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1.
北山地区黑红山一带出露的晚石炭世斑状花岗闪长岩大地构造位置位于北山-天山造山系、额济纳-北山弧盆系,至今未见可靠的同位素年龄报道。在运用阴极发光技术对岩石中的锆石进行内部结构分析的基础上,利用LA-ICP-MS锆石UPb同位素原位定年方法获得206Pb/238U年龄加权平均值为312.1±3.2Ma。岩石化学研究显示,斑状花岗闪长岩属中钾钙碱性、准铝质-弱过铝质系列,具I型花岗岩特征;轻稀土元素富集,轻、重稀土元素分馏明显,稀土元素配分曲线右倾;微量元素不同程度地富集Rb、Th、K、Hf,亏损Ta、Nb、Ti、P等元素,显示其形成于板块碰撞前的火山弧环境。结合区域地质背景分析,红石山-百合山-蓬勃山蛇绿岩带代表的洋盆在晚石炭世尚未消亡。  相似文献   

2.
提要：通过野外考察、岩石地球化学、锆石U-Pb测年和Re-Os同位素测试等手段,对里东坑似斑状花岗闪长岩及钼矿床的成因类型、成岩机制以及与壳幔作用的关系进行了分析讨论。测试结果显示：赋矿似斑状花岗闪长岩的LA-ICP-MS锆石U-Pb年龄为（153.01±0.90） Ma（MSWD=1.14）,辉钼矿Re-Os模式年龄为（144.9±1.9） Ma（MSWD=2.0）,成岩与成矿均发生于燕山早期。主微量元素分析结果显示：岩石富Si和K,贫Mg、Ca、P等元素,具有高Rb、低Yb+Ta的特征,稀土元素具有轻微负Eu异常,轻稀土富集;辉钼矿样品Re含量主要介于24.17～27.92μg.g-1。说明赋矿似斑状花岗闪长岩具有I型花岗岩的特征,并经历了壳幔混合作用,判断里东坑似斑状花岗闪长岩为碰撞花岗岩类,形成于挤压背景,具备良好的成矿条件。  相似文献   

3.
新疆西天山天山乡地区大面积分布片麻状花岗闪长岩,含较高的Na_2O+K_2O,A/CNK为0.74~0.97,为准铝质、钠质,成因类型为I型花岗岩,稀土元素富集、重稀土亏损的右倾型分布模式,δEu在弱片麻状似斑状花岗闪长岩中呈中等负异常,在强片麻状花岗闪长岩中基本无异常;微量元素总体富集大离子亲石元素,亏损高场强元素,Ba,Rb,K,Nb,Ta,Ti元素呈明显的亏损特征,具岛弧火山岩特征;锆石U-Pb年龄为(321.9±1.2)Ma,为早石炭世晚期。综合野外地质观察、区域地质构造,认为天山乡南部片麻状花岗闪长岩形成于南天山洋闭合时期,岛弧基本消亡逐渐向陆陆碰撞的过渡阶段。  相似文献   

4.
采用LA-ICP-MS同位素测定技术,测得内蒙古阿拉善北缘沙拉扎山温都尔毛道黑云母花岗闪长岩锆石U-Pb年龄为301±2Ma,属于晚石炭世侵入岩。地球化学分析结果显示,该黑云母花岗闪长岩SiO2含量为67.23%~72.57%,K2O为1.14%~1.61%,Al2O3为14.92%~17.23%,具有过铝质(A/CNK=1.06~1.1)和钙碱性特征。岩石的稀土元素总量较低(38.86×10-6~74.39×10-6),轻稀土元素相对富集,Eu总体呈弱异常(δEu=0.9~1.3)。在原始地幔标准化图解中,岩石具有大离子亲石元素(Rb、Th、K)富集及高场强元素(Nb、Ta、P、Ti)亏损的特征,显示出I型花岗岩的特点。结合区域地质背景,该黑云母花岗闪长岩可能形成于俯冲背景,是洋壳板片与新生的壳源物质混合形成的产物,表明晚古生代沿着阿拉善地块北缘的俯冲至少始于301Ma。  相似文献   

