The δ13C–δ18O variations in marble in the Hida Belt,Japan     

Hironobu Harada  Tatsuki Tsujimori  Keitaro Kunugiza  Katsuyuki Yamashita  Shogo Aoki  Kazumasa Aoki  Hideko Takayanagi  Yasufumi Iryu 《Island Arc》2021,30(1):e12389

Marble has a great potential to understand a history of various geological events occurring during tectonic processes. In order to decode metamorphic–metasomatic records on C–O isotope compositions of marble at mid-crustal conditions, we conducted a C–O–Sr isotope study on upper amphibolite-facies marbles and a carbonate–silicate rock from the Hida Belt, which was once a part of the crustal basement of the East Asian continental margin. Carbon and oxygen isotope analyses of calcite from marbles (Kamioka area) and a carbonate–silicate rock (Wadagawa area) show a large variation of δ¹³C [VPDB] and δ¹⁸O [VSMOW] values (from −4.4 to +4.2 ‰ and +1.6 to +20.8 ‰, respectively). The low δ¹³C values of calcites from the carbonate–silicate rock (from −4.4 to −2.9 ‰) can be explained by decarbonation (CO₂ releasing) reactions; carbon–oxygen isotope modeling suggests that a decrease of δ¹³C strongly depends on the amount of silicate reacting with carbonates. The occurrence of metamorphic clinopyroxene in marbles indicates that all samples have been affected by decarbonation reactions. All δ¹⁸O values of calcites are remarkably lower than the marine-carbonate values. The large δ¹⁸O variation can be explained by the isotope exchange via interactions between marble, external fluids, and/or silicates. Remarkably low δ¹⁸O values of marbles that are lower than mantle value (~+5 ‰) suggest the interaction with meteoric water at a later stage. Sr isotope ratios (⁸⁷Sr/⁸⁶Sr = 0.707255–0.708220) might be close to their protolith values. One zircon associated with wollastonite in a marble thin-section yields a U–Pb age of 222 ± 3 Ma, which represents the timing of the recrystallization of marble, triggered by H₂O-rich fluid infiltration at a relatively high-temperature condition. Our isotope study implies that the upper amphibolite-facies condition, like the Hida Belt, might be appropriate to cause decarbonation reactions which can modify original isotope compositions of marble if carbonates react with silicates.  相似文献   

Ubiquitous post-peak zircon in an eclogite from the Kumdy-Kol,Kokchetav UHP-HP Massif (Kazakhstan): Significance of exhumation-related zircon growth and modification in continental-subduction settings     

Sergei Yu. Skuzovatov  Vladislav S. Shatsky  Alexey L. Ragozin  Kuo-Lung Wang 《Island Arc》2021,30(1):e12385

U–Pb geochronological, trace-element and Lu–Hf isotopic studies have been made on zircons from ultrahigh-pressure (UHP) mafic eclogite from the Kumdy-Kol area, one of the diamond-facies domains of the Kokchetav Massif (northern Kazakhstan). The peak eclogitic assemblage equilibrated at > 900 °C, whereas the bulk sample composition displays light rare-earth element (LREE) and Th depletion evident of partial melting. Zircons from the eclogite are represented by exclusively newly formed metamorphic grains and have U–Pb age spread over 533–459 Ma, thus ranging from the time of peak subduction burial to that of the late post-orogenic collapse. The major zircon group with concordant age estimates have a concordia age of 508.1 ±4.4 Ma, which corresponds to exhumation of the eclogite-bearing UHP crustal slice to granulite- or amphibolite-facies depths. This may indicate potentially incoherent exhumation of different crustal blocks within a single Kumdy-Kol UHP domain. Model Hf isotopic characteristics of zircons (ε_Hf(t) +1.5 to +7.8, Neoproterozoic model Hf ages of 1.02–0.79 Ga) closely resemble the whole-rock values of the Kumdy-Kol eclogites and likely reflect in situ derivation of HFSE source for newly formed grains. The ages coupled with geochemical systematics of zircons confirm that predominantly late zircon growth occurred in Th–LREE-depleted eclogitic assemblage, that experienced incipient melting and monazite dissolution in melt at granulite-facies depths, followed by amphibolite-facies rehydration during late-stage exhumation-related retrogression.  相似文献   

