中国东部新生代玄武岩中巨晶矿物的地球化学

本文对安徽女山、河北汉诺坝和广东普宁碱性玄武岩中的单斜辉石和角闪石巨晶进行了主要元素、稀土元素、微量元天和Ｓｒ＿Ｎｄ同位素的综合分析。数据显示产出于３个研究区的单斜辉石巨晶有３类：Ａｌ普通辉石、透辉石和Ｆｅ＿Ｎａ透辉石。普宁地区的角闪石巨晶乃世界上罕见的绿钙闪石巨晶。女山和普宁的单斜辉石和角闪石巨晶是碱性玄武岩浆在幔源高压下的结晶产物；汉诺坝的单斜辉石巨晶既可以是碱性玄武岩浆又可以是拉斑玄武岩浆的高压结晶体。所有巨晶相对于寄主岩者属于偶然捕掳晶。巨晶的形成符合“流动结晶模式”。它们与共存的橄榄岩色体无成因     

冀东迁西-迁安地区早太古代变质岩系原岩恢复及其地质意义

冀东早太古代变质岩系的主体是一套呈层分布的,各种成分麻粒岩及其某些退变质产物——斜长角闪岩类。在其上部发育变质含铁建造,而在其下部常夹有变质的镁铁质和超镁铁质岩(如变闪辉岩、变辉石岩和蛇纹石化橄榄岩等)薄层或透镜体。 麻粒岩的矿物组合是斜方辉石+单斜辉石+斜长石(常常为反条纹长石)+石英+磁铁矿±角闪石±黑云母。在变质含铁建造中局部出现包括铝硅酸盐的矿物组合(蓝晶石-石榴石-黑云母-斜长石-石英)。变质铁硅质岩可以分为两类:辉石磁铁石英岩和英榴易熔岩(张儒瑗,从柏林,1981)。     

新疆尾亚含矿岩体锆石U-Pb年龄、 Sr-Nd同位素组成及其地质意义

东天山尾亚钒钛磁铁矿矿床是北疆地区最大的钒钛磁铁矿矿床,其含矿岩系为一套偏碱性的镁铁-超镁铁质杂岩。含矿岩石主要造岩矿物橄榄石、辉石、角闪石、黑云母和斜长石的化学成分与铁质系列的镁铁-超镁铁岩成分相似或相同;辉石、角闪石、黑云母等矿物以富钛为特点,这些矿物中Ti、Fe等在早期形成的岩石(辉橄岩、橄榄辉长岩)中较晚期岩石中有明显富集。含矿辉长岩的锆石LA-ICPMS U-Pb同位素定年结果为236±3Ma,主要成岩时代为中三叠世,代表后碰撞结束阶段的成矿作用。这套含矿镁铁-超镁铁杂岩的Sr-Nd同位素特征以ε_(Nd)(t)均为正值,(~(87)Sr/~(86)Sr)_i值较低为特征,与原始地幔相近,但在岩浆上移过程中可能有陆壳物质加入。     

中国东部某些地区碱性玄武岩中包体的温度、压力的计算

一、概述中国东部新生代碱性玄武岩系列的火山岩中广泛分布着超镁铁岩包体。这些包体是我们直接能观察到的该地区上地幔的标本。它对于了解该地区上地幔物质组成和地温分布具有重要的意义。现仅就收集到的包体资料,侧重对其温度压力条件进行估计,尝试着对这些地区上地幔的组成和地温分布进行一些讨论。超镁铁岩包体主要是尖晶石二辉橄榄岩。在浙江和福建等地还分布有石榴石二辉橄榄岩。此外,还有少量的纯橄榄岩、斜方辉石岩、单斜辉石岩、二辉石岩,含角闪石的尖晶石二辉橄榄岩     

