腾冲地块西缘那邦基性麻粒岩中石榴石Sm—Nd等时每年龄及其意义

石榴石Ｓｍ－Ｎｄ等时线法是近年来常用于较新年龄的测年方法。腾冲地块西缘新近发现的基性麻粒岩中石榴石和全岩的Ｓｍ－Ｎｄ等时线年龄为１７￣２５Ｍａ,是该麻粒岩经受后期变形变质作用的年龄,与区内右旋走滑断裂活动时限相一致,为确证腾冲地区的右旋走滑断裂是印支地块逸出的西部边界提供了Ｓｍ－Ｎｄ等时线方法的年龄约束。并推断石榴石Ｓｍ－Ｎｄ体系的封闭温度较低,应低于那邦变质基性岩晚期变质作用的６４０℃￣７２０℃     

滇西南那邦变质基性岩两期变质作用的40Ar/39Ar年代学研究

中缅边界那邦变质基性岩出露于东缅著名的 Mogok带的东缘。那邦基性麻粒岩经历了早期麻粒岩相、晚期角闪岩相的两期变质作用的改造。早期变质作用的矿物石榴石和单斜辉石的 40 Ar/ 39Ar激光微区等时线年龄是 74.44± 1.44 Ma;石榴石和单斜辉石的 40 Ar/ 39Ar年龄谱图和等时线年龄均显示两组年龄 :74～ 76 Ma和 2 3～ 2 4Ma。晚期变质作用矿物角闪石的K- Ar法得出 2 3Ma,角闪石和斜长石的 40 Ar/ 39Ar年龄谱图和等时线年龄均显示 2 3～ 2 4Ma的变质年龄。综合这些结果 ,可以确定那邦基性麻粒岩的早期麻粒岩相变质作用的年龄是 74～ 77Ma,可能与新特提斯洋壳俯冲事件有关 ;晚期角闪岩相变质作用的年龄是 2 3～ 2 4Ma,与区内喜山期以来陆内块体响应两大陆会聚作用发生的大型走滑事件有关。那邦基性麻粒岩是世界上最年轻的麻粒岩相岩石之一 ,而且 ,两期变质作用年龄的确定对揭示区内与变质作用相关的地质事件具有重要意义。     

柴达木盆地北缘麻粒岩的发现及地质特征

在柴达木盆地北缘东段,首次从古元代达肯大坂岩群中发现太古宙麻粒岩,并取得３４５０Ｍａ Ｓｍ－Ｎｄ等时线同位素年龄。该麻粒岩以包体地元古代变质出于元古代变质侵入体中,原岩为拉斑玄武质岩石,其形成于大洋岛弧构造环境,经高温高压麻粒岩相变质作用形成。     

滇西南新生代走滑断裂运动学、年代学、及对青藏高原东南部块体运动的意义

依据走滑断裂的运动学和年代学,确认滇西腾冲地区新生代大型走滑断裂带变形作用的三个阶段:1)始新世初(54-56Ma),在槟榔江两岸出露的与新特提斯俯冲和两大陆碰撞相关的左旋走滑-逆冲断裂,由此推断腾冲地块西缘南北向展布格局是两大陆碰撞后发生顺时针旋转达90°的结果.2)渐新世-中新世,腾冲地块东缘的高黎贡右旋走滑断裂和西缘的那邦右旋走滑断裂存在两个走滑活动的峰期:24-19Ma和11-14Ma,早期与Tapponnier模式中挤出块体东边界红河-哀牢山左旋走滑断裂活动的时限相一致,指示高黎贡和那邦右旋走滑断裂在此时期是挤出的印支地块的西边界;晚期与安达曼海的扩张、缅甸境内实皆断裂的右旋活动相一致,可能是此期地块再次发生挤出的结果.3)中新世末,约5-8Ma间两大陆的进一步会聚,引起了腾冲地区岩石圈结构的重要变化,腾冲地块发生了向南的挤出和顺时针的旋转,促成了一系列与此前右旋走滑相关的盆地的折返和南北向凹陷盆地的形成,制约了腾冲火山岩的喷发和整个地区的快速抬升.腾冲地块及其周缘新生代断裂带多阶段运动的转换对揭示青藏高原东南部块体运动型式具有重要的研究意义.     

