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Condensate in Impact Glass Samples from the Lonar Crater, India 印度洛纳尔陨石坑撞击玻璃样品中的冷凝物
IF 1.5 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-03-21 DOI: 10.1134/S0869591123010046
T. A. Gornostaeva, A. V. Mokhov, A. P. Rybchuk, P. M. Kartashov

Polycomponent condensate glasses found in nature provide an insight into condensation mechanisms, which are still understood inadequately poorly. Condensate glasses found in the impactites of the Lonar crater contain nanosized inclusions of metallic Fe, Cr, Cu, Zn, Ag, In, Te, Au, Pt, and Bi, along with Fe, Cu, and Zn sulfides. This combination may be indicative either of a brief condensation window for the almost simultaneous condensation of components with so different fugacity or of a possible mechanism of cluster condensation, provided that the condensation temperatures of such clusters are close.

在自然界中发现的多组分冷凝玻璃提供了对冷凝机制的深入了解,这些机制仍然不够充分。在月球陨石坑的撞击物中发现的冷凝玻璃含有纳米大小的金属铁、铬、铜、锌、银、银、碲、金、铂和铋,以及铁、铜和锌的硫化物。这种组合可能表明,具有如此不同逸度的组分几乎同时凝结的短暂凝结窗口,或可能的团簇凝结机制,只要这些团簇的凝结温度接近。
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引用次数: 0
Crystallization Parameters, Genesis of Melts, and Sources of Magmas of the Late Cenozoic Udokan Volcanic Plateau, Central Asia 中亚晚新生代乌多坎火山高原结晶参数、熔体成因及岩浆来源
IF 1.5 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-03-21 DOI: 10.1134/S0869591123010101
V. V. Yarmolyuk, V. M. Savatenkov, A. M. Kozlovsky, F. M. Stupak, M. V. Kuznetsov, L. V. Shpakovich

Similar to the other areas of the Late Cenozoic volcanic province of Central Asia, the Udokan volcanic plateau (UVP) was formed in the time span between the Middle Miocene and the Pleistocene. Its rocks are highly alkaline and vary from alkaline picrobasalts and basanites to alkaline trachytes. The compositional variations of the rocks were controlled by two differentiation trends, which corresponded to different generation conditions of the parental magmas. The rocks with low SiO2 contents (<45 wt %) were formed by melts of low degrees of melting, whose melts were derived under elevated pressures and temperatures. The formation of the rocks with 45–61 wt % SiO2 was associated with the differentiation of basalt melts, which were derived at shallower depths and at lower temperatures. The geochemical characteristics of the UVP basaltoids make them similar to OIB-type basalts. They are also close in Sr, Nd, and Pb isotopic composition, corresponding to the parameters of the moderately depleted mantle, which is close to the composition of oceanic basalt sources corresponding to the mantle of deep mantle plumes. The corresponding mantle component is present in the sources of other volcanic regions of the Late Cenozoic intraplate volcanic province in Central Asia, which indicates that the material of a lower mantle plume was involved in the formation of these regions.

与中亚晚新生代火山省的其他地区相似,乌多坎火山高原形成于中中新世至更新世之间。其岩石呈高碱性,从碱性微玄武岩和玄武岩到碱性粗叶岩不一而足。岩石成分的变化受两种分异趋势的控制,这两种分异趋势对应于母岩浆的不同生成条件。低SiO2含量(45 wt %)的岩石是由低熔融程度的熔体形成的,这些熔体是在高压和高温下形成的。SiO2含量为45 ~ 61 wt %的岩石的形成与玄武岩熔体的分异有关,这些熔体来源于较浅的深度和较低的温度。UVP玄武岩的地球化学特征与obb型玄武岩相似。Sr、Nd、Pb同位素组成接近,与中贫地幔参数相对应,与深部地幔柱相对应的洋玄武岩源组成接近。中亚晚新生代板内火山省其它火山岩源区中均存在相应的地幔成分,表明这些地区的形成中有下地幔柱物质参与。
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引用次数: 0
Ti and Cr in High-Pressure Mica: Experimental Study and Application to the Mantle Assemblages 高压云母中Ti和Cr的实验研究及其在地幔组合中的应用
IF 1.5 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-03-21 DOI: 10.1134/S0869591123010113
A. A. Bendeliani, A. V. Bobrov, L. Bindi, N. N. Eremin

