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91.
滇西马厂箐煌斑岩脉分为早晚两期,早期为云斜煌岩,晚期为云煌岩.对煌斑岩样品进行锆石LA-MC-ICP-MS U-Pb定年,获得33.77±0.11Ma的岩浆侵位年龄,表明马厂箐煌斑岩为马厂箐复式杂岩体中期岩浆结晶作用的产物,也是金沙江-哀牢山断裂带新生代早期岩浆活动的产物.岩石地球化学分析表明马厂箐煌斑岩高钾(K2O/NaO=2.88 ~4.60)、富碱(K2O+ Na2O =6.40% ~7.55%)、高Mg# (74.3~76.9),富集大离子亲石元素(LILE) (K、Rb、Ba)和轻稀土元素(LREE),亏损高场强元素(HFSE)(Nb、Zr、P)和重稀土元素.同位素以高(87Sr/86Sr)i(0.707406~0.706506),低εNd(t)(-1.78~-7.64),富集放射性Pb(208 pb/204 Pb=38.87 ~ 39.35,207Pb/204 Pb=15.6390~15.6431,206Pb/204 Pb=18.6579 ~ 18.8093)为特征.176Hf/177Hf为0.282712 ~0.282864,εHf(t)为-1.4~4.0,εNd(t)与εHf(t)存在Nd-Hf同位素解耦.根据岩石地球化学和同位素特征以及区域构造演化历史分析,马厂箐煌斑岩起源于金沙江洋壳俯冲交代作用形成的富集地幔,区域上软流圈物质上涌可能促使EMII的部分熔融形成煌斑岩岩浆,而金沙江-哀牢山断裂及其与其他断裂的交汇处则为岩浆上侵提供了良好的通道.  相似文献   
92.
胶北西留古元古代~2.1Ga变辉长岩岩石学与年代学初步研究   总被引:8,自引:7,他引:1  
刘平华  刘福来  王舫  刘建辉  蔡佳 《岩石学报》2013,29(7):2371-2390
胶北西留古元古代变辉长岩主要由二辉麻粒岩与辉石斜长角闪岩所组成,且以不规则透镜体的形式赋存于新太古代花岗质片麻岩与英云闪长质片麻岩之中.岩相学观察、矿物相转变分析、矿物化学研究、传统地质温压计计算与锆石LA-ICP-MS定年结果表明,胶北西留变辉长岩记录了十分复杂的演化历史,其中早期残留的原岩标志性岩浆结构以辉长辉绿结构为特征,早期残留的单斜辉石为高温低钙的普通辉石(M0),此阶段形成的岩浆锆石记录了其原岩形成时代为2102±3Ma.峰期麻粒岩相变质阶段(M1)的矿物组合以斜方辉石+单斜辉石+斜长石+石英为特征,记录的温压条件为T=800 ~ 850℃,P<0.65~0.75GPa;晚期角闪石的生长表明岩石又经历了降温冷却的过程(M2),其稳定的矿物组合为角闪石+斜长石+石英+单斜辉石,记录的温压条件为T=675~700℃,P=0.40 ~0.55GPa,变质阶段形成的变质锆石记录了其变质时代为1907±16Ma.胶北西留变辉长岩记录了含有近等压降温变质过程的顺时针P-T轨迹.结合本区其它研究资料,本文认为西留古元古代变辉长岩是胶北地区古元古代地层沉积之前一次地壳伸展作用的产物,并于古元古代晚期(1.95~1.80Ga)卷入了胶北碰撞造山作用过程.  相似文献   
93.
A major Mesoproterozoic paleo-plate boundary in the southwestern Amazonian Craton, the Guaporé Suture Zone, is investigated by U–Pb zircon geochronology, Sr–Nd isotope geochemistry and aeromagnetic data. This suture zone is constituted dominantly by ophiolitic mafic–ultramafic rocks of the Trincheira Complex, and minor proportion of tonalites of the Rio Galera and São Felipe complexes, Colorado Complex, amphibolites of the Rio Alegre Terrane and syn- to late-kinematic mafic to felsic plutonic rocks. The ophiolitic Trincheira Complex formed during an accretionary phase from 1470 to 1430 Ma and was overprinted by upper amphibolite–granulite facies metamorphism during the collisional phase of the Ectasian followed by syntectonic emplacement of gabbro and granite plutons (1350–1340 Ma). The ophiolites were intruded by syntectonic tonalitic–plagiogranitic plutons ca. 1435 Ma. Mafic–ultramafic rocks of the Trincheira ophiolites show moderate to highly positive initial epsilon Nd (t = 1.46 Ga) values (+2.6 to +8.8) and very low initial 87Sr/86Sr ratio (0.7013–0.7033). It is suggested that these magmas originated from a depleted mantle source in an island-arc–back-arc setting. The identification of a fossil ophiolite in the Guaporé Suture Zone early as 1470–1435 Ma and later collisional phase, as late as 1350 Ma, marks the impingement of the proto-Amazonian Craton against the Paragua Block, before the formation of the Rodinia supercontinent. The results provide important insights into the geodynamic history of the SW Amazonian Craton, with evidence for both accretionary orogen and subduction of oceanic lithosphere in the Mesoproterozoic, and provide information that allows other workers to evaluate the configuration of supercontinents.  相似文献   
94.
