Remeshk-Mokhtarabad和Fannux-Maskutan蛇绿岩(伊朗东南部Makran增生棱镜)火山岩和岩脉的地球化学:中东新地球系岩浆生成的新限制

Emilio Saccani , Morteza Delavari , Asghar Dolati , Luca Pandolfi , Edoardo Barbero , Valentina Brombin , Michele Marroni
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引用次数: 5

摘要

Remeshk Mokhtarabad和Fannuj Maskutan蛇绿岩代表了北马克兰地区的两个主要蛇绿岩单元(马克兰增生棱镜)。这些蛇绿岩的火山岩和岩脉主要由玄武岩和罕见的玄武岩安山岩、安山岩和英安岩组成。在这两个蛇绿岩单元的玄武岩中,或者在火山岩和岩脉之间,都没有发现化学区别。玄武岩表现出广泛的MORB型性质,但化学成分可变(例如,SiO2=42.64–52.63 wt%;TiO2=0.98–2.43 wt%;Mg#=71–50)。它们显示出N-MORB(1型)和E-MORB(2型)的成分(MORB:中海脊玄武岩;N:正常;E:富集)。1型岩石在两个蛇绿岩单元中都非常罕见,而2型岩石占主导地位。1型岩石的Th(0.10–0.16 ppm)、Nb(1.86–2.82 ppm)、Ta(0.09–0.17 ppm)丰度较低,(La/Yb)N(0.50–0.75)、(La/Sm)N(0.48–0.72)比值较低。与N-MORB相比,2型玄武岩显示出Th(0.42–1.60 ppm)、Nb(6.09–14.6 ppm)和Ta(0.227–0.792 ppm)的轻微富集,以及(La/Yb)N和(La/Sm)N比率>;1,类似于在典型E-MORB中观察到的那些。微量元素岩石成因模型表明,原始玄武岩来源于由羽流型(OIB-)成分可变交代的非均质亚洋地幔的部分熔融。1型玄武岩来源于地幔区的部分熔融,不富集OIB型组分,而2型玄武岩则来源于不同OIB组分富集的DMM源的部分熔融。这些岩石形成于受地幔柱活动和不同程度的羽流-山脊相互作用强烈影响的洋盆中。
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Geochemistry of volcanic rocks and dykes from the Remeshk-Mokhtarabad and Fannuj-Maskutan Ophiolites (Makran Accretionary Prism, SE Iran): New constraints for magma generation in the Middle East neo-Tethys

The Remeshk-Mokhtarabad and Fannuj-Maskutan ophiolites represent two major ophiolitic units in the North Makran Domain (Makran Accretionary Prism). Volcanic rocks and dykes of these ophiolites mainly consist of basalts and rare basaltic andesites, andesites and dacites. No chemical distinction can be seen in basalts from these two ophiolitic units, or between volcanic rocks and dykes. Basaltic rocks show a broad MORB-type nature but variable chemical composition (e.g., SiO2= 42.64–52.63 wt%; TiO2= 0.98–2.43 wt%; Mg# = 71–50). They show both N-MORB (Type 1) and E-MORB (Type 2) compositions (MORB: mid-ocean ridge basalt; N: normal; E: enriched). Type 1 rocks are very rare in both ophiolitic units, whereas Type 2 rocks are predominant. Type 1 rocks show low Th (0.10–0.16 ppm), Nb (1.86–2.82 ppm), Ta (0.09–0.17 ppm) abundance and low (La/Yb)N (0.50–0.75), (La/Sm)N (0.48–0.72) ratios. Compared to N-MORBs, Type 2 basalts show slight enrichment in Th (0.42–1.60 ppm), Nb (6.09–14.6 ppm), and Ta (0.227–0.792 ppm), as well as (La/Yb)N and (La/Sm)N ratios >1 like those observed in typical E-MORB. Trace element petrogenetic models indicate that primitive basalts derived from partial melting of a heterogeneous sub-oceanic mantle variably metasomatized by plume-type (OIB-) components. Type 1 basalts derived from partial melting of mantle regions with no enrichment in OIB-type components, whereas Type 2 basalts derived from partial melting of DMM sources variably enriched by OIB-components. These rocks formed in an oceanic basin that was strongly affected by mantle plume activity and different extents of plume-ridge interaction.

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