地幔柱活动对克拉通岩石圈地幔的影响：西伯利亚克拉通地幔橄榄岩包体Sr-Nd-Hf同位素制约

利用单矿物溶液法分析了Obnazhennaya金伯利岩中橄榄岩包体单矿物的Sr-Nd-Hf同位素组成,并且与Udachnaya金伯利岩中橄榄岩包体单矿物的Sr-Nd-Hf同位素组成进行了对比。结果显示,Obnazhennaya金伯利岩中橄榄岩包体单斜辉石具有亏损的Sr同位素组成和富集的Nd、Hf同位素组成。橄榄岩包体石榴子石的Sr-Nd-Hf同位素组成表现出原始的特征,没有受到交代作用的影响。通过对比Udachnaya和Obnazhennaya金伯利岩中地幔包体的特征和单斜辉石的二元混合模拟发现,Udachnaya金伯利岩中的地幔包体的Sr-Nd-Hf同位素组成更偏向于金伯利岩的特征,而与之相反,Obnazhennaya金伯利岩中的地幔包体的Sr-Nd-Hf同位素组成则位于金伯利岩和地幔柱溢流玄武岩之间,且更加偏向于溢流玄武岩的同位素特征。因此,地幔柱活动对西伯利亚克拉通岩石圈产生了影响,改变了其岩石圈地幔的同位素组成。     

中国东部新生代玄武岩及超镁铁岩包体研究

几年来作者以岩石学和矿物学为主体,结合中国东部地质构造、地层、同位素地质学、同位素年代学、稀土元素和地球化学等方面,对新生代火山岩及其中的超镁铁岩包体和高压巨晶,进行了比较全面、系统的多学科研究,取得了极丰富的实际资料和大量数据,进而对该区新生代玄武岩的岩浆性质、成因、时空分布、演化规律、构造控制因素和超镁铁岩包体及高压巨晶的类型、成因等一系列问题,提出了一些较成熟的见解和具有理论意义的讨论。     

浙江嵊县—新昌新生代玄武岩及包体的研究

浙江新生代玄武岩主要岩石类型为橄榄拉斑玄武岩.矿物组合、岩石化学和REE特征表明为碱性玄武岩系列,是非原生岩浆的结晶产物(M=36-60,SI=15-37)。K-Ar同位素年龄4—10Ma.碱性橄榄玄武岩内赋存幔源包体和高压巨晶,其中尖晶石二辉橄榄岩包体熔融程度8％,形成温度975℃,压力15.7×10~8Pa。     

我国东、南部玄武岩中尖晶石二辉橄榄岩包体的矿物研究

我国东部与南部新生代碱性玄武岩及火山角砾岩喷发过程中,携带了来自地幔及玄武岩浆深部结晶分异形成的包体,这些包体包括尖晶石二辉橄榄岩、石榴石二辉橄榄岩、辉石岩和辉长岩类,以及石榴石、辉石和歪长石巨晶等。我们收集了福建、江苏、河北及云南等地数十个包体,并对其中13个包体的矿物进行了研究,计算了包体形成的温度和压力,并讨论了成因。     

新生代碱性玄武岩中超镁铁质包体成因的新认识

全球范围内,新生代碱性玄武岩中常含有数量和大小不等的超镁铁质岩石包体(以下简称包体)。因其可供测定年龄的同位素含量甚少,因而迄今缺乏探讨其成因的年龄依据。本文对我国辽宁省宽甸地区第三纪碱性玄武岩中有代表性的两个包体的年龄进行方法研究和测定,获得了值得重视的结果。     

中国东南沿海中-新生代玄武岩微量元素和Nd-Sr-Pb同位素研究

本文对中国东南沿海不含幔源包体的中生代玄武岩和含幔源包体的新生代玄武岩进行了微量元素和Nd-Sr-Pb同位素对比研究。中生代玄武岩呈Ta、Nb和Hf负异常,低Ce/Pb、Nb/U比值和高La/Nb比值,与岛弧火山岩和陆壳岩石的微量元素特征相类似,说明在岩浆生成和上升过程中,幔源组分受到了陆壳组分的混染。新生代玄武岩呈Ta、Nb正异常和Pb负异常,高Ce/Pb、Nb/U比值和低La/Nb比值,与海岛玄武岩(OIB)相类似,Nd-Sr同位素成分与夏威夷玄武岩类似,因而它们未受明显的陆壳混染。143Nd/144Nd与206Pb/204Pb之间的负相关关系和87Sr/86Sr与206Pb/204Pb之间的正相关关系说明本区新生代玄武岩起源于中等亏损程度的软流圈地幔,并与EMII富集地幔组分发生了混合。     