甘肃宕昌好梯碱性超基性火山岩:一种含上地幔包体和巨晶的钾质超镁铁煌斑岩

甘肃宕昌好梯含上地幔包体和巨晶的碱性超基性火山岩为新生代火山作用的产物。该火山岩的岩相学、矿物学、岩石化学和地球化学特征显示了从碱性基性岩(霞石碱玄岩-碧玄岩)-超基性岩(苦橄岩-玻基辉橄岩)-钾镁煌斑岩之过渡类型岩石的特征。表明好榜火山岩是一种煌斑岩。根据火山岩的岩相学、矿物学、岩石化学和地球化学特征,火山岩的镁铁指数>90,特别是岩石中含一定数量的金云母以及含白榴石、原生方解石、碱性角闪石和碱性辉石的球状分异物等特征,将该火山岩命名为钾质超镁铁煌斑岩。本文还提出该钾质超镁铁煌斑岩代表一种原生煌斑岩浆的标志。     

西垄玄武质岩石中的橄榄岩类包体、捕虏晶以及巨晶的矿物化学研究

浙江衢县西垄和金华龙游一带分布有许多第三纪的霞石玄武岩、玻基橄辉岩、橄辉玢岩和超基性火山角砾岩岩体和岩脉。它们富含橄榄岩类包体和来源于破碎的橄榄岩包体的各种捕虏晶(橄榄石、斜方辉石、透辉石和石榴石)。此外,还常含有富铝普通辉石、石榴石和钛铁矿巨晶。本文试图在大量的单矿物分析数据基础上,讨论橄榄岩类包体、捕虏晶以及巨晶的矿物化学及其形成条件。关于橄榄岩包体的主要元素和微量元素地球化学以及成因岩石学的研究,笔者已在另一篇论文中专门论述(从柏林和张儒瑗,1983),这里不再重复。     

压力对稀土元素分配系数相对变化的影响——以宽甸、汉诺坝玄武岩中巨晶矿物为例

通过对与寄主岩(碱性玄武岩)具有化学平衡或近于化学平衡关系的巨晶(石榴石、辉石和角闪石)的REE分配系数的研究,发现其REE分配系数的对数值相对于元素半径呈抛物线性变化。抛物线的顶点位置不但随矿物种类的不同而不同,而且对同一矿物也是变化的。随压力增大,同一种矿物的分配系数抛物线顶点向离子半径小的元素方向偏移,可以认为在不同深度生成或演化的玄武岩岩浆的REE分布模式受压力的影响较大。     

昌乐地区新生代碱性玄武岩中刚玉巨晶和伴生地幔岩捕虏体与熔体作用的研究

<正>西太平洋板块大陆边缘火山活动区的蓝宝石矿床,分布于塔斯马尼亚岛、澳大利亚的南部到东部、中国东部及俄罗斯东部(Graham,et al.,2008)。中国东部广泛分布的新生代碱性玄武岩中,山东昌乐蕴含中国最大的蓝宝石矿床,与蓝宝石/刚玉相伴生的地幔岩捕虏体为辉石岩和橄榄岩(董振信等,1999)。野外勘察发现,赋存蓝宝石/刚玉的层位往往含地幔橄榄岩捕虏体及矿物巨晶,而不含捕虏体的玄武岩层则不见刚玉,     

内蒙古阿巴嘎旗新生代玄武岩中超镁铁岩包体的特征

内蒙古东部阿巴嘎旗及其以北地区第四纪更新世钠质碱性火山岩中发现的超镁铁岩包体,主要为尖晶石二辉橄榄岩、方辉橄榄岩、纯橄榄岩、橄榄二辉岩、尖晶石单斜辉石岩和单斜辉石巨晶以及辉长岩、花岗闪长岩、石英长石片麻岩等壳源包体。超镁铁岩包体和巨晶的岩相学特征显示它们不是寄主玄武岩岩浆分离结晶堆积体;其主要元素、稀土元素特征与阿尔卑斯型橄榄岩相似,其组成接近于原始地幔岩值;同位素地球化学特征表明它们与寄主岩-玄武岩浆不是同源的;尖晶石二辉橄榄岩包体形成的平衡温度和压力范围分别为1056.9℃～1103.1℃,压力为1.50～1.84GPa,形成相当深度为49.5～60.72km。辉石岩包体形成温度为887.1℃～958.6℃,压力为1.25～1.4GPa,形成相当深度为41.25～46.2km。寄主玄武岩形成温度1390℃～1450℃,压力1.75～2.20GPa,形成相当深度为60～70km。可以认为,研究区在新生代发生了软流圈地幔上涌,导致岩石圈减薄以及地壳的拉张,大量岩浆物质沿构造通道溢出地表。其中超镁铁岩包体与寄主玄武岩浆之间没有熔体与残余物这种成因联系,它们是寄主玄武岩浆在上升过程中捕获的岩石圈地幔碎块。     

