北大巴山早古生代辉绿岩地球化学特征及其地质意义     

张方毅  赖绍聪  秦江锋  朱韧之  杨航  朱毓 《岩石矿物学杂志》2020,39(1):35-46

对南秦岭北大巴山地区广泛分布的一套基性岩墙群中的辉绿岩进行采样,并进行了锆石U-Pb年代学、全岩地球化学分析。结果显示,岩石形成年龄为435~433 Ma,为早志留世晚期岩浆活动产物。这些辉绿岩具低硅、高碱、高钛的碱性岩特征。岩石微量及稀土元素具板内玄武岩特征,轻稀土元素相对富集,轻重稀土元素分异明显,富集不相容元素Ba、Nb、Ta,而K、Y、Yb相对亏损;K及Rb的负异常表明岩石源区残留角闪石或金云母,部分熔融模拟结果显示岩石起源于尖晶石角闪石岩高程度部分熔融。综合地球化学特征及前人研究结果,认为北大巴山地区在早古生代处于大规模伸展裂陷背景下,岩石圈的拉张诱发了低熔点的交代岩石圈地幔熔融,进而形成了这条碱性岩浆带。  相似文献   

Nishinoshima volcano in the Ogasawara Arc: New continent from the ocean?     

Yoshihiko Tamura  Osamu Ishizuka  Tomoki Sato  Alexander R. L. Nichols 《Island Arc》2019,28(1)

Nishinoshima, a submarine volcano in the Ogasawara Arc, approximately 1 000 km south of Tokyo, Japan, suddenly erupted in November 2013, after 40 years of dormancy. Olivine‐bearing phenocryst‐poor andesites found in older submarine lavas from the flanks of the volcano have been used to develop a model for the genesis of andesitic lavas from Nishinoshima. In this model, primary andesite magmas originate directly from the mantle as a result of shallow and hydrous melting of plagioclase peridotites. Thus, it only operates beneath Nishinoshima and submarine volcanoes in the Ogasawara Arc and other oceanic arcs, where the crust is thin. The primary magma compositions have changed from basalt, produced at considerable depth, to andesite, produced beneath the existing thinner crust at this location in the arc. This reflects the thermal and mechanical evolution of the mantle wedge and the overlying lithosphere. It is suggested that continental crust‐like andesitic magma builds up beneath submarine volcanoes on thin arc lithosphere today, and has built up beneath such volcanoes in the past. Andesites produced by this shallow and hydrous melting of the mantle could accumulate through collisions of plates to generate continental crust.  相似文献   

南秦岭早古生代玄武岩的岩浆源区及演化过程   总被引：1，自引：1，他引：0  

张方毅  赖绍聪  秦江锋  朱韧之  赵少伟  杨航  朱毓  张泽中 《岩石学报》2020,36(7):2149-2162

南秦岭地区早古生代玄武岩中发育的大量单斜辉石斑晶为研究火山岩的深部演化过程及源区属性提供了重要的载体。本文通过对早古生代玄武岩及其中的单斜辉石斑晶进行矿物学、岩石学及地球化学分析,讨论火山岩的演化历程及源区属性。电子探针分析结果表明玄武岩中单斜辉石斑晶属于透辉石,其成分与全岩成分并不平衡,暗示岩石经历了单斜辉石的堆晶作用。通过质量平衡计算得到了与单斜辉石斑晶平衡的熔体并计算了单斜辉石结晶的温压条件,结果显示单斜辉石斑晶结晶压力为7.6～14.0kbar,温度为1201～1268℃。高压下的分离结晶作用导致了单斜辉石成为主要的结晶相。重建后的玄武岩具有高镁、高钙、富钛,富集高场强元素Nb、Ta,亏损Rb、K、Sr和P,Dy/Yb比值高的地球化学特征,指示其源区为含单斜辉石、磷灰石及石榴石的交代岩石圈地幔。同地区发现的玄武质角砾也具高镁及高钙的特征,其富集Ba、Nb、Ta、Ti及低Dy/Yb比值表明源区为含单斜辉石、角闪石及尖晶石的交代岩石圈地幔。  相似文献   

