粤北大宝山志留纪次英安斑岩年代学、地球化学特征及其地质意义

粤北大宝山Cu-Mo-W-Pb-Zn多金属矿床位于钦杭矽卡岩型Cu-Mo成矿带南部。对于该矿床成因目前存在志留纪海底喷流沉积成因和燕山期斑岩矽卡岩成因2种争议。文章以大宝山次英安斑岩为研究对象,通过矿区填图和钻孔编录,查明次英安斑岩与矿体矿化的空间关系;通过年代学、岩石地球化学研究,提示成岩成矿时代与背景;结合区域资料探讨次英安斑岩与金属成矿关系。野外地质填图提示,层状铜矿体赋存在志留系东岗岭下亚组碳酸盐岩中,但存在透闪石化、绿泥石化等与斑岩型矽卡岩型岩体有关蚀变,而且周围发育侏罗纪花岗闪长斑岩;采用LAICP-MS锆石U-Pb同位素精确定年方法,获得次英安斑岩年龄为(434.3±1.0)Ma(DB009)、(431.50±0.12)Ma(DB022)和(417.00±0.87)Ma(DB031)。岩石地球化学数据显示,次英安斑岩为高钾钙碱性系列岩石,具有富集Hf同位素特征和古老模式年龄,指示岩石成因主要源于古老地壳重熔,这种重熔有可能伴生有钨、锡、铌、铊等矿化,但不会产生海底喷流沉积型矿床。结合辉钼矿Re-Os等时线成矿年龄(166.0±3.0)Ma,笔者认为大宝山矿床成矿主要与侏罗纪花岗质岩浆侵位密切相关,与志留纪次火山岩无关。     

腾冲地块西缘那邦基性麻粒岩中石榴石Sm-Nd等时线年龄及其意义

石榴石 Ｓｍ  Ｎｄ 等时线法是近年来常用于较新年龄的测年方法。腾冲地块西缘新近发现的基性麻粒岩中石榴石和全岩的 Ｓｍ  Ｎｄ 等时线年龄为 １７～２５ Ｍａ, 是该麻粒岩经受后期变形变质作用的年龄, 与区内右旋走滑断裂活动时限相一致,为确证腾冲地区的右旋走滑断裂是印支地块逸出的西部边界提供了 Ｓｍ  Ｎｄ 等时线方法的年龄约束。并推断石榴石 Ｓｍ  Ｎｄ 体系的封闭温度较低, 应低于那邦变质基性岩晚期变质作用的６４０℃～７２０℃。     

北祁连山小柳沟钨矿床中辉钼矿Re-Os年龄测定及其意义

小柳沟是中国在北方最新探明的一个大型钨矿床,本文概要地介绍了该矿床的成矿地质背景和矿床地质特征,用Re-Os同位素方法测试辉钼矿,获得等时线年龄462±13 Ma(2σ),模式年龄436～496 Ma。还证明了成矿发生于板块碰撞期前,成矿物质主要为壳源。     

滇西腾冲大硐厂铜-铅-锌矿床的辉钼矿Re-Os同位素定年

在环绕印度—亚洲大陆碰撞形成的东构造结波密—腾冲弧形构造带中,发育一组含锡铅_锌_铜多金属矿床,但一直没有准确的成矿年龄数据。文章通过对大硐厂铅_锌矿区红沟岩铜矿体中辉钼矿的Re_Os同位素测试,获得精确的成矿等时线年龄为(118.0±2.4)Ma。区内与成矿关系密切的斑岩成岩年龄在143～112Ma,认为斑岩成岩与成矿同期,同为燕山晚期。     

岩浆型Cu-Ni-PGE硫化物矿床研究的几个问题探讨

文章简述了岩浆型Cu—Ni—PGE硫化物矿床的主要特点和研究现状,探讨了矿床的成矿机制,认为其成矿的首要条件是岩浆中硫达到饱和而使硅酸盐岩浆与硫化物熔体发生熔离。综述了如何利用同位素方法确定其成矿物质来源,介绍了如何判别硫饱和度的方法。     

Isochron‐burial dating of glaciofluvial deposits: First results from the Swiss Alps

In this study, we use isochron‐burial dating to date the Swiss Deckenschotter, the oldest Quaternary deposits of the northern Alpine Foreland. Concentrations of cosmogenic ¹⁰Be and ²⁶Al in individual clasts from a single stratigraphic horizon can be used to calculate an isochron‐burial age based on an assumed initial ratio and the measured ²⁶Al/¹⁰Be ratio. We suggest that, owing to deep and repeated glacial erosion, the initial isochron ratio of glacial landscapes at the time of burial varies between 6.75 and 8.4. Analysis of 22 clasts of different lithology, shape, and size from one 0.5 m thick gravel bed at Siglistorf (Canton Aargau) indicates low nuclide concentrations: <20 000 ¹⁰Be atoms/g and <150 000 ²⁶Al atoms/g. Using an ²⁶Al/¹⁰Be ratio of 7.6 (arithmetical mean of 6.75 and 8.4), we calculate a mean isochron‐burial age of 1.5 ± 0.2 Ma. This age points to an average bedrock incision rate between 0.13 and 0.17 mm/a. Age data from the Irchel, Stadlerberg, and Siglistorf sites show that the Higher Swiss Deckenschotter was deposited between 2.5 and 1.3 Ma. Our results indicate that isochron‐burial dating can be successfully applied to glaciofluvial sediments despite very low cosmogenic nuclide concentrations. Copyright © 2017 John Wiley & Sons, Ltd.     

