赣南河草坑铀矿田蚀变特征

文章着重对河草坑铀矿田近矿围岩蚀变特征、分带特征以及蚀变期次进行研究,结果表明：因表生氧化作用,近地表蚀变岩石多表现为紫色,向下转变为绿色;碱交代以钾交代为主,而钠交代较弱;矿田蚀变依据时间先后可划分为5个阶段。剖面系统取样分析结果揭示：在蚀变、矿化及成矿过程中U与Fe2O3、Be、Pb、W等呈正相关关系;U与Cu、Zn因矿化类型不同而表现出不同的相关关系,而U与Mo无明显关系。     

Intraplate geodynamics and magmatism in the evolution of the Central Asian Orogenic Belt

The Central Asian Orogenic Belt (CAOB) was produced as a consequence of the successive closure of the Paleoasian Ocean and the accretion of structures formed within it (island arcs, oceanic islands, and backarc basins) to the Siberian continent. The belt started developing in the latest Late Neoproterozoic, and this process terminated in the latest Permian in response to the collision of the Siberian and North China continents that resulted in closure of the Paleoasian ocean (Metcalfe, 2006; Li et al., 2014; Liu et al., 2009; Xiao et al., 2010; Didenko et al., 2010). Throughout the whole evolutionary history of this Orogenic Belt, a leading role in its evolution was played by convergent processes. Along with these processes, an important contribution to the evolution of the composition and structure of the crust in the belt was made by deep geodynamic processes related to the activity of mantle plumes.Indicator complexes of the activity of mantle plumes are identified, and their major distribution patterns in CAOB structures are determined. A number of epochs and areas of intraplate magmatism are distinguished, including the Neoproterozoic one (Rodinia breakup and the origin of alkaline rock belt in the marginal part of the Siberian craton); Neoproterozoic–Early Cambrian (origin of oceanic islands in the Paleoasian Ocean); Late Cambrian–Early Ordovician (origin of LIP within the region of Early Caledonian structures in CAOB); Middle Paleozoic (origin of LIP in the Altai–Sayan rift system); Late Paleozoic–Early Mesozoic (origin of the Tarim flood-basalt province, Central Asian rift system, and a number of related zonal magmatic areas); Late Mesozoic–Cenozoic (origin of continental volcanic areas in Central Asia).Geochemical and isotopic characteristics are determined for magmatic complexes that are indicator complexes for areas of intraplate magmatism of various age, and their major evolutionary trends are discussed. Available data indicate that mantle plumes practically did not cease to affect crustal growth and transformations in CAOB in relation to the migration of the Siberian continent throughout the whole time span when the belt was formed above a cluster of hotspots, which is compared with the African superplume.     

前寒武纪富铀矿床与热液碱交代作用

本文根据国内外文献资料,提出前寒武纪富铀矿床的形成与碱交代作用在空间上、成因上蕾切相关的认识,并根据碱性热水溶液的性质将前寒武纪富铀矿床分为钠交代型和钾交代型。同时,简述了两种类型矿床的主要特征,成矿地质条件及机理。     

Ophiolite hosted chromitite formed by supra-subduction zone peridotite –plume interaction

Chromitite bodies hosted in peridotites typical of suboceanic mantle (s.l. ophiolitic) are found in the northern and central part of the Loma Caribe peridotite, in the Cordillera Central of the Dominican Republic. These chromitites are massive pods of small size (less than a few meters across) and veins that intrude both dunite and harzburgite. Compositionally, they are high-Cr chromitites [Cr# ​= ​Cr/(Cr ​+ ​Al) atomic ratio ​= ​0.71–0.83] singularly enriched in TiO₂ (up to 1.25 ​wt.%), Fe₂O₃ (2.77–9.16 ​wt.%) as well as some trace elements (Ga, V, Co, Mn, and Zn) and PGE (up to 4548 ​ppb in whole-rock). This geochemical signature is unknown for chromitites hosted in oceanic upper mantle but akin to those chromites crystallized from mantle plume derived melts. Noteworthy, the melt estimated to be in equilibrium with such chromite from the Loma Caribe chromitites is similar to basalts derived from different source regions of a heterogeneous Caribbean mantle plume. This mantle plume is responsible for the formation of the Caribbean Large Igneous Province (CLIP). Dolerite dykes with back-arc basin basalt (BABB) and enriched mid-ocean ridge basalt (E-MORB) affinities commonly intrude the Loma Caribe peridotite, and are interpreted as evidence of the impact that the Caribbean plume had in the off-axis magmatism of the back-arc basin, developed after the Caribbean island-arc extension in the Late Cretaceous. We propose a model in which chromitites were formed in the shallow portion of the back-arc mantle as a result of the metasomatic reaction between the supra-subduction zone (SSZ) peridotites and upwelling plume-related melts.     

中国东部新生代玄武岩及其地幔包体的氧逸度

地幔环境的氧逸度与温度和压力一样,是控制许多地幔过程的一个重要参数。本文计算了中国东部几个具有代表性地区的玄武岩和尖晶石二辉橄榄岩的氧逸度,尖晶石二辉橄榄岩的氧逸度变化不大,均位于１ｏｇ（ｆｏ２）＝ｌｏｇ（ｆｏ２ＦＭＱ）＋０．０左右,而各地区玄武岩的氧逸度却变化很大,其平均值从尚志地区的ｌｏｇ（ｆｏ２ＦＭＱ＋０．６到长白山地区的ｌｏｇ（ｆｏ２ＦＭＱ）＋３．３左右（其中东北地区钾质玄武岩的氧逸度比除尚志以外其它地区的低）,并且总体具有比地幔橄榄岩高得多的氧逸度。推测钾质玄武岩和尚志地区破性玄武岩的氧逸度比中国东部其它地区玄武岩的氧逸度低的可能原因是,前二个地区的玄武岩来源于更深部的（金云母）石榴石二辉橄榄岩,而其它地区的玄武岩来源于略浅部的尖晶石二辉橄榄岩。     

