign="middle" >Samples</td><td align="center" valign="middle" >Depth (m)</td><td align="center" valign="middle" >Coordinates by GPS</td><td align="center" valign="middle" >Samples</td><td align="center" valign="middle" >Depth (m)</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >1</td><td align="center" valign="middle"  rowspan="2"  >N 06˚41.084' E 002˚01000'</td><td align="center" valign="middle" >GNO1</td><td align="center" valign="middle" >0.2</td><td align="center" valign="middle"  rowspan="2"  >N 07˚04025' E 002˚07326'</td><td align="center" valign="middle"  rowspan="2"  >ZPO</td><td align="center" valign="middle"  rowspan="2"  >3</td><td align="center" valign="middle"  rowspan="2"  >N 06˚57602' E 002˚15249'</td><td align="center" valign="middle" >MNO1</td><td align="center" valign="middle" >0.05</td></tr><tr><td align="center" valign="middle" >GNO2</td><td align="center" valign="middle" >4.5</td><td align="center" valign="middle" >MNO2</td><td align="center" valign="middle" >5</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >2</td><td align="center" valign="middle"  rowspan="2"  >N 06˚41049' E 002˚00965'</td><td align="center" valign="middle" >GO1</td><td align="center" valign="middle" >0.2</td><td align="center" valign="middle"  rowspan="2"  >N 07˚04051' E 002˚06170'</td><td align="center" valign="middle" >ZPI1</td><td align="center" valign="middle" >2.95</td><td align="center" valign="middle"  rowspan="2"  >N 06˚57476' E 002˚15198'</td><td align="center" valign="middle" >MO1</td><td align="center" valign="middle" >0.12</td></tr><tr><td align="center" valign="middle" >GO2</td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >ZPI2</td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >MO2</td><td align="center" valign="middle" >1.82</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >3</td><td align="center" valign="middle"  rowspan="2"  >N 06˚41010' E 002˚00928'</td><td align="center" valign="middle" >GSO1</td><td align="center" valign="middle" >0.5</td><td align="center" valign="middle"  rowspan="2"  >N 07˚05022' E 002˚06309'</td><td align="center" valign="middle" >ZPII1</td><td align="center" valign="middle" >2.95</td><td align="center" valign="middle"  rowspan="2"  >N 06˚57429' E 002˚15232'</td><td align="center" valign="middle" >MSO1</td><td align="center" valign="middle" >0.15</td></tr><tr><td align="center" valign="middle" >GSO2</td><td align="center" valign="middle" >1.2</td><td align="center" valign="middle" >ZPII2</td><td align="center" valign="middle" >7</td><td align="center" valign="middle" >MSO2</td><td align="center" valign="middle" >5</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >4</td><td align="center" valign="middle"  rowspan="2"  >N 06˚41084' E 002˚01062'</td><td align="center" valign="middle" >GNN1</td><td align="center" valign="middle" >0.25</td><td align="center" valign="middle"  rowspan="2"  >N 07˚04148' E 002˚07170'</td><td align="center" valign="middle" >ZPIII1</td><td align="center" valign="middle" >3</td><td align="center" valign="middle"  rowspan="2"  >N 06˚57325' E 002˚15317'</td><td align="center" valign="middle" >MSSO1</td><td align="center" valign="middle" >0.05</td></tr><tr><td align="center" valign="middle" >GNN2</td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >ZPIII2</td><td align="center" valign="middle" >7</td><td align="center" valign="middle" >MSSO2</td><td align="center" valign="middle" >2.6</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >5</td><td align="center" valign="middle"  rowspan="2"  >N 06˚40985' E 002˚00995'</td><td align="center" valign="middle" >GN1</td><td align="center" valign="middle" >0.20</td><td align="center" valign="middle"  rowspan="2"  >N 07˚04821' E 002˚06176'</td><td align="center" valign="middle" >ZTI1</td><td align="center" valign="middle" >2.95</td><td align="center" valign="middle"  rowspan="2"  >N 06˚57556' E 002˚15204'</td><td align="center" valign="middle" >MN1</td><td align="center" valign="middle" >0.12</td></tr><tr><td align="center" valign="middle" >GN2</td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >ZTI2</td><td align="center" valign="middle" >6.2</td><td align="center" valign="middle" >MN2</td><td align="center" valign="middle" >5</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >6</td><td align="center" valign="middle"  rowspan="2"  >N 06˚40958' E 002˚00950'</td><td align="center" valign="middle" >GC1</td><td align="center" valign="middle" >0.25</td><td align="center" valign="middle"  rowspan="2"  >N 07˚04936' E 002˚06294'</td><td align="center" valign="middle" >ZTII1</td><td align="center" valign="middle" >3.05</td><td align="center" valign="middle"  rowspan="2"  >N 06˚57515' E 002˚15245'</td><td align="center" valign="middle" >MC1</td><td align="center" valign="middle" >0.42</td></tr><tr><td align="center" valign="middle" >GC2</td><td align="center" valign="middle" >5</td><td align="center" valign="middle" >ZTII2</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >MC2</td><td align="center" valign="middle" >5</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >7</td><td align="center" valign="middle"  rowspan="2"  >N 06˚40988' E 002˚01051'</td><td align="center" valign="middle" >GS1</td><td align="center" valign="middle" >0.20</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle"  rowspan="2"  >N 06˚57464' E 002˚15280'</td><td align="center" valign="middle" >MS1</td><td align="center" valign="middle" >0.4</td></tr><tr><td align="center" valign="middle" >GS2</td><td align="center" valign="middle" >5</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >MS2</td><td align="center" valign="middle" >5</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >8</td><td align="center" valign="middle"  