Origin of Neoproterozoic anorthosites in the Wadi El Dib ultramafic-mafic layered intrusions, Egypt

IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY
H.A. Eliwa , R. Deevsalar , N.M. Mahdy , Y. Pan , Kh. El-Gameel , H.A. El-Desouky , H. Khamis , M. Murata , A. Andresen , D. Chew , H. El Sundolly , M.M. Fawzy , Y. Kato , K. Fujinaga , K.-C. Shin , R. Shinjo
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引用次数: 0

Abstract

The Neoproterozoic ultramafic–mafic intrusions (NUIs) in the Wadi El Dib (WED) region of the Northeastern Desert, Egypt, consist of a gabbro-serpentinite sequence overlain by anorthosite intrusions. The WED anorthosites show two texturally distinct types of framework-dominated and intercumulus-rich and made of cumulus plagioclases (anorthite percentage: An60-45) and intercumulus mafic minerals along with granophyric materials. They are associated with rock types typically found alongside anorthosites within layered mafic intrusions. Zircon U-Pb age dating yielded Concordia age of 591.5 ± 3.5 Ma for both types of WED anorthosites. The measured crystallization age of the WED anorthosites matches the post-collisional stage of the Pan-African orogeny and coinciding with the emplacement of A-type granites in the Arabian Nubian Shield. The geochemical evidence suggests that gabbros and anorthosites likely formed from a common mafic parental magma. This is indicated by progressive decreases in concentrations of highly compatible elements and Mg# from gabbros to anorthosites, relatively high total REE contents in anorthosites, chondrite-normalized REE patterns with positive versus negative Eu anomalies, and the crystallization of transitional magmatic to metamorphic orthopyroxene in anorthosites. The low (87Sr/86Sr)i ratios and strongly positive εNd(t) values of the WED gabbros and anorthosites validate their genesis from an isotopically depleted mantle source. Trace-element geochemical modelling suggests that the older gabbros are denser mafic cumulates segregated from partially crystallized high alumina (high-Al) basaltic parent magma originated from low degree partial melting of mantle peridotite, whereas anorthosites settle out of the cooling residual melt through imperfect fractional crystallization process. The Sr-Nd systematics of the anorthosites coupled with distinct An% variations of cumulus plagioclases and the existence of both magmatic and inherited zircon in the granophyric materials verify a small contribution of lower crustal melts through the entrapment of felsic melt pockets within intercumulus spaces. The data and models indicate that the formation of WED anorthosites at the top of NUIs is triggered by post-collisional crustal thickening and asthenosphere upwelling consistent with previously proposed tectono-magmatic model for the NED.
埃及Wadi El Dib超基性-基性层状岩体中新元古代斜长岩的成因
埃及东北沙漠Wadi El Dib (WED)地区新元古代超镁铁质侵入岩(NUIs)由辉长岩-蛇纹岩层序和斜长岩侵入岩复盖而成。ww斜长岩由积云斜长石(钙长石比例为60-45)和积云间基性矿物及花岗质物质组成,呈框架型为主和富含积云间辉长岩两种结构类型。它们与岩石类型有关,通常在层状基性侵入体中与斜长岩一起发现。锆石U-Pb年龄测定结果表明,这两类斜长岩的Concordia年龄均为591.5±3.5 Ma。ww斜长岩的结晶年龄与泛非造山运动后碰撞阶段相吻合,与阿拉伯努比亚盾中a型花岗岩的侵位相吻合。地球化学证据表明辉长岩和斜长岩可能是由一种共同的基性母岩浆形成的。从辉长岩到斜长岩的高相容性元素和Mg#浓度逐渐降低,斜长岩中总稀土含量相对较高,球粒陨石归一化稀土模式呈正、负Eu异常,斜长岩中过渡型岩浆向变质正辉石结晶。w - w辉长岩和斜长岩具有较低的(87Sr/86Sr)比值和较强的正εNd(t)值,证明其成因为同位素亏缺的地幔源。微量元素地球化学模拟表明,较老的辉长岩是由部分结晶的高铝(高铝)玄武岩母岩浆分离而成的致密基性堆积物,源自地幔橄榄岩的低程度部分熔融,而斜长岩则是通过不完全的部分结晶过程沉淀于冷却残余熔体中。斜长岩的Sr-Nd分系统、明显的积云斜长石的An%变化以及花岗岩物质中岩浆锆石和继承锆石的存在,证实了下地壳熔体通过积云间空间内长英质熔体袋的夹带而产生的小贡献。数据和模型表明,NUIs顶部西向斜长岩的形成是由碰撞后地壳增厚和软流圈上升流触发的,与之前提出的内地壳构造-岩浆模型一致。
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来源期刊
Precambrian Research
Precambrian Research 地学-地球科学综合
CiteScore
7.20
自引率
28.90%
发文量
325
审稿时长
12 months
期刊介绍: Precambrian Research publishes studies on all aspects of the early stages of the composition, structure and evolution of the Earth and its planetary neighbours. With a focus on process-oriented and comparative studies, it covers, but is not restricted to, subjects such as: (1) Chemical, biological, biochemical and cosmochemical evolution; the origin of life; the evolution of the oceans and atmosphere; the early fossil record; palaeobiology; (2) Geochronology and isotope and elemental geochemistry; (3) Precambrian mineral deposits; (4) Geophysical aspects of the early Earth and Precambrian terrains; (5) Nature, formation and evolution of the Precambrian lithosphere and mantle including magmatic, depositional, metamorphic and tectonic processes. In addition, the editors particularly welcome integrated process-oriented studies that involve a combination of the above fields and comparative studies that demonstrate the effect of Precambrian evolution on Phanerozoic earth system processes. Regional and localised studies of Precambrian phenomena are considered appropriate only when the detail and quality allow illustration of a wider process, or when significant gaps in basic knowledge of a particular area can be filled.
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