Volatile element chemistry during accretion of the earth     

《Chemie der Erde / Geochemistry》2020,80(1):125594

We review some issues relevant to volatile element chemistry during accretion of the Earth with an emphasis on historical development of ideas during the past century and on issues we think are important. These ideas and issues include the following: (1) whether or not the Earth accreted hot and the geochemical evidence for high temperatures during its formation, (2) some chemical consequences of the Earth’s formation before dissipation of solar nebular gas, (3) the building blocks of the Earth, (4) the composition of the Earth and its lithophile volatility trend, (5) chemistry of silicate vapor and steam atmospheres during Earth’s formation, (6) vapor - melt partitioning and possible loss of volatile elements, (7) insights from hot rocky extrasolar planets. We include tabulated chemical kinetic data for high-temperature elementary reactions in silicate vapor and steam atmospheres. We finish with a summary of the known and unknown issues along with suggestions for future work.  相似文献   

热扩散驱动的元素分异和同位素分馏:一种不容忽视的硅酸盐成分分异机制     

常翱飞  丁兴 《岩石学报》2020,36(1):99-112

热扩散在地质过程中是否发挥重要作用一直存有争议。本文回顾了热扩散的研究历史和现状,重点总结了热扩散驱动的元素和同位素行为规律,并探讨了温度、硅酸盐组分、压力和氧逸度等因素对热扩散行为的影响。已有的研究表明,稳定热梯度下的硅酸盐热扩散效应类似于结晶分异或AFC过程,可以造成轻、重同位素分别在高温端和低温端富集,而主、微量元素的扩散方向则取决于两端化学势的高低和熔体中的电价平衡。从基性岩浆到酸性岩浆,熔体聚合度增大,黏度增加,热扩散速率明显降低,成网元素的热扩散效应减弱,变网元素则反之;水、氟、氯和硫化氢等挥发组分能增加熔体的非桥氧比例,降低熔体聚合度,因而能显著增强硅酸盐熔体中元素和同位素的热扩散效应。在此基础上,本文提出了当前硅酸盐体系热扩散研究中存在的五个亟需解决的问题,即:1)对不同硅酸盐体系的热扩散规律的研究还不够全面;2)对微量元素的热扩散行为认识不足;3)硅酸盐体系热扩散作用的影响因素及尺度还不够明确;4)热扩散作用的地质与地球化学关键识别标志有待确立;5)硅酸盐体系热扩散作用的理论模型有待建立。尽管硅酸盐体系热扩散的研究还存在诸多不足,但越来越多的证据表明,热扩散是地质过程中不容忽视的一种成分分异机制。这种机制会造成岩浆房或岩浆通道中的元素分异和同位素分馏,可能对于一些成分分异的岩石和矿床的形成具有重要的意义。  相似文献   

北山造山带中部(甘肃段)花岗岩成因及构造背景   总被引：2，自引：2，他引：0  

白荣龙  刘显凡  周慧玲 《岩石学报》2020,36(6):1731-1754

北山造山带中部花岗岩体以陶勒努图洪岩体和跃进山南岩体为代表,本文对这两个岩体进行了LA-ICP-MS锆石U-Pb定年、全岩地球化学和原位锆石Lu-Hf同位素分析,结果表明:岩体成岩年龄分别为410±2. 8Ma、427±2. 5Ma;主量元素呈现高硅、高钾钙碱性、准铝质-弱过铝质特征;微量元素表现为富集Th、Zr、Hf等及大离子亲石元素(Rb、U、K等),亏损Ba、Sr、Eu及高场强元素(Nb、Ta、P、Ti等);球粒陨石标准化稀土元素曲线呈轻稀土富集、重稀土亏损的右倾模式。综合分析认为跃进山南岩体属A型花岗岩,陶勒努图洪岩体属S型花岗岩。陶勒努图洪和跃进山岩体锆石ε_(Hf)(t)分别为-2. 90～-0. 12(平均值为-1. 53)、-1. 99～2. 82(平均值为0. 26),t_(DM2)分别为1. 41～1. 58Ga、1. 23～1. 54Ga。研究表明:陶勒努图洪黑云母花岗闪长岩岩浆源区主要为由元古界北山杂岩组成的以变质杂砂岩为主的古老地壳物质(含中基性岩石)部分熔融的产物,跃进山南二长花岗岩体可能在元古界北山杂岩组成的以变质杂砂岩为主的古老地壳物质重熔过程中有幔源岩浆的参与。在中志留世(427Ma)明水-小黄山洋已向南侧马鬃山-公婆泉弧之下俯冲至后期,板块后撤引发明水-旱山地体南缘弧后形成裂解环境导致幔源岩浆底侵,诱发地壳物质重熔形成花岗质岩浆,岩浆侵位形成跃进山南二长花岗岩体;至早泥盆世(410Ma),俯冲结束发生弧-陆碰撞造山导致地壳增厚,引发下地壳发生部分熔融产生的花岗质岩浆侵位形成陶勒努图洪岩体;两岩体是在早、晚古生代交接时段同一俯冲-碰撞构造背景下不同部位、不同亚构造环境下的产物。  相似文献   

