北冰洋西部楚科奇海盆晚第四纪生源沉积物及其古海洋学意义

通过北冰洋西部楚科奇海盆M03孔晚第四纪以来生源沉积物,有孔虫丰度和冰筏碎屑(Ice．Rafted Detritus,IRD)的综合研究表明,海洋氧同位素(Marine Isotope Stage,MIS)7期以来,碳酸钙(CaCO )含量和浮游有孔虫丰度在间冰期的增加和冰期的降低,分别指示大西洋水输入的加强和减弱。而有机碳(TOC)和生源蛋白石(Biogenic Opa1)含量的变化可能主要与输入到海底的TOC降解和Opal溶解作用与底层水中的溶解氧有关。间冰期低的TOC和Opal含量可能反映楚
科奇海盆海冰覆盖减少,营养盐供给多,表层生产力增加,通气作用好,底层水富氧,降解和溶解作用增强,保存在沉积物中的TOC和Opal减少;而冰期相对高的TOC和Opal含量可能反映楚科奇海盆海冰覆盖时间较长,营养盐供给少,表层生产力较低,通气作用差,底层水少氧,降解和溶解作用减弱,保存在沉积物中的TOC和Opal增多。     

SiO2 precipitation in olivine: ATEM investigation of two dunites annealed at 300 MPa in hydrous conditions

Two natural dunites were annealed at pressure P=300 MPa, temperature T=1373, 1473 and 1573 K, and fO₂ within the stability field of olivine. The starting materials contained small amounts of hydroxyls in the form of minor phases of hydrated minerals, which released an aqueous phase during the experiments. A detailed analytical transmission electron microscopy (ATEM) investigation of these materials revealed that small quantities of two types of silica-rich glass formed during heat treatment. The first type of glass, found at triple junctions as rare partially crystallized glass pockets, results from melting dehydration reactions involving the hydrous phases. The second type of glass is found as pure silica precipitates (0.1–0.5 μm in size, for a total of a few 0.1 vol%) within the olivine grains of specimens heated to ≥1473 K. From considerations of the kinetics of the precipitation at 1473 K, we interpret this silica precipitation as resulting from the condensation of olivine metallic vacancies promoted by increasing fluid fugacities during the runs. Our observations, thus, demonstrate that metastable silica can precipitate in olivine from dunites experiencing rapid changes in their thermodynamical environment.     

生物气CO2还原途径中碳同位素分馏作用研究及应用

地质历史中,CO2/H2还原产甲烷作用对生物气的形成具有十分重要的意义。中国柴达木盆地第四系生物气主要为CO2/H2还原型生物气。笔者以CO2/H2还原生气理论为指导,进行不同初始碳同位素值和不同赋存状态碳源的生物模拟实验,研究CO2/H2还原产气过程中发生的碳同位素分馏作用。实验结果表明,产物中δ13CH4值与底物的δ13C值呈很好的正相关关系;在反应母质过量的情况下,碳源的赋存状态可以影响产物甲烷的碳同位素组成。以游离形式CO2还原产生的甲烷δ13C值,相对于以HCO3-、CO23-离子形式产生的甲烷δ13C值轻。通过柴达木盆地东部第四系生物气田实例分析,探讨了该区生物气的主要底物CO2的来源及赋存状态,对评价盆地生物气资源和有利勘探区预测有重要的参考价值。     

新疆三塘湖盆地马朗凹陷中二叠统芦草沟组泥页岩层系SiO2赋存状态与成因

为了弄清新疆三塘湖盆地马朗凹陷芦草沟组泥页岩层系中SiO_2对储集层物性、脆性等特性的影响,通过全岩和黏土矿物X衍射、岩石力学性质、阴极发光、扫描电镜及电子能谱等实验手段对其中SiO_2的赋存状态进行了研究,初步探讨了SiO_2不同形态赋存的机理,并在此基础上探究了石英含量对储层的影响。研究表明:凝灰岩、泥页岩和粉砂质泥岩中二氧化硅多以非晶态形式存在。二氧化硅在凝灰岩中多呈不规则球粒状,而在泥页岩和粉砂质页岩中无固定形态。凝灰质泥岩、凝灰质白云岩和白云岩中二氧化硅呈现一定的晶体形态。在凝灰质泥岩中,二氧化硅以自生石英形态聚集呈条带状,在凝灰质白云岩中则以自生石英形态发育于孤立的孔、洞之中,而白云岩中二氧化硅只能生长成Opal-A/Opal-CT阶段。凝灰质成分及其脱玻化作用为自生石英的生长提供了二氧化硅和生长空间,是控制SiO_2赋存状态的根本因素。此外,储集层孔隙度、渗透率和抗压强度都与石英含量呈一定正相关性,泊松比则与其呈负相关性。     