rowspan="2"  >N 06˚40958' E 002˚00950'</td><td align="center" valign="middle" >GNE1</td><td align="center" valign="middle" >0.20</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle"  rowspan="2"  >N 06˚57602' E 002˚15107'</td><td align="center" valign="middle" >MNE1</td><td align="center" valign="middle" >0.05</td></tr><tr><td align="center" valign="middle" >GNE2</td><td align="center" valign="middle" >5</td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" >MNE2</td><td align="center" valign="middle" >5</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >9</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"  rowspan="2"  >N 06˚57556' E 002˚15289'</td><td align="center" valign="middle" >ME1</td><td align="center" valign="middle" >0.15</td></tr><tr><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" >ME2</td><td align="center" valign="middle" >4.5</td></tr><tr><td align="center" valign="middle"  rowspan="2"  >10</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"  rowspan="2"  >N 06˚58747' E 002˚13817'</td><td align="center" valign="middle" >MT1</td><td align="center" valign="middle" >4</td></tr><tr><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" >MT2</td><td align="center" valign="middle" >7</td></tr></tbody></table></table-wrap></sec></sec><sec id="s3"><title>3. Results and Discussion</title><sec id="s3_1"><title>3.1. Estimate of Quantitive Composition of Clayey Minerals</title><p>This quantification is based on the evaluation of surfaces of the peaks, of the harmonic reflections (00l), of argil laceous minerals on the diffractogram of the treatment ethylene glycol. They are the peaks with 17.10 and 7 &#197; respectively of the smectite, the illite and kaolinite. Surfaces obtained are brought back to a total of 100% [<xref ref-type="bibr" rid="scirp.61581-ref11">11</xref>] . The use of the diffractogram of the treatment glycol is justified by the fact that, our samples not comprising a chlorite, there is no overlap compared to the reflections of argillaceous minerals. Moreover, the estimate based on the surface of the peaks makes it possible to minimize the errors caused by the variation of the crystallinity of the samples. Indeed a low crystallinity would cause changes in the intensity of the peaks, but not of their surface [<xref ref-type="bibr" rid="scirp.61581-ref12">12</xref>] . The approximate mineralogical compositions of some of these samples were determined and are deferred in <xref ref-type="table" rid="table2">Table 2</xref>.</p><p>One can conclude that GN and MN contain on average, more smectite (respectively 82.46%, 92.22%) than kaolinite (respectively 15.77% and 7%) contrary to ZN (28.40% of smectite, 70.93% of kaolinite) <xref ref-type="fig" rid="fig3">Figure 3</xref> and <xref ref-type="table" rid="table2">Table 2</xref>. These fine fractions are enough good quality because a good part of quartz was eliminated by sedimentation <xref ref-type="fig" rid="fig3">Figure 3</xref>, <xref ref-type="fig" rid="fig4">Figure 4</xref>.</p></sec><sec id="s3_2"><title>3.2. Determination of the Nature of the Smectites: The Test of Hoffmann Then of Grenne-Kelly</title><p>For our samples the rate of iron (<xref ref-type="table" rid="table3">Table 3</xref>), on average of 7.5% allows to move aside the nontronite whose minimal content of ironis of 15% [<xref ref-type="bibr" rid="scirp.61581-ref7">7</xref>] . The test of Hoffmann [<xref ref-type="bibr" rid="scirp.61581-ref13">13</xref>] then of Grenne-Kelly [<xref ref-type="bibr" rid="scirp.61581-ref14">14</xref>] (saturation with Li,</p><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Quantitative composition of the argillaceous minerals of fraction &lt; 2 &#181;m</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Samples Saturated with Glycol</th><th align="center" valign="middle" >% Smectite</th><th align="center" valign="middle" >% Kaolinite</th><th align="center" valign="middle" >% Illite</th><th align="center" valign="middle" >% Quartz</th></tr></thead><tr><td align="center" valign="middle" >GC1G</td><td align="center" valign="middle" >89.13</td><td align="center" valign="middle" >9.84</td><td align="center" valign="middle" >Traces</td><td align="center" valign="middle" >1.03</td></tr><tr><td align="center" valign="middle" >GC2G</td><td align="center" valign="middle" >84.76</td><td align="center" valign="middle" >14.17</td><td align="center" valign="middle" >‘’</td><td align="center" valign="middle" >1.07</td></tr><tr><td align="center" valign="middle" >GNEIG</td><td align="center" valign="middle" >76,74</td><td align="center" valign="middle" >20.48</td><td align="center" valign="middle" >“</td><td align="center" valign="middle" >2.27</td></tr><tr><td align="center" valign="middle" >GNIG</td><td align="center" valign="middle" >77.30</td><td align="center" valign="middle" >20.07</td><td align="center" valign="middle" >“</td><td align="center" valign="middle" >2.63</td></tr><tr><td align="center" valign="middle" >GSO1G</td><td align="center" valign="middle" >84.37</td><td align="center" valign="middle" >15.01</td><td align="center" valign="middle" >“</td><td align="center" valign="middle" >0.62</td></tr><tr><td align="center" valign="middle" >GSO2G</td><td align="center" valign="middle" >82.47</td><td align="center" valign="middle" >15.02</td><td align="center" valign="middle" >“</td><td align="center" valign="middle" >2.51</td></tr><tr><td align="center" valign="middle" >Average GN</td><td align="center" valign="middle" >82.46</td><td align="center" valign="middle" >15.77</td><td align="center" valign="middle" >Traces</td><td align="center" valign="middle" >1.69</td></tr><tr><td align="center" valign="middle" >ME1G</td><td