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151.
We conducted axial compression and general shear experiments, at T = 900 °C and P = 1.5 GPa, on samples of banded iron formation (BIF) and synthetic aggregates of quartz, hematite and magnetite to investigate how dynamic recrystallization of quartz promotes strain localization, and the role of weak second phases (oxides) on the rheology and microstructural evolution of the aggregates. Experiments showed strain localization into oxide rich layers, and that the oxide content and oxide distribution are key factors for the strength of the aggregate. Only 2–10 wt.% hematite leads to pronounced weakening and increasing hematite content above ∼10% has only a minor additional effect. Where oxide grains are dispersed, the initial strength contrast with quartz induces stress concentrations at their tips, promoting high stress recrystallization-accommodated dislocation creep of quartz. Fine recrystallized quartz reacts with oxide, forming trails of fine reaction product (ferrosilite/fayalite) leading to the interconnection/percolation of a weaker matrix. The strength contrast between the quartz framework and these fine-grained trails promotes strain localization into micro-shear zones, inducing drastic strain weakening. Thus dynamic recrystallization of quartz promotes syn-deformational reactions leading to a microstructurally-controlled evolution of phase strength contrast. It results in a rheologic transition from load-bearing framework to a matrix-controlled rheology, with transition from S–C′ to S–C fabric with increasing strain. 相似文献
152.
新疆若羌坡北地区因发现了众多岩浆硫化物型镍矿而受到关注,坡一镍矿为近期发现评价的超大型岩浆硫化物型铜镍矿床.但未发现有规模的高品位富矿体,不能满足矿产开发的条件.文章从坡北镁铁-超镁铁岩带地质特征出发,对坡北地区已经发现的岩浆硫化物矿床含矿特征进行了归纳总结,分析岩体就位成矿有利部位,开展了富矿成矿预测.结合已经总结出的综合地质、物探、遥感、化探等的找矿方法组合,通过地质实践,取得了很好的找矿进展,首次在坡北一带发现了深熔贯入式镍矿床——坡东镍矿. 相似文献
153.
154.
滇东北伴(共)生锗矿地质特征及成因探讨 总被引:3,自引:1,他引:2
长期以来,习惯上将伴(共)生锗矿的成因,归属于主金属矿的成因。代表性的会泽矿其主流派的成因认识是沉积一改造成因,而且是与岩浆岩无关的改造作用。通过对滇东北伴(共)生锗与酸性岩有关的地质特性、另一组与酸性岩有关的伴生元素的存在和深受二次矿化叠加富矿存在的事实的分析与研究,认为会泽矿深部存在尚未被揭露的与晚期主要叠加矿化有关的酸性岩体。提出早期的火山热液与晚期岩浆热液复式成矿的新观点。合理解释了在相关准地台构造单调,地表又无岩浆岩的会泽地区会产出一个超大型富锗-铅锌矿床的根本原因。 相似文献
155.
Benjamin Jacobsen Qing-zhu Yin Frederic Moynier Yuri Amelin Alexander N. Krot Kazuhide Nagashima Ian D. Hutcheon Herbert Palme 《Earth and Planetary Science Letters》2008,272(1-2):353-364
The precise knowledge of the initial 26Al/27Al ratio [(26Al/27Al)0] is crucial if we are to use the very first solid objects formed in our Solar System, calcium–aluminum-rich inclusions (CAIs) as the “time zero” age-anchor and guide future work with other short-lived radio-chronometers in the early Solar System, as well as determining the inventory of heat budgets from radioactivities for early planetary differentiation. New high-precision multi-collector inductively-coupled plasma mass spectrometry (MC-ICP-MS) measurements of 27Al/24Mg ratios and Mg-isotopic compositions of nine whole-rock CAIs (six mineralogically characterized fragments and three micro-drilled inclusions) from the CV carbonaceous chondrite, Allende yield a well-defined 26Al–26Mg fossil isochron with an (26Al/27Al)0 of (5.23 ± 0.13) × 10− 5. Internal mineral isochrons obtained for three of these CAIs (A44A, AJEF, and A43) are consistent with the whole-rock CAI isochron. The mineral isochron of AJEF with (26Al/27Al)0 = (4.96 ± 0.25) × 10− 5, anchored to our precisely determined absolute 207Pb–206Pb age of 4567.60 ± 0.36 Ma for the same mineral separates, reinstate the “canonical” (26Al/27Al)0 of 5 × 10− 5 for the early Solar System. The uncertainty in (26Al/27Al)0 corresponds to a maximum time span of ± 20 Ka (thousand years), suggesting that the Allende CAI formation events were culminated within this time span. Although all Allende CAIs studied experienced multistage formation history, including melting and evaporation in the solar nebula and post-crystallization alteration likely on the asteroidal parent body, the 26Al–26Mg and U–Pb-isotopic systematics of the mineral separates and bulk CAIs behaved largely as closed-system since their formation. Our data do not support the “supra-canonical” 26Al/27Al ratio of individual minerals or their mixtures in CV CAIs, suggesting that the supra-canonical 26Al/27Al ratio in the CV CAIs may have resulted from post-crystallization inter-mineral redistribution of Mg isotopes within an individual inclusion. This redistribution must be volumetrically minor in order to satisfy the mass balance of the precisely defined bulk CAI and bulk mineral data obtained by MC-ICP-MS.The radiogenic 208Pb/206Pb ratio obtained as a by-product from the Pb–Pb age dating is used to estimate time-integrated 232Th/238U ratio (κ value) of CAIs. Limited κ variations among the minerals within a single CAI, contrasted by much larger variations among the bulk CAIs, suggest Th/U fractionation occurred prior to crystallization of igneous CAIs. If interpreted as primordial heterogeneity, the κ value can be used to calculate the mean age of the interstellar dust from which the CAIs condensed. 相似文献
156.
相山铀矿田特富矿成矿模式 总被引:10,自引:0,他引:10
相山铀矿田是我国最大的火山热液型铀矿田之一。大量的电子探针测试揭示该矿田特富铀矿体中普遍存在铀矿物与氟碳磷灰石紧密共生,对特富铀矿石的化学分析也显示铀含量与P2O5和CaO呈大体正相关关系。进一步研究表明磷、铀具有相似的地球化学特性并在热液条件下可以共迁移、共沉淀,据此作者提出:磷、铀胶体共沉淀是该区特富矿形成的主要机理。对采自相山盆地邻区地幔捕虏体研究证实地幔流体与相山矿田铀成矿热液化学成分具有相似性:即富含钾、钠离子和还原性气体。对相山铀矿田He、Ar同位素研究进一步证实该矿田铀成矿热液中有地幔流体参与。配合其他方面的研究,在本区首次提出特富矿铀成矿模式。 相似文献
157.
158.
等离子体发射光谱法同时测定大洋富钴结壳中硅锰铁钙镁铝钛 总被引:3,自引:0,他引:3
大洋富钴结壳试样经HCl+HNO3+HF溶解,在0.2mol/LHF和0.13mol/LH3BO3介质中,用感耦等离子发射光谱法同时测定Si、Mn、Fe、Ca、Mg、Al、Ti元素的含量。方法经国家标准物质GBW07249大洋多金属结核验证,其结果与标准值相符,精密度RSD〈3.2%(n=6);已应用于太平洋富钴结壳中多元素分析。 相似文献
159.
160.