Sedimentary records of the late Early Cretaceous compressional setting in the South China block: A case study of the Xingning Basin,Guangdong Province     

Jintao Kong  Zhongjie Xu  Yunyi Liang  Rihui Cheng 《Island Arc》2021,30(1):e12399

Recently, some scholars have proposed that the South China Block (SCB) was controlled by a compressive tectonic regime in the middle–late Early Cretaceous, challenging the belief that the SCB was under an extensional setting during the Cretaceous. The Early Cretaceous tectonic setting constraint in the SCB can offer vital insight to clarify the Mesozoic subduction history of the Paleo-Pacific. Therefore, to determine the SCB tectonic regime during the Early Cretaceous, this study investigated sedimentary rocks from the Lower Cretaceous Heshui Formation in the Xingning Basin, a foreland basin located in the southeastern SCB. Provenance analysis was performed using sandstone modal analysis, sandstone geochemical characteristics, and detrital zircon geochronology. Based on the results, we discussed basin sediment sources and the SCB tectonic regime during the Early Cretaceous. The results showed that the maximum Heshui Formation depositional age was 103 Ma ± 1.6 Ma in the Early Cretaceous Albian. Detrital framework modes and geochemical characteristics of sandstone indicated that Heshui Formation's source rocks were granites and sedimentary rocks. The detrital zircon U–Pb ages could be classified into two major and four subordinate age populations. The Wuyi Terrane to the north and southeast coastal regions to the east were the primary potential Heshui Formation source areas. However, the lower and upper sandstones are different in the peak ages, ~437 and ~146 to 104 Ma, respectively, indicating that the major source area shifted from the Wuyi Terrane to the southeastern coastal regions during the late Early Cretaceous. The sandstone modal analysis results indicated that the source area comprised mainly collisional–orogenic material. The SCB was under a compressive tectonic regime during the late Early Cretaceous and this compression action continued until at least 103 Ma ± 1.6 Ma.  相似文献   

扬子地台西南缘早三叠世层序地层格架   总被引：7，自引：0，他引：7  

肖加飞  魏家庸  胡瑞忠 《沉积学报》2004,22(2):310-318

扬子地台西南缘早三叠世地层被划分为4个沉积层序。通过综合研究已取得的牙形石生物地层资料,与Haq等人提出的三叠纪牙形石生物时带进行了对比,初步定出了各沉积层序及体系域的界面年龄(层序1底界年龄251Ma;层序2底界年龄245.2Ma;层序3底界年龄243Ma;层序4底界年龄240.5Ma,顶界年龄239.4Ma),从而建立了区内分辨率较高的早三叠世地层格架。格架中层序组合特征在碳酸盐岩台地边缘显示得非常清楚,其中,层序1-层序2高水位体系域的台地边缘依次向陆后退,呈退积或超覆(overlap)型组合关系;层序3-层序4高水位体系域的台地边缘则依次向海推进,呈进积或退覆(offlap)型组合关系。这种组合特征主要受沉积盆地的构造沉降及2级海平面升降亚旋回的海面变化的控制,构造沉降加速和海面上升期形成的层序呈退积型组合关系;构造沉降平缓及海面下降期形成的层序呈进积型组合关系。此外,还研究了斜坡地带(贵阳改毛)层序1-层序3底部的碳氧同位素组成变化规律:海侵体系域-高水位体系域碳、氧同位素组成变化不大,δ13C主要为正值,但在高水位体系域顶部明显负向偏移;低水位体系域碳、氧同位素组成变化剧烈,且均为负值。这为地层划分提供了地球化学方面的依据。  相似文献   