四川攀西红格矿区辉长岩和正长岩的SHRIMP U-Pb和Sm-Nd定年及其地质意义

用SHRIMP U-Pb和Sm-Nd定年技术,对攀西红格矿区含矿层状辉长岩、碱性正长岩进行了年龄测定。获得红格辉长岩中3种不同晶形锆石的U-Pb年龄分别为258.4±4.1Ma、1841±34Ma、2487±12Ma,由辉长岩、辉石和磷灰石所构成的Sm-Nd等时线年龄为253±14Ma;碱性正长岩中锆石的U-Pb年龄为257.2±1.5Ma。结果表明,红格辉长岩中具有典型基性岩锆石特征的锆石U-Pb年龄(258Ma)与同一地质样品的Sm-Nd年龄(全岩+矿物内部等时线年龄),以及同一矿区的正长岩锆石U-Pb年龄在测定误差范围内一致。鉴于层状辉长岩和碱性正长岩在空间上密切共生,在形成时间上一致,可以认为它们都属于晚二叠世末岩浆活动的产物;而1841Ma和2487Ma的锆石,可能是在基性-超基性岩浆的上侵过程中,从基底所捕获的岩浆锆石和继承锆石,其年龄信息,揭示了康滇地轴岩浆岩带的下部或结晶基底存在元古代甚至新太古代末期的岩石或物质。     

湖北随州黑龙潭金矿石英Rb-Sr同位素年龄及其地质意义

通过矿物流体包裹体Rb-Sr同位素测年,获得鄂北黑龙潭金矿石英Rb-Sr等时线年龄为132.6±2.7Ma,表明该金矿床形成于早白垩世中期。矿石石英中流体包裹体Sr同位素初始比(~(87)Sr/~(86)Sr)i平均值为0.710798,小于陆源硅酸盐的值(0.720),高于地幔Sr的初始值(0.707),暗示成矿物质来源于壳幔混合。结合各类岩矿石Au丰度变化,S、Pb、H、O等同位素组成,以及稀土和微量元素特征、成矿流体等研究,认为该矿床的形成可能与燕山期持续伸展阶段大规模构造-岩浆活动有关,燕山期中酸性岩浆活动为金矿成矿提供了主要矿源和热源。     

小兴安岭鹿鸣大型钼矿LA-ICP-MS锆石U-Pb和辉钼矿Re-Os年龄及其地质意义

鹿鸣钼矿是小兴安岭地区于近年发现的大型斑岩型钼矿床。为探讨研究区成岩成矿关系及其地质意义,在对矿化特征分析的基础上,采用LA-ICP-MS锆石U-Pb技术对鹿鸣地区含矿二长花岗岩测年,获得成岩年龄为 (187.1±1.2) Ma (n=15, MSWD=0.70) 。通过辉钼矿样品Re-Os同位素分析,获得等值线年龄为(177.4±3.5) Ma (n=11, MSWD=0.71) ,加权平均年龄为(178.08±0.79) Ma (n=11,MSWD=0.46)。两种方法获得的年龄大致相近,表明它们形成于同一成岩成矿系统。鹿鸣钼矿成岩成矿年龄,与乌奴格吐山铜钼矿、兰家沟钼矿和杨家杖子钼矿等矿床辉钼矿Re-Os同位素年龄相近,表明包括小兴安岭地区在内的我国东北地区广泛存在早侏罗世岩浆-成矿作用。微量元素和同位素指纹显示,鹿鸣钼矿形成于地壳挤压向拉伸转换的构造环境,成矿物质为壳幔混合来源。     

Origin of highly siderophile and chalcogen element fractionations in the components of unequilibrated H and LL chondrites

Osmium isotopic compositions, abundances of highly siderophile elements (HSE: platinum group elements, Re and Au), the chalcogen elements S, Se and Te and major and minor elements were analysed in physically separated size fractions and components of the ordinary chondrites WSG 95300 (H3.3, meteorite find) and Parnallee (LL3.6, meteorite fall). Fine grained magnetic fractions are 268-65 times enriched in HSE compared to the non-magnetic fractions. A significant deviation of some fractions of WSG 95300 from the 4.568 Ga ¹⁸⁷Re-¹⁸⁷Os isochron was caused by redistribution of Re due to weathering of metal. HSE abundance patterns show that at least four different types of HSE carriers are present in WSG 95300 and Parnallee. The HSE carriers display (i) CI chondritic HSE ratios, (ii) variable Re/Os ratios, (iii) lower than CI chondritic Pd/Ir and Au/Ir and (iv) higher Pt/Ir and Pt/Ru than in CI chondrites. These differences between components clearly indicate the loss of refractory HSE carrier phases before accretion of the components. Tellurium abundances correlate with Pd and are decoupled from S, suggesting that most Te partitioned into metal during the last high-temperature event. Tellurium is depleted in all fractions compared to CI chondrite normalized Se abundances. The depletion of Te is likely associated with the high temperature history of the metal precursors of H and LL chondrites and occurred independent of the metal loss event that depleted LL chondrites in siderophile elements. Most non-magnetic and slightly magnetic fractions have S/Se close to CI chondrites. In contrast, the decoupling of Te and Se from S in magnetic fractions suggests the influence of volatility and metal-silicate partitioning on the abundances of the chalcogen elements. The influence of terrestrial weathering on chalcogen element systematics of these meteorites appears to be negligible.