广东北部早白垩世粗面岩的成因:Sr-Nd-Pb同位素制约

广东北部大长沙盆地粗面岩锆石SHRIMP U-Pb年龄为(135.3±1.5) Ma,形成于早白垩世早期,其Sr-Nd-Pb同位素组成为:富放射性成因铅,(206pb/204Pb)i=18.23～18.39,(207pb/204pb )i=15.78～ 15.88,(208Pb/204Pb)i＝38.83～39.14,...     

内蒙古乌斯尼黑蛇绿混杂岩带形成时代的地质新证据

贺根山-乌斯尼黑蛇绿混杂岩带的属性和形成时代存在明显的认识上的分歧.早期认为是二叠纪侵入的超镁铁质岩体.该超镁铁质岩体侵入了下二叠统格根敖包组,并被哲斯组地层不整合覆盖,形成时代为二叠纪.20世纪80年代以来,通过中国北方板块构造研究,在硅质岩中采集到的一系列化石资料表明,贺根山地区蛇绿混杂岩的形成时代应为中-晚泥盆世...     

广东湛江湖光岩地区玄武岩风化壳Fe同位素研究

本文对广东湛江湖光岩地区厚度分别为4 m和7 m的两个不同喷发时代玄武岩形成的风化壳样品进行Fe同位素分析,分析结果显示:厚度4m风化壳样品Fe同位素组成δ57Fe范围为0.17‰～0.57‰;厚度7 m风化壳样品Fe同位素组成δ57Fe范围为0.20‰～0.68‰,相对于标准物质IRMM-014,不同深度风化壳样品均显示Fe的重同位素富集.两风化壳剖面自下而上,随风化程度增大,风化壳样品中Fe同位素分馏程度也呈现逐渐增大的趋势,表明风化壳样品中Fe的重同位素富集趋势与风化壳的发育程度正相关,风化壳土壤中Fe同位素组成是反映土壤风化程度的指标.另一方面,风化过程可将地球外部圈层(岩石圈、水圈、生物圈)有机结合起来,风化壳土壤Fe同位素组成变化是表生植物和水淋滤共同作用的结果,对化学风化过程中Fe同位素研究,将会极大地补充表生过程中同位素地球化学的知识,同时Fe同位素可作为表生过程中物质的循环、环境的变化等过程中有力的示踪/指示技术手段加以应用.     

新疆尼勒克县圆头山后碰撞花岗斑岩的同位素年代学及地球化学特征

圆头山黑云母花岗斑岩位于尼勒克县城南,岩体普遍发育的铜矿化,以中部碎裂带中矿化最强。岩石具有典型的斑状结构,斑晶由碱性长石和黑云母组成,基质以长石、云母和石英为主,并含有少量的硫化物。圆头山黑云母花岗斑岩的轻重稀土分馏明显,并且明显富集大离子亲石元素(LILE) (除Sr外)和Pb,同时亏损高场强元素(HFSE)和Nb、Ta、P、Ti,显示出弧火山岩的地球化学特征。圆头山黑云母花岗形成年龄为269±3Ma,其源区以具有弧火山岩特征的下地壳为主,同时含有少量的幔源物质,而且在岩体的侵位过程中有高(⁸⁷Sr/⁸⁶Sr)_i (0.706054~0.709228)和高Pb含量(5.05×10^-6~32.5×10^-6)的陆壳物质混染。在下地壳物质熔融过程中,位于下地壳底部的富水和成矿元素的MASH带物质也被圈入,使原始岩浆富水和成矿物质。圆头山黑云母花岗斑形成于碰撞后阶段,岩石的形成主要受岩石圈地幔拆沉作用的控制,而岩石圈地幔的拆沉可能与中亚造山带的垮塌或塔里木地幔柱活动有关。     