5.
首次对延边小西南岔富金铜矿床矿田内产出的燕山晚期花岗杂岩进行了系统的锆石SHRIMPU-Pb年龄测定,获得中细粒黑云母二长花岗岩、中细粒黑云母花岗闪长岩和似斑状角闪花岗闪长岩的3组锆石谐和年龄数据,分别为98.4~109.0Ma〔加权平均值为(104.6±2.5)Ma,n=10,MSWD=0.71,置信度0.70〕、98.3~108.3Ma〔加权平均值为(106.7±1.6)Ma,n=12〕和104.4~118.8Ma〔加权平均值为(111.7±2.8)Ma,n=12〕,指示它们的岩浆侵位时限在112~104Ma之间,相对侵位时序为似斑状角闪花岗闪长岩、中细粒黑云母花岗闪长岩到中细粒黑云母二长花岗岩;考虑到它们在成矿元素和地质上与矿化的密切程度以及控(容)矿断裂的张扭性特征,进而确定大规模的金铜矿化应发生在似斑状角闪花岗闪长岩、中细粒黑云母花岗闪长岩、中细粒黑云母二长花岗岩形成之后,闪长玢岩之前,或在104.6~102.1Ma之间,成矿环境应处于早白垩世晚期伊泽奈崎板块向古亚洲大陆边缘俯冲消亡、中国东部大陆边缘燕山造山期末的走滑、伸展构造转换过程。  相似文献   

6.
通过对福建紫金山矿田深部与成矿作用有关的主期似斑状花岗闪长岩3组锆石SHRIMP U-Pb和2组角闪石、钾长石~(40)Ar/~(39)Ar测年,获得锆石~(206)Pb/~(238()U加权平均年龄为101.8±1.5 Ma(n=34,MSWD=1.0),代表紫金山矿田深部与成矿作用有关的主期似斑状花岗闪长岩的成岩年龄;同时获得角闪石~(40)Ar/~(39)Ar冷却年龄为100±11 Ma、102.2 Ma,钾长石的~(40)Ar/~(39)Ar冷却年龄为96.3±1.7 Ma、98.5 Ma。依据矿物封闭温度理论,估算紫金山矿田深部与成矿作用有关的主期似斑状花岗闪长岩由锆石结晶至角闪石40Ar/39Ar体系封闭、再到钾长石~(40)Ar/~(39)Ar体系封闭的岩石冷却速率分别是40.7~67.1℃/Ma、116.9~216.3℃/Ma,显示岩石的冷却速率较大;由古地温梯度推算主期似斑状花岗闪长岩结晶(101.8±1.5 Ma)至钾长石~(40)Ar/~(39)Ar体系封闭(96.3±1.7 Ma)期间岩体隆升剥露了约3 km,暗示地壳在这一时期发生了快速隆升剥蚀作用。紫金山矿田深部似斑状花岗闪长岩锆石206Pb/238U年龄佐证了紫金山矿田深部存在一个大岩基,并约束了紫金山矿田斑岩型矿床的成矿时代,单矿物的~(40)Ar/~(39)Ar年龄为矿区的隆升剥露研究提供新资料。  相似文献   

7.
陈瑞莉  潘家永  伍俊杰  陈芳 《地质通报》2019,38(7):1219-1227
安徽茂林岩体为中国东部中生代皖南构造-岩浆带中的一个浅层侵入岩体,是檀树岭钼矿和湛岭钼矿的成矿母岩。该岩体的主要岩性为花岗闪长岩、花岗斑岩、斑状花岗闪长岩、二长花岗岩等。对茂林花岗闪长岩体进行LA-ICP-MS锆石UPb测年,结果显示锆石Th/U值为0.38~0.66,为典型的岩浆成因锆石。花岗闪长岩~(206)Pb/~(238)U年龄加权平均值为140.8±0.8Ma(n=19,MSWD=2.3),结合锆石自形、岩浆环带发育等特点,该年龄为茂林花岗闪长岩的成岩年龄,显示岩体形成于早白垩世。锆石Hf同位素分析结果显示,茂林花岗闪长岩锆石振荡岩浆环带具负εHf(t)值(-9.7~-6.2),揭示花岗闪长岩主要形成于下地壳的熔融。  相似文献   