Experiments aimed at the synthesis of Cr- and Ti-bearing phlogopite in the silicate-carbonate systems peridotite—K2CO3 + H2O and basalt—K2CO3 + H2O at 7 GPa and 900–1200°С were carried out. It is shown that the crystallization of titanium-bearing phlogopite requires subducted crustal material at mantle depths. However, the mantle peridotite should predominate over basalt for Ti-phlogopite crystallization; otherwise, dioctahedral mica (aluminoceladonite) with (Mg + Fe)/VIAl > 1 is formed via the scheme 2VIAl = VITi4+ + VI(Mg + Fe). The competitive behavior of Ti and Cr upon incorporation into phlogopite is considered. It is shown that the presence of >1.3 wt % TiO2 introduces a limitation on the high concentrations of Cr2O3 via the scheme VI(Mg2+) + IV(Si4+) = VI(Cr3+) + IV(Al3+). This can explain the compositional patterns of phlogopite from inclusions in natural diamonds, in which the Ti content is much higher than that of Cr. The results obtained support the original idea that the composition of phlogopite may be applied to distinguish the paragenetic associations of diamond.

在7 GPa、900 ~ 1200°С温度条件下,在硅酸盐-碳酸盐体系中,橄榄岩- k2co3 + H2O和玄武岩- k2co3 + H2O中合成了含Cr和含ti的云母。结果表明,含钛云母的结晶需要地幔深处俯冲的地壳物质。而在钛辉云母结晶过程中,地幔橄榄岩占主导地位,玄武岩占主导地位;反之,二八面体云母(铝钙石)与(Mg + Fe)/VIAl >1由方案2VIAl = VITi4+ + VI(Mg + Fe)组成。考虑了钛和铬掺入银云母后的竞争行为。结果表明,当掺杂>1.3 wt % TiO2时,通过VI(Mg2+) + IV(Si4+) = VI(Cr3+) + IV(Al3+)的方案限制了Cr2O3的高浓度。这可以解释天然金刚石中钛含量远高于铬含量的包裹体中金云母的组成模式。所得结果支持了用金云母的组成来区分金刚石共生组合的最初想法。
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引用次数: 0
The Monticellite-bearing Rocks of the Krestovskaya Intrusion: Genesis according to Melt Inclusion Study 克列斯托夫斯卡亚岩体含蒙地长辉石岩:熔融包裹体研究的成因
IF 1.5 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-03-21 DOI: 10.1134/S0869591123010071
L. I. Panina, A. T. Isakova, E. Yu. Rokosova

