E. Saccani, Edoardo Barbero, M. Delavari, A. Dolati, Valentina Brombin, M. Marroni, L. Pandolfi
{"title":"来自 Bajgan 复合体(伊朗东南部马克兰断积棱岩)的元玢岩的地球化学和岩浆岩石学:关于早白垩世中东新特提斯性质的新见解","authors":"E. Saccani, Edoardo Barbero, M. Delavari, A. Dolati, Valentina Brombin, M. Marroni, L. Pandolfi","doi":"10.1144/jgs2024-043","DOIUrl":null,"url":null,"abstract":"\n The Bajgan Complex in the North Makran Domain (Makran Accretionary Prism) comprises disrupted meta-ophiolitic sequences originating from oceanic crust protoliths. They include ultramafic and mafic cumulates, isotropic gabbros, plagiogranites, and basalts. Ultramafic-mafic cumulates and plagiogranites exhibit compositions akin to rocks formed in mid-ocean ridge settings. Isotropic gabbro and basalt protoliths can be subdivided in three distinct geochemical types. Type-1 rocks is sub-alkaline (Nb/Y < 0.1) with low Th, Nb, and Ta contents and La\n N\n /Yb\n N\n ratios <1, resembling those of normal-type (N-) mid-ocean ridge basalts (MORB). Type-2 rocks display slight enrichment in Th, Ta, Nb (Nb/Y = 0.36 – 0.45), and La\n N\n /Yb\n N\n = 2.12 – 3.20, resembling the chemistry of enriched-type (E-) MORB. Type-3 basalts show an alkaline nature (Nb/Y=0.88-1.82), significant Th, Ta, Nb enrichment, and high La\n N\n /Yb\n N\n ratios (7.01 – 20.08), resembling the chemistry of alkaline basalts (OIB). Petrogenetic modeling indicates that N-MORB protoliths originated from a depleted MORB mantle source, while E-MORB and OIB protoliths were generated from partial melting of sub-oceanic depleted sources that underwent varying degrees of OIB-type enrichment. The Bajgan meta-ophiolitic protoliths were formed within a Late Jurassic to Cretaceous oceanic basin influenced by mantle plume activity and plume-ridge interaction.\n \n \n Thematic collection:\n This article is part of the Ophiolites, melanges and blueschists collection available at:\n https://www.lyellcollection.org/topic/collections/ophiolites-melanges-and-blueschists\n \n \n Supplementary material:\n https://doi.org/10.6084/m9.figshare.c.7193937\n","PeriodicalId":507891,"journal":{"name":"Journal of the Geological Society","volume":"3 3","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-04-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Geochemistry and magmatic petrology of meta-ophiolites from the Bajgan Complex (Makran Accretionary Prism, SE Iran): New insights on the nature of the Early Cretaceous Middle East Neotethys\",\"authors\":\"E. Saccani, Edoardo Barbero, M. Delavari, A. Dolati, Valentina Brombin, M. Marroni, L. Pandolfi\",\"doi\":\"10.1144/jgs2024-043\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"\\n The Bajgan Complex in the North Makran Domain (Makran Accretionary Prism) comprises disrupted meta-ophiolitic sequences originating from oceanic crust protoliths. They include ultramafic and mafic cumulates, isotropic gabbros, plagiogranites, and basalts. Ultramafic-mafic cumulates and plagiogranites exhibit compositions akin to rocks formed in mid-ocean ridge settings. Isotropic gabbro and basalt protoliths can be subdivided in three distinct geochemical types. Type-1 rocks is sub-alkaline (Nb/Y < 0.1) with low Th, Nb, and Ta contents and La\\n N\\n /Yb\\n N\\n ratios <1, resembling those of