安徽省凤阳江山金矿床赋矿地层和相关岩浆岩锆石年代学研究及其意义

安徽省北部蚌埠隆起区被认为是山东胶东招远金成矿带以西的延伸部分,但蚌埠隆起区内之前一直未发现成规模的金矿床。江山金矿床是最近新发现的中型金矿床,区内成矿作用的时代、赋矿地层的归属仍缺乏系统的年代学证据。文章对蚌埠隆起区内江山金矿床的赋矿地层和相关岩浆岩开展系统的年代学研究,明确了赋矿地层时代归属,并限定了成矿时代的上限和下限。矿床赋矿围岩浅粒岩的结晶年龄为(2496±19)Ma,变质年龄为(2452±47)Ma;斜长角闪岩的变质年龄为(1824±11)Ma,对比区域地层岩性和时代,确定矿床的赋矿围岩为新太古代五河群西堌堆组,而非过去认为的庄子里组。矿床中穿切矿体的脉岩花岗闪长斑岩的结晶年龄为(121.2±1.4)Ma,代表成矿时代的下限;赋矿岩体巨斑花岗斑岩的结晶年龄为(128.3±1.7)Ma,代表了成矿时代的上限。通过与胶东金成矿带的对比,认为蚌埠隆起区与胶东地区的前寒武纪变质基底演化历史相似,江山金矿床的成矿作用类型属于胶东焦家式金矿,在此基础上,推测蚌埠隆起区西芦山岩体和淮光岩体有较大的成矿潜力。     

哈萨克斯坦楚—萨雷苏盆地砂岩型铀矿床地质—伊犁盆地蒙其古尔铀矿床含矿砂岩成岩蚀变特征及其有机-无机流体成岩成矿效应

伊犁盆地蒙其古尔铀矿床为典型的层间氧化带型铀矿床,虽然前人对该区铀矿的成矿流体进行了较为系统的研究,但对其成矿流体来源依然存在较大的分歧,尤其对该区成矿流体与蚀变特征、铀成矿的内在联系研究较少。本文为了研究蒙其古尔铀矿床成矿流体来源及其与成岩蚀变、铀成矿的内在联系,综合地应用了偏光显微镜、扫描电镜、电子探针等手段,对其含矿目的层砂岩成岩蚀变进行系统的分析,并对蚀变矿物高岭石H—O同位素、碳酸盐胶结物C—O同位素及黄铁矿S同位素进行了研究。研究表明：与砂岩型铀矿有关的成岩蚀变类型主要有黏土化、碳酸盐化、硅化及金属矿化;成矿流体中水δDH2O,V SMOW为-48.3‰～-93‰, δ18OH2O,V SMOW为-10.3‰～-5.1‰,碳酸盐胶结物δ13CV PDB为-10.9‰～-7.2‰,δ18OV SMOW为176‰～249‰,黄铁矿δ34SV CDT为-17.3‰～12‰,上述特征揭示蒙其古尔铀矿床成矿流体是由大气降水性质的地表水（无机）和煤系地层有机质脱羟基及热降解作用产生的有机酸及CH4等还原性气体（煤层气）（有机）两部分组成;成岩蚀变和铀成矿效应皆是有机—无机流体及流体与周围砂岩相互作用的结果。     

车排子凸起与沙湾凹陷过渡带的构造模型

车排子凸起位于准噶尔盆地扎伊尔山前,是夹持在南部四棵树凹陷和东部沙湾凹陷之间的三角构造带。然而对这个三角构造带是原地掩伏构造,山前推覆构造,还是走滑构造控制形成的认识存在争议。目前对于车排子凸起与沙湾凹陷过渡带的构造变形特征以及变形机制的认识尚不清楚。而过渡带是研究该区构造变形与演化的良好区域,精细研究该区域构造几何学与运动学对于揭示其构造变形机制以及认识盆山之间的关系具有积极作用,并对于该区油气勘探具有重要意义。本文以研究区的连片三维地震资料为基础,运用不整合面识别、轴面分析及平衡剖面等方法,对车排子凸起与沙湾凹陷过渡带进行精细的构造解析、建模与构造复原。研究表明,过渡带发育下二叠统（P₁j-P₁f）,中二叠统（P₂x-P₂w）,上二叠统（P₃w）,三叠系（T）,侏罗系（J）,白垩系（K）与古近系-第四系（E-Q）7个构造变形层序。发育佳木河组底部及石炭系内部滑脱层。深部（前二叠系）构造楔发育于整个过渡带,其个数和几何学形态的变化直接影响了上覆背斜形态。构造楔在早二叠世开始楔入,挤压作用持续至三叠纪末期。晚三叠世发育生长地层,显示了P-T构造层褶皱变形的时间,随后三叠纪末期,过渡带受到来自西北缘造山带方向的逆冲推覆构造的叠加作用,表现在后缘发育一系列叠瓦构造,推覆距离约为8 km,南部逆冲断层上盘二叠系-三叠系被剥蚀完全,北部残余少量下二叠统佳木河组。     