align="center" valign="middle" >82.01</td><td align="center" valign="middle" >17.70</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >0.29</td></tr><tr><td align="center" valign="middle" >MNIG</td><td align="center" valign="middle" >92.31</td><td align="center" valign="middle" >7.23</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >0.46</td></tr><tr><td align="center" valign="middle" >MNOIG</td><td align="center" valign="middle" >97.32</td><td align="center" valign="middle" >2.26</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >0.42</td></tr><tr><td align="center" valign="middle" >MO2G</td><td align="center" valign="middle" >98.74</td><td align="center" valign="middle" >0.87</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >0.39</td></tr><tr><td align="center" valign="middle" >MSG</td><td align="center" valign="middle" >90.72</td><td align="center" valign="middle" >6.94</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >2.34</td></tr><tr><td align="center" valign="middle" >Average MN</td><td align="center" valign="middle" >92.22</td><td align="center" valign="middle" >7</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >0.78</td></tr><tr><td align="center" valign="middle" >ZPI1 G</td><td align="center" valign="middle" >29.83</td><td align="center" valign="middle" >69.78</td><td align="center" valign="middle" >Traces</td><td align="center" valign="middle" >0.39</td></tr><tr><td align="center" valign="middle" >ZPI2G</td><td align="center" valign="middle" >28.86</td><td align="center" valign="middle" >70.84</td><td align="center" valign="middle" >“</td><td align="center" valign="middle" >0.30</td></tr><tr><td align="center" valign="middle" >ZPII1G</td><td align="center" valign="middle" >10.65</td><td align="center" valign="middle" >87.33</td><td align="center" valign="middle" >“</td><td align="center" valign="middle" >2.022</td></tr><tr><td align="center" valign="middle" >ZPOG</td><td align="center" valign="middle" >32.09</td><td align="center" valign="middle" >67.47</td><td align="center" valign="middle" >“</td><td align="center" valign="middle" >0.44</td></tr><tr><td align="center" valign="middle" >ZTI2G</td><td align="center" valign="middle" >29.93</td><td align="center" valign="middle" >69.64</td><td align="center" valign="middle" >“</td><td align="center" valign="middle" >0.43</td></tr><tr><td align="center" valign="middle" >ZTII1G</td><td align="center" valign="middle" >39.06</td><td align="center" valign="middle" >60.53</td><td align="center" valign="middle" >“</td><td align="center" valign="middle" >0.41</td></tr><tr><td align="center" valign="middle" >Average ZN</td><td align="center" valign="middle" >28.40</td><td align="center" valign="middle" >70.93</td><td align="center" valign="middle" >Traces</td><td align="center" valign="middle" >0.67</td></tr></tbody></table></table-wrap><table-wrap id="table3" ><label><xref ref-type="table" rid="table3">Table 3</xref></label><caption><title> Elementary chemical composition of the samples Massi, Zogbodomey, Gbedji- Kotovi and Sehoue-Massi</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Samples Elements</th><th align="center" valign="middle" >MNO1</th><th align="center" valign="middle" >MNO1N</th><th align="center" valign="middle" >GNE1</th><th align="center" valign="middle" >GNE1N</th><th align="center" valign="middle" >ZTI2</th><th align="center" valign="middle" >ZTI2N</th></tr></thead><tr><td align="center" valign="middle" >SiO<sub>2</sub></td><td align="center" valign="middle" >54.84</td><td align="center" valign="middle" >47.5</td><td align="center" valign="middle" >45.58</td><td align="center" valign="middle" >44.8</td><td align="center" valign="middle" >52.67</td><td align="center" valign="middle" >43.53</td></tr><tr><td align="center" valign="middle" >Al<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >16.75</td><td align="center" valign="middle" >22.02</td><td align="center" valign="middle" >21.13</td><td align="center" valign="middle" >21.58</td><td align="center" valign="middle" >21.07</td><td align="center" valign="middle" >28.88</td></tr><tr><td align="center" valign="middle" >Fe<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >7.11</td><td align="center" valign="middle" >8.49</td><td align="center" valign="middle" >9.61</td><td align="center" valign="middle" >8.18</td><td align="center" valign="middle" >11.25</td><td align="center" valign="middle" >7.34</td></tr><tr><td align="center" valign="middle" >MgO</td><td align="center" valign="middle" >1.51</td><td align="center" valign="middle" >1.91</td><td align="center" valign="middle" >1.72</td><td align="center" valign="middle" >1.8</td><td align="center" valign="middle" >0.45</td><td align="center" valign="middle" >1.46</td></tr><tr><td align="center" valign="middle" >CaO</td><td align="center" valign="middle" >1.1</td><td align="center" valign="middle" >1.25</td><td align="center" valign="middle" >0.87</td><td align="center" valign="middle" >0.88</td><td align="center" valign="middle" >0.3</td><td align="center" valign="middle" >0.48</td></tr><tr><td align="center" valign="middle" >Na<sub>2</sub>O</td><td align="center" valign="middle" >0.01</td><td align="center" valign="middle" >0.062</td><td align="center" valign="middle" >0.2</td><td align="center" valign="middle" >0.12</td><td align="center" valign="middle" >0.06</td><td align="center" valign="middle" >0.09</td></tr><tr><td align="center" valign="middle" >K<sub>2</sub>O</td><td align="center" valign="middle" >0.01</td><td align="center" valign="middle" >0.09</td><td align="center" valign="middle" >0.48</td><td align="center" valign="middle" >0.65</td><td align="center" valign="middle" >0.27</td><td align="center" valign="middle" >0.44</td></tr><tr><td