安徽栏杆含金刚石基性岩中辉石及钛铁矿矿物化学特征

在中国东部皖北地区分布着新元古代镁铁质岩,岩石类型为辉绿岩、辉绿辉长岩、辉绿玢岩等。其中主要组成矿物为辉石、斜长石、角闪石、铁钛氧化物等。利用电子探针对单斜辉石和钛铁矿进行了详细研究。单斜辉石分析表明,其端元分子组成硅灰石分子(Wo)为33.27～43.04,顽火辉石分子(En)为38.79～46.63,斜方铁辉石(Fs)为10.45～24.83,属于普通透辉石。计算结果及化学成分比值说明,单斜辉石应该是在寄主碱性玄武质岩浆晚期低压下结晶的,可能是碱性玄武质岩浆浅位岩浆房晶出的产物。单斜辉石的结晶温度为1109～1206℃,压力最高为0.6GPa,相当于深部19.8km。栏杆地区钛铁矿含MgO和Cr_2O_3较低,具有富FeO,并含少量MnO的特点,属于含镁锰钛铁矿。两类矿物特征均与典型金伯利岩中的指示矿物不同。     

Ultramafic inclusions and high pressure megacrysts from a nephelinite sill,Nandewar Mountains,north-eastern New South Wales,and their bearing on the origin of certain ultramafic inclusions in alkaline volcanic rocks

Ultramafic inclusions and megacrysts are unusually abundant in a nephelinite sill in the Nandewar Mountains in north-eastern New South Wales. The inclusions are divisible into a Cr-diopside group and a Ti-augite group, the former being dominated by Cr-spinel Iherzolites of restricted modal composition, the latter by olivine and titaniferous Al-rich clinopyroxene assemblages which vary widely in their modal proportions. The principal megacryst species are olivine and black, titaniferous Al-rich clinopyroxene; additional but comparatively rare megacrysts include titanphlogopite, kaersutitic amphibole, and deep green, relatively Fe-rich clinopyroxene. The Cr-spinel Iherzolites conform closely in mineralogy and chemistry with the spinel lherzolites which dominate upper mantle xenolith assemblages in alkaline mafic volcanic rocks from other provinces. Megacrysts and Ti-augite inclusion mineral assemblages are consistently more Fe-rich than analogous phases in the Cr-diopside xenoliths and also display more extensive cryptic variation. The available experimental data on the high pressure liquidus or near-liquidus phases in olivine nephelinite and related compositions indicate that the olivine and black clinopyroxene megacrysts were precipitated at pressures in the vicinity of 15–20 kb. The similarity in the nature and compositions of the principal megacryst species to analogous phases in the Tiaugite group of inclusions indicates that the latter also represent cognate cumulates derived from the olivine nephelinite at broadly comparable pressures. High pressure fractionation of the host olivine nephelinite liquid, controlled mainly by the separation of olivine and aluminous clinopyroxene, produced only comparatively minor compositional changes in the derivative liquid. The hiatus in olivine compositions at approximately Fo_86–88, apparently characteristic of the olivines in coexisting Cr-diopside and Ti-augite inclusions, is assessed in terms of the compositions of olivine in equilibrium with alkali basaltic liquids at high pressures.     

An Al-spinel ultramafic-mafic inclusion suite and high pressure megacrysts in an analcimite and their bearing on basaltic magma fractionation at elevated pressures

