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Assessment of Soil Cover Geochemical Composition in the Technogenically Altered Territory of the Pioneer Gold Deposit (Upper Amur Region) 评估先锋金矿床(上阿穆尔州)技术改造区域的土壤覆盖层地球化学成分
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-04-04 DOI: 10.1134/S0016702924700873
V. I. Radomskaya, L. M. Pavlova, N. V. Moiseenko, M. Yu. Lyapunov, D. V. Yusupov

The results of geochemical studies of soils and anthropogenic grounds within the territory of the large Pioneer gold ore deposit developed in the Amur Region are presented. Using the enrichment indices for the soil and ground cover of the Pioneer deposit territory, the following pollutant elements were determined: As, Sb, Mo, Bi, W, S, Cd, and Pb. Using the methods of mathematical statistics, the background contents of As, Sb, Bi, Mo, W, S, Cd, and Pb in the technogenically transformed territory at the sampling time accounted for 63, 8.84, 0.69, 3.54, 4.19, 529, 0.11, and 36.5 mg/kg, respectively. The exceedance of background values for As, Sb, Bi, Mo, W, and S is caused by the natural metallogenic features of the territory. It has been established that the sources of metal emissions into the environment are mining facilities and structures of the mining complex: quarries, waste dumps, heap leaching areas, gold extraction plant, and tailings dumps.

本文介绍了阿穆尔河地区大型先锋金矿床境内土壤和人为土壤地球化学研究的结果。利用先锋矿区土壤和地被物富集指数,确定了污染元素As、Sb、Mo、Bi、W、S、Cd和Pb。采用数理统计的方法,采样时技术转化区As、Sb、Bi、Mo、W、S、Cd、Pb的背景含量分别为63、8.84、0.69、3.54、4.19、529、0.11、36.5 mg/kg。As、Sb、Bi、Mo、W、S的背景值超标是由本区的自然成矿特征所致。已经确定,进入环境的金属排放的来源是采矿设施和采矿综合体的结构:采石场、废物倾倒场、堆浸出区、黄金提取厂和尾矿倾倒场。
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引用次数: 0
Formation Conditions of Gold Mineralization in the Spokoininsky Ore Cluster, Aldan Shield, Russia 俄罗斯Aldan地盾spokininsky矿群金矿化形成条件
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-02-25 DOI: 10.1134/S0016702924700824
V. N. Kardashevskaia, L. A. Kondratieva, E. O. Shaparenko, G. S. Anisimova

The paper presents the first data on individual fluid inclusions hosted in quartz in the ores of three types (polysulfide, gold–silver–telluride, and gold–bismuth) of the Spokoininsky ore cluster with gold ore mineralization. The three ore types show differences in the physicochemical parameters and composition of their fluids. The fluid of the Spokoininsky cluster polysulfide ores are characterized by a relatively low initial temperature (180‒350°C), a higher CO2 density (0.27‒0.71 g/cm3), and a higher fluid pressure (0.7‒1 kbar) compared to the fluids that formed the gold–silver–telluride ores (temperature 200–260°C, CO2 density 0.28–0.56 g/cm3, pressure 0.7 kbar). The dominant salts in the fluids of polysulfide ores are Na and Mg chlorides, whereas the mineral-forming fluids of the gold–silver–telluride ores are simpler saline aqueous fluids containing Na chlorides. The fluids that formed the polysulfide ores have a H2O–CO2–N2 composition, whereas the fluid of the gold–silver–telluride ores is mostly of H2O–CO2 composition. The gold–bismuth ores in the Mayskoe ore field were formed by H2O–CO2-bearing fluids with a salinity concentration of 4.0‒6.4 wt %-equiv. NaCl, a CO2 density of 0.56‒0.61 g/cm3, at a temperature of 280‒335°C and a pressure of 0.7 kbar. The data led us to conclude that the ore-forming fluid of the Spokoininsky ore cluster was similar to the fluids of orogenic gold deposits.