95.
The Fujiawu porphyry Cu–Mo deposit is one of several porphyry Cu–Mo deposits in the Dexing district, Jiangxi Province, Southeast China. New zircon SHRIMP U–Pb data yield a weighted mean 206Pb/238U age of 172.0 ± 2.1 and 168.5 ± 1.4 Ma from weakly altered granodiorite porphyry and quartz diorite porphyry, respectively. Two hydrothermal biotites from granodiorite porphyry give an Ar–Ar step-heating plateau age of 169.9 ± 1.8 and 168.7 ± 1.8 Ma. Hydrothermal apatite exsolved from altered biotite yields an isotope dilution thermal ionization mass spectrometry isochron age of 164.4 ± 0.9 Ma. The apatite age is similar to the ages obtained from hydrothermal rutile (165.0 ± 1.1 and 164.8 ± 1.6 Ma) and indicates that the magmatism and hydrothermal activity in the Fujiawu deposit occurred in the Middle Jurassic. Hydrothermal fluid circulation related to multiple stages of magma emplacement resulted in Cu–Mo mineralization in the Fujiawu porphyry deposit. The zircon SHRIMP U–Pb ages and the published molybdenite Re–Os age (170.9 ± 1.5 Ma) represent the timing of magma crystallization and Mo mineralization, whereas the rutile and apatite U–Pb ages reflect the timing of Cu mineralization following quartz diorite emplacement. The data suggest slow cooling after emplacement of the quartz diorite porphyry.  相似文献   
96.
The Palaeoproterozoic–Mesoproterozoic transition (~1600 Ma) is a significant event in the Earth history as a global thermal perturbation affected the pre-1600 Ma landmasses. Like other cratonic blocks of the world, lithospheric thinning, sedimentation, magmatism, metamorphism and crustal melting/anatexis are associated with this significant geological event in the Singhbhum cratonic province of India. This paper is a review of sedimentological, magmatic and tectono-thermal events in the Singhbhum craton at ~1600 Ma. The Palaeo-Mesoproterozoic sedimentation and volcanism in the Singhbhum craton took place in a terrestrial intracontinental rift setting. The available geochronological data are indicative of late Palaeoproterozoic to Neoproterozoic tectono-thermal events in the Chhotanagpur Granite Gneissic Complex (CGGC), an east–west trending arcuate belt of granite gneisses, migmatites and metasedimentary rocks. A detailed multidisciplinary geo-scientific investigation of the Dalma volcanic belt and the area to its north (Chandil Formation) and further north in CGGC will enable us to constrain the extant surface processes and crust-mantle interactions, the collision events between the North and South Indian cratonic blocks, and the position of India in the Columbia supercontinent.  相似文献   
97.
激光ICP-MS锆石年龄测定结果显示,出露于辽东半岛南部金州地区的太古宙花岗岩形成年龄为2440~2500Ma左右,比辽宁北部—吉林南部大致同时的太古宙花岗岩形成略晚,或基本相当。结合其它地质证据,上述两者在太古宙可能是相互独立的两个块体(分别称辽南地块和辽北—吉南地块),它们在古元古代晚期因造山作用而拼合在一起。古元古代花岗岩形成于两个时期,早期形成的条痕状花岗岩侵位年龄为2160Ma,为辽河群沉积的基底岩石;晚期形成的斑状二长花岗岩和角闪辉石正长岩形成于距今约1850Ma,标志着辽吉古元古代造山作用的结束。据此,可确定辽河群沉积—变质的时限为距今2160~1850Ma,其演化时间不超过300Ma。  相似文献   
98.
