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Petrological and mineralogical studies of Pan-African serpentinites at Bir Al-Edeid area,central Eastern Desert,Egypt
Institution:1. Department of Lithospheric Research, University of Vienna, Althanstrasse 14, A-1090 Vienna, Austria;2. Department of Geology, Faculty of Science, Minia University, El-Minia, 61519, Egypt;3. Institute of Mineralogy and Petrology, Karl-Franzens University, Graz, Austria;1. Instituto de Ciencias de la Tierra, Universidad Austral de Chile, Valdivia, Chile;2. Departamento de Mineralogía y Petrología, Facultad de Ciencias, Universidad de Granada, Avda. Fuentenueva s/n, 18002 Granada, Spain;3. Department of Geology, Andean Geothermal Center of Excellence (CEGA), Universidad de Chile, Plaza Ercilla #803, Santiago, Chile;4. Instituto de Geología, Universidad Nacional Autónoma de México, Ciudad Universitaria, 04510 Ciudad de México, Mexico;5. Géosciences environnement Toulouse, Université de Toulouse, CNES, CNRS, IRD, UPS, France;6. Nantes Univ., Angers Univ., CNRS, LPG, UMR 6112, F-44000 Nantes, France;7. Géosciences Montpellier, CNRS, Univ. Montpellier & Univ. des Antilles (UMR5243), 34095 Montpellier, France;8. La Rochelle University, FST, Av M Crepeau, 17042 La Rochelle, Cedex, France
Abstract:The studied serpentinites occur as isolated masses, imbricate slices of variable thicknesses and as small blocks or lenses incorporated in the sedimentary matrix of the mélange. They are thrusted over the associated island arc calc-alkaline metavolcanics and replaced by talc-carbonates along shear zones. Lack of thermal effect of the serpentinites upon the enveloping country rocks, as well as their association with thrust faults indicates their tectonic emplacement as solid bodies. Petrographically, they are composed essentially of antigorite, chrysotile and lizardite with subordinate amounts of carbonates, chromite, magnetite, magnesite, talc, tremolite and chlorite. Chrysotile occurs as cross-fiber veinlets traversing the antigorite matrix, which indicate a late crystallization under static conditions. The predominance of antigorite over other serpentine minerals indicates that the serpentinites have undergone prograde metamorphism or the parent ultramafic rocks were serpentinized under higher pressure. The parent rocks of the studied serpentinites are mainly harzburgite and less commonly dunite and wehrlite due to the prevalence of mesh and bastite textures. The serpentinites have suffered regional metamorphism up to the greenschist facies, which occurred during the collisional stage or back-arc basin closure, followed by thrusting over a continental margin. The microprobe analyses of the serpentine minerals show wide variation in SiO2, MgO, Al2O3, FeO and Cr2O3 due to different generations of serpentinization. The clinopyroxene relicts, from the partly serpentinized peridotite, are augite and similar to clinopyroxene in mantle-derived peridotites. The chromitite lenses associated with the serpentinites show common textures and structures typical of magmatic crystallization and podiform chromitites. The present data suggest that the serpentinites and associated chromitite lenses represent an ophiolitic mantle sequence from a supra-subduction zone, which were thrust over the continental margins during the collisional stage of back-arc basin.
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