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1.
Phanerozoic granitoids in South Korea are classified into four primary spatiotemporal groups showing geochemical and isotopic diversity. This study presents the first in situ Hf isotope data for zircons extracted from representative outcrops of each granitoid group. The core‐to‐rim variation in εHf values observed in some zircon grains provides evidence for open‐system processes influenced by the input of more primitive melts or interactions with pre‐existing crustal materials. A general core‐to‐rim decrease in Lu/Hf and Th/U ratios indicates a progressive compositional change in the melts during magmatic differentiation. Contrasting evolutionary paths demonstrated by zircon εHf values suggest that the Neoproterozoic to Palaeozoic crust including the Permian granitoids was recycled during the Cretaceous to Palaeogene magmatism in south‐eastern Korea, whereas the Palaeoarchaean to Palaeoproterozoic crust provided major source material for the Triassic to Jurassic granitoids in central Korea.  相似文献   

2.
Gangdese batholith in the southern Lhasa block is a key location for exploring the Tibetan Plateau uplift and exhumation history. We present the new low-temperature thermochronological data from two north–south traverses in the central Gangdese batholith to reveal their cooling histories and corresponding controls. Zircon fission track ages show prominent clusters ranging from 23.7 to 51.6 Ma, apatite fission track ages from 9.4 to 36.9 Ma, apatite (U–Th)/He ages between 9.5 and 12.3 Ma, and one zircon (U–Th)/He age around 77.8 Ma. These new data and thermal modeling, in combination with the regional geological data, suggest that the distinct parts of Gangdese batholith underwent different cooling histories resulted from various dynamic mechanisms. The Late Eocene–Early Oligocene exhumation of northern Gangdese batholith, coeval with the magmatic gap, might be triggered by crust thickening followed by the breakoff of Neotethyan slab, while this stage of exhumation in southern Gangdese batholith cannot be clearly elucidated probably because the most of plutonic rocks with the information of this cooling event were eroded away. Since then, the northern Gangdese batholith experienced a slow and stable exhumation, while the southern Gangdese batholith underwent two more stages of exhumation. The Late Oligocene–Early Miocene rapid cooling might be a response to denudation caused by the Gangdese Thrust or related to the regional uplift and exhumation in extensional background. By the early Miocene, the rapid exhumation was associated with localized river incision or intensification of Asian monsoon, or north–south normal fault.  相似文献   

3.
西藏中部拉萨地块大规模早白垩世花岗岩类的岩浆源区和岩石成因迄今尚未得到很好约束,对这些问题的深入理解将有助于揭示拉萨地块白垩纪时期的岩浆作用过程及成矿背景。本文报道了中部拉萨地块代表性花岗岩基——措勤麦嘎岩基的锆石U-Pb年代学、全岩元素地球化学、Sr-Nd同位素和锆石Hf同位素数据。本文锆石U-Pb定年结果表明,麦嘎岩基花岗质岩主要侵位于122±1Ma和113±2Ma,闪长质包体与后者同期(113±2Ma)。122±1Ma花岗质岩属I型弱过铝质高钾钙碱性系列,(87Sr/86Sr)i值高(0.7147),全岩εNd(t)(-12.0)和锆石εHf(t)(-15.7～-11.1)为较大的负值,表明其很可能来源于古老下地壳物质的重熔。113±2Ma寄主花岗质岩为I型偏铝质-弱过铝质高钾钙碱性系列,相对于122±1Ma花岗质岩石,其(87Sr/86Sr)i比值偏低(0.7094～0.7156)、全岩εNd(t)值(-12.1～-7.3)和锆石εHf(t)值(-11.1～0.1)较高,很可能来源于古老下地壳物质的部分熔融,并含有更多幔源物质。闪长质包体(113±2Ma)为偏铝质中-高钾钙碱性系列,以变化范围大的(87Sr/86Sr)i(0.7058～0.7105)、负的全岩εNd(t)值(-10.7～-9.8)及负的锆石εHf(t)值(-14.0～-5.6)为特征,可能是古老富集岩石圈地幔物质部分熔融的产物或亏损地幔物质经历强烈地壳混染作用的结果。在目前已有资料条件下(缺乏同期基性岩石的相关数据),本文暂将麦嘎岩基113±2Ma寄主花岗质岩及同期闪长质包体解释为镁铁质岩浆与长英质岩浆发生不同程度岩浆混合作用的产物,这一解释可能对中部拉萨地块同期花岗类的岩石成因具普遍意义。麦嘎岩基及中部拉萨地块同期岩浆岩约113Ma幔源物质增加现象,可能是南向俯冲的班公湖-怒江洋壳岩石圈板片断离的结果。  相似文献   