四川盆地：周缘活动主控下形成的叠合盆地

四川盆地位于扬子板块西缘和青藏高原东缘,地震勘探资料等揭示盆地前寒武纪基底保存完整的古俯冲带和地堑-地垒结构,说明盆地基底后期构造活动非常稳定;显生宙以来经历晚震旦世-石炭纪、二叠纪-中三叠世两幕克拉通边缘强拉张-强挤压,而克拉通内弱拉张-弱挤压的构造演化过程,体现出盆地内部稳定性结构沉积演化特征。克拉通内弱拉张初期以海相碳酸盐岩大面积稳定沉积（即震旦系灯影组和二叠系栖霞-茅口组）和随后的风化壳岩溶作用（即桐湾期、东吴期等不整合面）为特征,弱拉张期以拉张槽（如：绵阳-长宁拉张槽和开江-梁平拉张槽等）的形成为典型特征;弱挤压则以古隆起（如：加里东期乐山-龙女寺古隆起、印支期泸州古隆起等）的发育为典型特征。四川盆地晚三叠世后的前陆盆地演化阶段受控于其周缘造山带逆冲推覆构造活动,是现今地貌和构造盆地的主要建造期,形成了四川盆地周缘突变（线型）和渐变（弥散型）两种盆山结构。盆地西边界（龙门山）和北边界（米仓山-大巴山）即是线型突变边界,也是扬子地块（板块）的边界,边界几何形状和扬子板块刚性特征对盆山系统结构-构造特征等有较大的控制作用;四川盆地的东边界（齐岳山-大娄山）和西南边界（大凉山）即是渐变弥散型边界,同时也是板（陆）块内部的边界,它们受控于邻区（盆外）的构造变形和盆内沉积盖层中滑脱层的分布特征。受控于盆地（克拉通）周缘活动,四川盆地垂向上前寒武纪基底与盖层、盖层内早期和晚期构造具解耦特征。基底与盖层构造的解耦有利于盆地内部前寒武纪基底结构构造的保存和盖层内大型隆-坳结构的形成演化;盖层内早期和晚期构造的解耦有利于早期构造免遭后期破环,对深层油气藏的保存意义重大。总之,四川盆地可能是具独特形成过程和特征的叠合盆地新类型,其突出特征表现为周缘活动、内部稳定及早期和晚期构造解耦。     

准噶尔盆地腹部地区生烃增压定量化评价——东道海子北凹陷为例

目前准噶尔盆地腹部地区超压演化过程仅提供了相对时间、概念、定性的认识,并未达到定量化。本文以东道海子北凹陷为例,基于流体包裹体、单井一维和剖面二维烃源岩成熟生烃史模拟技术,采用生烃增压模型定量化评价了侏罗纪八道湾组顶部和底部烃源岩的生烃增压演化过程。研究结果表明侏罗纪八道湾组为东道海子北凹陷主力烃源岩,具有幕式排烃的特点。八道湾组底部烃源岩经历了3 次超压增加和两次超压释放的过程,顶部烃源岩经历了两次超压增加和一次超压释放的过程。八道湾底部烃源岩3 次超压增加的时间分别为距今170～70 Ma、55～23 Ma、10～0 Ma,对应最大压力系数均为2.0,最大剩余流体压力50 MPa,两次超压释放的时间分别为70～55 Ma、23～10 Ma;八道湾组顶部烃源岩两次超压增加的时间分别为130～40 Ma、23～0 Ma,对应流体最大压力系数最大亦可达2.0 左右,最大剩余流体压力44 MPa,超压释放的时间为40～23 Ma。     

大数据环境下内蒙古浩布高地区铅锌多金属矿智能矿产预测研究

传统机器学习算法已广泛应用于矿产预测,但面对地质大数据的高维稀疏、不平衡小样本等特性仍缺乏有效处理和分析的方法,设计适合地质大数据特点的机器学习算法是智能矿产预测亟需解决的新问题。本文以内蒙古浩布高地区的铅锌多金属矿产预测为例,提出了一种面向地质大数据的半监督协同训练矿产预测模型。首先对研究区地质找矿信息和地球化学异常信息进行定量分析,提取断裂构造、二叠系地层、燕山期侵入岩、地层与岩体接触带、围岩蚀变及Pb、Zn、Sn、Cu地球化学异常共9种找矿因子。然后利用递归特征消除法优选找矿因子组合,不包括Sn异常在内的8个找矿因子组合被选为最优组合。最后,利用支持向量机和随机森林算法作为基分类器进行半监督协同训练矿产预测,绘制成矿概率分布图。ROC曲线和预测度曲线分析结果表明,半监督协同训练模型的AUC值和预测效率都高于随机森林和支持向量机模型。研究结果也为大数据环境下的智能矿产预测提供了一种新的思路。     