8.
江西大湖塘地区发育多期次与钨、铜、钼多金属成矿关系密切的中生代花岗岩。本文对该地区出露的似斑状黑云母二长花岗岩和黑云母花岗斑岩进行矿物化学、岩石地球化学、锆石U-Pb年代学和Lu-Hf同位素研究。其中似斑状黑云母二长花岗岩样品的成岩年龄分别为145.6±1.4 Ma(昆山岩体)、148.4±2.4 Ma(燕子崖岩体中部)和145.7±2.9 Ma(燕子崖岩体边部);黑云母花岗斑岩成岩时代为143.7±2.4 Ma(狮尾洞岩体),四者的继承锆石均来自新元古代花岗岩源区。岩石地球化学特征显示主量元素特征相似,似斑状黑云母二长花岗岩和黑云母花岗斑岩普遍高硅(SiO_2分别为72.37%～73.33%和70.16%～73.8%);富铝,二者铝饱和指数A/CNK分别为1.23～1.47和1.30～3.02,均属过铝质高钾钙碱性系列,而稀土、微量元素特征存在明显差异,其中似斑状黑云母二长花岗岩轻重稀土分馏明显,(La/Yb)_N平均为26.18,Eu负异常明显,稀土元素配分曲线呈明显右倾型,富集大离子亲石元素(LILE)Cs、Rb、Th、U、K、Pb,亏损高场强元素(HFSE)Zr、Nb、Ti、Y,低Ba、Sr;而黑云母花岗斑岩轻重稀土分馏不显著,(La/Yb)_N平均为9.76,Eu负异常明显,稀土元素配分曲线呈"海鸥型",并显示"M"型四分组效应,微量元素富集LILE,亏损HFSE。似斑状黑云母二长花岗岩的锆石ε_(Hf)(t)值为-7.39～-5.19,两阶段模式年龄(T_(DM2))为1.53～1.67 Ga。综合分析表明,大湖塘晚侏罗世似斑状黑云母二长花岗岩应产于古太平洋板块向华南板块俯冲的构造背景之下,由中上地壳的新元古代黑云母花岗闪长岩部分熔融形成;而早白垩世黑云母花岗斑岩形成于古太平洋板块向华南板块俯冲—俯冲后伸展的构造转换背景之下,由于软流圈地幔上涌,诱发上地壳新元古代黑云母二长花岗岩部分熔融,且在结晶分异过程中还受到富Cl流体的交代。  相似文献   

9.
阿克图约克花岗闪长岩富黑云母,具较高SiO_2(61.53%~67.01%),低里特曼指数(1.8~2.25),富钠贫钾,A/CNK小于1,稀土元素总量中等(∑REE=64.64×10~(-6)~76.12×10~(-6)),弱Eu亏损,富集大离子亲石元素(Th,K,Ba,LREE),亏损HREE和高场强元素(Ti,Ta,Nb,P),Nb/Ta小于1等特征。该岩体为钙碱性系列准铝质花岗闪长岩,并具I型花岗岩特征。岩体LA-ICP-MS锆石U-Pb年龄为(329.7±1.9)Ma,早于苏云河含矿岩体,为早石炭世洋壳俯冲背景下的火山弧花岗岩,暗示洋壳闭合时限晚于(329.7±1.9)Ma。  相似文献   

10.
辽宁兴城新立屯地区岩浆杂岩主要由4种不同的岩石单元组成,分别为似斑状黑云母二长花岗岩,中细粒石英闪长岩,花岗细晶岩和花岗伟晶岩,前两者分布广泛且为研究区的主要岩石单元,后两者则呈脉状侵入到前两者中。应用LA-ICP-MS锆石U-Pb定年方法,测得似斑状黑云母二长花岗岩,中细粒石英闪长岩及花岗细晶岩的年龄分别为2 496±18 Ma,2 490±19 Ma,2 479±29 Ma,形成于古元古代早期。结合野外地质特征,侵位顺序由早到晚依次为:似斑状黑云母二长花岗岩,中细粒石英闪长岩,花岗细晶岩,花岗伟晶岩。岩石地球化学特征显示,新立屯地区岩浆杂岩主量元素方面具高硅(SiO2=61.38%~74.99%),富碱(Na2O+K2O=6.86%~9.41%),富Mg#(56~70)特征;A/CNK=0.91~1.18,属准铝质-过铝质岩石;微量元素方面,相对富集轻稀土元素,亏损重稀土元素,具有Eu异常(δEu=0.50~0.96);富集大离子亲石元素,亏损高场强元素;锆石Lu-Hf同位素特征εHf(t)值为-1.12~+6.13;TDM2(Hf)介于2 594~2 937 Ma,显示该套岩浆杂岩可能为地幔物质加入新生地壳再造的产物。  相似文献   