4.
The late- to post-collisional stage in orogenic systems is characterized by the coeval existence of bimodal potassic to ultrapotassic magmatic activity related to partial melting of an enriched lithospheric mantle together with crustal derived melts. In this paper, we present new whole rock geochemical analyses combined with zircon and titanite U–Pb and zircon Hf isotopic data from potassic to ultrapotassic rocks from six plutons that occur within the Archean Itacambira-Monte Azul block (BIMA), to discuss their petrogenesis and the tectonic implications for the São Francisco paleocontinent. The new U–Pb ages range from ca. 2.06 Ga to 1.98 Ga and reveal long-lasting potassic magmatism within the BIMA, which is within the late- to- post-collisional stage of the São Francisco paleocontinent evolution. The ultrapotassic rocks are compatible with a fluid-related metasomatized mantle source enriched by previous subduction events, whereas the potassic rocks are bimodal and have a transitional shoshonitic to A-type affinity. These rocks have a hybrid nature, possible related to the mixing between the mafic potassic/ultrapotassic rocks and high temperature crustal melts of the Archean continental crust. Our results also show an increase of within-plate signature towards the younger potassic magmas. The participation of an important Archean crustal component in the genesis of these rocks is highlighted by the common and occasionally abundant occurrence of Archean inherited zircons. The Hf isotopic record shows that most of the zircon inheritance has dominantly subchondritic εHf(t) values, which fits a crustal reworking derivation from a similar Eo- to Paleoarchean precursor crust. However, the presence of juvenile 2.36 Ga zircon inheritance in an ultrapotassic sample reveal the existence of a hidden reservoir that is somewhat similar to the described for the Mineiro Belt in southern São Francisco paleocontinent.  相似文献   

5.
SHRIMP zircon U-Pb dates, combined with in-situ Hf isotopic data, provide new constraints on the petrogenesis and protolith of peralkaline, metaluminous and peraluminous intrusions and rhyolitic tuffs in the Emeishan large igneous province, with significant bearing on crustal melting associated with mantle plumes. Syenite and A-type granitic intrusions from Huili, Miyi and Taihe in the center of this large igneous province yield U-Pb dates at ∼260 Ma, consistent with the ages obtained for mafic layered intrusions in the same province. Zircon from these rocks exhibits a wide range of initial Hf isotope ratios (εHf(t) = −1.4 to +13.4), with corresponding TDM1 of 400-900 Ma. The highest εHf(t) value is only marginally lower than that of depleted mantle reservoir at 260 Ma, suggesting that their source is primarily juvenile crust added during Emeishan volcanism, with incorporation of variable amounts of Neoproterozoic crust. The trigger of crustal melting is most likely related to advective heating associated with magmatic underplating. In contrast, the 255-251 Ma peraluminous granites from Ailanghe and 238 Ma rhyolitic tuff from Binchuan, have negative initial εHf values of −1.3 to −4.4, and of −7.7 to −14, respectively. Hf isotopic model ages and presence of inherited zircons indicate their derivation from Mesoproterozoic and Paleoproterozoic crust, respectively. Given the time lag relative to the plume impact (∼260 Ma) and insignificant mantle contribution to 255-238 Ma magmatism, conductive heating is suggested as the trigger of crustal melting that resulted in formation of delayed felsic magmas. The involvement of older crust in younger felsic magmas is consistent with upward heat transfer to the lithosphere during plume impregnation, if the age of crust is inversely stratified, i.e., changes from Paleoproterozoic to Mesoproterozoic to Neoproterozoic to Permian with increasing depth. Such crust may have resulted from episodic, downward crustal growth during the evolution of the western Yangtze Craton.  相似文献   