Detrital zircon U/Pb geochronology is a common tool used to resolve stratigraphic questions,inform basin evolution and constrain regional geological histories.In favourable circumstances,detrital zircon populations can contain a concomitant volcanic contribution that provides constraints on the age of deposition.However,for non-volcanic settings,proving isolated detrital zircon grains are from contemporaneous and potentially remote volcanism is challenging.Here we use same grain(U-Th)/He thermochronology coupled with U/Pb geochronology to identify detrital zircon grains of contemporary volcanic origin.(U-Th)/He ages from Cretaceous zircon grains in southern Australia define a single population with a weighted mean age of 104±6.1 Ma.indistinguishable from zircon U/Pb geochronology and palynology(~104.0-107.5 Ma).Detrital zircon trace-element geochemistry is consistent with a continental signature for parent rocks and coupled with detrital grain ages,supports derivation from a2000 km distant early-to mid-Cretaceous Whitsunday Volcanic Province in eastern Australia.Thus,integration of biostratigraphy,single-grain zircon double-dating(geochronology and thermochronology)and grain geochemistry enhances fingerprinting of zircon source region and transport history.A distal volcanic source and rapid continental-scale transport to southern Australia is supported here.  相似文献   
99.
The calculation of a maximum depositional age(MDA)from a detrital zircon sample can provide insight into a variety of geological problems.However,the impact of sample size and calculation method on the accuracy of a resulting MDA has not been evaluated.We use large populations of synthetic zircon dates(N≈25,000)to analyze the impact of varying sample size(n),measurement uncertainty,and the abundance of neardepositional-age zircons on the accuracy and uncertainty of 9 commonly used MDA calculation methods.Furthermore,a new method,the youngest statistical population is tested.For each method,500 samples of n synthetic dates were drawn from the parent population and MDAs were calculated.The mean and standard deviation of each method ove r the 500 trials at each n-value(50-1000,in increments of 50)were compa red to the known depositional age of the synthetic population and used to compare the methods quantitatively in two simulation scenarios.The first simulation scenario varied the proportion of near-depositional-age grains in the synthetic population.The second scenario varied the uncertainty of the dates used to calculate the MDAs.Increasing sample size initially decreased the mean residual error and standard deviation calculated by each method.At higher n-values(>~300 grains),calculated MDAs changed more slowly and the mean resid ual error increased or decreased depending on the method used.Increasing the p roportion of near-depositional-age grains and lowering measurement uncertainty decreased the number of measurements required for the calculated MDAs to stabilize and decreased the standard deviation in calculated MDAs of the 500 samples.Results of the two simulation scenarios show that the most successful way to increase the accuracy of a calculated M DA is by acquiring a large number of low-uncertainty measurements(300300)approach is used if the calculation of accurate MDAs are key to research goals.Other acquisition method s,such as high-to moderate-precision measurement methods(e.g.,1%-5%,2σ)acquiring low-to moderate-n datasets(50300).Additionally,they are most susceptible to producing erroneous MDAs due to contamination in the field or laboratory,or through disturbances of the youngest zircon’s U-Pb systematics(e.g.,lead loss).More conservative methods that still produce accurate MDAs and are less susceptible to contamination or lead loss include:youngest grain cluster at 1σunce rtainty(YGC 1σ),youngest grain clusterat 2σuncertainty(YGC 2σ),and youngest statistical population(YSP).The ages calculated by these methods may be more useful and appealing when fitting calculated MDAs in to pre-existing chronostratigraphic frameworks,as they are less likely to be younger than the true depositional age.From the results of our numerical models we illustrate what geologic processes(i.e.,tectonic or sedimentary)can be resolved using MDAs derived from strata of different ages.  相似文献   
100.
Granulitic lunar meteorites offer rare insights into the timing and nature of igneous,metamorphic and impact processes in the lunar crust.Accurately dating the different events recorded by these materials is very challenging,however,due to low trace element abundances(e.g.Sm,Nd,Lu,Hf),rare micrometerscale U-Th-bearing accessory minerals,and disturbed Ar-Ar systematics following a multi-stage history of shock and thermal metamorphism.Here we report on micro-baddeleyite grains in granulitic mafic breccia NWA 3163 for the first time and show that targeted microstructural analysis(electron backscatter diffraction)and nanoscale geochronology(atom probe tomography)can overcome these barriers to lunar chronology.A twinned(~90°/401)baddeleyite domain yields a ~(232)Th/~(208)Pb age of 4328 ± 309 Ma,which overlaps with a robust secondary ion mass spectrometry(SIMS)~(207)Pb/~(206)Pb age of 4308 ± 18.6 Ma and is interpreted here as the crystallization age for the igneous protolith of NWA 3163.A second microstructural domain,2μm in width,contains patchy overprinting baddeleyite and yields a Th-Pb age of 2175 ±143 Ma,interpreted as dating the last substantial impact event to affect the sample.This finding demonstrates the potential of combining microstructural characterization with nanoscale geochronology when resolving complex P-T-t histories in planetary materials,here yielding the oldest measured crystallization age for components of lunar granulite NWA 3163 and placing further constraints on the formation and evolution of lunar crust.  相似文献   
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