Geochemistry of Xenoliths in Rapakivi Granites of the Korsun-Novomyrhorod Pluton (Ukrainian Shield)

IF 0.5 Q4 MINERALOGY
K.Ye. Shniukova, L. Tomurko, N. Konoval
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Abstract

Rapakivi of the Korsun-Novomyrhorod pluton (KNP), being the latest Precambrian granites of the central part of the Ukrainian shield, contain older acidic and intermediate rocks as xenoliths, the geochemical features of which reflect the Early Proterozoic geodynamic situation. Rapakivi granites, their differentiates and three types of xenoliths in them, represented by plagiogneiss, pink granite and charnockitoid (mangerite), were selected in the northwestern part of the KNP for geochemical studies. Analysis findings were compared with the geochemical characteristics of similar rocks of igneous and metamorphic Precambrian complexes that surround the KNP and could serve as a source of xenoliths. Based on distribution patterns of rare earth elements, lithophile elements content and their ratios relations in the rocks, taking into account their petrographic composition, it was established that plagiogneiss belongs to the upper part of the Inhul-Inhulets series, pink granite belongs to the Kirovohrad complex, and charnokitoid belongs to the intermediate rocks of the Tashlyk complex. In the latter, acid charnockitoids (enderbites) are probably younger than intermediate ones and were formed in another geodynamic setting. Pink granite, like the granites of the Kirovohrad complex, shows collisional geochemical features, in contrast to the rapakivi granites containing these xenoliths, which have predominantly within-plate geochemical characteristics. Thus, in the form of xenoliths in rapakivi those rocks were preserved that had been generated before and during the collision that occurred about 2 billion years ago and constructed a crust thickening at the site of the Inhul megablock, under subsequent extension of which about 1.75 billion years ago the KNP was intruded. Acid charnockitoids of the Tashlyk complex and rocks of the Novoukrainian complex, which are absent in xenoliths, probably were formed after the collision.
korsun - novmyrhorod岩体Rapakivi花岗岩中包体地球化学特征
Korsun-Novomyrhorod岩体(KNP)的Rapakivi是乌克兰盾中部最新的前寒武纪花岗岩,其包体中含有较古老的酸性和中间岩石,其地球化学特征反映了早元古代的地球动力学状况。选取了华北西北地区的Rapakivi花岗岩及其分异体及其中以斜长麻岩、粉红花岗岩和绿斑岩(锰矿)为代表的3种捕虏体进行地球化学研究。分析结果与围绕KNP的火成岩和变质前寒武纪杂岩的类似岩石的地球化学特征进行了比较,这些岩石可以作为捕虏体的来源。根据岩石中稀土元素的分布规律、亲石元素含量及其比值关系,结合岩石学组成,确定斜长岩属于因胡尔—因胡莱特系列的上部,粉红色花岗岩属于基罗沃拉德杂岩,恰诺奇似岩属于塔什莱克杂岩的中间岩。在后者中,酸性类绿腐岩(endenbite)可能比中间类绿腐岩更年轻,形成于另一个地球动力学环境。粉红色花岗岩,如Kirovohrad杂岩的花岗岩,显示出碰撞地球化学特征,与含有这些包体的rapakivi花岗岩形成鲜明对比,后者主要具有板块内地球化学特征。因此,以rapakivi捕虏体的形式,这些岩石被保存下来,这些岩石是在大约20亿年前发生碰撞之前和碰撞期间产生的,并在Inhul巨锁的遗址上形成了地壳增厚,在随后的扩展下,大约17.5亿年前KNP被侵入。在捕虏体中不存在的Tashlyk杂岩和novoukukian杂岩的酸性类炭黑岩可能是在碰撞后形成的。
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CiteScore
0.70
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