广东麒麟绿钙闪石巨晶的地球化学特征

本文对罕见的幔源绿钙闪石巨晶进行了综合的地球化学分析，主要元素，稀土微量元素和Ｓｒ，Ｎｄ同位素的特征表明；绿钙闪石巨晶是碱性玄武岩浆在地幔条件下的结晶产物；相对于寄主玄武岩，绿钙闪石巨晶均属捕虏晶，它们与共存的橄榄岩包体无成因联系，其形成可能与共存的黑色包体有关。     

玄武岩及其深源包体学术讨论会会议报导

由中国矿物、岩石、地球化学学会召开的中国东部新生代玄武岩及其深源包体学术讨论会,于一九八二年七月二十七日至七月三十一日在黑龙江省德部县五大莲池举行。参加讨论会的有科研、院校、生产等五十几个单位130位代表。我国著名地质学家、岩石学家和大地构造学家尹赞勋、张文佑、马杏垣、徐克勤,吴利仁等参加了会议,并在会上作了学术报告,受到与会代表的欢迎。我院岩浆岩研究室和岩石教研室7位教师和研究生代表出席了会议。 讨论会是我国研究新生代玄武岩及其深源包体岩石学与地壳运动关系的一次盛大的学术交流会。会议收到论文74篇,其中我院教师及研究生提交8篇。这些论文提供了中国东部几十个地区新生代玄武岩及其深源包体的岩石学,造岩矿物学,岩石化学,同位素地球化学,     

我国东南部地区深源包体矿物中Mg同位素比值的离子探针研究

本文对产于我国东，南部地区新生代碱性玄武岩中尖晶石橄榄二辉岩和尖晶石二辉橄榄岩包体矿物，应用离子探针（SIMS）线性分析和深度分析方法，测定Mg同位素比值。从SIMS所揭示的深源包体矿物Mg同位素组成异常现象来看，可以为进一步探讨地幔矿物的物质来源与演化提供信息。     

湖南省道县虎子岩片麻岩包体的岩石学特征和年代学研究

通过对道县虎子岩碱性玄武岩中片麻岩包体的岩石化学、Ｎｄ同位素模式年龄ＴＤＭ和颗粒锆石Ｕ－Ｐｂ法测年结果，确定了本区片麻岩包体的变质反应、变质相和原岩类型，恢复了本区前寒武纪地壳的形成和演化历史     

滇西澜沧老厂地区玄武岩岩石成因与构造意义

对滇西澜沧老厂地区玄武岩进行了系统的主微量元素和Nd-Pb同位素地球化学研究,结果表明该玄武岩为典型的洋岛玄武岩(OIB)。Nd-Pb同位素研究表明,玄武岩浆含富集地幔组分。老厂地区玄武岩浆活动可能与地幔热柱有关,玄武岩可能为地幔热柱(软流圈)熔融产生的岩浆与富集的岩石圈地幔岩浆混合的产物。     

The 1996 Eruption of Karymsky Volcano, Kamchatka: Historical Record of Basaltic Replenishment of an Andesite Reservoir

The simultaneous eruption in 1996 of andesite from Karymskyvolcano and of basalt from the Academy Nauk vent 6 km away appearsto provide a case of mafic recharge of an andesite reservoirfor which the time of recharge is exactly known and direct samplesof the recharging magma are available. The explosive phreato-magmaticeruption of basalt was terminated in less than 24 h, whereasandesite erupted continuously during the following 4 years.Detailed petrological study of volcanic ash, bombs and lavasof Karymsky andesite erupted during the period 1996–1999provides evidence for basaltic replenishment at the beginningof the eruptive cycle, as well as a record of compositionalvariations within the Karymsky magma reservoir induced by basalticrecharge. Shortly after the beginning of the eruption the compositionof the matrix glass of the Karymsky tephra became more maficand then, within 2 months, gradually returned to its originalstate and remained almost constant for the following 3 years.Further evidence for basaltic replenishment is provided by thepresence of xenocrysts of basaltic origin in the andesite ofKarymsky. A conspicuous portion of the plagioclase phenocrystsin the Karymsky andesite has calcic cores, with compositionsand textures resembling those of plagioclases in the AcademyNauk basalt. Similarly, the earlier portion of the andesiteof the eruption sequence contains rare olivines, which occuras resorbed cores in pyroxenes. The composition of the olivinematches that of olivines in the Academy Nauk basalt. The sequenceof events appears to be: (1) injection of basaltic magma intothe Karymsky chamber with immediate, compensating expulsionof pre-existing chamber magma from the Karymsky central vent;(2) direct mixing of basaltic and andesitic magmas with dispersalof phenocrysts associated with the basalt throughout the andesiteso that newly mixed magma appeared at the vent within 2 months;(3) re-establishment of thermal and chemical equilibrium withinthe reservoir involving crystallization in the new hybrid liquid,which returned the melt composition to ‘normal’,formed rims on inherited calcic plagioclase, and caused theresorption of dispersed olivine xenocrysts. Taken together,these findings indicate that the Karymsky magma reservoir wasrecharged by basalt at the onset of the 1996 eruptive cycle.The rapidity and thoroughness of mixing of the basalt with thepre-existing andesite probably reflects the modest contrastin temperature, viscosity, and density between the two magmas. KEY WORDS: Karymsky; Kamchatka; magma mixing; andesite; volcanic glass; plagioclase     