鄂尔多斯盆地侏罗系低煤阶煤层气系统演化

低煤阶煤层气作为一种非常规天然气资源,具有良好的勘探开发前景。我国低煤阶煤层气资源丰富,进行低煤阶煤层气系统演化分析,对其富集成藏及开发具有重要的理论意义。鄂尔多斯盆地煤层甲烷的碳同位素δ13C₁为–33.1‰~–80.0‰,氢同位素δ_CH4为–235‰~–268‰。该盆地侏罗系煤层气藏主要有次生生物气与热成因气构成的混合型煤层气藏和热成因气藏两种类型。据构造热事件、煤层气组分及成因,结合不同阶段的煤层埋深、变质程度和生气特征等,将鄂尔多斯盆地侏罗系低煤阶煤层气系统演化划分为4个阶段:煤系浅埋–原生生物气阶段﹑煤系深埋–热成因气阶段﹑煤系抬升–吸附气逃逸散失阶段﹑煤系局部沉降–次生生物气补充阶段。其中,煤系深埋–热成因气阶段和局部沉降–次生生物气阶段是低煤阶煤层气资源的主要形成阶段。次生生物气的补充是鄂尔多斯盆地侏罗系低煤阶煤层气成功开发的重要气源。鄂尔多斯盆地侏罗系煤层气藏应属于单斜式富气成藏模式。      

柴达木盆地三湖地区第四系生物气的形成途径与运聚方式

柴达木盆地三湖(台吉乃尔湖、涩聂湖、达布逊湖)地区第四系生物气区是我国最大的生物气区。笔者系统采集了该气区21个天然气样品,测量了其组分和碳同位素组成,重点探讨了生物气形成途径和运聚方式。生物气δ~(13)C_1和δ~(13)C_(CO_2)均随深度增大而变重,显示了CO_2还原途径成气的特征。生物气δ~(13)C_1、δ~(13)C_(CO_2)和δD分布与CO_2还原方式形成的生物气的相应同位素值分布范围接近。在有关成因图解中这些数据主要位于CO_2还原途径成气范围内。生物气CO_2和CH_4之间的碳同位素分馏系数α_c>1.055,具有CO_2还原途径成气的特征。柴达木盆地第四纪干旱的古气候、较低的古温度、较高的沉积速率和水体中较高的硫酸盐含量使得甲烷菌的大量繁殖只能在较大的深度范围内才能实现,从而,有利于CO_2还原途径成气作用进行。涩北一号、涩北二号气田生物气δ~(13)C_1组成分布可能表明,生物气形成以后沿疏导层水平运移进入气藏,基本不存在垂向运移。该项研究对于进一步深入探讨生物气成因、形成条件,确定生物气模拟实验方式与条件,计算生物气资源量,建立成藏模式和选择天然气有利勘探区块均具有重要价值。     

Synthesis and characterization of zeolite X obtained from kaolin for adsorption of Zn（Ⅱ）

This study deals with the synthesis and characterization of low-silica zeolite X, from calcined Kalabsha kaolin, for adsorption of Zn(Ⅱ) ions from aqueous solution. The synthesis processes is performed under hydrothermal treatment in alkaline solutions. The obtained zeolite samples are characterized using X-ray diffraction, grain size distribution, surface area, and SEM. The critical molar ratios of both SiO2/Al2O3 and K2O/Na2O are about 2.9 and 0.16, respectively. Those ratios are needed to give individual low silica zeolite X in a minimum reaction time. The adsorption capacity of the synthesized products is determined by adsorption of Zn(Ⅱ) ions from solution. The results suggest that the zeolite obtained could be converted to a beneficial product, which will be used in future as an ion exchanger in removing heavy metals from wastewaters.     