塔里木盆地东南缘阿克塔什塔格地区新太古代陆壳增生:米兰岩群和TTG片麻岩的地球化学及年代学约束

塔里木盆地东南缘的阿克塔什塔格地区,保存有较为完好的早前寒武纪基底变质岩——阿克塔什塔格杂岩,主要由米兰岩群、新太古代TTG花岗片麻岩和侵入其中的各类古元古代花岗片麻岩构成。其中米兰岩群和TTG片麻岩发育塑性流变褶皱和高角闪岩相-麻粒岩相变质,具有强烈的混合岩化,并遭受后期的角闪岩相变质改造。米兰岩群中的长英质片麻岩和TTG岩系的锆石SHRIMP U-Pb年龄分别为(2 567±32)Ma和(2 592±15)Ma,二者普遍低Si高Al、富Na贫K、富Sr贫Mg、富集LILE和LREE,亏损HSFE和HREE、轻重稀土分馏强烈、Eu异常不明显,具有类似于埃达克岩的岩石地球化学特征,表明它们形成于俯冲带的岛弧环境,为岛弧玄武岩俯冲至下地壳部分熔融的产物,指示了塔里木盆地东南缘新太古代晚期古老克拉通的大陆地壳水平增生。在此基础上,文章还探讨了塔里木盆地周缘早前寒武纪基底岩系的年代格架问题,认为塔里木盆地具有统一的早前寒武纪变质基底。     

火山岩风化壳地层型油气藏评价预测方法研究——以新疆北部石炭系为例

针对火山岩风化壳地层型油气藏强非均质性,评价预测难度大,勘探成功率低等难题,本文采用重磁电剥层处理、沿层延拓信号增强反演方法有效顶测区域火山岩分布;建立风化淋滤剥蚀后不同岩石组合的不完整火山机构和形态识别模式,利用相干体和振幅分析等方法有效识别火山岩目标;在建立单次火山喷发岩石序列及储层分布模式基础上,开发了基于次生溶...     

Trace element geochemistry of coesite-bearing eclogites from the Roberts Victor kimberlite, Kaapvaal craton

Trace element characteristics of seven coesite-bearing eclogitic xenoliths from the Roberts Victor kimberlite demonstrate that this suite of eclogites originated as gabbroic cumulates in oceanic crust that was subsequently subducted. All but one of the garnets show positive Eu anomalies, accompanied by a flat heavy rare earth pattern, which is atypical of garnet, but characteristic of plagioclase, arguing for a considerable amount of plagioclase in the protoliths. Forward modelling of the accumulation of liquidus minerals from primitive komatiitic, picritic, and basaltic liquids suggests that at least some of the eclogite protoliths were not derived from basaltic parental liquids, whereas derivation from either komatiitic or picritic liquids is possible. The reconstructed eclogite bulk rocks compare favourably with oceanic gabbros from ODP hole 735B (SW Indian Ridge), even to the extent that oxygen isotopic systematics show signs of low-temperature seawater alteration. However, the oxygen isotope trends are the reverse of what is expected for cumulates in the lower section of the oceanic crust. These new findings show that δ¹⁸O values in eclogitic xenoliths, despite being sound indicators for their interaction with hydrothermal fluids at low pressure, do not necessarily bear a simple relationship with the inferred oceanic crustal stratigraphy of the protoliths.     

Crustal transect from the North Atlantic Knipovich Ridge to the Svalbard Margin west of Hornsund

The crustal structure along a 312 km transect, stretching from the axial mountains of the North Atlantic Knipovich Ridge to the continental shelf of Svalbard, has been obtained using seismic reflection data and wide angle OBS data. The resulting seismic V_p and V_s models are further constrained by a 2-D-gravity model. The principal objective of this study is to describe and resolve the physical and compositional properties of the crust in order to understand the processes and creation of oceanic crust in this extremely slow-spreading counterpart of the North Atlantic Ridge Systems. V_p is estimated to be 3.50–6.05 km/s for the upper oceanic crust (oceanic layer 2), with a marked increase away from the ridge. The measured V_p of 6.55–6.95 km/s for oceanic layer 3A and 7.10–7.25 km/s for layer 3B, both with a V_p/V_s ratio of 1.81, except for slightly higher values at the ridge axis, does not allow a clear distinction between gabbro and mantle-derived peridotite (10–40% serpentized). The thickness of the oceanic crust varies a lot along the transect from the minimum of 5.6 km to a maximum of 8.1 km. The mean thickness of 6.7 km for the oceanic crust is well above the average thickness for slow-spreading ridges (<10 mm/year half-spreading rate). The areas of increased thickness could be explained by large magma production-rates found in the zones of axial highs at the ridge axis, which also have generated the off-axial highs adjacent the ridge. We suggest that these axial and off-axial highs along the ridge control the lithological composition of the oceanic crust. This approach suggests normal gabbroic oceanic crust to be found in the areas bound by the active magma segments (the axial and off-axial highs) and mantle-derived peridotite outside these zone.