桑干地区高压麻粒岩中石榴石和斜长石的连续激光探针^40Ar—^39Ar等时年龄

采用微区激光探针＾４０Ａｒ－＾３９Ａｒ定年方法,对华北桑干地区高压基性麻粒岩中变质石榴石和斜长石直接进行了原位微区年代测定,石榴石变斑晶是高压麻粒岩相变质作用形成的矿物,石榴石周围后合成晶反应边组合中的斜长石是石榴石减压分解的产物。石榴石斑晶的４０Ａｒ－３９Ａｒ等时线年龄为２５１０Ｍａ证明高压变质作用发生在太古宙末,斜长石＾４０Ａｒ－＾３９Ａｒ等时线年龄为１９６８Ｍａ,代表石榴石中压麻粒岩相条件下     

浙西南八都群变火山岩系及变晶糜棱岩的同位素年龄及其构造意义

浙西南八都群变火山岩系的Ｓｍ－Ｎｄ全岩等时线参考年龄为２０１４±４３Ｍａ。其中变质玄武岩具有扁平的ＲＥＥ模型。这说明在早元古，华夏古陆张裂并发生一次陆壳增生事件。对该区与具有逆掩断层性质的Ｍ１大型韧性剪切带有关的含石榴石变晶糜棱岩给出１５１８±１６Ｍａ和１００１±１４Ｍａ的Ｓｍ－Ｎｄ和Ｒｂ－Ｓｒ石榴石十全岩等时线年龄。前者指示原含石榴石变质岩的变质时代；后者指示的是糜棱岩化时代。它们可能分别与中元古时华夏古陆的再次张裂，及晚元古时龙泉群沉积盆地闭合有关。     

桑干地区高压麻粒岩中石榴石和斜长石的连续激光探针~(40)Ar~-~(39)Ar等时年龄及其地质意义

采用微区激光探针４０Ａｒ－３９Ａｒ定年方法, 对华北桑干地区高压基性麻粒岩中变质石榴石和斜长石直接进行了原位微区年代测定。石榴石变斑晶是高压麻粒岩相变质作用形成的矿物,石榴石周围后成合晶反应边组合中的斜长石是石榴石减压分解的产物。石榴石斑晶的４０Ａｒ－３９Ａｒ等时线年龄为２５１０ Ｍａ, 证明高压变质作用发生在太古宙末。斜长石４０Ａｒ－３９Ａｒ等时线年龄为１９６８Ｍａ, 代表石榴石在中压麻粒岩相条件下分解的时代。它们之间年龄相差大于５００Ｍａ, 说明高压麻粒岩可能没有经历近等温减压的ＰＴ轨迹。后成合晶组合很可能代表中压麻粒岩相变质作用的叠加。这一结果对探讨华北克拉通桑干地区早期地壳的构造演化具有重要意义。     

浙西南八都群变火山岩及变晶糜棱岩的同位素年龄及其构造意义

浙西南八都群变火山岩系的Ｓｍ－Ｎｄ全岩等时线参考年龄为２０１４±４３Ｍａ。其中变质玄武岩具有扁平的ＲＥＥ模型。这说明在早元古，华夏古陆张裂并发生一次陆壳增生事件。对该区与具有逆掩断层性质的Ｍ１大型韧性剪切带有关的含石榴石变晶糜棱岩给出１５１８±１６Ｍａ和１００１±１４Ｍａ的Ｓｍ－Ｎｄ和Ｒｂ－Ｓｒ石榴石十全岩等时线年龄。前者指示原含石榴石变质岩的变质时代；后者指示的是糜棱岩化时代。它们可能分别与中元古时华夏古陆的再次张裂，及晚元古时龙泉群沉积盆地闭合有关。     