本文首次获得了含金矿化的spokininsky矿群中多硫化物、金银碲化物和金铋三种类型矿石中石英中单个流体包裹体的数据。三种矿石类型在物化参数和流体组成上存在差异。与形成金银碲化矿石的流体(温度200 ~ 260℃,CO2密度0.28 ~ 0.56 g/cm3,压力0.7 kbar)相比,spokininsky集群多硫化矿石流体具有较低的初始温度(180 ~ 350℃)、较高的CO2密度(0.27 ~ 0.71 g/cm3)和较高的流体压力(0.7 ~ 1 kbar)的特征。多硫化物矿石流体中的优势盐是钠和镁氯化物,而金银碲化矿石的成矿流体是含钠氯化物的简单盐水。形成多硫化物矿石的流体主要由H2O-CO2 - n2组成,而金银碲化矿石的流体主要由H2O-CO2组成。Mayskoe矿田金铋矿是由含盐量为4.0 ~ 6.4 wt %-当量的含h2o - co2流体形成的。NaCl, CO2密度为0.56 ~ 0.61 g/cm3,温度280 ~ 335℃,压力0.7 kbar。结果表明,斯波克林斯基矿群的成矿流体与造山带金矿流体相似。
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引用次数: 0
Differentiation Features of Alkaline Rocks in Ilmen Miaskite Massif: New Mineralogical and Geochemical Data 伊门紫岩地块碱性岩石分异特征:新的矿物学和地球化学资料
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-02-25 DOI: 10.1134/S0016702924700782
E. S. Sorokina, E. V. Medvedeva, A. B. Nemov, M. A. Rassomakhin, L. N. Kogarko

The Ilmen miaskite massif in the Southern Urals remains largely understudied from the mineralogical and geochemical standpoints, and theories of its formation are still debatable. The paper presents the first data on the mineral associations of the miaskite varieties and REE-rich minerals. Microchemical studies determined that the pyroxene–amphibole miaskites are the most promising rock variety for REE mineralization (REE content at ca. 1500 ppm). These rocks show clearly discernible positive Nb anomalies combined with a negative Pb anomaly. The temperatures of feldspar exsolution indicate their following formation sequence within the miaskite varieties (from higher temperature to lower temperature ones): pyroxene–amphibole miaskite → garnet–amphibole miaskite → amphibole miaskite → biotite miaskite

从矿物学和地球化学的角度来看,南乌拉尔地区的伊尔门miaskite岩群在很大程度上仍未得到充分研究,关于其形成的理论仍存在争议。本文首次提供了有关miaskite品种的矿物关联和富含REE矿物的数据。显微化学研究确定,辉石-闪石miaskite是最有希望形成REE矿化的岩石种类(REE含量约为1500 ppm)。这些岩石显示出明显的正铌异常和负铅异常。长石的溶解温度表明了它们在闪长岩中的形成顺序(从高温到低温):辉石-闪长闪长岩 → 石榴石-闪长闪长岩 → 闪长闪长岩 → 黑云母闪长岩
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引用次数: 0
Actinides in the Soil Chronosequence of the Amur River Floodplain 阿穆尔河漫滩土壤中锕系元素的年代序列
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-02-25 DOI: 10.1134/S0016702924700848
A. V. Martynov

For the first time, a study was conducted at the Russian Far East to assess the rate of accumulation of gross and mobile forms of actinides (U and Th) in a 5000-year-old soil chronosequence embedded within the floodplain of the middle reaches of the Amur River. The relationships between actinides and the properties of alluvial and residual alluvial soils are characterized using regression models. It was found that during the evolution, the content of the gross form of actinides in the soils of the automorphic series increased from 1 to 2 mg/kg for U and from 4 to 10 mg/kg for Th. In the soils of the hydromorphic series, the increase over a shorter time period (2600 years) was from 1 to 3 mg/kg for U and from 4 to 12 mg/kg for Th. The content of the mobile U form in automorphic and hydromorphic soils increased on average from 0.1 to 0.4 mg/kg, and that of Th, from 0.02 to 0.2 mg/kg. In the automorphic soils, the accumulation of U is observed as long as the floodplain is regularly flooded, while Th continues to accumulate even after the floodplain leaves the flood zone. In the hydromorphic soils, the accumulation of actinides continues over the entire chronological range. The results obtained show that the main soil properties determining the accumulation of actinides in soils are the content of clay minerals and iron oxides. The intake of actinides into the soils of the Amur River floodplain occurs mainly due to the weathering of melanocratic granitoid minerals in the alluvium. The mobilization of actinides is affected by pH in automorphic soils and Eh in hydromorphic soils.