6.
The Mozambique Ocean is postulated to mark the huge oceanic basin of the East African Orogen and separated the continental components of eastern and western Gondwana, but only limited studies have considered the production of its oceanic crust. Here we present a combined analysis of petrological, geochronological, geochemical, and Sr–Nd–Hf isotopic data for the Early Neoproterozoic gabbros in the North Lhasa terrane, Tibet. Zircons from the gabbros yielded concordant ages of ca. 913–901 Ma. The gabbros display N‐MORB compositions with limited subduction input and are characterized by high positive zircon εHf(t) (+5.3 to +12.1) and whole‐rock εNd(t) (+5.6 to +6.5) values. They have not experienced significant crustal contamination but their compositions have been modified by extensive fractional crystallization. They are most likely derived from relatively high degree partial melting (>20%) of a spinel lherzolite source in a depleted mantle. Combined with observations from previous studies, we suggest that the generation of these gabbros was probably related to the incipient formation of oceanic crust in a back‐arc basin and they may mark a relic of the eastern Mozambique Ocean. To our knowledge, they are the oldest oceanic relic in the Tibetan Plateau.  相似文献   

7.
The Khangai batholith is one of the largest groups of granitoid plutons produced in Central Asia in the Late Permian–Early Triassic, at 270–240 Ma. The batholith occurs in the Khangai collage of Precambrian terranes, which include Early Precambrian crustal blocks (Dzabkhan and Tarbagatai) and Early to Late Neoproterozoic structures of the Songino block in their surroundings. The axial zone of this collage is overprinted by a basin filled with Devonian volcanic–siliceous rocks and Early to Middle Carboniferous terrigenous rocks. The isotopic parameters (Nd and Pb) of granitoids in the Khangai batholith indicate that the melts were derived from compositionally contrasting crustal sources and a single mantle one. The massifs hosted in the Precambrian blocks were produced with the involvement of lower crustal material, with various ages of the origin of the crust and its differentiation into upper and lower ones. The crust of the Tarbagatai and Dzabkhan blocks was produced in the Early Archean and was differentiated at the Archean–Proterozoic boundary. The crust of the Songino block was formed in the Paleoproterozoic and differentiated in the Early Neoproterozoic. According to the Pb and Nd isotopic parameters of granitoids in the Khangai Basin, the regional continental crust was close to the juvenile one, i.e., the continental crust of the Khangai Basin had still not been differentiated by the time when the Khangai batholith was produced. A single mantle source was involved in the origin of the melts of granitoids of the Khangai batholith in various tectonic blocks. The evolution of the Pb isotopic composition of this sources is consistent with the Stacey–Kramers model at µ = 9.5. This source can be identified with the enriched mantle, which has a higher U/Pb ratio than the depleted mantle and lower εNd(T) of 0 to +2.  相似文献   

8.
青藏高原东部的隆升机制一直都是地学界的研究热点,研究学者们提出和发展了多种岩石圈变形模型,而存在多种模型的主要原因之一是对青藏高原东部地壳及岩石圈结构认识不足。本文主要针对SinoProbe-02项目横跨龙门山断裂带、全长400多公里的宽角、折射地震数据及重力数据进行联合反演和综合解释。研究结果表明,龙门山及邻近地区地壳结构可明确划分为上地壳、中地壳和下地壳。上地壳上层为沉积层,龙门山断裂带以西大部分区域被三叠纪复理岩覆盖,而在龙日坝断裂与岷江断裂之间出现了密度为2.7g/cm3的高速异常体;向东靠近龙门山地区,沉积层厚度逐渐减薄。中地壳速度变化不均一,而且变形强烈;若尔盖盆地和龙门山断裂带下方出现明显低速带;中地壳在龙门山西侧厚度加厚,在岷江断裂下方和四川盆地靠近龙门山断裂带地区附近厚度达到最大。莫霍面整体深度从东往西增厚,最厚可达56 km。本次研究得到的地壳结构和密度分布分析结果表明现有的地壳厚度和物质组成不足以支撑龙门山及邻近地区目前所达到的隆升高度,因此四川盆地刚性基底西缘因挤压作用产生的弯曲应力也是该地区抬升的重要条件之一。  相似文献   