The thermal maturity of sedimentary basins as revealed by magnetic mineralogy     

Mansour M. Abdelmalak  Stéphane Polteau 《Basin Research》2020,32(6):1510-1531

The thermal evolution of sedimentary basins is usually constrained by maturity data, which is interpreted from Rock-Eval pyrolysis and vitrinite reflectance analytical results on field or boreholes samples. However, some thermal evolution models may be inaccurate due to the use of elevated maturities measured in samples collected within an undetected metamorphic contact aureole surrounding a magmatic intrusion. In this context, we investigate the maturity and magnetic mineralogy of 16 claystone samples from Disko-Svartenhuk Basin, part of the SE Baffin Bay volcanic margin. Samples were collected within thermal contact metamorphic aureoles near magma intrusions, as well as equivalent reference samples not affected by intrusions. Rock-Eval pyrolysis (T_max), and vitrinite reflectance (Ro) analysis were performed to assess the thermal maturity, which lies in the oil window when 435°C ≤ T_max ≤ 470°C and 0.6%–0.7% ≤ Ro ≤ 1.3%. In addition, we performed low- (<300K) and high-temperature (>300K) investigations of isothermal remanent magnetization to assess the magnetic mineralogy of the selected samples. The maturity results (0.37% ≤ Ro ≤ 2%, 22°C ≤ T_max ≤ 604°C) show a predominance of immature to early mature Type III organic matter, but do not reliably identify the contact aureole when compared to the reference samples. The magnetic assemblage of the immature samples consists of iron sulphide (greigite), goethite and oxidized or non-stoichiometric magnetite. The magnetic assemblage of the early mature to mature samples consists of stoichiometric magnetite and fine-grained pyrrhotite (<1 μm). These results document the disappearance of the iron sulphide (greigite) and increase in content of magnetite during normal burial. On the other hand, magnetite is interpreted to be the dominant magnetic mineral inside the contact aureole surrounding dyke/sill intrusions where palaeotemperatures indicate mature to over-mature state. Interestingly, the iron sulphide (greigite) is still detected in the contact aureole where palaeotemperatures exceeded 130°C. Therefore, the magnetic mineralogy is a sensitive method that can characterize normal burial history, as well as identify hidden metamorphic contact aureoles where the iron sulphide greigite is present at temperatures beyond its stability field.  相似文献   

东南印度洋中脊澳大利亚-南极洲不整合带地区岩浆供应与构造作用沿洋脊的变化     

刘守金  林间  周志远  张帆 《海洋学报(英文版)》2020,39(1):118-129

We analyzed seafloor morphology and geophysical anomalies of the Southeast Indian Ridge(SEIR) to reveal the remarkable changes in magma supply along this intermediate fast-spreading ridge. We found systematic differences of the Australian-Antarctic Discordance(AAD) from adjacent ridge segments with the residual mantle Bouguer gravity anomaly(RMBA) being more positive, seafloor being deeper, morphology being more chaotic, M factors being smaller at the AAD. These systematic anomalies, as well as the observed Na_(8.0) being greater and Fe_(8.0) being smaller at AAD, suggest relatively starved magma supply and relatively thin crust within the AAD.Comparing to the adjacent ridges segments, the calculated average map-view M factors are relatively small for the AAD, where several Oceanic Core Complexes(OCCs) develop. Close to 30 OCCs were found to be distributed asymmetrically along the SEIR with 60% of OCCs at the northern flank. The OCCs are concentrated mainly in Segments B3 and B4 within the AAD at ～124°–126°E, as well as at the eastern end of Zone C at ～115°E. The relatively small map-view M factors within the AAD indicate stronger tectonism than the adjacent SEIR segments.The interaction between the westward migrating Pacific mantle and the relatively cold mantle beneath the AAD may have caused a reduction in magma supply, leading to the development of abundant OCCs.  相似文献   