藏南冈底斯岩基东段朗县杂岩早白垩世岩浆作用:新特提斯洋二次俯冲   总被引：1，自引：1，他引：0  

李广旭  曾令森  高利娥  高家昊  赵令浩 《岩石学报》2021,37(10):2995-3034

新特提斯洋长期俯冲消减作用在早白垩世可能经历二次俯冲启动或板片俯冲几何形态的重大转换。确定西藏南部冈底斯岩基早白垩世岩浆作用的岩石地球化学特征和作用方式是甄别上述过程的关键,对理解新特提斯洋的俯冲演化过程至关重要。本文就冈底斯岩基东段朗县杂岩中保存的各类早白垩世岩浆岩,开展了锆石U-Pb地质年代学和Hf同位素、全岩元素和同位素（Sr-Nd）组成分析。数据结果表明：1）基性岩侵位时代为早白垩世晚期（103.6~100.8Ma）,为高钾钙碱性偏铝质岩石,锆石ε_Hf（t）=+0.3~+5.7,全岩ε_Nd（t）=-0.8和-0.3,暗示其岩浆源区具有大量俯冲沉积物或流体的混入,为沉积物熔体和流体交代的地幔楔物质部分熔融的产物,经历了一定程度的角闪石分离结晶作用;2）中性岩形成于99.8~97.6Ma,略晚于基性岩,其主量元素与基性岩具有较好的线性关系,全岩ε_Nd（t）=+1.1,具有较多的地幔物质参与,为基性岩浆进一步演化形成;3）酸性岩（脉体）记录了多阶段岩浆作用（124.1~95.3Ma）,根据同位素组成不同进一步划分为两类,第一类具有较低的全岩ε_Nd（t）值（-8.3~-6.0）,其岩浆源区显示富集特征,t_DM2=1385~1586Ma,由古老地壳物质的再熔融形成;第二类的锆石ε_Hf（t）值（-2.8~+3.2）变化较大,岩脉的锆石ε_Hf（t）=+0.4~+8.1,t_DM=428~906Ma,全岩ε_Nd（t）=+0.1和+0.8,表明岩浆源区具有不均一性,为古老地壳物质被富流体地幔岩浆改造形成;和4）镁铁质包体的主量元素与寄主花岗岩具有较好的线性关系,锆石的Hf同位素组成变化较大（ε_Hf（t）=-9.3~+4.1）,变化范围可达13个ε单位,为岩浆混合成因。寄主花岗岩和角闪辉长岩分别作为酸性和基性端元,是基性岩浆与其诱发古老地壳熔融形成的花岗质岩浆经混合形成。结合冈底斯岩基早白垩世岩浆岩的研究结果,朗县杂岩在早白垩世（124~97Ma）的岩浆作用具有明显的岩浆混合现象,锆石Hf和全岩Sr-Nd同位素组成变化较大,可达13个ε单位,其岩浆源区复杂且富含流体,代表了新特提斯洋在早期（240~144Ma）经历漫长的俯冲之后,在早白垩世时期（~120Ma）俯冲带发生跃迁或俯冲角度达到临界点,导致大量俯冲沉积物和流体沿俯冲带俯冲下去,与发生部分熔融的地幔楔物质混合,底侵导致上覆古老地壳物质的再熔融,形成早白垩世复杂的岩浆岩组合,很可能是新特提斯洋二次俯冲开始的标志。  相似文献   

东天山云海铜镍矿地球化学特征及成因分析     

李大海  刘超  王成  唐毅 《新疆地质》2021,(1):75-81

云海铜镍矿位于觉罗塔格构造带西段,成矿岩体为多期次侵入的杂岩体,岩体分异演化充分,镁铁质和超镁铁质岩石均有发育,主要岩石类型为角闪辉石岩、橄榄苏长岩、辉长岩、闪长岩。主量元素化学组成表明,该杂岩体属拉斑玄武岩系列,岩石具同源演化特征,显示高铁、高镁、低钛、低铝特征,富集大离子亲石元素Rb,Ba,亏损Nb,Ta,轻稀土富集。岩浆源区有部分熔融而交代的岩石圈地幔,岩浆在上升过程中受到地壳物质混染,发生橄榄石、斜方辉石、斜长石的分离结晶。岩体形成于早二叠世,为构造活动和地幔柱双重作用下的产物。  相似文献   