The investigation of monticellitolites and olivine–monticellite rocks from the Krestovskaya Intrusion shows that the major minerals (olivine and monticellite) have higher MgO content than the same minerals in olivinites and kugdites of the intrusion. In the studied rocks olivine contains 90–93 mol % Fo and monticellite has 41.6–42.3 mol % Fo, whereas olivine and monticellite in olivinites and kugdites contain 86–87 and 37.2–41.2 mol % Fo, respectively. Melt inclusion study in minerals of monticellite rocks demonstrates that the monticellite rocks of the Krestovskaya Intrusion were formed by mixing of volatile-rich melts of different composition: K-rich high-iron low-alumina kamafugitic melt and Na-rich high-magnesium high-alumina picritic melt. Minerals crystallized at high temperatures in the following sequence: perovskite I (1250–1230°C) → perovskite II (≥1200°C) ↔ olivine (>1200°C) → monticellite (>1150°C). Perovskite I in monticellite rocks, as well as olivine in olivinites, crystallized from K-rich high-iron (Mg# = MgO/(MgO + FeO) = 0.37), low-alumina kamafugitic melt. During crystallization of late perovskite II in the monticellite rocks, the melt became more enriched in MgO (Mg# = 0.41) and richer in Na2O and Al2O3, which is intermediate in composition between kamafugite and alkali picrite. Olivine in the monticellite rocks crystallized from melts similar in composition to melilitite, having a K-rich composition with Mg# = 0.39, whereas monticellite formed from a heterogeneous high-Mg Si-undersaturated melt, which is highly enriched with volatile components (including H2O) and salts. The crystallization of minerals was accompanied by subsequent accumulation of volatile components in mixing melts, silicate–carbonate liquid immiscibility under 1250–1190°C, and polyphase carbonate–salt immiscibility under below 1190°C. In the latter event, the exsolved carbonate melt began to split into simpler immiscible fractions: alkali–sulfate–carbonate, alkali–phosphate–carbonate, and calcio–carbonate.

对克列斯托夫斯卡亚侵入岩的蒙长石和橄榄石-蒙长石岩石的研究表明,其主要矿物(橄榄石和蒙长石)的MgO含量高于侵入岩的橄榄岩和孔德岩中的相同矿物。研究岩石中橄榄石的Fo含量为90 ~ 93 mol %, monticellite的Fo含量为41.6 ~ 42.3 mol %,而橄榄岩中的橄榄石和铜榴石中的monticellite的Fo含量分别为86 ~ 87和37.2 ~ 41.2 mol %。蒙脱石岩石矿物熔体包裹体研究表明,Krestovskaya岩体的蒙脱石岩石是由富钾高铁低铝马马辉石熔体和富钠高镁高铝苦辉石熔体这两种不同组成的富挥发物混合形成的。矿物在高温下的结晶顺序如下:钙钛矿I(1250 ~ 1230℃)→钙钛矿II(≥1200℃)↔橄榄石(>1200℃)→蒙蒂石(>1150℃)。钙钛矿I和橄榄石中的橄榄石由富钾高铁(Mg# = MgO/(MgO + FeO) = 0.37)、低铝马马辉石熔体结晶而成。钙钛矿II型晚期钙钛矿在蒙脱石中结晶过程中,熔体中MgO (Mg# = 0.41)含量增加,Na2O和Al2O3含量增加,介于卡玛辉石和碱苦铁铁矿之间。monticellite岩石中的橄榄石是由组成类似于melmelite的熔体结晶而成,具有富k组成,Mg# = 0.39,而monticellite则是由非均质高Mg si欠饱和熔体结晶而成,其挥发性成分(包括H2O)和盐高度富集。矿物结晶过程伴随着挥发性组分在混合熔体中的积累,在1250 ~ 1190℃范围内硅酸盐-碳酸盐液体不混相,在1190℃以下范围内碳酸盐-盐多相不混相。在后一种情况下,溶解的碳酸盐熔体开始分裂成更简单的不可混溶的部分:碱-硫酸盐-碳酸盐、碱-磷酸盐-碳酸盐和碳酸钙。
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引用次数: 0
Staurolite in Metabasites: P–T–X Parameters and the Ratios of Major Components as Criteria of Staurolite Stability 变质岩中的小晶石:P-T-X参数和主要成分比值作为小晶石稳定性的判据
IF 1.5 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-03-21 DOI: 10.1134/S0869591123010034
E. B. Borisova, Sh. K. Baltybaev, J. A. D. Connolly