斑岩型钼矿床研究进展与问题   总被引：1，自引：0，他引：1  

曹冲  申萍 《地质论评》2018,64(2):477-497

本文在简要介绍全球重要成矿带斑岩型钼矿床品位、储量、时空分布以及构造背景的基础上,着重归纳了斑岩型钼矿床中Mo在岩浆—热液演化过程中的地球化学行为特征以及Mo在成矿流体中的迁移与沉淀机制两个方面的研究进展。取得了以下认识:形成斑岩型钼矿床成矿岩浆氧逸度(f_(O2))变化范围较大,但一般大于铁橄榄石—磁铁矿—石英(FMQ)缓冲体系。斑岩钼矿床形成的主要受岩浆房的大小,大体积的岩浆流体能否高效聚集到浅部岩株或岩脉,岩浆中的挥发分(例如F)含量等因素的控制,但与成矿花岗岩和出溶流体中Mo的含量高低无直接关系。成矿流体的氧逸度与p H降低对辉钼矿沉淀具有关键作用。除此之外,温度与盐度降低对辉钼矿沉淀也有重要作用。流体的多阶段沸腾可能对提高Mo品位具有重要意义。此外,应加强岩浆结晶分异过程、岩浆热液转化过程Mo的地球化学行为研究。  相似文献   

太行山南段安林地区侵入岩LA-ICP-MS锆石U-Pb年龄、 地球化学特征及其构造意义     

余智慧  吴园园  王巧玲  王剑锋  陈昊龙  王明明  祝少辉  陈春景  王昊  袁要伟  李玉芹 《地质论评》2022,68(3):877-890

太行山南段安林地区中生代侵入岩LA-ICP-MS锆石U-Pb测年表明侵入岩形成于129. 1±1. 0~129. 7±1. 1 Ma,属于早白垩世,与太行山其他地区乃至整个华北地区侵入杂岩体具有相近的形成年代,表明在晚中生代太行山地区与华北地区经历了相同的地球动力学背景和构造环境,即南太行山地区处于华北克拉通岩石圈减薄范围之内。安林地区中生代侵入岩轻稀土总量（LREE平均为113. 71×10-6）明显高于重稀土总量（HREE平均为11. 97×10-6）,具有相对明显的富集轻稀土元素的右倾型配分形式、Eu的弱正异常及大离子亲石元素相对富集的特征,且具有Sr、Ba含量高、Sr/Y、（La/Yb）N比值高的特征,表明壳幔岩浆混合是太行山南段安林地区中生代岩浆作用的主要成因机制。  相似文献   

热力学计算模拟对初始月幔结构的约束SCIEI北大核心CSCD     

鞠东阳  庞润连  李瑞  杜蔚 《岩石学报》2022,38(4):1025-1042

月球岩浆洋结晶形成的初始月球内部结构是其后续演化过程的开端,其结晶过程受月球岩浆洋的初始深度和物质组成这两个参数的制约。由于缺少直接来自月球深部的岩石样品,目前关于月球岩浆洋演化过程的探讨主要依赖实验和计算模拟手段。岩浆洋模型中形成的月壳厚度是否与探测结果一致是月球岩浆洋演化模型合理性的重要约束。最新的GRAIL(Gravity Recovery and Interior Laboratory)探测数据推算月壳厚度为34~43km,低于阿波罗时期认为的约70km,这对已有的月球岩浆洋演化模型提出了挑战。本文采用并修正FXMOTR程序包,针对月球岩浆洋在不同的初始深度和物质组成情况下的结晶过程,进行了一系列热力学计算模拟。通过量化月球岩浆洋的初始深度和物质组成对月壳厚度的影响,结合关于月球内部微量元素分配的研究结果,对比了月球岩浆洋结晶后期的残余熔体与原始克里普组分(urKREEP)的成分。本文的模拟结果显示,一个全月幔熔融且初始成分为月球初始上月幔组成(LPUM)的岩浆洋将在其深部结晶2.5%石榴子石,形成的月壳厚度符合GRAIL的约束,并且结晶出了合适的urKREEP成分。在此模型的基础上获取了月球初始的内部成分和密度结构,并对后期月幔翻转(Overturn)的程度进行了探讨。  相似文献   