敦煌地块变质岩系时代新认识

敦煌地块的中深变质系敦煌群，哟１／５万区调获得Ｓｍ－Ｎｄ等时线年龄值２９３５Ｍａ，３４８７Ｍａ，归属于太古界。北山南带的中深－浅变质岩系，经１／５万区调及１／２０万区调修测，中深变质岩系中获得Ｓｍ－Ｎｄ等时线年龄值２９４９Ｍａ，２９５６Ｍａ，３２３７Ｍａ及２０５９Ｍａ，分别划归敦粕群和厘定为早元古代。在浅变质岩系中获得Ｓｍ－Ｎｄ等时线年龄值１６２２Ｍａ，１６２４Ｍａ及Ｂａｉｃａｌｉａ等叠层石，归属     

敦煌地块变质岩系时代新认识

敦煌地块的中深变质岩系敦煌群,经１／５万区调获得Ｓｍ－Ｎｄ等时线年龄值２９３５Ｍａ、２９４６Ｍａ、３４８７Ｍａ,归属于太古界。北山南带的中深一浅变质岩系,经１／５万区调及１／２０万区调修测,在中深变质岩系中获得Ｓｍ－Ｎｄ等时线年龄值２９４９Ｍａ、２９５６Ｍａ、３２３７Ｍａ及２２０３Ｍａ、２０５９Ｍａ,分别划归敦煌群和厘定为早元古代。在浅变质岩系中获得Ｓｍ－Ｎｄ等时线年龄值１６２２Ｍａ、１６２４Ｍａ及Ｂａｉｃａｌｉａ等叠层石,归属于中上元古界。     

Thermobarometry, Sm/Nd Ages and Geophysical Evidence for the Location of the Suture Zone Between Cuyania and the Western Proto-Andean Margin of Gondwana

Basement rocks comprising ortho- and paragneisses and schists whose tectono-metamorphic evolution is poorly known, are exposed in the Sierras de Umango, Maz-Espinal and Las Ramaditas, in the northwest of the La Rioja Province, Argentina. These units were included in the Maz, El Taco, El Zaino complexes, as well as the Tambillos Metamorphics that would be part of the northern end of the Cuyania terrane, a microcontinent derived from Laurentia that collided with Western Gondwana during the early Paleozoic, or belong to the active margin of the continent. To recognize rocks belonging to each of these tectonic units and to understand the history and physical conditions of accretion were some of the main goals of the multidisciplinary investigation whose preliminary results are presented here. Geochemical studies, trace and REE elements and Sm-Nd model ages allowed the recognition of several episodes of crustal accretion in these rocks. The oldest one occurred at ca. 2.2 Ga in an arc/back-arc environment along the eastern segment of the Sierra de Maz, and was possibly coeval with development of a early Proterozoic continental crust that acted as source to sediments of Maz Complex. The following episode of crustal accretion that formed rocks in this region was at ca. 1.4 Ga and is registered by tonalites emplaced in an extensional environment cropping out in the western flank of the Sierra del Espinal.

In the Sierra de Umango, an arc/back-arc sequence registered an episode of crustal accretion during the Grenvillian Cycle (ca. 1.3 Ga). The last episode of crustal accretion detected in this area (800 Ma) is represented by an old alkaline volcanism in the Sierra de Umango. This episode could be representing the first stage of break-up of the Rodinia supercontinent during the Neoproterozoic.