9.
邱啸飞 《地质学报》2022,96(11):3784-3798
扬子克拉通前泥盆纪地壳演化过程一直是地学界研究的热点。本文报道了扬子克拉通北部武汉地区玉笋山剖面的志留系坟头组和泥盆系云台观组碎屑沉积岩中锆石U- Pb年龄和Hf同位素组成。结果表明，武汉地区坟头组和云台观组样品中最年轻的碎屑锆石年龄分别为430±5 Ma和415±5 Ma，将该地区坟头组和云台观组的沉积时代各限定在中志留世和晚泥盆世。碎屑锆石Hf同位素特点表明，沉积物源区在中太古代、新太古代以及新元古代形成了少量初生地壳，而古老地壳的再造主要发生在新太古代、新元古代和古生代，区域上最显著的初生地壳生长时期则是古元古代。综合对比扬子克拉通北部东、西两侧具有明显不同的锆石U- Pb年龄、微量元素和Hf同位素组成，暗示扬子克拉通可能由多个相对独立地壳演化过程的部分构成，而不具有统一的早前寒武纪基底。  相似文献   

10.
The Qinling Orogenic Belt (QOB) located between the North China Craton (NCC) and the Yangtze Craton (YZC) is composed of the North Qinling Belt (NQB), the South Qinling Belt (SQB) and the northern margin of the YZC. Detailed geological and geochronological investigations have revealed distinct Neoproterozoic blocks of various scales in the middle and western segments of the SQB, including the Madao block (MDB), Mihunzhen intrusion (MHI), Zhenggou block (ZGB), and Lengshuigou block (LSB) which constitute an east-west trending Neoproterozoic uplift zone of the basement continental blocks. These blocks are mainly composed of four lithological groups. Group #1 consists mainly of diorites in the LSB, the zircons from which yield a weighted mean 206Pb/ 238U age of ca. 941 Ma. Group #2 is chiefly composed of hornblende gabbros and diorites in the MHI and LSB, which were formed at ca. 885 Ma. Group #3 comprises massive diorites, quartz diorite, tonalites, granodiorites, and monzogranites in the MDB, MHI, ZGB and LSB, which were emplaced during ca. 785–740 Ma. Group #4 is composed of hornblende gabbros with an emplacement age of ca. 667 Ma in the ZGB.Detailed whole-rock geochemical and zircon Hf isotopic studies reveal the following: (1) The diorites of Group #1 were produced by partial melting of depleted mantle which was enriched by slab-derived melts, with the parental magmas contaminated by crustal materials. (2) The gabbros of Group #2 were derived from the partial melting of depleted mantle enriched by slab-derived melts and the diorites are the fractional crystallization products of the gabbroic magmas. (3) Group #3 which can be further sub-divided based on lithological assemblages and zircon Hf isotopic features into two subgroups, one representing massive diorites, quartz diorite, tonalites, granodiorites, and monzogranites (DTGMs) and the other composed of gneissic quartz diorites and granodiorites. Among these, the DTGMs were derived through magma mixing between melts derived from the depleted mantle wedge altered by slab-derived fluids and melts from juvenile sources, which subsequently underwent amphibole-dominated fractionation, whereas the gneissic granitoids formed through partial melting of thickened lower crust contaminated by depleted mantle melts. (4) The gabbros of Group #4 originated from a depleted lithospheric mantle that was enriched by slab-derived melts and fluids with contribution of asthenospheric mantle-derived materials. In conjunction with data from previous studies on the Neoproterozoic blocks in the SQB and basement blocks in the northern margin of the YZC, our new geological, geochronological and geochemical data suggest a large Neoproterozoic uplift zone in the SQB, which was destructed by Paleozoic to Mesozoic magmatism and deformation. The Neoproterozoic uplift zone of the SQB might have been separated from the northern margin of the YZC during the formation of the Mianlue Ocean, and might have evolved under an active continental margin setting and subsequent continental rift setting accompanied by significant crustal growth. The magmatism also resulted in the formation of important Neoproterozoic ore deposits and supplied the material sources for some of the major Mesozoic ore deposits.  相似文献   

