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81.
Plagioclase replacement textures in partially eclogitised gabbros from the Sanddal mafic-ultramafic complex, Greenland Caledonides 总被引:1,自引:0,他引:1
The Sanddal mafic‐ultramafic complex (SMUK) is a cluster of variably eclogitised mafic and ultramafic bodies that comprise the westernmost known eclogite facies locality in the North‐East Greenland eclogite province (NEGEP). Although there are no true eclogites in the SMUK, we interpret three distinct textural types of plagioclase replacement to record sequential stages in adjustment of SMUK olivine gabbro‐norites to eclogite facies conditions. The earliest stage, in which plagioclase was replaced by omphacite/spinel symplectite before nucleation of garnet (Type 1A & 1B) has not previously been described. Documentation of this texture provides clear evidence that, at least in some cases, garnet nucleation is delayed relative to nucleation of omphacite and is a rate‐limiting step for eclogitisation. Type 1C domains were produced by scattered nucleation of garnet in the same sample. In Type 2 domains, plagioclase was replaced by a layered corona with an outer layer of garnet, an inner layer of omphacite and an interior of inclusion‐rich plagioclase. In Type 3 domains, the omphacite layer was overgrown by the garnet rim, and omphacite is preserved only as inclusions in garnet. In more coarse grained leucogabbros, recrystallization was more complete, plagioclase replacement textures were less localised, and could not be divided into distinct stages. Plagioclase replacement in SMUK samples was not isochemical, and required diffusion of at least Mg and Fe from replacement of mafic phases in the surroundings. Strong compositional gradients in garnet reflect disequilibrium and were controlled by the different diffusion rates of Mg/Fe and Ca, different local chemical environments, and progress of the plagioclase breakdown reaction. The presence of small amounts of hydrous minerals (amphibole, phlogopite and clinozoisite) in local equilibrium in plagioclase domains of most SMUK samples indicates that a small amount of H2O was present during high pressure metamorphism. 相似文献
82.
Metastability of granulites and processes of eclogitisation in the UHP region of western Norway 总被引:1,自引:1,他引:1
The Flatraket Complex, a granulite facies low strain enclave within the Western Gneiss Region, provides an excellent example of metastability of plagioclase‐bearing assemblages under eclogite facies conditions. Coesite eclogites are found <200 m structurally above and <1 km below the Flatraket Complex, and are separated from it by amphibolite facies gneisses related to pervasive late‐orogenic deformation and overprinting. Granulites within the Flatraket Complex equilibrated at 9–11 kbar, 700–800°C. These predate eclogite facies metamorphism and were preserved metastably in dry undeformed zones under eclogite facies conditions. Approximately 5% of the complex was transformed to eclogite in zones of fluid infiltration and deformation, which were focused along lithological contacts in the margin of the complex. Eclogitisation proceeded by domainal re‐equilibration and disequilibrium breakdown of plagioclase by predominantly hydration reactions. Both hydration and anhydrous plagioclase breakdown reactions were kinetically linked to input of fluid. More pervasive hydration of the complex occurred during exhumation, with fluid infiltration linked to dehydration of external gneisses. Eclogite facies shear zones within the complex equilibrated at 20–23 kbar, 650–800°C, consistent with the lack of coesite and with the equilibration conditions of external HP eclogites. If the complex experienced pressures equivalent to those of nearby coesite eclogites (> 28 kbar), unprecedented metastability of plagioclase and quartz is implied. Alternatively, a tectonic break exists between the Flatraket Complex and UHP eclogites, supporting the concept of a tectonic boundary to the UHP zone of the Western Gneiss Region. The distribution of eclogite and amphibolite facies metamorphic overprints demonstrates that the reactivity of the crust during deep burial and exhumation is strongly controlled by fluid availability, and is a function of the protolith. 相似文献
83.
84.
鲁南苏北榴辉岩的特征及其成因 总被引:2,自引:0,他引:2
鲁南苏北榴辉岩按产状分为两类:一类是呈条带状、透镜状或肠状鳌合赋存于胶南混杂岩系中,另一类是呈透镜状赋存于石榴石橄榄岩中,以前者分布最为广泛,后者仅见于日照及东海地区。胶南混杂岩系中的榴辉岩由橄榄拉斑玄武岩深成变质作用形成,石榴石橄榄岩中的榴辉岩为地幔来源,它们共同经历了早期2.8 GPa,800℃的高温高压平衡结晶及后期600—700℃,1.1—1.3 GPa的退变质作用改造。Sm-Nd等时年龄为222±6Ma,~(143)Nd/~(144)Nd初始比值为0.511 36±3,推测本区榴辉岩形成于早三叠世华南陆块与华北陆块的碰撞事件。 相似文献
85.
