𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Origin of I- and A-type granitoids from the Eastern Desert of Egypt: Implications for crustal growth in the northern Arabian–Nubian Shield

✍ Scribed by E.S. Farahat; H.A. Mohamed; A.F. Ahmed; M.M. El Mahallawi


Publisher
Elsevier Science
Year
2007
Tongue
English
Weight
738 KB
Volume
49
Category
Article
ISSN
1464-343X

No coin nor oath required. For personal study only.

✦ Synopsis


I-and A-type granitoid rocks, emplaced during pre-and post-collision stages, respectively, of the Neoproterozoic Pan-African Orogeny, are widely distributed in the Eastern Desert of Egypt, constituting $60% of the basement outcrop. Petrological and geochemical data are presented for a selection of the two groups, the I-type, El Bula tonalite-granodiorite suite, and the A-type, Lo ˆma ˆn alkali granites, with the aim of discussing their origin and geotectonic implications. The El Bula (EB) rocks have geochemical characteristics of medium-K calc-alkaline, metaluminous to mildly peraluminous, granitoids formed in an island-arc environment. The Lo ˆma ˆn (LM) granites display midalkaline, metaluminous, post-orogenic, A-type characteristics. With respect to the EB granitoids, the LM granites contain lower Al 2 O 3 , Fe 2 O 3 , MgO, MnO, CaO, TiO 2 , Sr, Ba, and V, but higher Na 2 O, K 2 O, Nb, Zr, Th, and Rb. The I-type granitoids were presumably formed by high degrees of partial melting ($40%) of a mafic (amphibolitic), lower crustal source, whereas the A-type granites are derived from a tonalitic, middle crustal source, followed by some crystal fractionation. Such high degrees of partial melting attest to the large areal distribution of these rocks and require broad thermal anomalies, likely related to significant geodynamic features of the Arabian-Nubian Shield (ANS) evolution. We propose petrogenetic models involving an upwelling of hot asthenospheric mantle, due to oblique convergence during the pre-collision stage, and following a lithospheric delamination during the post-collision stage. Such asthenosphere uprise could account for the high crustal growth rate of the ANS.