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Genesis of gabbroic intrusions in the Arabian Shield, Saudi Arabia: mineralogical, geochemical and tectonic fingerprints of the Neoproterozoic arc magmatism

Published online by Cambridge University Press:  12 April 2021

Shehata Ali Open the ORCID record for Shehata Ali [Opens in a new window]  and
Abdullah S. Alshammari
Shehata Ali*
Affiliation:
Geology Department, Faculty of Science, Minia University, 61519El-Minia, Egypt
Abdullah S. Alshammari
Affiliation:
Faculty of Science, Hail University, 2440Hail, Saudi Arabia
*
Author for correspondence: Shehata Ali, Email: shehata.ali@mu.edu.eg
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Abstract

The Arabian Shield of Saudi Arabia represents part of the Arabian–Nubian Shield and forms an exposure of juvenile continental crust on the eastern side of the Red Sea rift. Gabbroic intrusions in Saudi Arabia constitute a significant part of the mafic magmatism in the Neoproterozoic Arabian Shield. This study records the first detailed geological, mineralogical and geochemical data for gabbroic intrusions located in the Gabal Samra and Gabal Abd areas of the Hail region in the Arabian Shield of Saudi Arabia. Geological field relations and investigations, supported by mineralogical and geochemical data, indicate that the gabbroic intrusions are generally unmetamorphosed and undeformed, and argue for their post-collisional emplacement. Their mineralogical and geochemical features reveal crystallization from hydrous, mainly tholeiitic, mafic magmas with arc-like signatures, which were probably inherited from the previous subduction event in the Arabian–Nubian Shield. The gabbroic rocks exhibit sub-chondritic Nb/U, Nb/Ta and Zr/Hf ratios, revealing depletion of their mantle source. Moreover, the high ratios of (Gd/Yb)N and (Dy/Yb)N indicate that their parental mafic melts were derived from a garnet-peridotite source with a garnet signature in the mantle residue. This implication suggests that the melting region was at a depth exceeding ∼70–80 km at the garnet stability field. They have geochemical characteristics similar to other post-collisional gabbros of the Arabian–Nubian Shield. Their origin could be explained by adiabatic decompression melting of depleted asthenosphere that interacted during ascent with metasomatized lithospheric mantle in an extensional regime, likely related to the activity of the Najd Fault System, at the end of the Pan-African Orogeny.

Keywords

gabbroNeoproterozoicpost-collisional magmatismArabian ShieldSaudi Arabia
Type
Original Article
Information
Geological Magazine , Volume 158 , Issue 9 , September 2021 , pp. 1639 - 1656
Copyright
© The Author(s), 2021. Published by Cambridge University Press

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