The metamorphic grade reached by these rocks is mostly represented by fabrics with mineral assemblages of intermediate to high pressures and high temperatures, typical of collisional environments. The oldest rock-forming fabrics tectono-metamorphic episode recognized is of middle Proterozoic age (ca. 1.04 to 0.969 Ga, garnet-whole-rock Sm/Nd age) being registered by metapelites from Maz Complex that attained temperatures of 650°C-6.3 kbar. A younger metamorphic event (463 Ma, garnet - whole-rock Sm/Nd age) is verified in metatonalites intrusive in these metapelites. Another metamorphic event at ca. 301 Ma (garnet-WR Sm/Nd age) was recognized in metasediments from El Taco Complex. Peak metamorphic conditions of this event, probably registering the last major tectonic episode that affected rocks of this area was established in 868°C-9.8 kbar. It is impossible to distinguish fabrics belonging to totally different tectonic episodes based on structural or metamorphic data. Therefore, distinction between major tectono-thermal events of totally different ages such as the high-T middle Proterozoic deformation and with N-NWestwards tectonic transport direction registered in the Sierras de Maz-Espinal and Umango from the youngest one (ca. 301 Ma) that attained the highest-P/T conditions, recognized in the Sierra de Las Ramaditas, had to be done on the basis of Sm/Nd ages.

Geophysical evidence indicates the presence of extensive WNW-oriented lineaments that separate basements blocks of different magnetic and gravimetric signatures that are thought to represent ancient Grenvillian age suture zones. On the other hand, the northern segment of the Valle Fértil lineament that runs between Sierras de Umango and Maz-Espinal is at present interpreted as marking the eastern boundary of the Cuyania terrane. This is supported by isotopic data as well as the contrasting history of tectono-metamorphic events as determined for both of these segments of the NW Sierras Pampeanas.     

河北矾山钾质碱性超镁铁岩—正长岩杂岩体Sm—Nd年龄和Sr、Nd同位素特征

河北矾山侵入杂岩,由层状钾质超镁铁岩--正长岩组成,已知它含有大型磁铁矿磷灰石矿床.现在已测定了岩体的岩石和矿物的Sm-Nd同位素资料,并获得了杂岩体的Sm-Nd同位素年龄.4个矿物样品和2个全岩样品Sm-Nd等时线年龄为243.4±9.7Ma,INd=0.512045,εNd(t)=-5.4;4个矿物样品和7个全岩样品等时线年龄为239±19Ma,INd=0.512055,εNd(t)=-5.3.这些年龄资料表明,矾山岩体可能侵位于早三叠.而矾山岩体的Rb-Sr等时线年龄为218±8Ma,Isr=0.70554,εsr=18.4的事实可能暗示矾山岩体在中三叠才完全固结并达到Rb-Sr体系封闭的温度.上述矾山岩体的Sr、Nd同位素特征表明,矾山岩体的物质源自富集的上地幔.     

白云鄂博矿区H_9变质岩的Sm-Nd年龄、成因及与成矿关系

本文报道了白云鄂博矿区Ｈ９变质岩富钾板岩，暗色板岩和变质基性火山岩的Ｓｍ－Ｎｄ年龄数据，讨论了上述变质岩的成因及与稀土矿床成矿关系。     

冀东青龙地区浅变质岩系的钐-钕同位素年龄及其地质意义

冀东青龙地区出露的浅变质岩系主要由角闪黑云变粒岩、变质基性—酸性火山岩、浅粒岩、二云石英片岩等组成,夹变质砾岩和铁英岩。姚家沟附近变质砾岩上下的斜长角闪岩的ＳｍＮｄ等时年龄为（２６９６±１８５）Ｍａ,７个样品的ｔＤＭ为２８９０～２９５５Ｍａ。西汉沟具变余枕状构造的斜长角闪岩的ＳｍＮｄ等时线年龄为（２７９３±６９）Ｍａ,其平均模式年龄为２８８４Ｍａ。两套样品相对集中的模式年龄（２．９Ｇａ）代表这套火山岩从地幔分异出的时间,等时线年龄则代表火山岩系形成的时间。     

Determination of Sm‐Nd Isotopic Compositions in Fifteen Geological Materials Using Laser Ablation MC‐ICP‐MS and Application to Monazite Geochronology of Metasedimentary Rock in the North China Craton