11.
The dissolution of H2O and CO2 in structurally dense, nominally anhydrous and non-carbonate oxide matrices such as MgO and CaO is reviewed. H2O and CO2 are treated as gaseous oxide components which enter into solid solution with the refractory oxide hosts. They form anion complexes associated with cation vacancy sites. Evidence is presented that OH? pairs which derive from the dissolution of H2O are subject to a charge transfer (CT) conversion into peroxy moieties and molecular hydrogen, O 2 2? ... H2. Because the O 2 2? moiety is small (O?-O? distance ≈ 1.5 Å) high pressure probably favors the CT conversion. Mass spectroscopic studies show that molecular H2 may be lost from the solid which retains excess oxygen in the form of O 2 2? , leading to the release of atomic O. The dissociation of O 2 2? moieties into a vacancy-bound O? state and an unbound O? state can be followed by measuring the internal redox reactions involving transition metal impurities, the transient paramagnetism of the O? and their effect on the d.c. conductivity. Evidence is presented that CO2 molecules dissolve dissociatively in the structurally dense oxide matrix, as if they were first to dissociate into CO+O and then to form separate solute moieties CO 2 2? and O 2 2? , both associated with cation vacancy sites. In the CO 2 2? moiety (C-O? distance 1.2–1.3 Å, OCO angle ≈ 130°) the C atom probably sits off center. The transition of the C atom into interstitial sites is accompanied by dissociation of the CO 2 2? moiety into CO? and O?. This transition can be followed by infrared spectroscopy, using OH? as local probes. Further support derives from magnetic susceptibility, thermal expansion, low frequency dielectric loss and low temperature deformation measurements. The recently observed emission of O and Mg atoms besides a variety of molecules such as CO, CO2, CH4, HCN and other hydrocarbons during impact fracture of MgO single crystals is presented and discussed in the light of the other experimental data.  相似文献   

12.
There are few inter-African country urban analyses because of the continent’s enormous size and socioeconomic diversity, language barriers, and wide variations in national and regional urban research capacity. Nevertheless, comparative urban studies are critical in understanding contemporary African urbanization. In this comparative spatial and temporal analysis of Ghana and Kenya’s urbanization, we find that both countries are urbanizing rapidly and are faced with many common urban problems. Moreover, Ghana is more urbanized than Kenya and has a larger indigenous urban imprint and a more widely dispersed urban pattern. Besides their physiographic and population conditions, we trace these countries’ convergent and divergent urban trends to their shared but unique experiences of colonialism, nationalism and globalization.  相似文献   

13.
利用GC-MS（气相色谱—质谱仪）,对采自湖北清江流域和尚洞洞顶的土壤样品与洞内石笋样品进行分析,发现土壤中存在的七个系列单甲基支链烷烃在所有的石笋样品中均可以找到,呈现相似的分布模式,石笋中七个系列支链烷烃有可能来自洞穴滴水携带的土壤中的支链烷烃,但是也不能排除石笋原地生长的微生物的贡献。烷基环己烷的分布在土壤与石笋中呈现了相似的分布模式,但是主峰碳数有所变化,高碳数部分与低碳数部分的相对含量也发生了变化。主要原因可能是微生物选择性降解的结果,也有可能是土壤与石笋中微生物种类分布差异所造成的。本次研究初步显示了相对封闭稳定的洞穴沉积物与上覆土壤层中生物标志化合物的异同。   相似文献   

14.
煤中气孔和镶嵌结构及其在煤变质研究中的意义   总被引：1，自引：0，他引：1  
河南省禹县、新密和荥巩煤田山西组Ⅱ1煤的贫煤和无烟煤中,气孔发育。气孔形态有椭圆状（图版1）、圆状及不规则状（图版2）,有的几个气孔连在一起呈大的朵状气孔(图版3)。此外,在荥巩煤田西部无烟煤中还发育有镀嵌结构(图版4)。   相似文献   