Fe–Mg staurolite is a typical and widespread mineral of medium-temperature high-alumina metapelites, whereas magnesian staurolite is only relatively rarely found in metamorphosed mafic rocks (metabasites). The most significant factors controlling staurolite stability in metabasites were identified by thermodynamic modeling and analysis of the common features of the mineral-forming processes. In contrast to staurolite in low- and medium-pressure metapelites, staurolite in metabasites is stable at medium- and high-pressure metamorphism. An increase in the proportion of carbon dioxide in the water–carbon dioxide fluid shifts the staurolite-forming mineral reactions to lower temperatures and higher pressures. Al, Fe, Mg, and Ca are the major components of rocks that are critically important for the formation of magnesian staurolite in these rocks, and the contents and ratios of these components are of crucial importance for the stability of staurolite in metabasites. To understand the processes forming the mineral in metabasites, it is instrumental to subdivide metabasites into subgroups of predominantly magnesian, ferruginous–magnesian, and ferruginous protoliths. With regard to this subdivision, three petrochemical modules are proposed in the form of ratios of major components: MgO/CaO, CaO/FM, and Al2O3/FM, based on which it is possible to predict the stability of staurolite in mafic rocks at appropriate P–T parameters of metamorphism.

铁镁双晶石是中温高铝偏长岩中常见的典型矿物,镁质双晶石仅在变质基性岩(变质岩)中相对较少发现。通过热力学模拟和矿物形成过程的共同特征分析,确定了控制变质岩中橄榄石稳定性的最重要因素。相对于中、低压变质岩中的橄榄石,变质岩中的橄榄石在中、高压变质作用下是稳定的。水-二氧化碳流体中二氧化碳比例的增加使形成星黄岩的矿物反应转向更低的温度和更高的压力。Al、Fe、Mg和Ca是岩石的主要成分,它们对镁质小沸石的形成起着至关重要的作用,其含量和比例对变质岩中小沸石的稳定性起着至关重要的作用。为了了解变质岩中矿物的形成过程,将变质岩细分为主要为镁质原岩、含铁-镁质原岩和含铁原岩的亚群是很有帮助的。在此基础上,提出了MgO/CaO、CaO/FM和Al2O3/FM三个主要组分比值的石化模块,并以此为基础,在适当的变质P-T参数下,预测基性岩中橄榄石的稳定性。
{"title":"Staurolite in Metabasites: P–T–X Parameters and the Ratios of Major Components as Criteria of Staurolite Stability","authors":"E. B. Borisova,&nbsp;Sh. K. Baltybaev,&nbsp;J. A. D. Connolly","doi":"10.1134/S0869591123010034","DOIUrl":"10.1134/S0869591123010034","url":null,"abstract":"<p>Fe–Mg staurolite is a typical and widespread mineral of medium-temperature high-alumina metapelites, whereas magnesian staurolite is only relatively rarely found in metamorphosed mafic rocks (metabasites). The most significant factors controlling staurolite stability in metabasites were identified by thermodynamic modeling and analysis of the common features of the mineral-forming processes. In contrast to staurolite in low- and medium-pressure metapelites, staurolite in metabasites is stable at medium- and high-pressure metamorphism. An increase in the proportion of carbon dioxide in the water–carbon dioxide fluid shifts the staurolite-forming mineral reactions to lower temperatures and higher pressures. Al, Fe, Mg, and Ca are the major components of rocks that are critically important for the formation of magnesian staurolite in these rocks, and the contents and ratios of these components are of crucial importance for the stability of staurolite in metabasites. To understand the processes forming the mineral in metabasites, it is instrumental to subdivide metabasites into subgroups of predominantly magnesian, ferruginous–magnesian, and ferruginous protoliths. With regard to this subdivision, three petrochemical modules are proposed in the form of ratios of major components: MgO/CaO, CaO/FM, and Al<sub>2</sub>O<sub>3</sub>/FM, based on which it is possible to predict the stability of staurolite in mafic rocks at appropriate <i>P–T</i> parameters of metamorphism.</p>","PeriodicalId":20026,"journal":{"name":"Petrology","volume":"30 1","pages":"S53 - S71"},"PeriodicalIF":1.5,"publicationDate":"2023-03-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"4829855","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Grenville and Valhalla Tectonic Events at the Western Margin of the Siberian Craton: Evidence from Rocks of the Garevka Complex, Northern Yenisei Range, Russia 西伯利亚克拉通西缘的Grenville和Valhalla构造事件:来自俄罗斯叶尼塞山脉北部Garevka杂岩的证据
IF 1.5 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-03-21 DOI: 10.1134/S0869591123010058
I. I. Likhanov