In this study, we report both ¹⁴³Nd/¹⁴⁴Nd and ¹⁴⁷Sm/¹⁴⁴Nd values in twelve minerals (apatite, titanite, monazite and eudialyte) based on analyses over 4 years using LA‐MC‐ICP‐MS. The positive correlation between the measured β_Sm and β_Nd (r² = 0.9981) over this time in our laboratory demonstrates the excellent long‐term stability of the method. Compared with the normal method, Sm and Nd signal intensities were improved by a factor of 2.9 with the use of X skimmer and Jet sample cones in combination with the addition of nitrogen at 3–6 ml min^?1 to the central gas flow. The enhancement of signal intensity benefits the accurate in situ determination of the Sm‐Nd isotopes of samples poor in these elements. ¹⁴³Nd/¹⁴⁴Nd values were also determined in two manganese nodules and GSMC Co‐rich crust with low mass fractions of Nd (94–293 μg g^?1). Generally, most of the obtained Sm‐Nd isotopic compositions in these geological materials are consistent with published values. ‘External reproducibility’ (2s) of ¹⁴³Nd/¹⁴⁴Nd and ¹⁴⁷Sm/¹⁴⁴Nd was typically better than 0.06‰ and 2.5‰, respectively, demonstrating that the Durango, Otter Lake, NW‐1 and MAD apatites, the Khan, and OLT‐1 titanites, MGMH#117531 monazite and LV01 eudialyte are promising candidate reference materials for in situ Sm‐Nd isotopic determinations. The Trebilcock, Mae Klang and 44069 monazites are only suitable for in situ Nd isotopic determinations because of their heterogeneous Sm/Nd compositions. The heterogeneous Sm‐Nd composition of titanite BLR‐1 demonstrates that it is not a suitable reference material for in situ Sm‐Nd isotopic determinations. Deep‐sea samples (NOD‐A‐1 and NOD‐P‐1 manganese nodule, GSMC Co‐rich crust) with low mass fractions of Nd also show homogenous Nd isotopic compositions. Sm‐Nd isotopic ratios of a monazite (MQG‐22) from the North China Craton were measured as a case study and gave a ¹⁴⁷Sm‐¹⁴³Nd isochron age of 1792 ± 35 Ma (MSWD = 3.2) consistent with the published metamorphic age of the host metasedimentary rocks. The results for both candidate reference materials and geological samples demonstrate that the in situ LA‐MC‐ICP‐MS analytical protocol described is feasible and robust for research in geological evolution.     

柴达木北缘德令哈地区基性麻粒岩的发现及其形成时代

德令哈地区的基性麻粒岩呈透镜状或脉状分布于长英质片麻岩和泥质片麻岩中.基性麻粒岩的主要矿物组成为紫苏辉石、单斜辉石、斜长石、角闪石,含有少量的铁铁矿、锆石等副矿物.单斜辉石中具有针状的斜方辉石和铁铁矿的出熔片晶,代表了高温条件下的出熔结构.采用不同方法的二辉石温度计,估算出其麻粒岩相的温度为720～925℃.基性麻粒岩的微量及稀土元素分析显示其原岩的形成环境可能为大陆边缘环境.全岩及矿物的Sm-Nd等时线年龄为1791士37Ma,代表了麻粒岩相的变质时代.基性麻粒岩及其围岩的Nd模式年龄显示出这一地区可能有太古宙的地壳物质存在.     

兴蒙造山带正Σ（Nd,t）值花岗岩的成因和大陆地壳生长

大陆地壳的生长速率和地壳生长的位置均是地球科学中的最基本的问题。现有的许多大陆地壳生长模式认为,９０％的大陆地壳生长于１８亿年以前,显生宙以来的地壳生长不到整个地壳的１０％,主要位于活动大陆边缘。近年来在兴蒙造山带发现大量具有新生地壳来源性质的花岗岩产生于５００～１００Ｍa,对上述传统看法提出了挑战。现有的Ｎd同位素资料表明,兴蒙造山带的显生宙花岗岩,不论形成于什么时代和什么构造背影,也不论属于何种     

兴蒙造山带正ε(Nd,t)值花岗岩的成因和大陆地壳生长

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