15.
Using improved analytical techniques, which reduce the Re blanks by factors of 8 to 10, we report new Re-Os data on low Re and low PGE pallasites (PAL-anom) and IIIAB irons. The new pallasite samples nearly double the observed range in Re/Os for pallasites and allow the determination of an isochron of slope 0.0775 ± 0.0008 (T = 4.50 ± 0.04 Ga, using the adjusted λ187Re = 1.66 × 10−11 a−1) and initial (187Os/188Os)0 = 0.09599 ± 0.00046. If the data on different groups of pallasites (including the “anomalous” pallasites) are considered to define a whole-rock isochron, their formation would appear to be distinctly younger than for the iron meteorites by ∼60 Ma. Five IIIAB irons (Acuna, Bella Roca, Chupaderos, Grant, and Bear Creek), with Re contents ranging from 0.9 to 2.8 ppb, show limited Re/Os fractionation and plot within errors on the IIAB iron meteorite isochron of slope 0.07848 ± 0.00018 (T = 4.56 ± 0.01 Ga) and initial (187Os/188Os)0 = 0.09563 ± 0.00011. Many of the meteorites were analyzed also for Pd-Ag and show 107Ag enrichments correlated with Pd/Ag, requiring early formation and fractionation of the FeNi metal, in a narrow time interval, after injection of live 107Pd (t1/2 = 6.5 Ma) into the solar nebula. Based on Pd-Ag, the typical range in relative ages of these meteorites is ≤10 Ma. The Pd-Ag results suggest early formation and preservation of the 107Pd-107Ag systematics, both for IIIAB irons and for pallasites, while the younger Re-Os apparent age for pallasites suggests that the Re-Os system in pallasites was subject to re-equilibration. The low Re and low PGE pallasites show significant Re/Os fractionation (higher Re/Os) as the Re and PGE contents decrease. By contrast, the IIIAB irons show a restricted range in Re/Os, even for samples with extremely low Re and PGE contents. There is a good correlation of Re and Ir contents. The correlation of Re and Os contents for IIIAB irons shows a similar complex pattern as observed for IIAB irons (Morgan et al., 1995), and neither can be ascribed to a continuous fractional crystallization process with uniform solid-metal/liquid-metal distribution coefficients.  相似文献   

16.
At 31 sites in Finland the Zn content was determined of the epiphytic lichen Hypogymnia physodes (L.) Nyl. growing on pine and birch, the terricolous lichen Cladina spp. in pine bark, and the inner part of birch bark. The anomalous contents of Zn in H. physodes on pine and Cladina spp. in soil appeared to be strongly related to sulphide ore deposits. Anthropogenic Zn correlated closely with S and Fe in H. physodes on pine and with Fe in Cladina spp. The binding of geogenic Zn was related to iron hydroxides, and was attributed to the different uptake mechanism of S in these lichens. Elevated values of Zn in H. physodes on birch were due to both geogenic and anthropogenic sources. Zinc in pine bark increased with the Zn content in H. physodes and reached a limiting value.  相似文献   