11.
陈小宇  刘俊来  翁少腾 《岩石学报》2020,36(8):2558-2570
通常认为位于青藏高原东南缘的巽他地块侧向刚性块体挤出调节了印度-欧亚板块碰撞及后碰撞。然而,最近的研究表明,低粘度的中下地壳流动可以解释青藏高原向外扩张的现象。关于哪种机制在巽他地块挤出过程中起着主导作用仍未解决。在本研究中,我们重点围绕哀牢山-红河构造带南部的瑶山杂岩以及构造带北部邻区的玉龙杂岩开展构造研究。详细的宏观构造解析、显微构造以及组构分析说明切向剪切作用在瑶山与玉龙穹隆的形成与剥露中起着重要作用,组成穹窿的岩石均具有分层流变学特点。瑶山穹隆是发育在较深岩石层位的穹隆构造,而玉龙穹隆是发育在较浅岩石层位的穹隆构造。向南或东南切向剪切可能是上地壳向南的重力滑动和粘滞下地壳相对中上地壳向北流动共同作用的结果。前者可能与高原重力塌陷有关,但后者的驱动力有待进一步研究。  相似文献   

12.
根据松辽盆地北部林深3 井火山岩的岩相、全岩主微量元素、锆石U--Pb 同位素和锆石Hf 同位素特征的分析结果,探讨了该火山岩的形成时代和岩浆源区。锆石LA--MC--ICPMS U--Pb 研究结果表明: 林深3 井火山岩形成时代约为120 Ma,处于早白垩世中晚期,属于营城组火山岩。锆石的LA-- MC--ICPMS Hf 同位素研究显示,本区火山岩的锆石εHf ( t) 全部为较高的正值,二阶段Hf 模式年龄为789 ～ 1 494 Ma,表明其主要起源于中--新元古代增生的地壳物质,暗示中--新元古代时期兴蒙造山带东段存在地壳增生事件。  相似文献   

13.
莫宣学 《地球科学》2020,45(7):2245-2257
青藏巨厚陆壳的性质和形成机制，是重要的科学问题.通过对青藏岩浆岩，特别是其Nd、Hf同位素的研究，证明青藏高原并存着新生地壳和再循环地壳两类地壳.地壳的结构和属性对成矿矿种、矿床类型和分布有重要的控制作用.青藏巨厚地壳是由两种机制（构造加厚；地幔物质通过岩浆作用注入加厚）共同造成的，二者贡献比例约6:4.地壳增厚主要发生在50~25 Ma期间.大陆碰撞带是造成地壳净生长的重要构造部位.   相似文献   

14.
对喜马拉雅前陆盆地和孟加拉海扇中各地层的碎屑白云母40Ar/39Ar资料的系统分析揭示了喜马拉雅造山带自印度-欧亚板块碰撞开始造山以来的整个剥落历史：剥落速率开始较为稳定,然后开始上升,在22Ma左右达到峰值,为4～5mm/a,随后急剧下降,最终以2mm/a的速率保持平稳。喜马拉雅造山带与青藏高原周缘剥落历史的对比约束了印度-欧亚板块碰撞造成青藏高原东缘和北缘的不同反应方式。即开始时的挤压主要被青藏高原北缘的大规模左旋走滑吸收,到30Ma左右,喜马拉雅造山带冷却、剥落速率显著增强,北缘左旋走滑造成的柴达木地块的向东运动被华北板块阻挡而停滞,因此在北缘发生了一些重要的冷却和抬升剥落事件。至18Ma左右,喜马拉雅造山带的冷却、剥落速率继续增高并维持在较高水平,而该时间段内无论是北缘还是东缘,均未发生显著的抬升剥落事件,因此青藏高原的整体隆升和地壳增厚可能发生在此期间。中新世末—上新世初开始至今,青藏高原东缘龙门山地区发生了一些显著的抬升剥落事件,导致了大量的山崩和河流侵蚀,即此时来自喜马拉雅的挤压主要被青藏高原向东方向的地壳逃逸所吸收。  相似文献   

