korsun’-novomyrhorod斜长岩- rapakivi花岗岩岩体主要岩石类型地球化学特征

IF 0.5 Q4 MINERALOGY Mineralogical Journal-Ukraine Pub Date : 2022-01-01 DOI:10.15407/mineraljournal.44.01.020
O. Dubyna, S. Kryvdik, I. Shvaika, I. Shvaika, P. Yakubenko, L. Proskurka
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引用次数: 2

摘要

本文考虑了Korsun -Novomyrhorod岩体大部分分布岩石的地球化学特征。所获得的资料使我们有理由认为,该岩体的基性岩和中间岩的结合是由于原生熔体的分异而形成的,其成分与高铝拉斑岩相似。推测斜长岩是斜长石结晶早期最早出现的岩石。斜长岩的稀土元素球粒陨石归一化模式具有典型的稀土元素分布特征,在低稀土浓度下具有明显的正eu异常。富含基性成分的残余熔体进一步演化可形成辉长岩斜长岩。辉长岩与辉长岩-辉长岩堆积物分离后,残余熔体结晶,形成分布较少的辉长岩和黑长岩。考虑到所有类型岩石中铁含量高,基性岩石是由与斜长岩有关的残余熔体结晶而成。但是,与大多数分布的基性岩不同,含矿岩(nosachiv型)是在早期形成的,因为长石和钛铁矿同时聚集,随后在岩浆室的较低水平发生了重力沉淀。二长岩-正长岩的成因则更加神秘。它们的地球化学特征与辉长岩中的地球化学特征非常相似,因此有理由认为它们是辉长岩和斜长岩体逸出后残余熔体结晶的结果。这些富钾熔体随后的迁移和长时间的分异会导致Velyka vyska型高铁正长岩的出现,这些正长岩富集REE、Y、Zr和部分Nb,而贫Sr和Ba。虽然其地球化学特征与二长岩具有明显的相似性,但其成因仍是一个问题。值得注意的是,我们的发现更符合由上升的基本成分侵入引起的大陆地壳融化。
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GEOCHEMICAL CHARACTERISTICS OF THE MAIN ROCKS TYPES OF THE KORSUN'-NOVOMYRHOROD ANORTHOSITE-RAPAKIVI GRANITE PLUTON
The geochemical features of most distributed rocks from the Korsun'-Novomyrhorod Pluton are considered. The obtained data give reason to assume that the association of basic and intermediate rocks of the pluton was formed because of the differentiation of the primary melt, similar in composition to high alumina tholeiites. It can be inferred that anorthosites were the earliest rocks that appeared in the early stages of plagioclase crystallization. The chondrite-normalized patterns of REE from anorthosites are characterized by the classical distribution of REE for such rocks, with significant positive Eu-anomalies at low REE concentrations. Further evolution of the residual melts enriched by mafic components could lead to the formation of gabbro-anorthosites. Less distributed gabbronorites and norites were formed because of crystallization of residual melts after segregation of anorthositic and gabbro-anorthositic cumulates. Considering the high iron content in all types of rocks, the basic rocks crystallized from residual melts that were genetically related to anorthosites. But ore-bearing norites (Nosachiv-type), in contrast to most distributed basic rocks, had been formed in the early stages because of simultaneous accumulation of feldspar and ilmenite, followed by gravitational precipitation at lower levels of magmatic chambers. The genesis of monzonite-syenite rocks is more enigmatic. Their geochemical features very resemble those in gabbroic rocks, which gives reason to consider them as a result of residual melts crystallization after escaping from anorthositic and gabbronoritic bodies. Subsequent migration and protracted differentiation of such K-enriched melts could cause the appearance of the high-Fe syenites of the Velyka Vyska-type, enriched in REE, Y, Zr, partially Nb, and depleted in Sr and Ba. Although the geochemical characteristics of rapakivi show significant similarities to monzonitic rocks, their genesis remains problematic. It's worth noting that our findings are more consistent with continental crust melting caused by ascending intrusions of basic composition.
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