align="center" valign="middle" >TiO<sub>2</sub></td><td align="center" valign="middle" >1.09</td><td align="center" valign="middle" >1.15</td><td align="center" valign="middle" >1.34</td><td align="center" valign="middle" >1.22</td><td align="center" valign="middle" >1.46</td><td align="center" valign="middle" >1.34</td></tr><tr><td align="center" valign="middle" >P<sub>2</sub>O<sub>5</sub></td><td align="center" valign="middle" >0.07</td><td align="center" valign="middle" >0.08</td><td align="center" valign="middle" >0.06</td><td align="center" valign="middle" >0.05</td><td align="center" valign="middle" >0.05</td><td align="center" valign="middle" >0.10</td></tr><tr><td align="center" valign="middle" >LOI</td><td align="center" valign="middle" >17.12</td><td align="center" valign="middle" >18.03</td><td align="center" valign="middle" >19.36</td><td align="center" valign="middle" >20.8</td><td align="center" valign="middle" >12.44</td><td align="center" valign="middle" >15.96</td></tr><tr><td align="center" valign="middle" >TOTAL</td><td align="center" valign="middle" >99.61</td><td align="center" valign="middle" >100.58</td><td align="center" valign="middle" >100.35</td><td align="center" valign="middle" >100.08</td><td align="center" valign="middle" >100.02</td><td align="center" valign="middle" >99.62</td></tr></tbody></table></table-wrap><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> The diffractogram of the treatment ethylene glycol</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x9.png"/></fig><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Diffractograms of fine (normal) fractions</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x10.png"/></fig><p>heating at 250˚C one night, then saturation with ethylene glycol) allows to differentiate in the dioctaedric smectites, montmorillonites of the beidellites. smectitetake place then between 12 and 13 &#197;. Then, one heats at approximately 300˚C during one night the saturated smectite. Lithium migrates in octahedral position, thus cancelling the octahedral charges. Afterwards exchange of Li and heating, the oriented preparations of the smectites give to the X-ray a peak between 9 and 10 &#197;. After having added glycol, the beidellites which have moreover a tetrahedral charge will pass to 17&#197; because they can still fix ethylene glycol molecules. On the other hand montmorillonites which do not have any more octahedral charges and not having tetrahedral charges initially, cannot fix any ethylene glycol and will remain between 9 and 10 &#197; [<xref ref-type="bibr" rid="scirp.61581-ref15">15</xref>] . Practically the difficulty consists in exchanging the smectites with lithium. Lithium takes with difficulty the place of the other ions in interfoliaceous position and if little lithium penetrates in the smectite then, the octahedral charges all are not neutralized. Thus the test loses all its significance. To be certain that the exchange was well made, it is necessary in each series, to treat a montmorillonite standard at the same time, as witness [<xref ref-type="bibr" rid="scirp.61581-ref16">16</xref>] . The diffractograms obtained for this purpose are regrouped on Figures 5-8.</p><p>On <xref ref-type="fig" rid="fig5">Figure 5</xref>, normal montmorillonite (reference MTMN) is to 12.62 &#197;. Saturated with lithium, it (MTMLN) passes to 12.40 &#197;. Then heated, it (MTMLC) is reduced to 9.8 &#197;, value that montmorillonite keeps even after addition glycol thereafter (MTMLCG) On <xref ref-type="fig" rid="fig6">Figure 6</xref> the smectite of GNEI of the normal fraction (GNEIN) is at 15 &#197;. Saturated with lithium (GNEILN), it is at 12.40 &#197;, then heated (GNEILC) it passes to 10 to find 17 &#197; after addition glycol (GNEILCG). GNEILCG contrary to the montmorillonite remains with 9.80 &#197;. One concludes from it that the smectite of GBEDJI-KOTOVI is well a beidellite. By considering the diffractograms contained in <xref ref-type="fig" rid="fig7">Figure 7</xref> and <xref ref-type="fig" rid="fig8">Figure 8</xref> relating to sample MNO1 of Sehoue-Massi and sample ZTII2 of Zogbodomey,</p><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Diffractograms of clayey fractions treated of Montm- orillonite reference</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x11.png"/></fig><fig id="fig6"  position="float"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Diffractograms of treated samples GNE1</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x12.png"/></fig><fig id="fig7"  position="float"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> Diffractogramsof treated samples MNO1</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x13.png"/></fig><fig id="fig8"  position="float"><label><xref ref-type="fig" rid="fig8">Figure 8</xref></label><caption><title> Diffractogramsof treated samples MNO1</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x14.png"/></fig><p>one thus leads to the same observations with the same conclusion with knowing that the smectites of the studied samples are beidellites.