The Precambrian Homrit-Waggat granite is a post-orogenic batholithic intrusion located in the northern region of the Nubian Shield,characterized by a typical annular morphology and significant secondary alteration.Thi...The Precambrian Homrit-Waggat granite is a post-orogenic batholithic intrusion located in the northern region of the Nubian Shield,characterized by a typical annular morphology and significant secondary alteration.This study aims to elucidate the processes that have shaped the intrusion in both macroscopic and microscopic perspectives,employing a combination of field observation and petrographic analysis alongside major and trace element compositions of minerals.Within the central region of the pluton,biotite and amphibole are observed sporadically,while the predominant crystallization of anhydrous oligoclase in the outer regions has led to a progressive increase in volatile components within the residual melt,ultimately resulting in a volatile-saturated aluminosilicate melt.The exsolved fluids subsequently interacted with the previously crystallized mineral assemblage,producing metasomatic overprinting.As the cooling and crystallization continued,the water pressure within the magma chamber gradually escalated until it equaled or surpassed the confining pressure,leading to the formation of fractures and veins filled with minerals that crystallized from the residual aqueous fluids.The ongoing degassing and expulsion of aqueous fluids from the magma chamber’s interior ultimately contributed to the collapse of the chamber’s roof,resulting in the annular ring-dike morphology observed in the Homrit Waggat pluton.展开更多
The Shaitian granite complex(SGC)spans more than 80 Ma of crustal growth in the Arabian–Nubian Shield in southeast Egypt.It is a voluminous composite intrusion(60 km2)comprising a host tonalite massif intruded by sub...The Shaitian granite complex(SGC)spans more than 80 Ma of crustal growth in the Arabian–Nubian Shield in southeast Egypt.It is a voluminous composite intrusion(60 km2)comprising a host tonalite massif intruded by subordinate dyke-like masses of trondhjemite,granodiorite and monzogranite.The host tonalite,in turn,encloses several,fine-grained amphibolite enclaves.U-Pb zircon dating indicates a wide range of crystallization ages within the SGC(800±18Ma for tonalites;754±3.9 Ma for trondhjemite;738±3.8 Ma for granodiorite;and 717±3.2 Ma for monzogranite),suggesting crystallization of independent magma pulses.The high positiveεNdi(+6–+8)indicate that the melting sources were dominated by juvenile material without any significant input from older crust.Application of zircon saturation geothermometry indicates increasing temperatures during the generation of melts from 745±31℃ for tonalite to 810±25℃ for trondhjemite;840±10℃ for granodiorite;and 868±10℃ for monzogranite.The pressure of partial melting is loosely constrained to be below the stability of residual garnet(<10 kbar)as inferred fromthe almost flat HREE pattern((Gd/Lu)N=0.9–1.1),but>3 kbar for the stability of residual amphibole as inferred from the significantly lower NbN and TaN compared with LREEN and the sub-chondrite Nb/Ta ratios exhibited by the granitic phases.The inverse relation between the generation temperatures and the ages estimates of the granitoid lithologies argue against a significant role of fractional crystallization.The major and trace element contents indicate the emplacement of the SGC within a subduction zone setting.It lacks distinctive features for melt derived from a subducted slab(e.g.high Sr/Y and high(La/Yb)N ratios),and the relatively low MgO and Ni contents in all granite phases within the SGC suggest melting within the lower crust of an island arc overlying a mantlewedge.Comparisonwith melts produced during melting experiments indicates an amphibolite of basaltic composition is the best candidate as source for the tonalite,trondhjemite and granodiorite magmas whereas the monzogranite magma is most consistent with fusion of a tonalite protolith.Given the overlapping Sm-Nd isotope ratios as well as several trace element ratios between monzogranite and tonalite samples,it is reasonable to suggest that the renewed basaltic underplating may have caused partialmelting of tonalite and the emplacement ofmonzogranite melt within the SGC.The emplacement of potassic granite(monzogranite)melts subsequent to the emplacement of Na-rich granites(tonalitetrondhjemite-granodiorite)most likely suggests major crustal thickening prior arc collision and amalgamation into the over thickened proto-crust of the Arabian-Nubian shield.Eventually,after complete consolidation,the whole SGC was subjected to regional deformation,most probably during accretion to the Saharan Metacraton(arc–continent collisions)in the late Cryogenian-Ediacaran times(650–542 Ma).展开更多
基金supported by Science and Technology Development Fund(STDF)of the Arab Republic of Egypt(No.23080)entitled―Rare Metal Ore Deposits in Egypt:A comparative survey in altered granites from selected areas in the Central Eastern Desert‖(to M.A.ABU EL-RUS)National Key Research and Development Program of China(No.2023YFF0804200).