15.
Zircon U-Pb and hornblende Ar-Ar ages, major and trace elements, and Sr, Nd and O isotope compositions of Neoproterozoic and Mesozoic granitoids from the Wulian region in the Sulu orogen of China demonstrate that post-collisional granitoids were generated by Early Cretaceous melting of subduction-thickened continental crust that has geochemical affinities to Neoproterozoic protolith of ultrahigh-pressure metaigneous rocks that were derived from the Yangtze Block. The Mesozoic granitoids share the following features with the Neoproterozoic granites: (1) occurrence of Neoproterozoic U-Pb ages in zircon; (2) strong LREE enrichment but HFSE (Nb, P and Ti) depletion; (3) variable δ18O values for constituent minerals; (4) significantly negative εNd(t) values with Paleoproterozoic Nd model ages. Thus the two ages of granitoids have a genetic relationship in source nature. However, they differ significantly in both the O isotope composition of zircon and the concentration ratios of fluid-mobile to fluid-immobile elements. These differences are interpreted to reflect differences in the depth of magma sources, and in the nature of subsequent water-rock alteration. The Neoproterozoic granites were derived from hydration melting of Paleoproterozoic crust during breakup of the supercontinent Rodinia at ca. 780 to 740 Ma along the northern margin of the Yangtze Block, with subsequent overprinting of high-T meteoric-hydrothermal alteration and rifting-induced low-18O magmatism. In contrast, the Mesozoic granitoids were derived from dehydration melting of subduction-thickened crust that was unaffected by meteoric-hydrothermal alteration. The source of the Mesozoic granitoids may be coeval middle-lower crustal counterparts of the Neoproterozoic granites.  相似文献   

16.
段亮 《地质通报》2010,29(1):70-78
对喜马拉雅前陆盆地和孟加拉海扇中各地层的碎屑白云母40Ar/39Ar资料的系统分析揭示了喜马拉雅造山带自印度-欧亚板块碰撞开始造山以来的整个剥落历史: 剥落速率开始较为稳定,然后开始上升,在22Ma左右达到峰值,为4~5mm/a,随后急剧下降,最终以2mm/a的速率保持平稳。喜马拉雅造山带与青藏高原周缘剥落历史的对比约束了印度-欧亚板块碰撞造成青藏高原东缘和北缘的不同反应方式。即开始时的挤压主要被青藏高原北缘的大规模左旋走滑吸收, 到30Ma左右,喜马拉雅造山带冷却、剥落速率显著增强,北缘左旋走滑造成的柴达木地块的向东运动被华北板块阻挡而停滞,因此在北缘发生了一些重要的冷却和抬升剥落事件。至18Ma左右,喜马拉雅造山带的冷却、剥落速率继续增高并维持在较高水平,而该时间段内无论是北缘还是东缘,均未发生显著的抬升剥落事件,因此青藏高原的整体隆升和地壳增厚可能发生在此期间。中新世末—上新世初开始至今,青藏高原东缘龙门山地区发生了一些显著的抬升剥落事件,导致了大量的山崩和河流侵蚀,即此时来自喜马拉雅的挤压主要被青藏高原向东方向的地壳逃逸所吸收。  相似文献   

