湘中锑(金)矿床成矿物质来源——Ⅰ.微量元素及其实验地球化学证据

为了查明湘中盆地中-低温梯（金）矿床的成矿物质来源，文章应用高分辨率ICP-MS、ICP-AES等方法对岩石与矿石进行了系统测定，并结合作者以往分析数据和实验地球化学结果，对该区盆地及周边基底地层与矿床中的微量元素分布特征及其水/岩反应效应进行了综合分析和系统研究。结果表明：Sb、Au等成矿元素在元古界基底碎屑岩中具有高的背景含量，在近似成矿条件下的水/岩反应实验中，成矿元素的淋出率达20%～90%，元古界基底碎屑岩中的金（锑、钨）矿床的周围蚀变围岩中出现明显的金负异常区。而盆地内泥盆系统地层中的高锑含量仅局限于锑矿床（化）及其蚀变围岩中；湘中锑（金）矿床中的矿石与基底碎屑岩具有相似的稀土元素球粒陨石标准化配分曲线特征，以上微量元素地球化学特征充分证明该区锑（金）矿床锑、金等成矿物质主要来源于元古界底碎屑岩。     

山东金青顶金矿床和七宝山金矿床的流体包裹体REE组成

文章运用电感耦合等离子体质谱（ICP-MS）方法，研究了金青顶金矿床和七宝山金矿床的脉石英中流体包裹体REE组成特征，结果表明流体包裹体的REE均为LREE富集型，并显示Eu正异常。成矿流体REE配分模式和REE参数特征表明它们具有相当的来源。与金矿有关的成矿母岩，即昆嵛山花岗岩和七宝山次火山岩的REE特征也极为相似，反映成矿流体的REE组成都有从成岩向成矿过程演化继承的关系。矿床流体包裹体REE组成的相似特征及矿床碳氧同位素等特点表明，金青顶金矿床和七宝山金矿床是华北东部中生代同一构造热事件的产物。     

采矿环境地球化学研究

阐述了采矿对环境造成的负面影响 ,包括 :尾矿或废石堆中的杂质元素会进入表生地球化学循环 ,在不同气候条件下 ,呈现不同的特征模式 ,尾矿氧化带的酸性水的排放 ;矿山污染源对周围土壤和植物的影响使重金属元素等进入食物链 ,对人类和动物健康造成威胁。根据国内外的最新研究动向 ,指出建立环境地球化学模式 ,对采矿环境污染作出客观的监测和评价 ,能为防止污染和治理环境提供可靠的地球化学依据。     

吉林集安铅锌矿地球化学与分散元素

吉林集安铅锌矿床是我国最早报导的少数几个典型低温铅锌矿床之一。矿化具有多期次特点 ,富矿体都是多期次矿化叠加的产物。根据矿化先后和矿物生成顺序将矿化分为五个阶段 :①石英 黄铁矿矿化阶段 ;②重晶石 闪锌矿矿化阶段 ;③石英 方铅矿矿化阶段 ;④石英 黄铁矿矿化阶段 ;⑤碳酸盐 氧化矿物矿化阶段。用均一法和爆裂法测得石英、重晶石、闪锌矿包裹体成矿温度变化在 1 1 0℃～ 1 97℃之间。矿床中除含铅锌矿外 ,还有微量的Pt和Pd,并普遍含分散元素Cd、Ga、Tl、In、Se、Ge、Te,其中以Cd含量最高 ,闪锌矿中Cd含量最高可达 71 5 5× 1 0 6。分散元素主要呈类质同象形式赋存在各种矿物之中 ,未发现独立矿物。通过矿床地质和硫铅同位素研究表明该铅锌矿床属低温沉积 改造型层控矿床。     

河北矾山燕山期侵入岩地球化学特征及成因

河北矾山地区燕山期侵入岩可分为早、晚两期。早期（中侏罗世-晚侏罗世）侵入岩主要由二长闪长岩、石英二长闪长岩、石英二长岩、正长岩构成，以高钾钙碱性岩系列岩石为主；SiO2=53.58%-60.57%,Al2O3=16.16%-17.23%,Na2O K2O=5.76%-8.96%,K2O=2.25%-4.55%,Na2O/K2O=1.14-1.56;ACNK=0.72-0.86,NKA=0.47-0.77;Eu^*/Eu=0.80-0.95,轻稀土富集，重稀土和Nb、Ta、Hf、Ti亏损，相对低Zr、Rb和Rb/Sr，但高Sr和Sr/Y，具有埃达史质岩石质岩石的部分特征。晚期（白垩纪）侵入岩由碱长石英正长岩、石英正长岩、石英二长岩、碱工花岗岩、钾长花岗岩构成，以钾玄岩系列岩石为主；比早期岩石富SiO2，低Al2O3、富Na2O K2O和K2O，但低Na2O/K2O;ACNK=0.82-1.07,NKA=0.77-0.92;Eu^*/Eu=0.65-1.00，轻稀土富集，重稀土和Nb、Ta、Hf、Ti亏损，相对高Zr、Rb和Rb/Sr，但低Sr和Sr/Y。矾山地区早期侵入岩的形成可能与伊泽奈崎（Izanaqi)板块向欧亚大陆板块的俯冲所导致的挤压增厚有关；晚期侵入岩可能形成于拉张环境中。     

REE Geochemistry of the Lead—Zinc Ores from the Jinding Lead—Zinc Deposit,Lanping,Yunnan

Nineteen volcanic and magmatic rock samples were collectecd from the Jinding leadzinc deposit and its surrounding areas in Yunnan.The ICP and AES analyses,feferred to the previous results,show that the metal minerals and altered rocks in the Jinding lead-zinc deposit display a decreasing trend of ∑REE from the early to late stages of mineralization,and similarities in REE distribution patterns,indicating that the ore fluids are characterized by high LREE enrichment,markedly negative δCe anomaly and slight δEu anomaly.These REE distribution paterns exhibit striking similarities to those of the Pliocene trachyte in the study area,both of which are similar in ∑REE,LREE/HREE ratio,δEu and δCe.The ore fluids besides the basin fluids in the deposit are also closely related to those associated with Pliocene trachyte magmas.     