An analcimite sill, which intrudes Carboniferous sedimentary rocks northwest of the township of Barraba in northeastern New South Wales, is exceedingly rich in ultramafic and mafic inclusions and also contains a varied megacryst assemblage. The majority of inclusions belong to an ultramafic-mafic granulite suite whose members generally contain a Cr-poor green spinel. Layering is preserved in many inclusions and their textures are appropriate to those arising from recrystallization at subsolidus temperatures. Ultramafic granulites of the Al-spinel suite are mainly pyroxenites, with rarer lherzolites, and mafic granulites usually consist of the assemblage plagioclasea-luminous pyroxenes-spinel. Ca-rich tschermakitic clinopyroxenes and coexisting aluminous Ca-poor orthopyroxenes define a trend of moderate iron enrichment. Spinels also display significant Fe²⁺ → Mg substitution. Plagioclase in some plagioclase-bearing pyroxenites and mafic granulites contains numerous rod-like inclusions of spinel, compositionally similar to the discrete spinels unassociated with plagioclase. The formation of spinel in plagioclase is believed to have resulted largely from the migration of (Mg, Fe²⁺) to Al-rich nucleation sites in the feldspar. Other inclusion types include Cr-spinel lherzolites —more Fe-rich than Cr-diopside lherzolite inclusions in alkaline volcanics — and rare wehrlite heteradcumulates, probably cognate with the host analcimite. The megacryst assemblage is dominated by anorthoclase megacrysts, which are accompanied, in order of decreasing abundance, by megacrysts of tschermakitic clinopyroxene, titanbiotite, kaersutite, and aluminous titanomagnetite. The Al-spinel mafic granulites have low Ti, K and P contents and their petrochemical affinities are high-alumina mafic alkaline to transitional. They compare closely in major and minor element chemistry with some ocean ridge basalts. The Al-spinel ultramafic-mafic inclusions suite is interpreted as the remnants of a layered ultramafic-mafic “pluton ” which initially crystallized at pressures in the vicinity of 10 kb and subsequently re-equilibrated at subsolidus temperatures (ca 950° C) and comparable pressures. The parent magma was K-poor, ol-normative subalkaline and its fractionation at moderate pressures, controlled mainly by olivine and subcalcic clinopyroxene, resulted in decreases in the derivative liquids in their saturation levels and ol contents, and increases in Al and Ca. These trends are reflected in the compositions of the mafic granulites. The pressure regime of megacryst formation apparently was greater than 10–12 kb i.e. the megacrysts precipitated before acquisition of xenoliths of the Al-spinel granulite suite by the analcimite host. Anorthoclase fractionation produced only limited compositional changes in the original alkali basaltic melt.     

Trace element abundances in megacrysts and their host basalts: Constraints on partition coefficients and megacryst genesis

In an effort to obtain information about mineral/melt trace element partitioning during the high pressure petrogenesis of basic rocks, we determined rare earth and other trace element abundances in megacrysts of clinopyroxene, orthopyroxene, amphibole, mica, anorthoclase, apatite and zircon, and in their host basalts. In general, the ranges of mineral/melt partition coefficients established from experimental partitioning studies and phenocryst/matrix measurements overlap with the ranges of megacryst/host abundance ratios. Our data for Hf, Sc, Ta and Th partitioning represent some of the only estimates available. Consideration of phase equilibria, major element partitioning and isotopic ratios indicate that most of the pyroxene and amphibole megacrysts may have been in equilibrium with their host magmas at high pressures (mostly 10–25 kb). In contrast, it is unlikely that mica, anorthoclase, apatite and zircon megacrysts formed in equilibrium with their host basalts; instead, we conclude that they were precipitated from more evolved magmas and have been mixed into their present host magmas. Consequently, the trace element abundance ratios for megacryst/host should not be interpreted as partition coefficients, but only as guides for understanding trace element partitioning during high pressure petrogenesis. With this caveat, we conclude that the megacryst/ host trace element abundance data indicate that mineral/melt partition coefficients in basaltic systems during high pressure fractionation are not drastically different from partition coefficients valid for low pressure fractionation.     