首次在俄罗斯远东地区进行了一项研究,以评估阿穆尔河中游漫滩内5000年历史的土壤时间序列中锕系元素(U和Th)总量和流动形式的积累速度。利用回归模型表征了锕系元素与冲积土和残余冲积土性质的关系。结果表明,在演化过程中,自同态系列土壤中锕系元素总形态的含量由U的1 mg/kg增加到2 mg/kg, Th的4 mg/kg增加到10 mg/kg。在水态系列土壤中,在较短的时间内(2600年),U的增加幅度为1 ~ 3 mg/kg, Th的增加幅度为4 ~ 12 mg/kg。自形态和水形态土壤中流动态U和Th的含量分别从0.1 ~ 0.4 mg/kg和0.02 ~ 0.2 mg/kg增加。在自同构土壤中,只要洪泛区被定期淹没,就会观察到U的积累,而即使洪泛区离开洪泛区,Th也会继续积累。在水态土壤中,锕系元素的积累在整个年代范围内持续进行。结果表明,决定锕系元素在土壤中积累的主要土壤性质是粘土矿物和氧化铁的含量。阿穆尔河漫滩土壤中锕系元素的摄入主要是由于冲积层中黑色花岗岩类矿物的风化作用。自同构土壤的pH值和水成态土壤的Eh值分别影响锕系元素的动员。
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引用次数: 0
Low Pb Isotopic Variations in the Extensive Chatkal–Kurama Ore Province, Middle Tien Shan, and Sources of the Large Scale Au, Ag, and Multimetal Mineralization: Evidence from High-Precision Pb Isotope Data 中天山察卡尔-库拉玛矿省低铅同位素变化与大规模金、银及多金属成矿来源:来自高精度Pb同位素数据的证据
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-02-25 DOI: 10.1134/S0016702924700800
I. V. Chernyshev, A. V. Chugaev, V. A. Kovalenker

The Chatkal–Kurama region in the central Tien Shan is a superlarge porphyry–epithermal gold ore province. The paleovolcanic area hosts world-class Au, Ag, and base-metal deposits (Kalmakyr, Kochbulak, Kanimansur, etc.). Using the high-precision (±0.02%) MC-ICP-MS method of lead isotope analysis, we studied a collection of 63 ore samples (47 of them are galena) from 18 deposits, which represent all types of Au–Ag, Au–Ag–base metal, and Cu–Au–Mo deposits known in the region. The same method was applied to study 21 samples of igneous rocks from this region, for which lead isotope composition was determined in monomineralic feldspar separates. The Pb isotope ratios 206Pb/204Pb, 207Pb/204Pb, and 208Pb/204Pb from the ore deposits vary within narrow ranges: 17.9885–18.1598, 15.5897–15.6412, and 38.0385–38.2380, respectively. These variations in relative terms are 0.94, 0.33, and 0.52%, respectively, and are among the smallest among ore provinces around the world. An even higher (two to five times) degree of homogeneity is typical of the Pb isotopic composition at individual deposits in the region. The lead isotope composition of deposits and ore fields in the Chatkal–Kurama region does not depend on their mineralogical and geochemical features but is instead controlled by the geological settings of the deposits. The discovered close similarity between ore deposits and Late Paleozoic granitoids in Pb isotope composition provides evidence in support of the hypothesis that genetic connection of the large-scale Au, Ag, and base-metal is genetically related to magmatism, which developed in a subduction environment. An interesting fact is that the Pb isotope composition is identical at the Kalmakyr Cu–Au–Mo porphyry deposit and the neighboring Akturpak Au epithermal deposit, which provides evidence that metals for these deposits (which are different in composition and were formed under different PT parameters) were derived from a common source. The isotope composition and its evolutionary model characteristics according to the Stacey–Kramers model indicate (in agreement with the data on Sr and Nd) that Pb of the rocks and deposits in the region is mid-crustal, typical of island-arc regions of the Andean type. The mantle component of the source of the regional ore-bearing magmas was the material of mantle lithosphere and oceanic crust that was partially melted in a subduction environment in the mantle wedge zone. The ratio Th/U = 3.86–3.99, which is higher than the average crustal value, indicates a significant contribution of Precambrian basement rocks of the Chatkal–Kurama terrane to the petrogenesis of the ore-bearing magmas.