Garnet-Pyroxenite-Derived End-Member Magma Type in Kamchatka: Evidence from Composition of Olivine and Olivine-Hosted Melt Inclusions in Holocene Rocks of Kekuknaisky Volcano

Late Quaternary volcanoes of Sredinny Range (Kamchatka) attract geoscientists’ attention by their unusual geochemical features and geodynamic setting. They produced volcanic rocks that are enriched relative to N-MORB in most of incompatible trace elements (except HREE), including strong enrichment in large-ion lithophile elements, and show a negative Nb–Ta anomaly, which is typical for rocks formed in supra-subduction settings. However, modern subduction of the Pacific Plate does not reach the most part of Sredinny Range, as inferred by mapping of Wadati–Benioff zone or seismic tomography. We constrain the source of parental magmas for Sredinny Range volcanic rocks by combining major and trace element geochemical data for olivine and naturally quenched olivine-hosed melt inclusions for Holocene tephra layers of the Kekuknaisky field. Composition of the most magnesian olivine (Ni > 2000 ppm, Fe/Mn ≈ 75 at Mg# ~ 84–85 mol %) and geochemical characteristics of the most primitive melts (FC3MS = 0.61 ± 0.04 (2s)) are consistent with their derivation from a pyroxenite source, while elevated LREE/HREE ratios in lavas indicate that it contained garnet. This garnet-bearing pyroxenite likely originated from the lower crust or lithospheric mantle. Its melting could have occurred due to delamination and sinking into the hotter mantle.     

Phase Relations in the Harzburgite–Hydrous Carbonate Melt at 5.5–7.5 GPa and 1200–1350°С

Phase relations are studied experimentally in the harzburgite–hydrous carbonate melt system, the bulk composition of which represents primary kimberlite. Experiments were carried out at 5.5 and 7.5 GPa, 1200–1350°С, and \({{X}_{{{\text{C}}{{{\text{O}}}_{2}}}}}\) = 0.39–0.57, and lasted 60 hours. It is established that olivine–orthopyroxene–garnet–magnesite–melt assemblage is stable within the entire range of the studied parameters. With increase of temperature and \({{X}_{{{\text{C}}{{{\text{O}}}_{2}}}}}\) in the system, Ca# in the melt and the olivine fraction in the peridotite matrix significantly decrease. The composition of silicate phases in run products is close to those of high-temperature mantle peridotite. Analysis of obtained data suggest that magnesite at the base of subcontinental lithosphere could be derived by metasomatic alteration of peridotite by asthenospheric hydrous carbonate melts. The process is possible in the temperature range typical of heat flux of 40–45 mW/m², which corresponds to the conditions of formation of the deepest peridotite xenoliths. Crystallization of magnesite during interaction with peridotite matrix can be considered as experimentally substantiated mechanism of CO₂ accumulation in subcratonic lithosphere.     

Biostratigraphy and Sedimentary Settings of the Middle Devonian Succession of the Yuryung-Tumus Peninsula,Khatanga Gulf of the Laptev Sea

The age of the Paleozoic sedimentary successions of the Yuryung-Tumus Peninsula in the Khatanga Gulf is determined as Middle Devonian, late Eifelian, and the beginning of the early Givetian on the basis of the study of brachiopods, ammonoids, nautiloids, bactritoids, gastropods, and conodonts, and in the terminology of the standard conodont succession, these deposits are not older than the late Eifelian Tortodus kockelianus Zone, but include the terminal Eifelian Polygnathus ensensis Zone and the first Givetian Polygnathus hemiansatus Zone and are no younger than the beginning of the early Givetian Polygnathus varcus Zone. The Middle Devonian sedimentary successions of the Yuryung-Tumus Peninsula show the level of the global sedimentary Ka?ak Event. The areas of distribution of the Devonian sedimentary deposits in the Yuryung-Tumus Peninsula in the Khatanga Gulf should be considered as one of the fragments of the regional geological structures of a remote (isolated?) region of the Taymyr Fold System rather than a component of the structures of the northern Siberian Platform.     

Jurassic and Early Cretaceous Radiolarians of Siliceous Sequences of the Vaamychgyn–Podgornaya Interfluve,Econai Zone,Koryak Highland

The assemblages of the Early Jurassic (Hettangian–Pliensbachian) and Late Jurassic–Early Cretaceous (Tithonian–Berriasian) radiolarians were described for the first time in the eastern part of the Ekonai Zone of the Koryak Highland. The Hettangian–Pliensbachian assemblage was found in siliceous rocks of the Ionai Nappe and this finding expands the stratigraphic interval of its siliceous sequences from the Carboniferous to the Early Jurassic. The Tithonian–Berriasian assemblage was found in volcanosiliceous rocks of the Yanranai accretionary complex. Both assemblages contain taxa abundant in the Tethyan regions.