华北晚中生代和新生代玄武岩中单斜辉石巨晶来源及其对寄主岩岩浆过程的制约:以莒南和鹤壁为例

本文对华北克拉通晚中生代和新生代碱性玄武质岩石中的单斜辉石巨晶进行了主、微量元素和Sr-Nd同位素的综合研究,发现晚中生代和新生代单斜辉石巨晶存在明显的主、微量元素和同位素组成上的差异。新生代单斜辉石巨晶有Al-普通辉石和次透辉石两类;而中生代单斜辉石巨晶只有Al-普通辉石。新生代单斜辉石SiO_2含量高、REE配分型式为上凸型、LILE和放射性元素含量高,并具有比寄主碱性玄武岩更亏损的Sr和Nd同位素组成;而中生代单斜辉石SiO_2含量低、REE配分型式为LREE富集型、LILE和部分HFSE以及放射性元素含量低,并具有比寄主碱性玄武岩稍富集的Sr和Nd同位素组成;巨晶的结构、矿物成分和地球化学特征,以及Mg-Fe在熔体与单斜辉石间的分配状况皆说明,新生代碱性玄武岩中单斜辉石巨晶是碱性玄武岩浆在高压下结晶的,因此二者是同源的;而中生代单斜辉石巨晶是被寄主岩浆偶然捕获的捕虏晶,是不同源的。华北新生代单斜辉石巨晶存在于碱性玄武岩和拉斑玄武岩中,它们具有比寄主碱性玄武岩更亏损的Sr和Nd同位素组成,说明即使是碱性玄武岩也不能完全代表软流圈来源的原始岩浆,其在上升过程中或多或少存在同位素组成富集的物质的混入。同时,拉斑玄武岩不是碱性玄武质岩浆直接结晶分异的产物,亦不是完全由部分熔融程度的不同造成的。拉斑玄武岩中存在岩石圈地幔物质的贡献或是岩浆房内碱性玄武质岩浆受地壳混染作用的结果。     

Kaersutite-peridotite inclusions and kindred megacrysts in basanitic lavas,Grand Canyon,Arizona

Essentially two types of ultramafic inclusions occur in the basanitic lavas and ejecta deposits of the northwestern Grand Canyon, Arizona. Abundant, olivine-rich nodules contain an emerald green, chrome-rich diopside and chrome-rich spinels. A much less common group of inclusions generally containing poikilitic kaersutite have more variable modal compositions, more variable but iron-rich and chrome-poor mineral compositions, and are characterized by the presence of a titaniferous clinopyroxene which appears black in hand specimen. The nature and petrologic significance of these black clinopyroxene-bearing inclusions, together with megacrysts of kaersutite and black clinopyroxene, are discussed in this paper.Petrographic aspects indicate an origin as cumulates of fractionating basaltic magma. Compositions of pyroxenes suggest high pressures of crystallization. The co-precipitation of orthopyroxene, clinopyroxene, olivine and Mg-spinel from what in all probability was under-saturated magma, together with the total absence of feldspar as a cumulate or intercumulate phase, is compatible with crystallization near 10 kb, on the basis of quite limited experimental data on anhydrous basaltic compositions. Pressures of this sort are attained at depths close to the mantle-crust boundary in the western Grand Canyon. By way of comparison, cumulate-textured inclusions from central Nevada containing rare orthopyroxene, widespread plagioclase, and more Fe-enriched clinopyroxenes, kaersutites, olivines and spinels are postulated to have crystallized at lower temperatures (or at a more advanced stage of fractionation) and possibly at lower pressures.Numerous occurrences, worldwide, of kaersutite-bearing inclusions, always in undersaturated host rocks, have recently been reported. Compositionally, the kaersutites are quite uniform, whether coexistent with pyropic garnet-clinopyroxene (Kakanui, New Zealand), with ortho-pyroxene-clinopyroxene-olivine-Mg spinel (Grand Canyon), or with plagioclase-clinopyroxene-olivine-magnetite. The last assemblage is found in shallow-seated igneous bodies of alkalic, mafic composition, as well as in inclusions within basaltic rocks. These occurrences imply the precipitation of kaersutite amphibole over a broad range of pressures, and as high as those prevailing in the upper mantle.     

苏鲁皖新生代玄武岩中巨晶组合的稀土元素特征

我国东部苏鲁皖地区新生代碱性玄武岩中,除了含有大量地幔橄榄岩类捕虏体以外,尚含有一定数量的石榴石、普通辉石和歪长石巨晶。这些巨晶是在地幔不同深度上从玄武岩中晶出的。巨晶组合的分离结晶作用对熔体稀土元素含量有很大影响。赋存巨晶的碱性玄武岩所具有的LREE富集、HREE亏损的稀土元素分配型式是由地幔橄榄岩类部分熔融程度、石榴石巨晶和普通辉石巨晶的早期高压熔离和玄武岩的结晶分异作用等综合因素造成的。     