延吉地区古新世埃达克岩成因的岩浆混合证据   总被引：2，自引：0，他引：2  

郭锋  范蔚茗  李超文 《矿物岩石地球化学通报》2011,30(1):1-10

本文通过年代学、矿物学、主量元素、微量元素和同位素的研究,指出延吉地区古新世富镁埃达克岩起源于被俯冲板片熔体交代的地幔楔。单斜辉石和角闪石斑晶所显示的反环带结构为幔源富镁埃达克熔体于壳源中酸性岩浆混合的结果,而非前人普遍认为的熔体—地幔的反应产物;其地球化学特征表现出的岩浆演化趋势可以很好地用地壳混染/AFC过程来解释。延吉古新世埃达克岩形成于俯冲后岩石圈伸展作用背景,与太平洋板块的俯冲后撤作用有关。因此,我们认为富镁埃达克岩的形成不必强调同期洋脊的俯冲作用,只要早先或同时有俯冲板片熔体交代,在合适的p-t条件下交代地幔并发生熔融作用,就能形成这一类岩石。  相似文献   

http://www.sciencedirect.com/science/article/pii/S1674987111000429   总被引：1，自引：0，他引：1  

Xieyan Song  Yushan Wang  Liemeng Chen 《地学前缘(英文版)》2011,2(3):375-384

The three most crucial factors for the formation of large and super-large magmatic sulfide deposits are: (1) a large volume of mantle-derived mafic-ultramafic magmas that participated in the formation of the deposits; (2) fractional crystallization and crustal contamination, particularly the input of sulfur from crustal rocks, resulting in sulfide immiscibility and segregation; and (3) the timing of sulfide concentration in the intrusion. The super-large magmatic Ni-Cu sulfide deposits around the world have been found in small mafic-ultramafic intrusions, except for the Sudbury deposit. Studies in the past decade indicated that the intrusions hosting large and super-large magmatic sulfide deposits occur in magma conduits, such as those in China, including Jinchuan (Gansu), Yangliuping (Sichuan), Kalatongke (Xinjiang), and Hongqiling (Jilin). Magma conduits as open magma systems provide a perfect environment for extensive concentration of immiscible sulfide melts, which have been found to occur along deep regional faults. The origin of many mantle-derived magmas is closely associated with mantle plumes, intracontinental rifts, or post-collisional extension. Although it has been confirmed that sulfide immiscibility results from crustal contamination, grades of sulfide ores are also related to the nature of the parental magmas, the ratio between silicate magma and immiscible sulfide melt, the reaction between the sulfide melts and newly injected silicate magmas, and fractionation of the sulfide melt. The field relationships of the ore-bearing intrusion and the sulfide ore body are controlled by the geological features of the wall rocks. In this paper, we attempt to demonstrate the general characteristics, formation mechanism,tectonic settings, and indicators of magmatic sulfide deposits occurring in magmatic conduits which would provide guidelines for further exploration.  相似文献   

Lower crustal melting via magma underplating: Elemental and Sr–Nd–Pb isotopic constraints from late Mesozoic intermediate–felsic volcanic rocks in the northeastern North China Block     

CHAOWEN LI  FENG GUO  WEIMING FAN 《Island Arc》2011,20(4):477-499

Ar–Ar dating, major and trace element analyses, and Sr–Nd–Pb isotope results of two groups of Lower Cretaceous (erupted at 126 and 119 Ma, respectively) intermediate–felsic lava from the northeastern North China Block (NCB) suggest their derivation from melting of mixtures between the heterogeneous lower crust and underplated basalts. Both groups exhibit high‐K calc‐alkaline to shoshonitic affinities, characterized by light rare earth element (LREE) and large ion lithophile element (LILE) enrichment and variable high field strength element (HFSE, e.g. Nb, Ta and Ti) depletion, and moderately radiogenic Sr and unradiogenic Nd and Pb isotopic compositions. Compared with Group 2, Group 1 rocks have relatively higher K₂O and Al₂O₃/(CaO + K₂O + Na₂O) in molar ratio, higher HFSE concentrations and lower Nb/Ta ratios, and higher Sr–Nd–Pb isotope ratios. Group 1 rocks were derived from a mixture of an enriched mantle‐derived magma and a lower crust that has developed radiogenic Sr and unradiogenic Nd and Pb isotopic compositions, whereas the Group 2 magmas were melts of another mixture between the same mantle‐derived component and another type of lower crust having even lower Sr, Nd, and Pb isotopic ratios. Shift in source region from Group 1 to Group 2 coincided with a change in melting conditions: hydrous melting of both the underplated basalt and the lower crust produced the earlier high‐Nb and low‐Nb/Ta melts with little or no residual Ti‐rich phases; while the younger low‐Nb and high‐Nb/Ta magmas were melted under a water‐deficient system, in which Ti‐rich phases were retained in the source. Generation of the two groups of intermediate–felsic volcanic rocks was genetically linked with the contemporaneous magma underplating event as a result of lithospheric thinning in the eastern NCB.  相似文献   