</p></sec><sec id="s3_3"><title>3.3. Determination of the Origin of Smectites: Test of Behaviour with the Potassium</title><p>This determination by diffraction of X-rays, was carried out on the fine fraction (normal) and the fine fraction saturated with potassium with a representative sample of each site thus G, M and Z. he behavior of minerals 2/1 saturated with potassium bring several information on their properties [<xref ref-type="bibr" rid="scirp.61581-ref17">17</xref>] . It allows particularly to distinguish the smectites of transformation (resulting from the micas) of the true smectites (newly formed or neogenetic) [<xref ref-type="bibr" rid="scirp.61581-ref11">11</xref>] , [<xref ref-type="bibr" rid="scirp.61581-ref15">15</xref>] . Indeed it is well-known that not very hydratable cations like K, whose diameter corresponds approximately to This causes the contraction of mineral towards 10 &#197; what one calls the “retrogradation of potassium”, this cation becoming not easily exchangeable then and especially for the smectites of transformation. For the true smectites closing to 10 &#197; generally does not intervene and their interfoliaceous distances are between 12 &#197; and 15 &#197; [<xref ref-type="bibr" rid="scirp.61581-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.61581-ref18">18</xref>] . The diffractograms obtained are recorded on <xref ref-type="fig" rid="fig9">Figure 9</xref>.</p><p>For GNE1, the peak at 15 &#197; of fine fraction (GNE1N or G normal) is replaced with two peaks of the fraction saturated with potassium (G-K) at 13 &#197; and at 10.2 &#197; (<xref ref-type="fig" rid="fig9">Figure 9</xref>), corresponding respectively to the presence of a true smectite and of a smectite of transformation. This is explained by the fact that this sample is in the bed of a river which receives a bit from everything. For MNO1, the peak at 14.7 &#197; of its fine part (MNO1N or M normal) is towards 12.7 &#197; with (M-K) its part saturated with K. We are in the presence of a true, neoformed smectite by the ions accumulated in the depression of the LAMA. Lastly, with its fine fraction (ZTI2N or Z normal), ZTI2 has a peak towards 15 &#197; which moves at 10 &#197; while becoming Z-K ( saturated with potassium) because of closing due to the saturation with K (<xref ref-type="fig" rid="fig9">Figure 9</xref>). Indeed its smectite is of transformation resulting from the mica probably coming from deterioration from the granite, because ZTI2 come from Zogbodomey which is beside of the base granito-migmatic.</p></sec><sec id="s3_4"><title>3.4. Elementary Chemical Analysis</title><p>The chemical analysis gave the results gathered in <xref ref-type="table" rid="table3">Table 3</xref> and <xref ref-type="table" rid="table4">Table 4</xref>. Quantitatively the samples contain all mainly the oxides SiO<sub>2</sub> (43.5% - 54.8%) and Al<sub>2</sub>O<sub>3</sub> (16.7% - 28.9%). Follow-up in the minority of Fe<sub>2</sub>O<sub>3</sub> or and FeO (7.1% - 11.2%), and of TiO<sub>2</sub> (1.09% - 1.5%) and according to each site of Na<sub>2</sub>O, P<sub>2</sub>O<sub>5</sub> of MgO of CaO and K<sub>2</sub>O in variable quantity. The chemical analyses correctly translate the results of the analysis by diffraction of the X-ray. They show indeed that the samples contain all, a content of (SiO<sub>2</sub> + Al<sub>2</sub>O<sub>3</sub>) ranging between 66.4 and 71.6. They are thus essentially silico-aluminous minerals with prevalence of SiO<sub>2</sub>.</p><p>The relationship α = SiO<sub>2</sub>/Al<sub>2</sub>O<sub>3</sub> about total fraction, variable between 2.2 and 3.3 (<xref ref-type="table" rid="table4">Table 4</xref>) is quite characteristic of argillaceous minerals. These values largely higher than 1.1, that of standard kaolinite [<xref ref-type="bibr" rid="scirp.61581-ref19">19</xref>] confirm the presence of free silica (quartz, amorphous silica…) and other argillaceous minerals detected with the X-ray.</p><fig id="fig9"  position="float"><label><xref ref-type="fig" rid="fig9">Figure 9</xref></label><caption><title> Diffractograms of fine (normal) fractions and fractions saturated with the potassium</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x15.png"/></fig><table-wrap id="table4" ><label><xref ref-type="table" rid="table4">Table 4</xref></label><caption><title> Rapportsα and of β for samples of Zogbodomey, Gb&#233;dji-Kotovi and Sehoue-Massi</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Samples Rapports α and β</th><th align="center" valign="middle" >MNO1</th><th align="center" valign="middle" >MNO1N</th><th align="center" valign="middle" >GNE1</th><th align="center" valign="middle" >GNE1N</th><th align="center" valign="middle" >ZTI2</th><th align="center" valign="middle" >ZTI2N</th></tr></thead><tr><td align="center" valign="middle" >α = SiO<sub>2</sub>/Al<sub>2</sub>O<sub>3</sub></td><td align="center" valign="middle" >3,3</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >2,2</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >2,5</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" >β = SiO<sub>2</sub>/ (Al<sub>2</sub>O<sub>3</sub> + Fe<sub>2</sub>O<sub>3</sub>)</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >1,6</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >1,5</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >1,2</td></tr></tbody></table></table-wrap><p>The rapport β = SiO<sub>2</sub>/(Al<sub>2</sub>O<sub>3</sub> + Fe<sub>2</sub>O<sub>3</sub>) concerning the fine fraction and varying between 1.6 for MNOIN and 1.2 for ZTI2N (<xref ref-type="table" rid="table4">Table 4</xref>), indicates the presence of clays of the type 2/1 the more so as this value would be close to 2 [<xref ref-type="bibr" rid="scirp.61581-ref20">20</xref>] . Indeed GNE1N, MNO1N and ZTI2N respectively contain 82%, 92% and 28% of smectite (<xref ref-type="table" rid="table2">Table 2</xref>)</p><p>All the samples also contain, of small quantities of TiO<sub>2</sub> indicating the presence on average of 1.27% of anatase also detected with the diffraction of x-rays. Moreover, only the materials of GNE1contain an appreciable average quantity of (K<sub>2</sub>O + Na<sub>2</sub>O) equalizes at 1.5%, suggesting the presence of feldspar detectable also by the diffraction of x-rays to the presence is from the goethite found in ZTI2 or from the structural iron in the smectites of 3 sites. This will be also confirmed by Spectrometry M&#246;ssbauer.