Silica depleted melting of pelites. Petrogenetic grid and application to the Susqueda Aureole, Spain

Metapelitic rocks in the low pressure contact metamorphic aureole around the Susqueda igneous complex, Spain show a number of features that make them an ideal testing ground for the modelling of silica‐undersaturated melting. Rocks in the aureole experienced localized depletion in silica by the segregation of quartz veins during a pre‐anatectic, regional cordierite‐andalusite grade metamorphic event. These rocks were then intruded by gabbroic to dioritic rocks of the Susqueda igneous complex that formed a migmatitic contact metamorphic aureole in the country rocks. This migmatisation event caused quartz‐saturated hornfels and restite formation in rocks that had experienced no quartz vein segregation in the previous regional metamorphic event, but silica‐undersaturated melting in those rocks that were previously depleted in silica. Silica‐undersaturated melting is investigated using a new petrogenetic P–T projection and equilibrium pseudosections calculated in the KFMASH and NCKFMASH systems, respectively. The grid considers quartz absent equilibria and a range of phases that form typically in silica‐undersaturated bulk compositions, for example corundum. It is shown that the quartz‐rich precursors in the Susqueda contact aureole produced about 10% melt during contact metamorphism. However, most of this melt was extracted leaving behind rocks with restitic bulk compositions and minor leucosome segregation. It is suggested that the melt mixed with the host igneous rocks causing an apparent magmatic zoning from diorite in the centre of the complex to tonalite at the margins. In contrast, the quartz‐poor precursors (from which the quartz veins segregated) melted in the silica‐undersaturated field producing a range of assemblages including peritectic corundum and spinel. Melting of the silica‐undersaturated rocks produced only negligible melt and no subsequent melt loss.     

FTIR Spectrum of Phenocryst Olivine as an Indicator of Silica Saturation in Magmas

Fourier Transform infrared (FTIR) absorption spectra of hydroxylwere measured on olivine phenocrysts from hydrous basaltic meltsthat originated in island-arc tectonic settings. The basalticmelts encompass a wide range of silica activities from orthopyroxene-saturatedhypersthene-normative to nepheline-normative compositions. Theintensities and wavenumber placement of hydroxyl absorptionbands correlate with the degree of silica saturation of theparent melt from which the olivine crystallized. Olivines fromsilica-undersaturated nepheline-normative melts absorb IR radiationin the wavenumber range 3430–3590 cm^–1 (Group 1).In contrast, olivines from orthopyroxene-saturated boniniticmelts exhibit hydroxyl absorption bands in the wavenumber range3285–3380 cm^–1 (Group 2). Olivines crystallizedat intermediate silica activities exhibit a combination of thetwo groups of hydroxyl IR bands, where the proportion of Group2 bands increases with increasing silica saturation of the parentmelt. The positions of hydroxyl absorption peaks observed herefor natural samples are consistent with previous measurementson experimentally annealed olivines. Thus protonation experimentscan be employed to make spectroscopically dry olivine structuresvisible by IR, yielding information on the silica saturationof the parental magmas. Hydroxyl concentrations in the studiedolivines were estimated to be 1–2 ppm, corresponding toan olivine–melt partition coefficient of (1·0 ±0·3) x 10^–4. KEY WORDS: nominally anhydrous minerals; olivine; water; mantle; silica activity; melt inclusions     

黑海西北部冷泉碳酸盐岩的沉积岩石学特征及氧化还原条件的稀土元素地球化学示踪

黑海西北部罗马尼亚大陆架(水深120m)和乌克兰陆坡(水深190m)发育冷泉碳酸盐岩结壳。XRD测试表明此结壳主要由高镁方解石和文石组成。结壳中与渗漏系统微生物活动有关的凝块和葡萄状文石等特殊的沉积组构非常发育。冷泉碳酸盐岩酸可溶部分(碳酸盐岩相矿物)的稀土元素含量很低(0.068×10-6~2.817×10-6),稀土元素页岩标准化配分模式显示罗马尼亚大陆架冷泉碳酸盐岩具有明显的Ce负异常,乌克兰陆坡冷泉碳酸盐岩具Ce的正异常,表明它们是分别在氧化和还原环境中沉积的。稀土元素和V、Cd和U等微量元素的含量在泥晶中最高,亮晶中最低,可能反映成岩过程对元素含量有控制作用。