Understanding the tectonic evolution of the Yenisei Range offers important clues not only for the tectonic evolution of orogenic belts at margins of ancient cratons but also for solving the problem of the incorporation of the Siberian craton into the Rodinia supercontinent. Results of mineralogical−petrological, geochemical, and isotope–geochemical studies provide an insight into the petrogenesis, geotectonic settings, thermodynamic parameters of formation, and the ages of the metamorphism and protoliths for the contrastingly compositionally different rocks of the Garevka metamorphic complex. The paper discusses the possible models for the origin of the rock complexes and the geodynamic settings in which they were formed. The western margin of the Siberian craton was determined to have been affected by two pulses of Neoproterozoic endogenic activity, which were related to the origin of the Rodinia supercontinent (930–900 and 880–845 Ma), and which correlated with Grenville and post-Grenville processes responsible for Valhalla folding. The regional geodynamic history is correlated with the coeval sequence and similar style of tectono−thermal events in the peripheries of the large Precambrian cratons Laurentia and Baltica, which is consistent with the proposed Neoproterozoic paleogeographic reconstructions of close spatiotemporal relationships between these cratons and their incorporation into Rodinia configuration.

了解叶尼塞山脉的构造演化,不仅为古克拉通边缘造山带的构造演化提供了重要线索,而且为解决西伯利亚克拉通并入罗迪尼亚超大陆的问题提供了重要线索。矿物-岩石学、地球化学和同位素-地球化学研究的结果,为了解Garevka变质杂岩的岩石成因、大地构造背景、形成的热力学参数以及变质作用和原岩的年龄提供了依据。本文讨论了杂岩的可能成因模式及其形成的地球动力学背景。西伯利亚克拉通西缘受两次新元古代内生活动的影响,这两次内生活动与Rodinia超大陆的起源(930-900和880-845 Ma)有关,并与导致Valhalla褶皱的Grenville和后Grenville过程相关。区域地球动力学历史与Laurentia和Baltica大型前寒武纪克拉通周缘的同期序列和相似的构造-热事件类型相关联,这与新元古代古地理重建所提出的这两个克拉通与它们并入Rodinia构造之间密切的时空关系相一致。
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引用次数: 1
Carbonation of Serpentinites of the Mid-Atlantic Ridge: 1. Geochemical Trends and Mineral Assemblages 大西洋中脊蛇纹岩的碳酸化作用:1。地球化学趋势与矿物组合
IF 1.5 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2023-03-21 DOI: 10.1134/S0869591123010095
S. A. Silantyev, E. A. Krasnova, D. D. Badyukov, A. V. Zhilkina, T. G. Kuzmina, A. S. Gryaznova, V. D. Shcherbakov

Abyssal peridotite outcrops compose vast areas of the ocean floor in the Atlantic, Indian, and Arctic Oceans, where they are an indispensable part of the oceanic crust section formed in the slow-spreading oceanic ridges (Mid-Atlantic Ridge, Southwest Indian Ridge, and Gakkel Ridge). The final stage in the evolution of abyssal peridotites in the oceanic crust is their carbonation, which they experience on the ocean floor surface or near it. The main goal of this study was to reconstruct the geochemical trends accompanying the carbonation of abyssal peridotites using MAR ultramafic rocks as an example and to identify the main factors that determine their geochemical and mineralogical differences. The composition variations of rock-forming minerals and their characteristic assemblages indicate that the initial stages of carbonation of abyssal peridotites occurred in crustal conditions simultaneously with the serpentinization of these rocks. The final stage in the crustal evolution of the abyssal peridotites is their exhumation on the ocean floor where they were brought up along the detachment faults. On the ocean floor, the abyssal peridotites in close association with gabbro form oceanic core complexes, and the degree of their carbonation sharply increases with time of their exposure on the ocean floor. The presented data made it possible to qualitatively reconstruct the sequence of events that determined the mineralogical and geochemical features of carbonatized abyssal peridotites of the MAR.

