Trace element geochemistry of mantle xenoliths from Zarnitsa kimberlite pipe, Daldyn field, Yakutia: Complex history of melts interactions with lithospheric mantle

I.V. Ashchepkov , N. Ntaflos , N.S. Medvedev , G.P. Shmarov
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Abstract

Mantle xenoliths from Zarnitsa pipe studied in gray eruptive breccias (early) brown autholitic breccia (BAB) and black macrocrystic kimberlites (last dike; BMK), include garnet and spinel dunites-harzburgites, pyroxenites, eclogites, glimmerites and megacrysts. PT reconstructions using xenoliths reveal sharply layered structure (8 levels), estimated with the single grain mineral estimates mark hot (Cpx, Ilm) and cold (OPx, Gar) inflected geotherm. The interaction with plume melts is found at the lithosphere asthenosphere boundary (LAB), pyroxenite layer (3-4 GPa), Gar-Sp transition and Moho. Eclogites reveal Fe# growth from LAB to middle pyroxenites layer. Clinopyroxenes and ilmenite estimates marks melt refertilisations in interlayers between coupled subduction slabs. Source of capture from first to third stage deepening to LAB and Cr- rich garnets (to 19.5 Cr2O3) are below the LAB.
The grey erupted breccia (GEB) includes mainly depleted and deformed peridotites. The later BAB includes pyroxenites, eclogites, and refertilised, deformed, and veined peridotites in BMK. Geochemistry of minerals changes from primary mid ocean ridge basalts (MORB) and back arc peridotites with low REE and large ion lithophile elements (LILE) and deeps in high field strength elements (HFSE) to metasomatized by alkaline (high Na and LILE) and adakitic melts (high Al, Na, Sr, and elevated HFSE) varieties and refertilised lherzolites due to plume at last stage. Mantle column metasomatized with scattered phlogopites in early grey eruptive breccia to amphibole-phlogopite ilmenite veins at last stages. Amphiboles trace mantle from lithosphere – asthenosphere boundary to Moho.
Growth of the diamond grade from early eruptive breccia to later kimberlite phases refer to decreasing of the crust material and deepening of the xenoliths capture level. Metasomatism dissolve the diamonds but growth of megacrystic diamond crystals increase diamond grade.

Abstract Image

来自雅库特达尔丁油田扎尔尼察金伯利岩管的地幔异岩石的微量元素地球化学:熔体与岩石圈地幔相互作用的复杂历史
在灰色喷发角砾岩(早期)、褐色自成角砾岩(BAB)和黑色巨晶金伯利岩(最后的堤坝;BMK)中研究了来自扎尔尼察岩管的地幔异长岩,其中包括石榴石和尖晶石云母-哈尔茨堡石、辉石、夕闪石、霞石和巨晶。利用异长岩进行的 PT 重建显示出明显的分层结构(8 层),并通过单颗粒矿物估算标记出热(Cpx、Ilm)和冷(OPx、Gar)偏转地温。在岩石圈星体层边界(LAB)、辉石层(3-4 GPa)、Gar-Sp 过渡和莫霍面发现了与羽流熔体的相互作用。蚀变岩显示了从岩石圈边界到中间辉绿岩层的铁#增长。霞石和钛铁矿的估计标志着耦合俯冲板块之间夹层中的熔体再充填。捕获源从第一阶段到第三阶段深化到 LAB,富铬石榴石(至 19.5 Cr2O3)位于 LAB 层以下。后期的 BAB 包括辉长岩、斜长岩以及 BMK 中的再营养、变形和脉状橄榄岩。矿物的地球化学发生了变化,从原生中洋脊玄武岩(MORB)和后弧橄榄岩(REE和大离子亲岩元素含量低,高场强元素含量深),到由碱性(高Na和大离子亲岩元素含量高)和赤铁矿熔体(高Al、Na、Sr和高HFSE)变质,以及在最后阶段由于羽流造成的再营养化橄榄岩。地幔柱变质,早期灰色喷发角砾岩中散布着辉绿岩,最后阶段变成闪石-辉绿岩钛铁矿脉。从早期的喷发角砾岩到后期的金伯利岩,金刚石品级的增长是由于地壳物质的减少和俘获异长岩程度的加深。变质作用溶解了金刚石,但巨晶金刚石晶体的生长提高了金刚石品位。
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