天山中部查特卡尔-库拉马地区是一个超大型斑岩-浅成热液型金矿大省。古火山区拥有世界级的金、银、贱金属矿床(Kalmakyr、Kochbulak、Kanimansur等)。采用高精度(±0.02%)MC-ICP-MS铅同位素分析方法,对18个矿床的63个矿石样品(其中方铅矿47个)进行了研究,这些样品代表了该地区已知的所有类型的Au-Ag、Au-Ag基金属和Cu-Au-Mo矿床。用同样的方法研究了该地区21个火成岩样品,测定了单矿物长石分离物中的铅同位素组成。矿床Pb同位素比值(206Pb/204Pb、207Pb/204Pb、208Pb/204Pb)在17.9885 ~ 18.1598、15.5897 ~ 15.6412、38.0385 ~ 38.2380范围内变化较窄。相对而言,这些差异分别为0.94、0.33和0.52%,是世界上最小的省份之一。该地区个别矿床的铅同位素组成的均匀性甚至更高(2至5倍)。Chatkal-Kurama地区矿床和矿田的铅同位素组成不取决于其矿物学和地球化学特征,而是由矿床的地质环境控制。发现矿床Pb同位素组成与晚古生代花岗岩类非常相似,为大规模金、银、贱金属的成因联系与俯冲环境下发育的岩浆活动有关的假说提供了证据。一个有趣的事实是,Kalmakyr Cu-Au-Mo斑岩矿床和邻近的Akturpak Au浅成热液矿床的Pb同位素组成相同,这证明了这些矿床的金属(成分不同,形成于不同的P-T参数下)来自一个共同的来源。根据stey - kramers模式的同位素组成及其演化模式特征(与Sr和Nd数据一致)表明,该地区岩石和矿床的Pb为中地壳,属于典型的安第斯型岛弧地区。区域含矿岩浆源的地幔成分为地幔楔带俯冲环境下部分熔融的地幔岩石圈和洋壳物质。Th/U = 3.86 ~ 3.99,高于地壳平均值,表明Chatkal-Kurama地体前寒武纪基底岩对含矿岩浆的成岩作用有重要贡献。
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引用次数: 0
The Archean Age of Granite-Gneiss Complexes from the Kama–Vyatka Zone (the Volga-Ural Segment, East European Craton) 东欧克拉通伏尔加-乌拉尔段卡马-维亚特卡带太古宙花岗岩-片麻岩杂岩时代
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-02-25 DOI: 10.1134/S0016702924700794
M. O. Anosova, O. V. Astrakhantsev, A. V. Postnikov, A. A. Fedotova, T. I. Kirnozova, M. M. Fugzan, I. A. Sabirov

The formation history of granulite complexes is fundamental significance for understanding the growth of early continental crust. The work presents the results of an isotope-geochronological study of rock samples from the main lithotectonic complexes of the Kama–Vyatka zone (the Volga–Ural segment of the East European Craton)—enderbites of the Otradnenskaya Group and quartz diorites of the Tanaisky plagiogranitoid massif. The model ages of quartz diorites of the Tanaisky plagiogranitoid massif and enderbites of the Otradnenskaya Groups calculated from Sm–Nd data are 3.2 and 3.0 Ga, respectively. Zircons from the quartz diorites of the Tanaisky plagiogranitoid massif and the enderbites of the Otradnenskaya Group were dated by U–Pb LA-ICP-MS method. Zircon from quartz diorites yielded the Archean age of protolith of the plagiogranitoids of the Tanaisky Massif. This time interval of 3.04–2.98 Ga marks the stage of the oldest granulite metamorphism immediately following the magmatic event. Zircons from weakly gneissose enderbites of the Otradnenskaya Group is subdivided into two age groups: 3.0–2.8 and 2.750–2.60 Ga. Based on the morphology, internal structure of the crystals, and their isotope-geochemical characteristics (Th and U contents, Th/U ratio), each of the indicated age groups includes several zircon generations. Within a time interval of 3.0–2.8 Ga, the identified zircon generations record the following events: the formation of primary enderbites, local partial melting under the granulite-facies conditions, and retrograde metamorphism under transitional granulite–amphibolite facies. With allowance for the model age of the enderbites, the Otradnenskaya Group of the Kama–Vyatka zone of the Volga–Ural segment was dated for the first time at 3.0 ± 0.1 Ga. In the time interval of 2.75–2.60 Ga, zircon from weakly gneissose enderbites records the peak granulite metamorphism, which spanned the entire Volga-Ural segment, and subsequent retrograde metamorphism accompanying by the input of hydrous fluid and temperature decrease.