17.
Aqueous extraction contributes to the formation and weathering of planetary materials and renders electrolytes such as phosphate available for biology. In this context, the solubility of phosphate is measured in planetary materials, represented by the Mars meteorites Nakhla, Dar al Gani 476 (DaG 476), Elephant Morraine 79001 (EETA 79001), and terrestrial analogs, and in the Murchison CM2 and Allende CV3 carbonaceous chondrites. The Mars meteorites contain high levels of phosphate that is readily extracted by water, up to 15 mg kg−1 in Nakhla and DaG 476 and 38 mg kg−1 in EETA 79001, while the terrestrial analogs and the carbonaceous chondrites contain 0.5 to 6 mg kg−1. Correspondingly, high phosphate concentrations of 4 to >28 mg L−1 are obtained in extracts of the Mars meteorites at high solid/solution ratios, exceeding the concentrations of 0.4 to 2.0 mg L−1 in the extracts of the terrestrial analogs. A wide range of planetary conditions, including N2 and CO2 atmospheres, solid/solution ratios of 0.01 to 1.0 kg L−1, extraction times of 1 to 21 d, and temperatures of 20 to 121°C affect the amounts of extractable phosphate by factors of only 2 to 5 in most materials. Phosphate-fixing capacity and exchangeable phosphate are assessed by the isotopic exchange kinetics (IEK) method, which quantifies the amount of P isotopically exchangeable within 1 min (E1min) and between 1 min and 3 months (E1min-3m) and the amount of P that cannot be exchanged within 3 months (E>3m). The IEK results show that the DaG 476 Mars meteorite and terrestrial analogs have low P-fixing capacities, while the carbonaceous chondrites have high P-fixing capacities. Aqueous processing under early planetary CO2 atmospheres has large effects on the available phosphate. For example, the fraction of total P that is exchangeable in 3 months increases from 1.6 to 11%, 13 to 51.6%, and 43.9 to 90.4% in the DaG 476 Mars meteorite, Allende, and Murchison, respectively. The results show that solutions with high phosphate concentrations can form in the pores of planetary lava ash and basalts and in carbonaceous asteroids and meteorites. These solutions can help prebiotic synthesis and early microbial nutrition. The Martian and carbonaceous chondrite materials contain sufficient phosphate for space-based agriculture.  相似文献   

18.
Stabilities of amphibole and chlorite in mafic and ultramafic compositions have been considered in the model system CaO+MgO+Al2O3+SiO2+H2O. From topological arguments two petrogenetic grids have been constructed. Although available experimental data in CMASH are compatible with the grid in which amphibole reacts out before chlorite in model ultramafic compositions for the pressure range 6 to 15 kbar, naturally observed mineral assemblages and some experimental data in more complex systems favour the other grid in which chlorite reacts out before amphibole at all pressures. This discrepancy between natural and model systems is due to differential movement of the dehydration equilibria of the two hydrates reflecting the variation of activity of H2O or of components other than CMASH.  相似文献   

19.
The evolution of the border region of part or all of a craton, on the basis of geological data gathered from Mexico, may best be described in terms of geotectonic cycles. These consist, in chronological order, of (1) an orthogeosynclinal phase (eu- and miogeosynclines) with or without initial magmatic activity, (2) an anatexitic phase consisting of batholith emplacement with attendant regional metamorphism in the eugeosyncline and deposition of a clastic or flysch wedge over the miogeosyncline, (3) an orogenic phase consisting principally of the folding and thrusting of the sediments of the miogeosyncline together with the clastic or flysch wedge against the foreland, and (4) a taphrogenic or block-faulting phase accompanied by (a) accumulation of post-orogenic debris or molasse, (b) subsequent magmatic activity consisting largely of igneous extrusions with fewer intrusions, and (c) final magmatic activity consisting of igneous extrusions. A region that has gone through the above phases of a geotectonic cycle may be termed a structural belt. In the post-Precambrian geologic history of Mexico, three geotectonic cycles are recognized: one occurred along the Pacific border of Mexico between Cambrian and middle Jurassic (?) time (Jaliscoan geotectonic cycle), the second occurred along the present Gulf of Mexico border of the country at the same time (Huastecan geotectonic cycle), and the third occurred over the entire country from the United States border to the Guatemalan border between Late Jurassic and Pliocene time (Mexican geotectonic cycle). The early Mesozoic clastic rocks in northwestern Mexico may signify a fourth geotectonic cycle in that region. In the three recognized geotectonic cycles, however, the geologic record shows only two orogenic phases, one of which occurred in late Paleozoic time in an arcuate belt along the eastern side of Mexico (Coahuilan orogeny), and the other in early Tertiary time in a belt traversing central Mexico from the United States border to the Guatemalan border (Hidalgoan orogeny).  相似文献   

20.
As a result of systematic study on heavy minerals in soils at city and town areas and their surroundings,cinnabar was discovered for the first time in areas of Hg anomalies in China, and it was found that the distribution of cinnabar was basically coincident in scope with that of Hg anomalies, showing that Hg anomalies were‘closely related to cinnabar. This finding provides a theoretical basis for a verification of Hg anomalies in soils in city and town areas and their surroundings, as well as evaluation of its ecological effects, and is significant to revealing the occurrence modes and origin of Hg in soils.  相似文献   

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