阿尔金造山带南缘晚奥陶世赞岐质闪长岩的发现及其地质意义     

曾忠诚  洪增林  边小卫  陈宁  张若愚  李琦 《地学前缘》2022,29(4):345-357

本文以阿尔金造山带南缘出露的高镁赞岐质闪长岩为研究对象,通过系统的野外地质工作、显微岩相学、年代学和全岩地球化学分析,探讨其成因类型和源区性质,限定了阿尔金造山带构造演化格架。闪长岩LA-ICP-MS锆石U-Pb测年结果表明其形成年龄为(445±3) Ma,属晚奥陶世。地球化学数据显示:闪长岩Al₂O₃含量为15.11%~16.19%,且具有高MgO(3.93%~5.29%)和K₂O(1.68%~2.67%)含量的特征,属于高镁钙碱性准铝质岩石;闪长岩具有较高的Cr(29.3×10^-6~140×10^-6)、Ni(27.1×10^-6~43.5×10^-6)、Ba(606×10^-6~936×10^-6)、Sr(513×10^-6~734×10^-6)和Y(26.4×10^-6~31.1×10^-6)含量,与典型的高镁赞岐岩类地球化学特征一致;稀土配分图和微量元素蛛网图显示闪长岩样品富集轻稀土元素和大离子亲石元素(如Rb和K),而亏损高场强元素(如Nb、Ti和Zr),表现出与俯冲带环境岩浆岩相似的性质;高Ti/Zr比值(48~60)与Mg^#(46.74~53.06)、高Cr(29.3×10^-6~140×10^-6)与高Ni(27.1×10^-6~43.5×10^-6)含量等暗示闪长岩岩浆源区来自遭受俯冲组分交代过的富集岩石圈地幔。岩石成因分析表明,阿尔金造山带南缘晚奥陶世高镁赞岐质闪长岩是后碰撞构造环境下俯冲板片断离诱发地幔楔发生减压熔融而形成,代表了早古生代最强烈的区域性幔源基性岩浆侵入事件。  相似文献   

江西印支期蔡江岩体中暗色微粒包体的发现及其地质意义     

刘运超  姜耀辉  青龙  杜佛光 《高校地质学报》2022,28(4):473-483

文章报道了江西蔡江花岗质岩体中发现暗色微粒包体,以及这些包体的地质、岩相学、LA-ICP-MS锆石U-Pb年代学和元素地球化学特征。包体多呈椭圆状,显示淬冷边和反向脉,具有典型的岩浆结构并含有针状磷灰石,有的包体含有长石捕虏晶。包体具有相对较低的SiO₂（低至57.05 wt%）和较高的MgO+Fe₂O₃（高达14.21 wt%）含量。LA-ICP-MS锆石U-Pb定年数据表明,包体形成于晚三叠世（224 Ma）,与寄主花岗岩（230~228 Ma）在误差范围内基本一致。上述特征表明,包体是离散的幔源偏基性岩浆团或者是幔源与寄主岩浆混合的产物。原始包体岩浆属于超钾质岩浆,可能是通过岩石圈地幔中交代成因的金云母辉石岩脉发生部分熔融而形成的。暗色微粒包体的发现为幔源岩浆底侵提供了直接证据,从而为蔡江花岗质岩石形成于较高温度提供佐证。该研究对于进一步探讨华南印支期花岗岩形成的热源机制具有意义。  相似文献