Geochemistry and geothermobarometry of the Um Eleiga Neoproterozoic island arc intrusive complex, SE Egypt: genesis of a potential gold-hosting intrusion

Abstract

Gabbro-diorite-tonalite¡granodiorite complexes, derived from subduction-related, calc alkaline magmas represent a distinct unit in the Precambrian basement of Egypt. These intrusive complexes are commonly intruded into ophiolitic mé lange, schistose or gneissic rock assemblages. Well-constrained geological mapping of the Um Eleiga complex, combined with geochemical studies, should enable a better understanding of its genesis, especially its potential as a host for gold mineralisation. This complex represents a composite pluton intruded into the allochthonous, ophiolitic Abu Dahr massif and its associated undifferentiated metavolcanosedimentary mé lange matrix in the southern Eastern Desert of Egypt. Field and petrographic investigations have revealed a compositional continuum from gabbro to granodiorite through diorite and subordinate tonalite. Petrography and bulk rock geochemical data have been used to determine the magma type and tectonic setting of the Um Eleiga complex, whereas the electron microprobe data were valuable for the purpose of determining the pressure-temperature and oxygen fugacity conditions. The compositional continuum, pattern of zonation, shallow magma origin and marked common negative Nb anomalies suggest that a close petrogenetic relationship between the gabbro, diorite, tonalite and granodiorite units of the Um Eleiga complex. Subducted upper mantle wedge is proposed as being the source region for the gabbroic magma, whereas zoning of the complex is attributed to interplay of fractional crystallisation and assimilation. Pressure estimates based on the Al (iv) -in-hornblende geobarometry indicate that the gabbroic and dioritic rocks crystallised under 4-5 kbar, whereas tonalite and granodiorite were formed at 3-4 kbar. The hornblende-plagioclase thermometer indicates a formation temperature range of about 720 to 880uC for the complex. Varied oxidation states are inferred from the mineral assemblages, including magnetite, titanite and ilmenite and checked by Fe/(FezMg) ratios of biotite in the granitoid rocks. The tectonic setting, mineralogical, geochemical characteristics and varied redox state of the Um Eleiga intrusive complex are typical for arc-related intrusives potential for hosting intrusion-related gold in a collisional environment.

Geochemistry and geochronology of the ~620 Ma gold-associated Batouri granitoids, Cameroon

“…These trends may indicate a co-magmatic origin for all rock variants. This hypothesis is further reinforced by the clustering of the rocks around the metaluminous-peraluminous boundary (Heinhorst et al 1996;Zoheir et al 2008) and the overlapping ages of the rock varieties. Tonalites and granodiorites partially Figure 10.…”

Multispectral and Radar Data for the Setting of Gold Mineralization in the South Eastern Desert, Egypt

“…A later barren generation of N-, NW-, and E-trending quartz veins are restricted to fault intersections and tension gashes in the highly deformed gabbroic rocks. Zoheir et al [71] suggested that fault/joint intersections are the main structural control of intensely hydrothermal alteration zones and high gold contents in the central part of the Um Eleiga complex. The E-trending fractures cutting the gabbroic rocks are locally associated with chlorite-calcite and chalcedonic quartz alteration assemblage.…”

Petrographic and geochemical study of Doua granitoids (adamawa-yade domain, center Cameroon): Petrogenesis and geodynamic implication

“…The abundance of ferromagnesian minerals such as amphibole in the rocks suggests on one hand that the fusion that took place has a magmatic source of mantle origin [55]. The global parallelism of the profiles of rare earths elements indicates that these rocks are cogenetic ( [56]; [57]). The high negative anomalies in Nb-Ta on the profil of these rocks are classically interpreted as corresponding to the characteristics of rocks originating from the continental crust ( [58]; [59]).…”