西藏南部康马岩体岩石类型及其同位素测年   总被引：9，自引：1，他引：8  

刘文灿  王瑜  张祥信  李惠民  周志广  赵兴国 《地学前缘》2004,11(4):491-501

康马岩体位于西藏南部康马县城北侧 ,其内部可划分出 5种不同的岩石类型 :(1)片麻状黑云二长花岗岩 ;(2 )眼球状黑云二长花岗岩 ;(3)片麻状二云母二长花岗岩 ;(4 )弱片麻状细粒黑云二长花岗岩 ;(5 )变质的暗色辉长辉绿岩。前两类为康马岩体的主体岩石类型 ,侵位时代为加里东早期 (约4 78～ 4 6 1Ma) ;其余均呈脉状产出 ,其中片麻状二云母二长花岗岩与康马岩体主体岩石类型属于同期产物 ,弱片麻状细粒黑云二长花岗岩形成于海西早期 ((339.0± 1.2 )Ma) ,暗色辉长辉绿岩的形成时代目前还不十分清楚。不同类型的岩石其Ar Ar冷却年龄约为 18～ 14Ma。  相似文献   

Open star clusters in the spiral arms of our Galaxy     

M. E. Popova  A. V. Loktin 《Astronomy Letters》2008,34(8):551-557

We consider the age distributions of open star clusters attributed to three segments of Galactic spiral arms. The smoothed distributions of clusters on the age-Galactocentric angle plane show a great nonuniformity. The time dependence of the formation rate of Galactic disk clusters recovered by taking into account selection effects and dynamical evolution of clusters shows that, on average, the formation rate of open star clusters decreases with time. This is in agreement with the increase in star formation rate into the past, as follows from the study of this process by the method of stellar population synthesis. The present time is the epoch of a current maximum of the cluster formation rate. In addition to the current maximum, there have been at least three more maxima with a period of 300–400 Myr and a duration of no more than 300 Myr. The age distributions are consistent with the pattern of star formation governed by the successive passages of density waves through each examined volume of the Galactic disk. The spiral structure becomes more complex when passing from the inner regions of the Galaxy to its outer regions.  相似文献   

Spectroscopic study of the peculiar galaxy UGC 5119     

O. A. Merkulova  L. V. Shalyapina  V. A. Yakovleva  G. M. Karataeva 《Astronomy Letters》2008,34(8):542-550

We present the results of our study of the stellar kinematics in the elliptical galaxy UGC 5119, which has previously been suspected to be a polar-ring galaxy. We have detected a rapidly rotating disk in the central region (r ≤ 3.2 kpc) of the galaxy’s main body and found a radial velocity gradient along its minor axis (in the putative ring). We conclude that UGC 5119 is a medium-luminosity elliptical galaxy with a rapidly rotating disk component and a stellar (probably polar) ring. We have calculated the Lick indices of the Hβ, Mggb, Fe 5270, and Fe 5335 absorption lines and compared them with evolutionary synthesis models. Differences in the [Mg/Fe] ratios, metallicities, and ages of the stars have been found: the young stellar population with a solar [Mg/Fe] ratio and a high metallicity dominates in the circumnuclear region (r ≤ 1 kpc), while the old one with a low metal abundance dominates in the ring.  相似文献   

湖南九嶷山复式花岗岩体SHRIMP锆石定年及其地质意义   总被引：53，自引：11，他引：42  

付建明  马昌前  谢才富  张业明  彭松柏 《大地构造与成矿学》2004,28(4):370-378

应用SHRIMP锆石U-Pb法获得九嶷山复式花岗岩中的主要岩体形成年龄为:雪花顶花岗岩(432±21)Ma、金鸡岭花岗岩(156±2)Ma、砂子岭花岗岩(157±1)Ma和西山火山-侵入杂岩(156±2)Ma。结果显示砂子岭岩体属燕山早期而非印支期;西山火山-侵入杂岩属燕山早期而非燕山晚期。花岗岩中继承锆石复杂,其形成时代为1579Ma、2108Ma和2669Ma,提供了九嶷山地区存在古-中元古代,甚至太古代基底的年龄信息。新元古代(912Ma)锆石的大量出现为扬子陆块和华夏陆块碰撞带通过本区的认识提供了一个间接证据。  相似文献   