早古生代古亚洲洋俯冲作用:来自新疆哈尔里克侵入岩的锆石U-Pb年代学、岩石地球化学和Sr-Nd同位素证据   总被引：7，自引：3，他引：4  

马星华  陈斌  王超  鄢雪龙 《岩石学报》2015,31(1):89-104

新疆哈尔里克造山带的形成时间(早古生代/晚古生代)及其构造属性(岛弧/弧后盆地)一直是有争议的问题。本文选择位于哈尔里克带内的奥尔达乌台克侵入体,对其成因及所揭示的地质意义进行了探讨。奥尔达乌台克岩体由一套成份连续的岩石组合构成,包括辉长岩、辉长闪长岩、闪长岩和花岗闪长岩。对闪长岩及其内部暗色包体进行的LA-ICP-MS锆石U-Pb定年结果显示两者同时形成于~450Ma,为晚奥陶世岩浆活动的产物。岩石学和地球化学证据反映奥尔达乌台克岩体普遍具有富H2O、高fO2的湿岩浆性质,富集LREE、Sr、Ba等大离子亲石元素(LILE)而亏损Nb、Ta、Ti等高场强元素(HFSE),与典型的岛弧岩浆岩类似。高放射成因Nd(εNd(t)=+4.4~+5.9)和低初始Sr(0.7032~0.7044)同位素组成表明偏基性的岩浆很可能起源于年轻的俯冲带岩石圈地幔,生成的镁铁质岩浆一部分与壳源长英质熔体发生混合形成各类岩浆,另一部分则是经历演化后(分离结晶)直接添加到地壳中。因此,壳幔岩浆混合作用和幔源物质的直接加入是古亚洲洋俯冲阶段陆壳增生的两种主要方式。Sr-Nd同位素模拟排除了区内存在古老前寒武纪陆壳的可能,陆壳主体应该是年轻的古生代大洋岛弧和洋壳。哈尔里克早古生代岛弧的确立改变了该带是泥盆纪岛弧或弧后盆地的原有认识,将古亚洲洋俯冲作用的时间追溯至奥陶纪。  相似文献   

中亚萨亚克矿田成矿岩体矿物学和地球化学:岩浆性质与成矿意义   总被引：3，自引：1，他引：2  

安芳  王居里  朱永峰  王建其  魏少妮  赖绍聪  SEITMURATOVA Eleonora 《岩石学报》2015,31(2):555-570

萨亚克大型铜矿田位于哈萨克斯坦北巴尔喀什斑岩成矿带中部,以矽卡岩型矿床为主。通过对矿区石英闪长岩的矿物化学和地球化学研究,发现石英闪长岩呈斑状结构,斑晶为斜长石和角闪石,其中的斜长石斑晶主要为中长石,角闪石斑晶为镁质普通角闪石;岩石属于高钾钙碱性系列,富集Rb、Sr、Ba等大离子亲石元素和轻稀土元素,亏损Nb、Ta和重稀土元素,高Sr/Y、La/Yb比值,与埃达克岩相似。地球化学特征指示萨亚克矿区侵入岩形成于岛弧环境,为矽卡岩-斑岩型成矿提供了有利的构造背景,岩石可能是岛弧玄武质岩浆在高压下经结晶分异而成。根据角闪石温压计及其成分与氧逸度和岩浆中水含量之间的关系,确定萨亚克石英闪长玢岩中角闪石斑晶结晶时岩浆的温度为799~843℃、处于3.6~9.6km深度范围内(P=1.2~3.2kbar)、氧逸度logfO2=-11.5~-12.0(ΔFMQ=2.0~2.8)、平均水含量为1.2%,相对较高的氧逸度和水含量有利于形成富含挥发分和Cu、Au等成矿物质的岩浆,是最终演化形成大型岩浆-热液型铜矿田(斑岩型、矽卡岩型)的有利条件。  相似文献