麻粒岩杂岩体的形成历史对认识早期大陆地壳的生长具有重要意义。本文介绍了对卡马-维亚特卡带(东欧克拉通的伏尔加-乌拉尔段)、奥特拉德涅斯卡亚群的主要岩石构造复合体和塔纳斯基斜花岗质地块的石英闪长岩的岩石样品进行同位素-地质年代学研究的结果。根据Sm-Nd资料计算的Tanaisky斜花岗岩体和Otradnenskaya群的石英闪长岩模型年龄分别为3.2 Ga和3.0 Ga。用U-Pb LA-ICP-MS法测定了Tanaisky斜花岗质地块石英闪长岩和Otradnenskaya群残余岩体的锆石年龄。石英闪长岩的锆石测定了塔纳斯基地块斜花岗质的太古宙原岩。3.04-2.98 Ga的时间间隔标志着紧随岩浆事件之后最古老的麻粒岩变质阶段。奥特拉德涅斯卡亚群弱片麻岩岩中锆石可划分为3.0 ~ 2.8 Ga和2.750 ~ 2.60 Ga两个年龄组。根据晶体的形态、内部结构及其同位素地球化学特征(Th和U含量、Th/U比值),每个指示年龄组都包含若干代锆石。在3.0 ~ 2.8 Ga的时间间隔内,确定的锆石世代记录了原生原生岩体的形成、麻粒岩相条件下的局部熔融和过渡麻粒岩-角闪岩相条件下的逆行变质作用。考虑到岩体的模式年龄,首次确定了伏尔加-乌拉尔段卡马-维亚特卡带的Otradnenskaya群的年龄为3.0±0.1 Ga。2.75 ~ 2.60 Ga弱片麻岩岩体锆石记录了贯穿整个伏尔加—乌拉尔段的麻粒岩变质峰,以及随后伴随含水流体输入和温度下降的逆变质作用。
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引用次数: 0
Carbon Isotope Type-Curves of Organic Matter in Sediments of the Laptev Sea (Seep Area) 拉普捷夫海(渗漏区)沉积物中有机物的碳同位素类型曲线
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-02-20 DOI: 10.1134/S0016702924700903
V. S. Sevastyanov, V. Yu. Fedulova, O. V. Kuznetsova, N. V. Dushenko, V. S. Fedulov, A. E. Bazhanova

Organic carbon content combined with organic carbon isotope composition have been applied for the study of organic matter transformation in marine sediments during upward gas migration at seep areas of the Laptev Sea. Organic matter extracted from marine sediments was separated into five fractions (hexane, hexane-benzene, benzene, benzene-methanol, asphaltenes) using solvents of increasing polarity. It has been shown that in the seep the destruction of asphaltenes fractions leads to enrichment of benzene-methanol fraction by isotope-light components. δ13C values of benzene-methanol fractions were much lower than δ13C values of asphaltenes fractions and were associated with the accumulation of bacterial biomass in the sediment core through which the upward methane flow was passed. The organic matter of seep area sediment cores can be classified by two clusters, according to δ13C values of benzene fractions of organic matter. The first cluster center was in the surface layer (about 10 cm) of marine sediments. The second cluster center was in a deeper sediment layer. The difference in carbon isotope composition between the cluster centers was 2–3‰. The use of carbon isotope type-curves for different horizons of a sediment core has enabled a better understanding of the biological effects related to upward gas migration in seep areas of the Arctic Seas.