阴山—燕山北麓富碱侵入岩体的岩石地球化学特征、锆石SHRIMP U-Pb年龄及构造意义     

龚弥  蔡剑辉  阎国翰  刘楚雄  刘钊 《地质论评》2019,65(4):894-915

本文研究的达茂旗黄合少、察哈尔右后旗古城和河北尚义县八道沟岩体位于华北克拉通北缘阴山—燕山北麓,索伦缝合带以南,沿近东西方向展布。主要岩石类型为正长岩、二长岩和石英二长岩。岩石地球化学研究表明其SiO2含量59. 08%~66. 52%, Al2O3= 15. 34%~21. 67%,A/CNK<1。属于准铝质中性岩范畴。全碱含量（Na2O+K2O）均在8%以上,在岩石的碱度率AR—SiO2图解上大多数样品落入碱性与过碱性区域,里特曼指数σ值从3. 73~10. 83均位于碱性或过碱性系列,属于碱性岩。岩体的微量元素以富集大离子亲石元素（LILE）如Rb、Ba和Sr等,亏损高场强元素（HFSE）如Ti、P、Nb和Ta等为特征。岩石稀土元素特征显示富集轻稀土元素（LREE）,亏损重稀土元素（HREE）并且轻重稀土元素分馏比较明显的特征。除极个别样品外,岩石具有Eu负异常（δEu= 0. 35~0. 91）。通过对察哈尔右后旗古城正长岩体和河北尚义县八道沟富碱侵入岩体的高精度测年研究,获得其SHRIMP锆石U- Pb年龄分别为413. 2±3. 3~415. 0±5. 9 Ma和366. 8±5. 2~372. 3±4. 7 Ma,表明其均为古生代泥盆纪富碱侵入岩浆活动的产物。结合前人关于阴山—燕山北麓其它富碱侵入岩体（内蒙古固阳东高家村碱性正长岩体、黄合少碱性正长岩和冀北水泉沟碱性杂岩体 ）的研究成果,推断在华北克拉通北缘阴山—燕山北麓一带,可能存在一条东西方向展布的晚古生代泥盆纪富碱侵入岩带。根据该岩带岩石地球化学特征,以及Ta/Yb—Th/Yb与Zr/Nb—Zr/Nb—Y/Nb判别图推测其岩浆物质来源可能与富集地幔有关,按照成岩温压环境指示,其形成深度位置约为下地壳,岩浆上升侵位过程中明显受到地壳物质的混染。依据前人关于碱性岩特征的研究,结合本文研究岩体的岩石化学特征和及Rb—Nb+Y构造判别图解指示,推测岩体形成于张性构造环境,可能与古生代志留纪末兴蒙造山带南部发育的白乃庙岛弧带和华北克拉通发生弧—陆碰撞后的伸展背景相关。  相似文献   

新疆阿尔泰阿勒泰组沉积时代及其形成环境          下载免费PDF全文

李彦  耿新霞  李强  张志欣  王旭  杨俊杰 《地质科学》2019,(1):34-61

阿勒泰组变质碎屑岩局部夹变质火山岩广泛分布于南阿尔泰的冲乎尔、克兰和麦兹盆地,其沉积时代和构造环境对于研究阿尔泰造山带的演化过程有重要意义。阿勒泰组碎屑锆石的年代学研究表明,碎唐锆石年龄主要集中在417-383 Ma和507-445 Ma,并出现少量元古宙和太古宙碎屑锆石。少数锆石年龄为380-354 Ma,与阿勒泰组凝灰岩和流纹岩年龄一致(376~354 Ma)。综合研究认为阿勒泰组时代为中-晚泥盆世(382-354 Ma)。阿勒泰组长石石英砂岩分选性和磨圆度较差,为近源沉积,物源岩石主要来自泥盆纪火山岩,其次是晚寒武一早奥陶世火山岩和奥陶纪花岗岩。长石石英砂岩样品具有高的La/Sc(3.9-6.3),La/Y(1.0~1.6),较低的Sc/Cr(0.2~0.4)比值,类似于大陆岛弧相关环境碎屑沉积物,结合Th-Co-Zr/10和Th-Sc-Zr/10以及La-Th-Sc判别图,认为阿勒泰组形成于与岛弧相关的构造环境(弧后盆地),为研究阿尔泰造山带泥盆纪构造演化提供了重要证据。  相似文献