Zhang Zeming You Zhendong Han Yujing Yang Weiran Wei BizeFaculty of Earth Sciences China University of Geosciences Wuhan 《中国地质大学学报(英文版)》1995,(2)
There are four units of high-pressure to ultrahigh-pressure metamorphism extending from south to north across the Tongbai-Dabie Mountains: the epidote-blueschist-facies unit, the low-temperature eclogite facies unit , the ultrahigh-pressure eclngite facies unit and the medium-temperature eclogite facies unit . The later two units were formed during the Caledonian subduction between the Tongbai-Dabie microplate and the North China plate ,the former two units are the products of Indosinian continental-continental subduction and collision between the Yangtze and the North China plates. 相似文献
86.
齐大山铁矿黑云变粒岩单锆石年龄及意义 总被引:3,自引:1,他引:3
齐大山特大型鞍山式铁矿的成矿时代,以往都是根据铁矿的构造和建造特征,以及与铁矿伴生的花岗岩类岩体的同位素年龄数据间接推断的。本文最近获得了该铁矿的黑云变粒岩中,单颗粒锆石U-Pb同位素年龄为(2533±53)×10 ̄6a。这是迄今为止研究该矿床成矿时代较为可靠的直接测年数据。 相似文献
87.
北秦岭官坡地区高压—超高压榴辉岩岩相学及变质作用研究 总被引:19,自引:2,他引:19
北秦岭官坡地区的榴辉岩及含柯石英榴辉岩产在帮岭岩群的北侧,主要由绿辉石和石榴石组成,部分石榴石和绿辉石中含柯石英包体。此外还含有退变质的多硅白云母、角闪石、黝帘石和纳长石等矿物,根据变质矿物之间的替代关系及共生组合规律,榴辉岩退变质作用可划分为四个阶段,各阶段代表性矿物组合依次为:柯石英+绿辉石+石榴石;石英+绿辉石+石榴石;多硅白云母+绿辉石+石榴石+石英;角闪石+斜长石+白云母+黑云母。这四个 相似文献
88.
胶东威海地区榴辉岩退变质的地球动力学信息 总被引:2,自引:0,他引:2
威海地区榴辉岩退变质过程表现为三个阶段:第一阶段,原生绿辉石分解形成钠质单斜辉石+斜长石合晶体;第二阶段,原生石榴石及钢质单斜辉石+斜长石合晶体,周边出现角闪石+斜长石 状反应边;第三阶段,石榴石及钢质单斜辉石消失。其后榴辉岩相退变质的p-t演化轨迹是压力相对温度快速降低的顺时针形式,反映本区榴辉岩折返的地球动力学过程可能是在经历了快速上升的构造侵位同时,晚元古宙巨量花岗岩浆可将相辉岩块体携带到上部地壳。 相似文献
89.
笔者在"关于板块运动启动时间的争论"一文(陆松年等,2016)基础上,参阅公开发表的部分文章,介绍了前板块岩浆洋和停滞盖研究的新进展,并再次讨论有关板块运动启动时间的不同认识和观点。根据太阳系30个类地行星天体图像资料,硅酸盐质行星体在它的生命期由于冷却和岩石圈增厚似乎经历过多种构造样式,包括岩浆洋、多类型停滞盖以及板块构造。硅酸盐类行星由于增生、分异、撞击和放射性活动,使星体变热,发生熔融反应而形成"岩浆洋"。硅酸盐星球体早期很可能是大面积但寿命很短的岩浆洋,之后的星球可能受两种构造模型控制:停滞盖构造和板块构造。已有资料表明,停滞盖构造是类地行星的主要构造类型,而板块构造在类地行星中是十分罕见的。停滞盖构造是一个单一的、围绕天体的板块,基本由硅酸盐质岩石圈组成。停滞盖构造有三种主要变化形态——热管、滴状及柱状体、拆沉及上涌流。板块构造启动时间从>4.4Ga到0.85Ga至少有11种不同观点:认为板块构造始于冥古宙的有1种、始于始-古太古代的有3种、始于中-新太古代的有4种、始于古元古代有1种、始于新元古代的有2种。本文重点介绍了地球冥古宙-太古宙板块运动启动的地质学证据和特点。 相似文献
90.