</p></sec><sec id="s3_5"><title>3.5. Physico-Chemical and Granulometric Analyses</title><p>The results of granulometry are represented on <xref ref-type="fig" rid="fig1">Figure 1</xref>0. The definition of the clay from the particle with a lower diameter than 2 &#181;m must be reservedly taken. Indeed, some clayey particles have the upper size than 2 &#181;m while some particles of minerals linked to clay (feldspar, quartz, goethite, etc.) have a lower size than 2 &#181;m. It is why ones think that the clayey minerals begin being present from fine silts [<xref ref-type="bibr" rid="scirp.61581-ref8">8</xref>] and that in lower fraction than 2 μm can be traces of associate minerals. The particles of these samples are divided into four great classes as shown it on <xref ref-type="fig" rid="fig8">Figure 8</xref>. Clays (diameter &lt; 2 μm) are in a decreasing way, 48.9; 31.4% and 23.4% respectively for the samples G, M and Z. The fine silts (2 - 20 &#181;m) are more numerous in M (64.8%), than G (48.2%) and Z (39%). The coarse silts (20 - 50 &#181;m) are more significant in Z (22.9%), than M (3.2%) and G (1.9%). Fine sands (50 - 200 &#181;m) are in an increasing way 1; 0.7% and 14.6% respectively for samples G, M and Z. The three samples are primarily silty-argillaceous (more than 62% clay + silt) with more clay for G (48.9%), more fine silt for M (64.8%) and a texture balanced enough for ZY with a little bit of every element.</p><p>The results of the physico-chemical analysis (<xref ref-type="table" rid="table5">Table 5</xref>) come to confirm those of the mineralogical analysis. It is noticed whereas clays of the three sites have capacities of cationic exchange lower than those their majority clay components. 40.9 meq/100 g for the G, 39.8 meq/100 g for M and 4.17 meq/100 g for the Z against 80 - 150 meq/100 g for the smectites and 5 - 15 meq/100 g for kaolinites [<xref ref-type="bibr" rid="scirp.61581-ref21">21</xref>] . These low values would be explained</p><fig id="fig10"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>0</label><caption><title> Granulom&#233;tric composition of GNE1, MNO1 and ZTI2</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x16.png"/></fig><table-wrap id="table5" ><label><xref ref-type="table" rid="table5">Table 5</xref></label><caption><title> Cationic Exchange Capacity (CEC), specific surface and density GNE1, MNO1 and ZTI2</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Samples</th><th align="center" valign="middle" >CEC in meq/100 g</th><th align="center" valign="middle" >Density</th><th align="center" valign="middle" >Specific Surface (m&#178;/g)</th></tr></thead><tr><td align="center" valign="middle" >GNE1</td><td align="center" valign="middle" >40,9</td><td align="center" valign="middle" >2,36</td><td align="center" valign="middle" >105,41</td></tr><tr><td align="center" valign="middle" >MNO1</td><td align="center" valign="middle" >39,8</td><td align="center" valign="middle" >2,33</td><td align="center" valign="middle" >100,59</td></tr><tr><td align="center" valign="middle" >ZTI2</td><td align="center" valign="middle" >3,8</td><td align="center" valign="middle" >2,66</td><td align="center" valign="middle" >69,2</td></tr></tbody></table></table-wrap><p>by the fact that in the method used measurements are done on the total samples which contains in our case a considerable quantity of quartz unable to exchange cations. Moreover, kaolinites are not very exchanger of cations what explain the low value 3.8 meq/100 g of Z which contains more kaolinite than G and M. The density gives an idea of the prevalent species in samples. Thus the samples G (density = 2.36) and M (density = 2.37) are smectitic (2.08 - 2.35) whereas the density of Z (2.64) are kaolinitic (density = 2.40 - 2.64) and/or quartz (density = 2.65). It is noticed that moreover GNE1 and MNO1, which are smectitic than ZTI2, have a greater specific surface (100.59 meq/100 g against 69.2 m<sup>2</sup>/g for ZTI2 ) and ZTI2 which contains more kaolinite, a little smectite and a little goethite which has raised more this by rapport of the specific surface of kaolinite (10 - 30 m<sup>2</sup>/g) [<xref ref-type="bibr" rid="scirp.61581-ref22">22</xref>] .</p></sec><sec id="s3_6"><title>3.6. Study Carried out by Infrared and M&#246;ssbauer Spectroscopies</title><p>For IR, the analysis of samples GNEIN, MNOIN and ZTI2N are going in field from 50 cm<sup>−1</sup> to 400 cm<sup>−1</sup> and 400 cm<sup>−1</sup> to 4000 cm<sup>−1</sup>. The spectra obtained are represented on <xref ref-type="fig" rid="fig1">Figure 1</xref>1(a) and <xref ref-type="fig" rid="fig1">Figure 1</xref>1(b). On <xref ref-type="fig" rid="fig1">Figure 1</xref>1(a) are observed:</p><p>・ 3 bands due to the vibrations of isosceles triangle H-O-H of symmetry C2v [<xref ref-type="bibr" rid="scirp.61581-ref23">23</xref>] which are roughly to 277. cm<sup>−1</sup> (symmetrical elongation), to 244 cm<sup>−1 </sup>(asymmetrical elongation) and to 199 cm<sup>−1</sup> (symmetrical deformation).</p><p>・ The beginning of a series of bands around 346 cm<sup>−1</sup> which characterizes the Si0<sub>4</sub> tetrahedron. This series continues on the <xref ref-type="fig" rid="fig1">Figure 1</xref>1(b) by the bands with 427 cm<sup>−1</sup> and 467 cm<sup>−1</sup> approximately previously notified.</p><p><xref ref-type="fig" rid="fig1">Figure 1</xref>1(b) in particular makes it possible to highlight the following differences:</p><p>・ Around 623 cm<sup>−1</sup> is a band hardly visible on the spectrum of GNEIN but non-existent on ZTI2N which would correspond to the elongation Al-O of a smectite [<xref ref-type="bibr" rid="scirp.61581-ref24">24</xref>] .