应用有机碳含量结合有机碳同位素组成研究了拉普捷夫海渗漏区海相沉积物在天然气向上运移过程中的有机质转化。采用极性递增的溶剂将海洋沉积物中提取的有机物分成5个组分(正己烷、正己烷-苯、苯、苯-甲醇、沥青烯)。研究表明,在渗流中沥青质组分的破坏导致了苯甲醇组分的同位素轻组分富集。苯甲醇馏分的δ13C值远低于沥青质馏分的δ13C值,这与甲烷向上流动通过的沉积物岩心中细菌生物量的积累有关。根据有机质中苯组分的δ13C值可将渗漏区沉积物岩心的有机质分为两类。第一个簇中心位于海洋沉积物表层(约10 cm)。第二个集群中心位于较深的沉积层中。簇中心碳同位素组成差异为2 ~ 3‰。对沉积物岩心不同层位的碳同位素类型曲线的使用,使人们能够更好地理解北冰洋渗漏区向上运移天然气的生物效应。
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引用次数: 0
Provenance, Paleoweathering and Paleotectonics of Cobalt Bearing Metasedimentary Rocks of the Delhi Supergroup, North Delhi Fold Belt, NW India 印度西北部北德里褶皱带德里超群含钴成岩的成因、古风化作用和古构造作用
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-02-20 DOI: 10.1134/S0016702924600913
Swati Rana, Naresh Kumar, A. Krishnakanta Singh

Cobalt bearing metasedimentary rocks from the Nasibpur and surrounding areas of North Delhi Fold Belt, NW India has been studied to elucidate their provenance, palaeoweathering, palaeoclimatological conditions and depositional environment. The investigated area is characterized by metasedimentary formations such as quartzites, mica schists, garnet mica schist, phyllites, gneiss, amphibolites and magmatic phases like granites and pegmatites. Petrographic analysis affirmed that quartzites are mineralogical mature, fine to medium grained. On the basis of modal compositions these quartzites range from Fe-sand and quartz arenite in composition. The calculated chemical index of alteration (CIA) values (31.98 to 75.87 with an average of 48.60 indicates low to moderate weathering under semiarid to humid climatic conditions. Most of the quartzites samples have SiO2/Al2O3 (>10, avg. 43) which indicates high maturity. Cobalt concentration in these quartzites, mica schist, pegmatites range from 166 to 3657, 62–166, and 167–519 ppm respectively. Quartz dilution during hydraulic sorting has led to low concentrations of rare earth elements in the quartzites. The rocks exhibit enrichment in LREE with (La/Sm)n (1.2–7.41 avg. 4.56) with noticeable negative Eu anomalies (Eu/Eu* = 0.34–0.74). Evaluation of mineral and whole rock geochemistry collectively indicate their predominant derivation from a felsic source and deposition in an active to passive continental setting.

对印度北部德里褶皱带纳西布尔及周边地区含钴变质沉积岩进行了研究,以阐明其物源、古风化、古气候条件和沉积环境。研究区以石英岩、云母片岩、石榴云母片岩、千层岩、片麻岩、角闪岩等变质沉积岩和花岗岩、伟晶岩等岩浆相为特征。岩相分析证实石英岩矿物学成熟,细粒至中粒。从模态组成上看,这些石英岩的成分介于铁砂和石英砂岩之间。计算得到的化学蚀变指数(CIA)值为31.98 ~ 75.87,平均值为48.60,表明在半干旱~湿润气候条件下,风化程度为低至中度。大部分石英岩样品SiO2/Al2O3 (>10,平均43),成熟度较高。石英岩、云母片岩、伟晶岩中的钴含量分别为166 ~ 3657、62 ~ 166和167 ~ 519 ppm。水力分选过程中石英的稀释作用导致石英岩中稀土元素浓度较低。LREE富集,(La/Sm)n(1.2 ~ 7.41,平均值4.56),Eu负异常显著(Eu/Eu* = 0.34 ~ 0.74)。矿物和整个岩石的地球化学评价共同表明,它们的主要来源是长英质烃源岩,沉积在主动到被动的大陆环境中。
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引用次数: 0
Different Types of CaSiO3 in the Earth’s Mantle and Its Geochemical Heterogeneity: the Juina Area in Brazil as an Example 地幔不同类型CaSiO3及其地球化学非均质性——以巴西Juina地区为例
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-02-20 DOI: 10.1134/S0016702924601761
F. V. Kaminsky, Yu. A. Kostitsyn