深海橄榄岩露头构成了大西洋、印度洋和北冰洋海底的大片区域,它们是缓慢扩张的海洋脊(大西洋中脊、西南印度洋脊和Gakkel脊)形成的海洋地壳部分不可或缺的一部分。海洋地壳中深海橄榄岩演化的最后阶段是它们在海底表面或海底附近经历的碳酸化。以MAR超镁质岩为例,重建深海橄榄岩碳酸化过程中的地球化学趋势,并找出影响其地球化学和矿物学差异的主要因素。造岩矿物组成变化及其特征组合表明,深海橄榄岩碳酸化的初始阶段与蛇纹岩化同时发生在地壳条件下。深海橄榄岩地壳演化的最后阶段是它们在海底的发掘,它们是沿着拆离断层被带上来的。在海底,与辉长岩密切联系的深海橄榄岩形成海洋岩心杂岩,其碳酸化程度随着暴露时间的增加而急剧增加。所提供的数据使定性地重建事件序列成为可能,这些事件序列决定了MAR碳酸化深海橄榄岩的矿物学和地球化学特征。
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引用次数: 0
The Great Dyke of the Kola Peninsula as a Marker of an Archean Cratonization in the Northern Fennoscandian Shield 科拉半岛大堤作为芬诺斯坎地盾北部太古宙克拉通化的标志
IF 1.5 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2022-11-15 DOI: 10.1134/S086959112206008X
A. V. Stepanova, A. V. Samsonov, E. B. Salnikova, S. V. Egorova, Yu. O. Larionova, A. A. Arzamastsev, A. N. Larionov, M. A. Sukhanova, R. V. Veselovskiy

The results of geochronological and petrological studies of the largest mafic dyke in the northern part of the Fennoscandian Shield, called the Great Dyke of the Kola Peninsula (GDK), are presented. According to U-Pb D-TIMS baddeleyite dating, the GDK crystallization age is 2680 ± 6 Ma. The age of host granites is 2.75–2.72 Ga (U-Pb, zircon, SHRIMP-II). The dyke has a simple internal structure with no signs of multistage melt injection. It comprises equigranular and plagioclase-porphyritic dolerites and gabbro that are amphibolitized to varying degrees. All rocks are low-Mg (Mg# less than 0.37) with low concentrations of Cr and Ni, and were derived through differentiation of more primitive melts. The analysis of geochemical and Sr-Nd isotopic data suggests that GDK melts could be formed by mixing of two types of mantle melts: depleted asthenospheric melt and enriched melt formed via melting of a lithospheric mantle. The weakly fractionated HREE patterns indicate that primary GDK melts originated at shallow (<60 km) depths outside the garnet stability field. The generation and injection of melts of the Neoarchean GDK occurred immediately after large-scale granitic magmatism and main crustal growth event in the Murmansk Craton and marked the cratonization of the continental lithosphere in the northeastern part of the Fennoscandian Shield.