Amphibole megacrysts as a probe into the deep plumbing system of Merapi volcano,Central Java,Indonesia

Amphibole has been discussed to potentially represent an important phase during early chemical evolution of arc magmas, but is not commonly observed in eruptive arc rocks. Here, we present an in-depth study of metastable calcic amphibole megacrysts in basaltic andesites of Merapi volcano, Indonesia. Radiogenic Sr and Nd isotope compositions of the amphibole megacrysts overlap with the host rock range, indicating that they represent antecrysts to the host magmas rather than xenocrysts. Amphibole-based barometry suggests that the megacrysts crystallised at pressures of >500 MPa, i.e., in the mid- to lower crust beneath Merapi. Rare-earth element concentrations, in turn, require the absence of magmatic garnet in the Merapi feeding system and, therefore, place an uppermost limit for the pressure of amphibole crystallisation at ca. 800 MPa. The host magmas of the megacrysts seem to have fractionated significant amounts of amphibole and/or clinopyroxene, because of their low Dy/Yb ratios relative to the estimated compositions of the parent magmas to the megacrysts. The megacrysts’ parent magmas at depth may thus have evolved by amphibole fractionation, in line with apparently coupled variations of trace element ratios in the megacrysts, such as e.g., decreasing Zr/Hf with Dy/Yb. Moreover, the Th/U ratios of the amphibole megacrysts decrease with increasing Dy/Yb and are lower than Th/U ratios in the basaltic andesite host rocks. Uranium in the megacrysts’ parent magmas, therefore, may have occurred predominantly in the tetravalent state, suggesting that magmatic fO₂ in the Merapi plumbing system increased from below the FMQ buffer in the mid-to-lower crust to 0.6–2.2 log units above it in the near surface environment. In addition, some of the amphibole megacrysts experienced dehydrogenation (H₂ loss) and/or dehydration (H₂O loss), as recorded by their variable H₂O contents and D/H and Fe³⁺/Fe²⁺ ratios, and the release of these volatile species into the shallow plumbing system may facilitate Merapi’s often erratic eruptive behaviour.     

强烈热液交代金矿石Rb—Sr等时线意义讨论

本文以曾经遭受强烈热液交代的含金石英闪长岩为研究对象，首次尝试性探索金矿石ＲｂＳｒ等时线测年研究。结果表明，在特定的热液蚀变矿物组合（不含绿帘石，以石英±绿泥石±绢云母±钠长石为主），强烈热液蚀变（黄铁矿化度（ＤＯＰ）＞７０％）以及锶同位素初始组成基本达到均一化的前提条件下，其ＲｂＳｒ等时线具确定的成矿地质意义，可代表后期热液蚀变年龄，这将为研究热液成矿年龄并进而探讨成矿机理提供又一可能的新途经。     

The conditions of formation of sapphire and zircon in the areas of alkali-basaltoid volcanism in Central Vietnam

Study of the chemical composition of clinopyroxene and garnet megacrysts from the Dak Nong sapphire deposit and model calculations have shown that megacrysts originated from the crystallization of alkali basaltoid magma in a deep-seated intermediate chamber at 14–15 kbar, which is close to the Moho depth (50 km) in this part of southeastern Asia. The chamber was a source of heat and CO₂ fluids for the generation of crustal syenitic melts producing sapphires and zircons. The formation conditions of sapphires and zircons are significantly different. The presence of jadeite inclusions in placer zircons points to high pressures during their crystallization, which is confirmed by the ubiquitous decrepitation of CO₂-rich melt inclusions. Sapphires crystallized from iron-rich syenitic melt in the shallower Earth’s crust horizons with the participation of CO₂ and carbonate–H₂O–CO₂ fluids. The subsequent eruptions of alkali basalts favored the transportation of garnet and pyroxene megacrysts as well as sapphire and zircon xenocrysts to the surface. It is shown that sapphire deposits can be produced only during multistage basaltic volcanism with deep-seated intermediate chambers in the regions with thick continental crust. The widespread megacryst mineral assemblage (clinopyroxene, garnet, sanidine, ilmenite) and the presence of placer zircon megacrysts can be used as indicators for sapphire prospecting.