CaSiO3 inclusions in diamonds from the Juina area in Brazil have low Fe (0.08–0.53 wt % FeO) and Al (0–1.52 wt % Al2O3) concentrations; they belong to the ultramafic association. Two different types exist among CaSiO3 grains. Type I has a normal REEn pattern, while type II has a sinusoidal REEn pattern. Type I CaSiO3 associates with high-Mg–high-Ni protogenetic ferropericlase, and type II associates with high-Fe–low-Ni syngenetic ferropericlase. Thus, type I CaSiO3 grains are protogenetic, formed, like high-Mg–high-Ni ferropericlase, in the upper part of the lower mantle as davemaoite (CaSi-perovskite), and type II CaSiO3 were formed in the transition zone as breyite. The enrichment of CaSiO3 in REE, particularly in LREE, corresponds to high values of their partition coefficient CaSiO3/melt and shows the CaSiO3’s origin from a mantle material under high pressures. The isotope characteristics of the studied CaSiO3 demonstrate strong geochemical heterogeneity in the inclusions. The 87Rb/86Sr ratios in type II CaSiO3 (0.127–3.23) are 3–4 orders higher than in type I (0.0008). Even within a single diamond, different CaSiO3 grains have 87Rb/86Sr ratios varying from 0.014 to 3.23. The same is true for U/Pb isotope systematics (e.g., 238U/206Pb varies in one sample in an order of magnitude from 0.031 to 0.312) and, to some extent, for Sm/Nd ratios. This implies the geochemical heterogeneity in Deep Earth on a very small scale.