文摘The Precambrian Homrit-Waggat granite is a post-orogenic batholithic intrusion located in the northern region of the Nubian Shield,characterized by a typical annular morphology and significant secondary alteration.This study aims to elucidate the processes that have shaped the intrusion in both macroscopic and microscopic perspectives,employing a combination of field observation and petrographic analysis alongside major and trace element compositions of minerals.Within the central region of the pluton,biotite and amphibole are observed sporadically,while the predominant crystallization of anhydrous oligoclase in the outer regions has led to a progressive increase in volatile components within the residual melt,ultimately resulting in a volatile-saturated aluminosilicate melt.The exsolved fluids subsequently interacted with the previously crystallized mineral assemblage,producing metasomatic overprinting.As the cooling and crystallization continued,the water pressure within the magma chamber gradually escalated until it equaled or surpassed the confining pressure,leading to the formation of fractures and veins filled with minerals that crystallized from the residual aqueous fluids.The ongoing degassing and expulsion of aqueous fluids from the magma chamber’s interior ultimately contributed to the collapse of the chamber’s roof,resulting in the annular ring-dike morphology observed in the Homrit Waggat pluton.
基金the outcome of a joint research project between Assiut University,Université Clermont-Auvergne,Ball State University,Swedish Museum of Natural History,Michigan State University and Notre Dame Universityfinancial support from the Geology Department,Assiut University+1 种基金Major and trace elements analyses were carried out with a grant from Science and Technology Development Fund(STDF),Egypt to Ali Abu El-Rus(contract no.6107)U-Pb analyses of zircons were funded through a Ball-State University internal grant to K.Nicholson and S.Malone.
文摘The Shaitian granite complex(SGC)spans more than 80 Ma of crustal growth in the Arabian–Nubian Shield in southeast Egypt.It is a voluminous composite intrusion(60 km2)comprising a host tonalite massif intruded by subordinate dyke-like masses of trondhjemite,granodiorite and monzogranite.The host tonalite,in turn,encloses several,fine-grained amphibolite enclaves.U-Pb zircon dating indicates a wide range of crystallization ages within the SGC(800±18Ma for tonalites;754±3.9 Ma for trondhjemite;738±3.8 Ma for granodiorite;and 717±3.2 Ma for monzogranite),suggesting crystallization of independent magma pulses.The high positiveεNdi(+6–+8)indicate that the melting sources were dominated by juvenile material without any significant input from older crust.Application of zircon saturation geothermometry indicates increasing temperatures during the generation of melts from 745±31℃ for tonalite to 810±25℃ for trondhjemite;840±10℃ for granodiorite;and 868±10℃ for monzogranite.The pressure of partial melting is loosely constrained to be below the stability of residual garnet(<10 kbar)as inferred fromthe almost flat HREE pattern((Gd/Lu)N=0.9–1.1),but>3 kbar for the stability of residual amphibole as inferred from the significantly lower NbN and TaN compared with LREEN and the sub-chondrite Nb/Ta ratios exhibited by the granitic phases.The inverse relation between the generation temperatures and the ages estimates of the granitoid lithologies argue against a significant role of fractional crystallization.The major and trace element contents indicate the emplacement of the SGC within a subduction zone setting.It lacks distinctive features for melt derived from a subducted slab(e.g.high Sr/Y and high(La/Yb)N ratios),and the relatively low MgO and Ni contents in all granite phases within the SGC suggest melting within the lower crust of an island arc overlying a mantlewedge.Comparisonwith melts produced during melting experiments indicates an amphibolite of basaltic composition is the best candidate as source for the tonalite,trondhjemite and granodiorite magmas whereas the monzogranite magma is most consistent with fusion of a tonalite protolith.Given the overlapping Sm-Nd isotope ratios as well as several trace element ratios between monzogranite and tonalite samples,it is reasonable to suggest that the renewed basaltic underplating may have caused partialmelting of tonalite and the emplacement ofmonzogranite melt within the SGC.The emplacement of potassic granite(monzogranite)melts subsequent to the emplacement of Na-rich granites(tonalitetrondhjemite-granodiorite)most likely suggests major crustal thickening prior arc collision and amalgamation into the over thickened proto-crust of the Arabian-Nubian shield.Eventually,after complete consolidation,the whole SGC was subjected to regional deformation,most probably during accretion to the Saharan Metacraton(arc–continent collisions)in the late Cryogenian-Ediacaran times(650–542 Ma).