本文介绍了芬诺斯坎地盾北部最大的基性堤坝——科拉半岛大堤(GDK)的年代学和岩石学研究结果。根据U-Pb D-TIMS bad - yite测年,GDK的结晶年龄为2680±6 Ma。寄主花岗岩年龄为2.75 ~ 2.72 Ga (U-Pb、锆石、SHRIMP-II)。岩脉内部结构简单,没有多级熔体注入的迹象。由不同程度角闪化的等粒状和斜长状斑岩白云岩和辉长岩组成。所有岩石均为低Mg (Mg# < 0.37),含低浓度的Cr和Ni,由更原始的熔体分异而成。地球化学和Sr-Nd同位素数据分析表明,GDK熔体可能是由两种类型的地幔熔体混合形成的:贫软流圈熔体和由岩石圈地幔熔融形成的富集熔体。弱分馏的ree模式表明初生GDK熔体起源于石榴石稳定场外的浅层(<60 km)深度。新太古代GDK熔体的生成和注入发生在摩尔曼斯克克拉通大规模花岗岩岩浆活动和主要地壳生长事件之后,标志着芬诺斯坎德盾东北部大陆岩石圈的克拉通化。
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引用次数: 0
А History of Coronitic Metagabbronorites in the Belomorian Province, Fennoscandian Shield: U-Pb (CA-ID-TIMS) Dating of Zircon–Baddeleyite Aggregates А Fennoscandian地盾Belomorian省冠状变辉长岩的历史:锆石- baddeleite聚落的U-Pb (CA-ID-TIMS)定年
IF 1.5 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2022-11-15 DOI: 10.1134/S0869591122060066
E. B. Salnikova, A. V. Stepanova, P. Ya. Azimov, M. A. Sukhanova, A. B. Kotov, S. V. Egorova, Yu. V. Plotkina, E. V. Tolmacheva, A. V. Kervinen, N. V. Rodionov, V. S. Stepanov

The estimation of crystallization and metamorphic reworking ages of mafic rocks in the polycyclic Precambrian areas is a difficult problem. Magmatic baddeleyite can be partially or completely replaced by polycrystalline zircon within a wide range of temperature and pressures, from greenschist to granulite facies. Evaluation of the age of each phase of the zircon–baddeleyite aggregates can provide information on both the age of the magmatic crystallization and metamorphism. U-Th-Pb (SHRIMP-II) and U-Pb (ID-TIMS) geochronological studies were carried out for single baddeleyite grains and zircon–baddeleyite aggregates from gabbronorites (“drusites”) of the Ambarnsky massif (Belomorian Province, Fennoscandian Shield). The petrological studies indicate the simultaneous growth of coronas at the olivine–plagioclase boundary and zircon rims around baddeleyite. U-Pb (ID-TIMS) dating of single baddeleyite grains yielded 2411 ± 6 Ma crystallization age of gabbronorites of the Ambarnsky massif. U-Pb (ID-TIMS) dating coupled with the discrete chemical abrasion give an age of 1911 ± 35 Ma for metamorphic zircon rims. The obtained results indicate that coronitic textures in the gabbronorites were formed 500 million years later than the magmatic crystallization of rocks as a result of the granulite-facies metamorphism that was probably related to the Lapland-Kola orogeny.

多旋回前寒武纪地区基性岩结晶和变质改造时代的确定是一个难题。从绿片岩到麻粒岩相,多晶锆石在温度和压力范围内均可部分或完全取代岩浆坏辉岩。对锆石-坏辉石集合体各相年龄的评价可以提供岩浆结晶和变质作用年龄的信息。对Fennoscandian地盾省Belomorian省Ambarnsky地块辉长岩(“drusites”)中的单个坏辉长岩颗粒和锆石-坏辉长岩聚集体进行了U-Th-Pb (SHRIMP-II)和U-Pb (ID-TIMS)年代学研究。岩石学研究表明,在橄榄石-斜长石边界和坏长岩周围的锆石边缘同时生长。U-Pb (ID-TIMS)定年法测定了Ambarnsky地块辉长岩的结晶年龄(2411±6 Ma)。U-Pb (ID-TIMS)测年与离散化学磨损相结合,确定变质锆石的年龄为1911±35 Ma。结果表明,辉长岩中的冕状结构形成时间比岩石岩浆结晶晚5亿年,其成因可能与拉普兰—科拉造山运动有关。
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引用次数: 2
Eocene Calc-Alkaline Volcanic Rocks from Central Iran (Southeast of Khur, Isfahan Province); an Evidence of Neotethys Syn-Subduction Magmatism 伊朗中部(伊斯法罕省Khur东南部)始新世钙碱性火山岩新特提斯同步俯冲岩浆活动的证据
IF 1.5 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2022-11-15 DOI: 10.1134/S0869591122060042
Paniz Shadman, Ghodrat Torabi, Tomoaki Morishita