</p><p>・ The three bands with 691 cm<sup>−1</sup>, 743 cm<sup>−1</sup> and 777 cm<sup>−1</sup> approximately visible on the three spectra are characteristic of a kaolinite [<xref ref-type="bibr" rid="scirp.61581-ref25">25</xref>] [<xref ref-type="bibr" rid="scirp.61581-ref26">26</xref>] . If the two last bands are equal intensities, kaolinite is then of a good crystal</p><fig-group id="fig11"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>1</label><caption><title> (a) Infra-red spectrum of GNE1N, MNO1N and ZTI2N between 50 cm<sup>−1</sup> and 450 cm<sup>−1</sup>; (b) Infra-red spectrum of GNE1N, MNO1N and ZTI2N between 400 cm<sup>−1</sup> and 4000 cm<sup>−1</sup>.</title></caption><fig id ="fig11_1"><label>(b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x17.png"/></fig><fig id ="fig11_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x18.png"/></fig></fig-group><p>linity [<xref ref-type="bibr" rid="scirp.61581-ref27">27</xref>] . It is the case of ZTI2N which is kaolinitique besides than the two others.</p><p>・ Moreover GNEIN and MNOIN present three other bands towards 797 cm<sup>−1</sup>, 871 cm<sup>−1</sup> and 1155 cm<sup>−1</sup>. The two first are characteristic of the deformation of O-H surrounded by two ions of Fe<sup>3+</sup> or Al<sup>3+</sup> and Fe<sup>3+</sup> following substitution of aluminum of a smectite by iron. The last band (shoulder) could be allotted to the elongation of Si-O-Si of a smectite.</p><p>We notice a resolved OH deformation band at 915 cm<sup>−1</sup> for Al-OH in beidellite, and 3 bands with positions of about 1007 cm<sup>−1</sup>, 1030 cm<sup>−1</sup> and 1087 cm<sup>−1</sup> which can be allotted to the vibrations of valence of the Si-O.</p><p>Finally between 3500 cm<sup>−1</sup> to 3800 cm<sup>−1</sup>, it is necessary notably to signalize the presence of the vibrations of valence of groupings OH related to the aluminum atoms which result in 4 following absorption bands:</p><p>・ 1 band solved enough around 3620 cm<sup>−1</sup> for the internal OH [<xref ref-type="bibr" rid="scirp.61581-ref28">28</xref>] as well in the minerals 1:1 that in the 2:1.</p><p>・ a 2<sup>nd</sup> band with approximately 3650 cm<sup>−1</sup>, sometimes a 3rd towards 3660 cm<sup>−1</sup> and a 4<sup>th</sup> also enough solved to approximately 3695 cm<sup>−1</sup>, for the external OH [<xref ref-type="bibr" rid="scirp.61581-ref29">29</xref>] , [<xref ref-type="bibr" rid="scirp.61581-ref30">30</xref>] . this only in the minerals 1:1.</p><p>These fine fractions contain primarily kaolinite and smectite thus confirming the analyses with the X-ray.</p><p>For M&#246;ssbauer, the study is made at the room temperature. The results are represented on <xref ref-type="fig" rid="fig1">Figure 1</xref>2 and are consigned in <xref ref-type="table" rid="table6">Table 6</xref>.</p><p>For GNE1 magnetic 1, pas de spectrum. One observes a doublet allotted to 100% of Fe III in an octahedral environment more or less distorted with an isomeric displacement δ1 = 0.36 m/s, a quadripolar bursting Δ1 = 0.54 m/s, and a width of line at middle height Γ = 0.55 m/s. This iron can be structural iron in substitution for the aluminum in clay or of super paramagnetic iron impurity [<xref ref-type="bibr" rid="scirp.61581-ref23">23</xref>] , [<xref ref-type="bibr" rid="scirp.61581-ref31">31</xref>] .</p><p>For MNO1, there is either magnetic spectrum; simulation gives two characteristic doublets:</p><p>・ A doublet, very broad (δ1 = 0.34 m/s, Δ1 = 0.53 m/s and Γ = 0.34 mm/s), corresponds to Fe III in octahedral site with 94% There too one can allot it either to iron substituted for aluminum in the structure of silico-</p><fig-group id="fig12"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>2</label><caption><title> Mossbauer spectra of the three samples at the ambient temperature.</title></caption><fig id ="fig12_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x20.png"/></fig><fig id ="fig12_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x19.png"/></fig><fig id ="fig12_3"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/9-6702756x21.png"/></fig></fig-group><table-wrap id="table6" ><label><xref ref-type="table" rid="table6">Table 6</xref></label><caption><title> Fe M&#246;ssbauer data relating to the studied samples (at ambient temperature)</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Samples</th><th align="center" valign="middle" >d (mm/s)</th><th align="center" valign="middle" >D (mm/s)</th><th align="center" valign="middle" >G<sub>(mm/s) </sub></th><th align="center" valign="middle" >H (T)</th><th align="center" valign="middle" >Contr. (%)</th><th align="center" valign="middle" >Attribution</th></tr></thead><tr><td align="center" valign="middle" >GNE1</td><td align="center" valign="middle" >0.36</td><td align="center" valign="middle" >0.54</td><td align="center" valign="middle" >0.55<sub> </sub></td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >100</td><td align="center" valign="middle" >Fe <sup>III</sup> octahedral</td></tr><tr><td align="center" valign="middle" >MNO1</td><td align="center" valign="middle" >0.34</td><td align="center" valign="middle" >0.53</td><td align="center" valign="middle" >0.34<sub> </sub></td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >94</td><td align="center" valign="middle" >Fe <sup>III</sup> octahedral</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >0.29</td><td align="center" valign="middle" >2.46</td><td align="center" valign="middle" >0.34<sub> </sub></td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >6</td><td align="center" valign="middle" >Fe <sup>III</sup> tetrahedral</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >0.37</td><td