Negative Ce Anomaly in the Indian Banded Iron Formations: Evidence for the Emergence of Oxygenated Deep-Sea at 2.9-2.7 Ga

Abstract: Major and rare earth element contents are reported for Late Archean banded iron formations (BIFs) in the Bababudan Group of the Dharwar Craton, South India. The BIFs are mostly composed of SiO₂ (average1ρ = 54.88.1 wt%) and Fe₂O₃* (44.38.2 wt%). The Al₂O₃ and TiO₂ contents are remarkably low, suggesting that detrital components were starved during the BIF deposition. The BIFs have a LREE-enriched pattern with a relatively high (La/Yb)_N (6.644.07). Total REE concentrations (RE) vary from 5.2 to 65.3 ppm. The REE patterns are characterized by the presence of a very large negative Ce anomaly (Ce/Ce*: 0.13-0.83) and a positive Eu anomaly (Eu/Eu*: 0.96-2.45). The Eu/Eu* decreases and (La/Yb)_N increases with a increase of RE. These correlations of REE indices are similar to those of modern hydrothermal iron-rich sediments near a mid-ocean ridge (MOR). Greenstones associated with the BIFs have MORB-like geochemical features. These geochemical and geological lines of evidence indicate that the depositional site of the BIFs was remote from a continent and/or island arc and that the BIFs were in situ hydrothermal sediments near a MOR. A striking negative Ce anomaly in the BIFs indicates that oxygenated deep-sea environments emerged at 2.9-2.7 Ga. The existence of contemporaneous Mn deposits in the Dharwar Craton supports this assertion. Our scenario of oxygen in the Earth's surface of the Late Archean is different from long-held notion that the atmosphere and ocean were persistently anoxic throughout the Archean.     

Volcanological and petrological evolution of Marsili Seamount (southern Tyrrhenian Sea)

A swath bathymetric survey was conducted on Marsili Volcano, the biggest seamount in the Tyrrhenian Sea. It stands 3000 m above the surrounding oceanic crust of the 3500 m-deep Marsili back-arc basin and is axially located within the basin. The seamount has an elongated shape and presents distinctive morphology, with narrow (<1000 m) ridges, made up of several elongated cones, on the summit zone and extensive cone fields on its lower flanks. A dredging campaign carried out at water depths varying between 3400 and 600 m indicates that most of Marsili Seamount is composed of medium-K calc-alkaline basalts. Evolved high-K andesites were only recovered from the small cones on the summit axis zone. Petrological and geochemical characteristics of the least differentiated basalts reveal that at least two varieties of magmas have been erupted on the Marsili Volcano. Group 1 basalts have plagioclase and olivine as dominant phases and show lower Al, Ca, K, Ba, Rb and Sr, and higher Fe, Na, Ti and Zr with respect to a second type of basaltic magma. Group 2 basalts reveal the presence of clinopyroxene as an additional phenocryst phase. In addition, the two basaltic magmas have different original pre-eruptive H₂O content (group 1, H₂O-poor and group 2, H₂O-rich). Moreover, comparison of the compositional trends and mineralogical compositions obtained from MELTS [Ghiorso, M.S., Sack, R.O., Contrib. Mineral. Petrol. 119 (1995) 197–212] fractional crystallization calculations reveal that the evolved andesites can only exclusively be derived from a low-pressure (0.3 kbar) fractionation of magmas compositionally similar to the least evolved group 2 basalts. Finally, we suggest that the high vesicularity of the basalts sampled at relatively great depths (>2400 m) on the edifice is governed by H₂O and, probably, CO₂ exsolution and is not a feature indicative of shallow water depth eruption.     

Les dykes basiques du massif ancien de l'Ourika (Atlas de Marrakech,Maroc) : géochimie et significationThe basic dykes of the Ourika old massif (High Atlas of Marrakech): Geochemistry and significance

The Precambrian massif of Ourika is crosscut by two systems of basic dykes, striking N40°E and N90–120°E. Using incompatible trace elements, the two systems form two distinct chemical groups, displaying a continental tholeiitic affinity. The composition variations between the two defined groups can be due to heterogeneities of mantle sources and to contamination, during the magma ascent, by the continental crust. The emplacement of these basic dykes, before the late-PIII formations, can be related to the Neoproterozoic distension generalised to the Anti-Atlas chain. To cite this article: A. Barakat et al., C. R. Geoscience 334 (2002) 827–833.     

辽东青城子矿集区金、银成矿时代及地质意义

为确定辽宁青城子矿集区金、银的成矿时代 ,分别以含金硅化岩和含银网脉状石英晶体内流体包裹体为对象 ,应用Rb_Sr法测得金、银成矿的等时线年龄为 (2 33± 31)Ma～ (2 34± 14 )Ma ;作为对Rb_Sr法测年结果的验证 ,又以与贵金属矿石矿物共生的热液石英为对象 ,用40 Ar/3 9Ar快中子活化法测得坪年龄tp=(2 38.78± 0 .74 )Ma～ (2 38.80± 0 .6 0 )Ma,等时线年龄ti=(2 39.4 6± 1.13)Ma～ (2 4 0 .35± 0 .88)Ma。Rb_Sr和40 Ar/3 9Ar两种方法的测年结果基本一致 ,与本区印支期岩浆活动时代〔2 17.6Ma～ (2 30 .7± 5 )Ma〕吻合。