歧口凹陷火成岩的地球化学特征、形成时代及构造意义

歧口凹陷侏罗系火成岩主要以中-酸性的流纹岩、粗面岩和粗面安山岩为主,白垩系主要为中-基性的粗面玄武岩和玄武质粗面安山岩,第三系火成岩以粗面玄武岩、碱性玄武岩及辉绿岩为主。同位素定年结果获得白垩系玄武岩的年龄为133±20 Ma,安山岩和粗安岩年龄分别为111.8±0.9 Ma和122.1±3.1 Ma,第三系辉绿岩年龄为16.57±0.23 Ma。地球化学特征显示,侏罗系火成岩相对低钛、高碱和钠、低铁镁,轻重稀土元素强烈分馏、微量元素相对富集LILE、贫化HFSE、亏损Nb和Ti、P,部分高Sr、低Yb,总体指示为挤压环境下加厚地壳物质的熔融产物,白垩系火成岩中等钛和碱的含量,高钠、铁和镁,稀土和微量元素显示其来自于伸展背景的富集地幔源,但受到陆壳物质的混染,第三系火成岩高钛含量、中等碱含量但变化大、高钠、富铁镁,轻重稀土元素分馏弱到中等、微量元素富集LILE和HFSE,同样来自板内伸展环境的富集地幔源的产物。表明歧口凹陷构造转换发生在晚侏罗世和早白垩世之间。     

贵东花岗岩体中煌斑岩的成因

本文主要从大地构造环境、煌斑岩的空间分布及其硫同位素、微量元素和稀土元素组成等方面,探讨贵东花岗岩体中煌斑岩的成因.结果表明,煌斑岩与周围的壳型花岗岩不同源,形成煌斑岩的原始岩浆,应为幔源大陆拉斑玄武岩浆。     

Nickel content of basaltic magmas: identification of primary magmas and a measure of the degree of olivine fractionation

Available NiO analyses of olivine in peridotites of probable mantle origin are consistent in giving values around 0.40 weight per cent. Assuming that basaltic magma forming from the mantle was in equilibrium with such peridotitic olivine, the NiO content of primary basaltic magmas is estimated to be about 0.030–0.050 weight per cent. The fractionation behaviour of nickel in basaltic magma due to the crystallization of olivine has been calculated using constant NiMg and FeMg exchange partition coefficients between olivine and magma. It is shown that the NiO content of both magma and olivine decreases by 50 per cent after fractional crystallization of 6–12 per cent of olivine. The nickel distribution in some basaltic rocks and olivines is examined in the light of these results, and it is suggested that basaltic magmas, such as some of the ocean-floor basalt and the Hawaiian tholeiite and alkali basalts, represent primary magmas from mantle peridotites.     

峨眉山玄武岩和白马层状岩体的铬镍地球化学

文章讨论了峨眉山玄武岩及白马基性、超基性岩体的微量元素地球化学特征。对Cr、Ni富集的地球化学条件进行了探讨,认为在母岩浆分离结晶早期形成的堆积层,即结晶度很小的橄榄岩有利于寻找富Cr、Ni层位。     

广西平南玄武岩的地球化学特征

平南碱性玄武岩产于 NE向的区域性断裂中 ,岩石类型有两类 ,一为碧玄岩 ,全岩 K- Ar年龄为 50 .8Ma,含各类包体 ,有以下特征 :1)含地幔岩包体 ,2 ) [Mg]=0 .78,3)在 Fe O/mol- Mgo/mol图解上液相线橄榄石的成分位于 Fo90～ Fo94之间 ,与橄榄岩包体中的橄榄石成分完全一致。4 ) Ni=0 .0 4 ( % ) <0 .0 5( % ) ,5)其熔浆密度为 2 .62 g/cm3,粘度为 2 .52 Pa· s,携带 4 cm直径包体上升的速度为 37.7cm/s,上升的速度较快 ,具原生碧玄岩浆的特点 ,岩浆液相线的温度为12 86℃ ,起源压力为 1.8GPa,玄武岩富集轻稀土可能与地幔性质有关。一为粗面玄武岩 ,不含包体 ,全岩 K- Ar年龄为 4 9.9Ma,岩浆液相线的温度为 1162℃ ,是进化岩浆。玄武岩的 Nd、Sr同位素显示为亏损地幔源区。它们都是大陆拉张环境下的产物 ,与中国东部新生代玄武岩的形成背景一致。     

