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25th International Meeting on Organic Geochemistry IMOG 2011

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P-050<br />

Informati<strong>on</strong> provided by the <strong>Organic</strong> Matter c<strong>on</strong>tained in cherts<br />

of the Ras-Draâ phosphate deposit (Tunisia) <strong>on</strong> their<br />

depositi<strong>on</strong>al envir<strong>on</strong>ment<br />

Aïda Ben Hassen 1 , Jean Trichet 2 , Jean-Robert Disnar 2 , Habib Belayouni 3<br />

1 Centre de Recherche et des Technologies de l'Energie, Technopôle Borj Cédria, Hammam-Lif, Tunisia,<br />

2 Institut des Sciences de la Terre d'Orléans, Orléans, France, 3 Faculté des Sciences de Tunis, El Manar,<br />

Tunisia<br />

In the Paleocene-Early Eocene Ras-Draâ (Tunisia)<br />

phosphate outcrop formati<strong>on</strong> a laminated (siliceous)<br />

chert level is interbedded between two phosphatic<br />

strata (CVI and CVII phosphorites; P2O5 > 18%). The<br />

study of the organic matter (OM) associated to the<br />

chert aims at bringing some light <strong>on</strong> the nature and<br />

the geochemical properties of this OM and then to<br />

draw some c<strong>on</strong>clusi<strong>on</strong>s <strong>on</strong> the genesis of these<br />

sediments.<br />

The main results of this study can be summarized<br />

as follows:<br />

1. The Total <strong>Organic</strong> Carb<strong>on</strong> (TOC) c<strong>on</strong>tent, given<br />

by Rock-Eval pyrolysis, is about 1.6%.<br />

2. The geochemical characterizati<strong>on</strong> of the OM<br />

c<strong>on</strong>tained in cherts, by Rock-Eval (RE) pyrolysis<br />

c<strong>on</strong>cludes to: (i) a high aliphatic character (Hydrogen<br />

Index IH value ~ 499 mg d‘HC/g TOC) and thus to a<br />

marine plankt<strong>on</strong>ic origin of the OM (Type II), (ii) a low<br />

degree of OM maturity (Rock Eval Tmax = 429 °C)<br />

and (iii) to the presence of little oxidized organic<br />

comp<strong>on</strong>ents due to the lower Oxygen Index IO (about<br />

50 mg de CO2/g TOC).<br />

3. The chemical extracti<strong>on</strong> of the humic substances<br />

(HS) associated to the cherty sediments (following the<br />

<str<strong>on</strong>g>Internati<strong>on</strong>al</str<strong>on</strong>g> Humic Substances Society protocol)<br />

evidences significant amounts of extractable humic<br />

compounds (~20% TOC) and higher proporti<strong>on</strong>s of<br />

n<strong>on</strong> extractible residue or "humin" (~ 80% TOC). Such<br />

significant amounts of HS were reported by Kahouach<br />

(1989) (up to 27% TOC) in chert interlayers from<br />

tunisian phosphatic series. However, higher HS<br />

proporti<strong>on</strong>s were found by Bein et Amit (1982), in<br />

cherts associated to Negev phosphorites (more than<br />

40% of OM are in humic form). According to Kolod<strong>on</strong>y<br />

(1969), such results suppose that the cherts formati<strong>on</strong><br />

is due to the silicificati<strong>on</strong> of phosphatic materials that<br />

were probably rich in HS. In our study, RE parameters<br />

– markedly high HI and distinctly low OI values –<br />

respectively suggest the autochth<strong>on</strong>ous origin of this<br />

OM and, the absence of oxidative destructi<strong>on</strong> of the<br />

initial organic material during chert formati<strong>on</strong>.<br />

4. The main geochemical and spectroscopic<br />

features of the humic acids (HA) extracted from the<br />

cherts are the following <strong>on</strong>es: (i) atomic O/C and H/C<br />

ratio values of 0.27 and 1.53% signify that these<br />

humic compounds originated from marine aliphatic<br />

OM; (ii) FTIR analysis of cherts-extracted HA show<br />

that these organic compounds are rich in aliphatic<br />

structures that is typical for an algae derived material.<br />

5. The occurrence of fossil molecules in chert lipidic<br />

extract (C22 predominance in n-alkane distributi<strong>on</strong>s,<br />

presence of steroids and benzohopanoids) c<strong>on</strong>firms<br />

the autochth<strong>on</strong>ous marine origin and the low degree<br />

of maturity of the OM. With regards to chert age, the<br />

abundance of HS implies their good preservati<strong>on</strong> in a<br />

reducing depositi<strong>on</strong>al envir<strong>on</strong>ment (Belayouni et<br />

Trichet, 1983).<br />

Finally, the study of the OM associated to the<br />

cherts interbedded within P-rich levels brings clear<br />

evidence that these sediments were deposited in a<br />

reducing marine envir<strong>on</strong>ment marine and that they<br />

<strong>on</strong>ly experienced limited diagenesis (that led them to<br />

the humic stage).<br />

References<br />

[1] Bein, A., Amit, O., 1982. Depositi<strong>on</strong>nal<br />

envir<strong>on</strong>ments of the Sen<strong>on</strong>ian chert phosphorites and<br />

oil shales sequence in Israel as deduced from their<br />

organic matter compositi<strong>on</strong>. Sedimentology 29, 81-90.<br />

[2] Belayouni, H. and Trichet, J. [1983] Preliminary<br />

data <strong>on</strong> the origin and diagenesis of the organic<br />

matter in the phosphate basin of Gafsa (Tunisia).<br />

Advances in <strong>Organic</strong> <strong>Geochemistry</strong> 1981, 328-335.<br />

[3] Ben Hassen, A. [2007] D<strong>on</strong>nées nouvelles sur la<br />

matière organique associée aux séries du bassin<br />

phosphaté du sud-tunisien (Gisement de Ras-Draâ)<br />

et sur la phosphatogenèse. Thèse de Doctorat,<br />

Université d‘Orléans. France.<br />

[4] Kahouach, H., 1986. Ab<strong>on</strong>dance, nature et<br />

compositi<strong>on</strong> de la matière organique c<strong>on</strong>tenue dans<br />

les sédiments de la série phosphatée du gisement de<br />

Ras-Draâ (Nefta-Tozeur). Applicati<strong>on</strong> à la valorisati<strong>on</strong><br />

des minerais phosphatés. Rapport de DEA. Université<br />

de Tunis. Tunisie.<br />

[5] Kolod<strong>on</strong>y, Y. 1969. Petrology of siliceous rocks in<br />

the Mishtah Formati<strong>on</strong> (Negev, Israel). J. Sedim.<br />

Petrol. 39, 166-175.<br />

197

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