align="center" valign="middle" >0.52</td><td align="center" valign="middle" >0.49</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >36.4</td><td align="center" valign="middle" >Fe <sup>III</sup> octahedral</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >0.54</td><td align="center" valign="middle" >1.53</td><td align="center" valign="middle" >0.49</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >8.3</td><td align="center" valign="middle" >Fe <sup>III</sup> octahedral</td></tr><tr><td align="center" valign="middle" >ZTI2</td><td align="center" valign="middle" >0.40</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >0.75</td><td align="center" valign="middle" >29.5</td><td align="center" valign="middle" >24.9</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >0.53</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >0.75</td><td align="center" valign="middle" >19.2</td><td align="center" valign="middle" >19.2</td><td align="center" valign="middle" ></td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >0.92</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >0.75</td><td align="center" valign="middle" >13.7</td><td align="center" valign="middle" >11.2</td><td align="center" valign="middle" ></td></tr></tbody></table></table-wrap><p>(d = someric displacement compared to a Fe; D = quadripolar bursting; G=width of line at middle height; H = hyperfine magnetic field).</p><p>aluminous or for iron super paramagnetic impurity.</p><p>・ The other, of small surface represents tetrahedral Fe III (δ2 = 0.29 m/s, Δ2 = 2.46 m/s, Γ = 0.34 m/s) for 6% of the total iron. This could agree with structural iron which replaced silicon in a tetrahedral environment relating to the presence of the beidellite in the sample as the X-ray indicates it.</p><p>Finally ZTI2 has a spectrum with different sites:</p><p>・ Two no magnetic contributions which form the central envelope with 40% on average. Contributions, which can be allotted to FeIII in octahedral site.</p><p>・ And three magnetic contributions which give the envelope widened in the spectrum and correspond to approximately 60%. This with H &lt; with 50 T, signalize the presence of the goethite detected to x-rays, [<xref ref-type="bibr" rid="scirp.61581-ref23">23</xref>] [<xref ref-type="bibr" rid="scirp.61581-ref32">32</xref>] .</p><p>On the whole, it is deduced that the beidellite of GNE1 contains Al<sup>3+</sup> and Si<sup>4+</sup> in its tetrahedron and that of MNO1 contains in addition, Fe<sup>3+</sup>.</p></sec><sec id="s3_7"><title>3.7. Determination of Chemical Formula of Samples GNE1N and MNO1N</title><p>For that, we regarded GNE1N and MNO1N as smectites considering the strong proportion of smectite contained in these samples (respectively 82.46%, 92.22%) and we used the method of M. &#214;NAL [<xref ref-type="bibr" rid="scirp.61581-ref33">33</xref>] supported in particular of the results of M&#246;ssbauer. What gives:</p><p>GNO1N: Na<sup>+</sup><sub>0,02</sub>K<sup>+</sup><sub>0,06</sub>Ca<sup>2+</sup><sub>0,07</sub>Mg<sup>2+</sup><sub>0,16</sub>[(Al<sup>3+</sup>, Fe<sup>3+</sup>)<sub>1,95</sub>Mg<sup>2+</sup><sub>0,05</sub>)] [Si<sup>4+</sup><sub>3,49</sub>Al<sup>3+</sup><sub>0,51</sub>]O<sub>10,00</sub>(OH)<sub>2,00</sub>H<sub>2</sub>O<sub>n</sub>.</p><p>MNO1N: Na<sup>+</sup><sub>0,01</sub>K<sup>+</sup><sub>0,01</sub>Ca<sup>2+</sup><sub>0,10</sub>Mg<sup>2+</sup><sub>0,15</sub>[(Al<sup>3+</sup>, Fe<sup>3+</sup>)<sub>1,94</sub>Mg<sup>2+</sup><sub>0,06</sub>)] [Si<sup>4+</sup><sub>3,53</sub>(Al<sup>3+</sup>, Fe<sup>3+</sup>)<sub>0,47</sub>]O<sub>10,00</sub>(OH)<sub>2,00</sub>H<sub>2</sub>O<sub>n</sub>.</p></sec></sec><sec id="s4"><title>4. Conclusion</title><p>Globally, the three samples are essentially silty-argillaceous (more than 62% clay + silt) with 48.9% of clay for GNE1, 31.4% of clay for MNO1 and 23.4% of clay for ZTI2. The principal minerals highlighted in the clayey fraction lower than 2 μm are the beidellite and kaolinite. GNE1N and MNO1N are practically beillidelitic (more than 82% of beillidelite) and ZTI2N practically kaolinitic (70% of kaolinite). Consequently, GNE1 and MNO1 have largest specific surfaces and capacities of exchange of cation relatively to ZTI2 (respectively40.9 meq/100 g; 39.8 meq/100 g; 3.8 meq/100 g and 105.4 meq/100 g; 100.6 meq/100 g; 69.2 m&#178;/g. It comes out from these analyses that the clay of GBEDJI-KOTOVI and MASSI will induce an enteric methane reduction more than clay of Zogbodomey. This study will be followed in further investigations by the use of clay as an additive food in Djallonk&#233; sheep.</p></sec><sec id="s5"><title>Cite this paper</title><p>EtienneSagbo,MarielleAgbahoungbata,WilfriedKangbode,ArthurCakpo,JacquesKinlehoume,Jean-BaptiseMensah,YvesNoack, (2015) Characterization of Clay of the Benin Used in Ruminale Feeding. Complete Determination of the Smectites Contained in These Clays. Journal of Environmental Protection,06,1322-1336. doi: 10.4236/jep.2015.611115</p></sec><sec id="s6"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.61581-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Chenoweth, D.P. (1996) Environmental Impact of Methanogenesis. Environmental Monitoring and Assessment, 42, 3-18. http://dx.doi.org/10.1007/BF00394039</mixed-citation></ref><ref id="scirp.61581-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Ouachem, D., Soltane, M. and Kalli, A. (2008) Les pailles de céréales: Profil des fermentations et production de méthane. Sciences &amp; Technologie, 27, 23-28.</mixed-citation></ref><ref id="scirp.61581-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Iheta, B., Kirov, M., Tsawlassou, G. and Houessou, A. 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