Eocene volcanic rocks with basaltic-trachyandesite and trachybasalt composition which cross-cut the Cretaceous sedimentary rocks, are exposed in the northwestern part of the Central-East Iranian Microcontient (CEIM) (SE of Khur, Isfahan Province, Iran). The rock-forming minerals of these volcanic rocks are olivine (chrysolite and hyalosiderite, Mg# = 0.69–0.71), clinopyroxene (augite with Mg# = 0.74–0.84), orthopyroxene (enstatite with Mg# = 0.61–0.62) and plagioclase (andesine and labradorite with An48.3-65.1). Phenocrysts set in a fine-grained matrix of the same minerals plus sanidine (Or59.1Ab36.6An4.3) with minor amounts of opaque minerals (magnetite and ilmenite). Secondary minerals are chlorite and calcite. The main textures of these volcanic rocks are porphyritic, microlitic porphyritic, poikilitic, and glomeroporphyritic. The Eocene volcanic rocks of the Khur area are characterized by SiO2 content of 51.8 to 54.9 wt %, Al2O3 amounts of 14.35 to 16.47 wt %, and TiO2 values of 0.88 to 0.92 wt %. They exhibit strong enrichment in light rare earth elements (LREE) relative to heavy REE (HREE) (La/Lu ratio up to 102.35), enrichment in large ion lithophile elements (LILEs), depletion in high field strength elements (HFSE), and present negative anomaly in Eu (Eu/Eu* = 0.72–0.87). Chemical characteristics and homogeneity of these volcanic rocks reveal their calc-alkaline nature and suggest that they were derived from a same parental magma and underwent a similar melt extraction. Major and trace elements geochemical features of the analyzed samples indicate that the parental magma was possibly derived from relatively low degrees of partial melting of a mantle wedge spinel lherzolite which was previously enriched by fluids/melts released from the Neo-Tethyan subducted slab.

在伊朗中东部微大陆(伊朗伊斯法罕省Khur东南)西北部,暴露出与白垩系沉积岩相交叉的玄武岩-粗面玄武岩和粗面玄武岩组成的始新世火山岩。这些火山岩的造岩矿物为橄榄石(黄璧石和透明黄铁矿,Mg# = 0.69 ~ 0.71)、斜辉石(辉石,Mg# = 0.74 ~ 0.84)、正辉石(顽辉石,Mg# = 0.61 ~ 0.62)和斜长石(安长石和拉长石,Mg# = 48.3 ~ 65.1)。斑晶镶嵌在由相同矿物加水晶石(Or59.1Ab36.6An4.3)和少量不透明矿物(磁铁矿和钛铁矿)组成的细粒基质中。次生矿物为绿泥石和方解石。这些火山岩的主要结构为斑岩、微岩屑斑岩、斑岩和肾小球斑岩。呼尔地区始新世火山岩的SiO2含量为51.8 ~ 54.9 wt %, Al2O3含量为14.35 ~ 16.47 wt %, TiO2含量为0.88 ~ 0.92 wt %。它们表现出轻稀土元素(LREE)相对重稀土元素(HREE)的强富集(La/Lu比值高达102.35),大离子亲石元素(LILEs)富集,高场强元素(HFSE)亏缺,Eu呈负异常(Eu/Eu* = 0.72 ~ 0.87)。这些火山岩的化学特征和均匀性揭示了它们的钙碱性特征,表明它们起源于相同的母岩浆,并经历了相似的熔融提取过程。分析样品的主要元素和微量元素地球化学特征表明,母岩浆可能来源于地幔楔尖晶石橄榄岩相对较低程度的部分熔融,该岩浆先前被新特提斯俯冲板块释放的流体/熔体富集。
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Petrology
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