内蒙古温都尔庙和巴彦敖包-交其尔蛇绿岩的元素与同位素地球化学：对古亚洲洋东部地幔域特征的限制

内蒙古中部发育的三条蛇绿岩带是华北板块和西伯利亚板块之间的缝合带。本文系统研究了其中的温都尔庙和巴彦敖包．交其尔两个蛇绿岩带中变质玄武岩的元素和Sr、Nd、Pb同位素地球化学。苏右旗温都尔庙碱性玄武岩为轻稀土富集型;岩石具有板内和大陆裂谷区玄武岩的特征,可能代表了600Ma左右,温都尔庙地区开始发育的新洋盆。采自苏左旗的巴彦敖包．交其尔玄武岩分为两类,一类呈现轻稀土富集型,呈洋岛玄武岩特征;另一类具有明显的Nb、Ta负异常,显示大洋岛孤玄武岩特征。洋岛玄武岩的存在表明古亚洲洋曾经发育洋盆,大洋岛弧玄武岩的存在表明古亚洲洋内部有大洋岩石圈之间的俯冲。将本文的古亚洲洋洋岛玄武岩与中国西南地区的特提斯洋岛玄武岩进行系统的元素和同位素地球化学特征对比表明,古亚洲洋的洋岛玄武岩显示高U／Pb（HU）和北大西洋和太平洋省的特征,而特提斯洋岛玄武岩属于印度洋省。这些说明古亚洲洋地幔域与特提斯地幔域是两个独立的构造域,它们代表了长期演化的两个不同的地幔地球化学域。     

地幔交代作用的微区微量元素证据——云南双沟蛇绿岩的质子探针研究

用质子探针技术对双沟地幔交代熔融物的微区微量元素进行了测定。研究表明,地幔橄榄岩中的残留矿物橄榄石和斜方辉石仅含Ni和Zn,而Ga、Ge、Sr、Rb、Zr、Y、As、Pb等微量元素主要集中在地幔部分熔融所产生的矿物(尤其是尖晶石和绿泥石)中。微区范围内微量元素的分布表明,尖晶石二辉橄榄岩地幔不均一性的尺度可达微米级,通常解释为尖晶石二辉橄榄岩在开放系统下地幔交代作用的结果。     

利用P波接收函数研究青藏高原东南缘地幔转换带结构

研究青藏高原东南缘的深部结构对于理解印度-欧亚板块的碰撞机理和青藏高原的形成演化具有重要的科学意义.本研究对布设在研究区域内566个固定和流动地震台站的波形资料进行了处理,获得77853条高质量P波接收函数,应用接收函数共转换点（CCP）叠加技术获得了研究区域下方精细的地幔转换带间断面起伏形态及转换带厚度变化图像.结果表明：研究区域南北方向上具有两个明显的转换带增厚异常区,南侧异常区位于滇中次级块体与印支块体下方,可能是新特提斯洋板片与上部印度板块间断离并部分滞留在转换带底部的结果;北侧川西地区异常增厚可能与上方岩石圈拆沉并降至转换带有关;腾冲火山起源可能是板块俯冲过程中发生断离造成软流圈物质部分熔融,湿热物质上涌所致.

     

新疆可可托海地区花岗岩成因的研究

新疆可可托海地区有三种花岗岩,它们形成于造山运动不同阶段:片麻状黑云母花岗岩是海西造山运动早期的产物;似斑状花岗岩形成于海西晚期;二云母花岗岩是印支一燕山期侵入而成。三者的岩石、岩石化学、CMF值和QAP图解、亲合度、微量无素、稀土元素、铅和氧同位素组成等研究表明,它们是陆壳交代重熔成因的一个连续成岩系列。     

Pyroxenite xenoliths from Marsabit (Northern Kenya): evidence for different magmatic events in the lithospheric mantle and interaction between peridotite and pyroxenite

Garnet-bearing and garnet-free pyroxenite xenoliths from Quaternary basanites of Marsabit, northern Kenya, were analysed for microstructures and mineral compositions (major and trace elements) to constrain the thermal and compositional evolution of the lithospheric mantle in this region. Garnet-bearing rocks are amphibole-bearing websterite with ~5–10 vol% orthopyroxene. Clinopyroxene is LREE-depleted and garnet has high HREE contents, in agreement with an origin as cumulates from basaltic mantle melts. Primary orthopyroxene inclusions in garnet suggest that the parental melts were orthopyroxene-saturated. Rock fabrics vary from weakly to strongly deformed. Thermobarometry indicates extensive decompression and cooling (~970–1,100°C at ~2.3–2.6 GPa to ~700–800°C at ~0.5–1.0 GPa) during deformation, best interpreted as pyroxenite intrusion into thick Paleozoic continental lithosphere subsequently followed by continental rifting (i.e., formation of the Mesozoic Anza Graben). During continental rifting, garnet websterites were decompressed (garnet-to-spinel transition) and experienced the same P–T evolution as their host peridotites. Strongly deformed samples show compositional overlaps with cpx-rich, initially garnet-bearing lherzolite, best explained by partial re-equilibration of peridotite and pyroxenite during deformation and mechanical mingling. In contrast, garnet-free pyroxenites include undeformed, cumulate-like samples, indicating that they are younger than the garnet websterites. Major and trace element compositions of clinopyroxene and calculated equilibrium melts suggest crystallisation from alkaline basaltic melt similar to the host basanite, which suggests formation in the context of alkaline magmatism during the development of the Kenya rift. Electronic supplementary material  The online version of this article (doi:) contains supplementary material, which is available to authorized users.