normal-type (N-) mid-ocean ridge basalts (MORB). Type-2 rocks display slight enrichment in Th, Ta, Nb (Nb/Y = 0.36 – 0.45), and La\\n N\\n /Yb\\n N\\n = 2.12 – 3.20, resembling the chemistry of enriched-type (E-) MORB. Type-3 basalts show an alkaline nature (Nb/Y=0.88-1.82), significant Th, Ta, Nb enrichment, and high La\\n N\\n /Yb\\n N\\n ratios (7.01 – 20.08), resembling the chemistry of alkaline basalts (OIB). Petrogenetic modeling indicates that N-MORB protoliths originated from a depleted MORB mantle source, while E-MORB and OIB protoliths were generated from partial melting of sub-oceanic depleted sources that underwent varying degrees of OIB-type enrichment. 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引用次数: 0
摘要
北迈克兰地区(迈克兰断积棱岩)的巴吉甘复合体由源自大洋地壳原岩的破碎元沸石序列组成。它们包括超闪长岩和黑云母积岩、各向同性辉长岩、斜长岩和玄武岩。超基性黑云母-黑云母积岩和长花岗岩的成分类似于在大洋中脊环境中形成的岩石。各向同性辉长岩和玄武岩原岩可细分为三种不同的地球化学类型。第一类岩石为亚碱性(Nb/Y < 0.1),Th、Nb 和 Ta 含量低,La N /Yb N 比率 < 1,与正常类型(N-)洋中脊玄武岩(MORB)相似。第二类岩石的钍、钽、铌含量略有富集(铌/镱比=0.36-0.45),镧/镱比=2.12-3.20,与富集型(E-)MORB 的化学成分相似。3型玄武岩呈碱性(Nb/Y=0.88-1.82),Th、Ta、Nb富集显著,La N /Yb N比值较高(7.01-20.08),类似于碱性玄武岩(OIB)的化学性质。岩石学模型表明,N-MORB原岩源于贫化的MORB地幔源,而E-MORB和OIB原岩则产生于经历了不同程度的OIB型富集的洋底贫化源的部分熔融。Bajgan元沸石原岩是在晚侏罗世至白垩纪大洋盆地内受地幔羽流活动和羽桥相互作用的影响而形成的。 专题文集:本文是蛇绿岩、熔岩和蓝晶岩专题集的一部分,可在以下网址查阅: https://www.lyellcollection.org/topic/collections/ophiolites-melanges-and-blueschists 补充材料: https://doi.org/10.6084/m9.figshare.c.7193937
Geochemistry and magmatic petrology of meta-ophiolites from the Bajgan Complex (Makran Accretionary Prism, SE Iran): New insights on the nature of the Early Cretaceous Middle East Neotethys
The Bajgan Complex in the North Makran Domain (Makran Accretionary Prism) comprises disrupted meta-ophiolitic sequences originating from oceanic crust protoliths. They include ultramafic and mafic cumulates, isotropic gabbros, plagiogranites, and basalts. Ultramafic-mafic cumulates and plagiogranites exhibit compositions akin to rocks formed in mid-ocean ridge settings. Isotropic gabbro and basalt protoliths can be subdivided in three distinct geochemical types. Type-1 rocks is sub-alkaline (Nb/Y < 0.1) with low Th, Nb, and Ta contents and La
N
/Yb
N
ratios <1, resembling those of normal-type (N-) mid-ocean ridge basalts (MORB). Type-2 rocks display slight enrichment in Th, Ta, Nb (Nb/Y = 0.36 – 0.45), and La
N
/Yb
N
= 2.12 – 3.20, resembling the chemistry of enriched-type (E-) MORB. Type-3 basalts show an alkaline nature (Nb/Y=0.88-1.82), significant Th, Ta, Nb enrichment, and high La
N
/Yb
N
ratios (7.01 – 20.08), resembling the chemistry of alkaline basalts (OIB). Petrogenetic modeling indicates that N-MORB protoliths originated from a depleted MORB mantle source, while E-MORB and OIB protoliths were generated from partial melting of sub-oceanic depleted sources that underwent varying degrees of OIB-type enrichment. The Bajgan meta-ophiolitic protoliths were formed within a Late Jurassic to Cretaceous oceanic basin influenced by mantle plume activity and plume-ridge interaction.
Thematic collection:
This article is part of the Ophiolites, melanges and blueschists collection available at:
https://www.lyellcollection.org/topic/collections/ophiolites-melanges-and-blueschists
Supplementary material:
https://doi.org/10.6084/m9.figshare.c.7193937