Evolution of Holocene Dacite and Compositionally Zoned Magma, Volcan San Pedro, Southern Volcanic Zone, Chile

Volcán San Pedro in the Andean Southern Volcanic Zone(SVZ) Chile, comprises Holocene basaltic to dacitic lavas withtrace element and strontium isotope ratios more variable thanthose of most Pleistocene lavas of the underlying Tatara–SanPedro complex. Older Holocene activity built a composite coneof basaltic andesitic and silicic andesitic lavas with traceelement ratios distinct from those of younger lavas. Collapseof the ancestral volcano triggered the Younger Holocene eruptivephase including a sequence of lava flows zoned from high-K calc-alkalinehornblende–biotite dacite to two-pyroxene andesite. Notably,hornblende–phlogopite gabbroic xenoliths in the daciticlava have relatively low ⁸⁷Sr/⁸⁶Sr ratios identical to theirhost, whereas abundant quenched basaltic inclusions are moreradiogenic than any silicic lava. The latest volcanism rebuiltthe modern 3621 m high summit cone from basaltic andesite thatis also more radiogenic than the dacitic lavas. We propose thefollowing model for the zoned magma: (1) generation of hornblende–biotitedacite by dehydration partial melting of phlogopite-bearingrock similar to the gabbroic xenoliths; (2) forceful intrusionof basaltic magma into the dacite, producing quenched basalticinclusions and dispersion of olivine and plagioclase xenocryststhroughout the dacite; (3) cooling and crystallization–differentiationof the basalt to basaltic andesite; (4) mixing of the basalticandesite with dacite to form a small volume of two-pyroxenehybrid andesite. The modern volcano comprises basaltic andesitethat developed independently from the zoned magma reservoir.Evolution of dacitic and andesitic magma during the Holoceneand over the past 350 kyr reflects the intrusion of multiplemafic magmas that on occasion partially melted or assimilatedhydrous gabbro within the shallow crust. The chemical and isotopiczoning of Holocene magma at Volcán San Pedro is paralleledby that of historically erupted magma at neighboring VolcánQuizapu. Consequently, the role of young, unradiogenic hydrousgabbro in generating dacite and contaminating basalt may beunderappreciated in the SVZ. KEY WORDS: Andes; dacite; gabbro; Holocene; strontium isotopes     

云南景洪南联山橄榄岩—闪长岩型岩体的特征及地质意义

岩相学和地球化学特征表明,南联山岩体是岩浆侵位的,岩石的分布显示环带构造;从中心向外依次为角闪橄榄岩、辉绿(辉长)岩和闪长岩。它们的结构和化学特征指示,这些岩石是由辉长-闪长岩质的岩浆结晶分异作用而形成的,角闪橄榄岩和部分辉绿岩为堆晶岩,其它的岩石为堆晶作用后分异而成的岩浆共结结晶作用所形成。原始岩浆的成分类似于高铝玄武岩和(或)玄武质安山岩。     

月球雨海地区玄武质岩浆充填活动期次的重新厘定及地质意义

雨海盆地是月球上研究程度最高的多环结构盆地,月球上古老的和年轻的玄武岩在盆地中均有分布,因此雨海是研究月海玄武岩岩浆活动的理想区域。为了更合理的厘定雨海地区的玄武质岩浆演化历史,本文主要结合岩石学、年代学等工作对本区玄武岩的充填期次进行重新划分。利用嫦娥一号IIM光谱数据进行岩石类型分布图编制,初步划分了5类不同钛含量的月海玄武岩;基于高分辨率100m LRO宽视角影像数据通过撞击坑尺寸-频率定年法(CSFD)对本区玄武岩单元模式年龄进行厘定,共划分35个玄武岩单元,发现本区在3.49~2.23Ga均有玄武质岩浆充填活动,具有多期次性。在建立不同类别玄武岩、形貌特征与模式年龄的对应关系基础上,将玄武岩充填划分为4个期次:极低钛玄武岩(3.49~3.20Ga)、低钛玄武岩(3.29~2.83Ga)、中钛玄武岩(3.13~2.52Ga)、(极)高钛玄武岩(2.92~2.23Ga)。本区地形地貌高程特征与不同表面年龄的玄武岩单元之间总体上呈现出一定的负相关性。因此在本区玄武质岩浆期次划分考虑上,不仅要考虑玄武岩的成分特征,更要考虑结合与玄武岩演化密切相关的年代学及形貌学特征,利用形貌、成分数据和年代学信息来共同约束玄武质岩浆期次划分及演化历史。