巴西Juina地区钻石中的CaSiO3包裹体Fe (0.08 ~ 0.53 wt % FeO)和Al (0 ~ 1.52 wt % Al2O3)浓度较低;他们属于超级联盟。CaSiO3颗粒中存在两种不同的类型。I型具有正常的green模式,而II型具有正弦green模式。I型CaSiO3与高mg -高ni原生铁方石酶结合,II型CaSiO3与高fe -低ni同生铁方石酶结合。因此,ⅰ型CaSiO3晶粒是原生形成的,像高镁高镍铁方长石一样形成于下地幔上部的钙钛矿(钙钛矿),ⅱ型CaSiO3晶粒形成于过渡带的白晶石。CaSiO3在REE中富集,特别是在LREE中富集,对应于它们的分配系数CaSiO3/melt的高值,表明CaSiO3来源于高压下的地幔物质。包裹体中CaSiO3的同位素特征显示出较强的地球化学非均质性。ⅱ型CaSiO3的87Rb/86Sr比值(0.127 ~ 3.23)比ⅰ型CaSiO3(0.0008)高3 ~ 4个数量级。即使在单个钻石中,不同的CaSiO3颗粒的87Rb/86Sr比值也从0.014到3.23不等。U/Pb同位素系统也是如此(例如,238U/206Pb在一个样品中变化的数量级从0.031到0.312),在某种程度上,Sm/Nd比率也是如此。这表明地球深部的地球化学非均匀性在很小的范围内。
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引用次数: 0
Chemical Composition, Mineralogy, and Physical Properties of the Moon’s Mantle: A Review 月球地幔的化学组成、矿物学和物理性质:综述
IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2025-01-27 DOI: 10.1134/S0016702924700733
O. L. Kuskov, E. V. Kronrod, V. A. Kronrod
<p>The problem of the internal structure of the Moon plays a special role in understanding its geochemistry and geophysics. The principal sources of information about the chemical composition and physical state of the deep interior are seismic experiments of the Apollo expeditions, gravity data from the GRAIL mission, and geochemical and isotopic studies of lunar samples. Despite the high degree of similarity of terrestrial and lunar matter in the isotopic composition of several elements, the problem of the similarity and/or difference in the major-component composition of the silicate shells of the Earth and its satellite remains unresolved. This review paper summarizes and critically analyzes information on the composition and structure of the Moon, examines the main contradictions between geochemical and geophysical classes models for the mantle structure, both within each class and between the classes, related to the estimation of the abundance of Fe, Mg, Si, Al, and Ca oxides, and analyzes bulk silicate Moon (BSM) models. The paper describes the principles of the approach to modeling the internal structure of a planetary body, based on the joint inversion of an integrated set of selenophysical, seismic, and geochemical parameters combined with calculations of phase equilibria and physical properties. Two new classes of the chemical composition of the Moon enriched in silica (∼50% SiO<sub>2</sub>) and ferrous iron (11–13% FeO, Mg# 79–81) relative to the bulk composition of the silicate component of the Earth (BSE) are discussed: (i) models E with terrestrial concentrations of CaO and Al<sub>2</sub>O<sub>3</sub> (Earth-like models) and (ii) models M with higher contents of refractory oxides (Moon-like models), which determine the features of the mineralogical and seismic structure of the lunar interior. A probabilistic distribution of geochemical (oxide concentrations) and geophysical (<i>P</i>-, <i>S</i>-wave velocities and density) parameters in the four-layer lunar mantle within the range of permissible selenotherms was obtained. Systematic differences are revealed between contents of major oxides in the silicate shells of the Earth and the Moon. Calculations were carried out for the mineral composition, <i>P</i>-, <i>S</i>-wave velocities, and density of the E/M models, and two classes of conceptual geochemical models: LPUM (Lunar Primitive Upper Mantle) and TWM (Taylor Whole Moon) with Earth’s silica content (∼45 wt % SiO<sub>2</sub>) and different FeO and Al<sub>2</sub>O<sub>3</sub> contents. Arguments are presented in support of the SiO<sub>2</sub>- and FeO-enriched (olivine pyroxenite) lunar mantle, which has no genetic similarity with Earth’s pyrolitic mantle, as a geochemical consequence of the inversion of geophysical parameters and determined by cosmochemical conditions and the mechanism that formed the Moon. The dominant mineral of the lunar upper mantle is high-magnesium orthopyroxene with a low calcium content (rather than olivi
月球的内部结构问题对了解月球的地球化学和地球物理学起着特殊的作用。关于月球深处化学成分和物理状态的主要信息来源是阿波罗探测器的地震实验、GRAIL任务的重力数据以及月球样本的地球化学和同位素研究。尽管陆地和月球物质在若干元素的同位素组成方面高度相似,但地球及其卫星的硅酸盐壳的主要成分组成的相似和(或)不同的问题仍然没有解决。本文总结并批判性地分析了有关月球成分和结构的信息,探讨了地球化学和地球物理类地幔结构模型之间的主要矛盾,无论是在每个类别内还是在类别之间,与铁、镁、硅、铝和钙氧化物丰度的估计有关,并分析了大块硅酸盐月球(BSM)模型。本文介绍了基于硒物理、地震和地球化学参数综合反演结合相平衡和物性计算的行星体内部结构建模方法的原理。本文讨论了相对于地球硅酸盐组分(BSE)的总体组成,富含二氧化硅(~ 50% SiO2)和亚铁(11-13% FeO, Mg# 79-81)的两类新的月球化学组成:(i)具有地球浓度CaO和Al2O3的E模型(类地模型)和(ii)具有较高含量耐火氧化物的M模型(类月模型),它们决定了月球内部的矿物学和地震结构特征。得到了四层月幔中地球化学(氧化物浓度)和地球物理(纵波、横波速度和密度)参数在允许硒温范围内的概率分布。揭示了地球和月球硅酸盐壳层中主要氧化物含量的系统性差异。计算了E/M模型的矿物组成、P波、s波速度和密度,以及两类概念地球化学模型:LPUM(月球原始上地幔)和TWM (Taylor Whole Moon),其中地球的二氧化硅含量(~ 45 wt % SiO2)和不同的FeO和Al2O3含量。在地球物理参数反演的地球化学结果和月球形成的宇宙化学条件和机制的作用下,提出了支持SiO2-和feo富集(橄榄辉石岩)月球地幔与地球的辉石岩地幔没有遗传相似性的观点。月球上地幔的主要矿物是钙含量低的高镁正辉石(而不是橄榄石),这一点得到了阿波罗地震数据的证实,并得到了航天器对许多撞击盆地岩石光谱数据分析的支持。相比之下,以橄榄石为主要矿物的TWM和LPUM地球化学模型的纵波和横波速度与阿波罗地震数据不匹配。考虑了月球形成情景中的地球化学约束。月球相对于地球的热石质地幔同时富集SiO2和FeO,这与月球是由陆地物质或球粒陨石组成的撞击体巨大撞击而形成的说法不相容,也与月球形成的现代假设相冲突,与月球和陆地样品同位素组成的相似性相冲突。讨论了如何将这些不同的地球化学因素拟合到地球-月球系统形成的宇宙演化模型的普罗克鲁斯坦床中。
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引用次数: 0
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Geochemistry International
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