17.
Granitic rocks are the principle agent of crustal differentiation, therefore their origins yield important information on crustal formation and reworking. An extensive survey of zircon Hf isotopes from granitic rocks in a large region can provide a profile of crustal characteristics that may be further linked to previous crustal evolution. In this study, we measured U–Pb ages and Hf isotope compositions of zircon grains extracted from twenty-five Jurassic, five Triassic and two Ordovician granitic plutons from the Nanling Range, South China Block (SCB). Combined with the published Lu–Hf isotopic data for the granitic rocks in the studied and adjacent areas, three domains with different crustal formation histories have been identified in the southern part of the SCB: eastern side, middle part and western side. The eastern side extends to the coastal area of the SCB, with dominant Hf crustal model ages (TDM2) in zircons falling within the range of 2.2–1.6 Ga. The middle part is partly coincided with the low-Nd model age belt proposed by Chen and Jahn (1998), with zircon Hf TDM2 ranging from 1.6 to 1.0 Ga. The western side covers the westernmost Nanling Range and the western end of the Jiangnan orogen, in which the granitoids have zircon Hf TDM2 model ages spanning 2.2–1.8 Ga. The Paleo- to Meso-Proterozoic model ages of the Phanerozoic granitoids in the Nanling Range imply a long-term crustal reworking. Zircons from the western and eastern sides have an average εHf(155 Ma) at around −10, about 4 epsilon units lower than the middle part (εHf(155 Ma) = −6). Hf TDM2 histogram from the western Nanling Range is similar to that of the Neoproterozoic granitoids in northern Guangxi Province to the west but much lower to the granites in the middle part to the east. The eastern side has a broader range of Hf model ages in zircons, with the main peak low to ca 1.6 Ga, suggesting the reworking of Mesoproterozoic crust. However, granitoids in the middle part have zircon Hf TDM2 ages at 1.6–1.0 Ga, which indicates the incorporation of younger crust materials into the magma sources. The Hf model ages of granitoids, as well as four zircon xenocrysts with ages around 920 Ma within the Mesozoic granitoids in the middle part, indicate that the middle part has similar crustal features with the eastern Jiangnan orogen. We propose that this low TDM2 granite belt is probably part of the early Neoproterozoic arc-continent collision belt between different continents (possibly Yangtze and Cathaysia) during the early assembling processes, while the granitoids in the western and eastern sides have similar crustal compositions.  相似文献   

18.
Zircons of 10–100μm size and monazites of up to 10μm size are present in rhyolite and trachyte dikes associated with Deccan basalts around Rajula in the southern Saurashtra Peninsula of Gujarat. On the basis of structural conformity of the felsic and basaltic dikes, K-Ar ages and trace element considerations, a previous study concluded that the felsic rocks are coeval with the Deccan Volcanics and originated by crustal anatexis. The felsic rocks contain two populations of zircons and monazites, one that crystallized from the felsic melt and the other that contains inherited crustal material. Trace element variations in the rhyolites and trachytes indicate that zircons and monazites crystallized from the felsic melts, but compositional analysis of a zircon indicates the presence of a small core possibly inherited from the crust. Hf compositional zoning profile of this zircon indicates that it grew from the host rhyolitic melt while the melt differentiated, and Y and LREE contents suggest that this zircon crystallized from the host melt. Pb contents of some monazites also suggest the presence of inherited crustal cores. Hence, any age determination by the U-Th-Pb isotopic method should be interpreted with due consideration to crustal inheritance. Temperatures estimated from zircon and monazite saturation thermometry indicate that the crust around Rajula may have been heated to a maximum of approximately 900°C by the intruding Deccan magma. Crustal melting models of other workers indicate that a 1–2 million year emplacement time for the Deccan Traps may be appropriate for crustal melting characteristics observed in the Rajula area through the felsic dikes.  相似文献   

19.
《地学前缘(英文版)》2018,9(6):1921-1936
The origin of zircon grains, and other exotic minerals of typical crustal origin, in mantle-hosted ophiolitic chromitites are hotly debated. We report a population of zircon grains with ages ranging from Cretaceous (99 Ma) to Neoarchean (2750 Ma), separated from massive chromitite bodies hosted in the mantle section of the supra-subduction (SSZ)-type Mayarí-Baracoa Ophiolitic Belt in eastern Cuba. Most analyzed zircon grains (n = 20, 287 ± 3 Ma to 2750 ± 60 Ma) are older than the early Cretaceous age of the ophiolite body, show negative εHf(t) (−26 to −0.6) and occasional inclusions of quartz, K-feldspar, biotite, and apatite that indicate derivation from a granitic continental crust. In contrast, 5 mainly rounded zircon grains (297 ± 5 Ma to 2126 ± 27 Ma) show positive εHf(t) (+0.7 to +13.5) and occasional apatite inclusions, suggesting their possible crystallization from melts derived from juvenile (mantle) sources. Interestingly, younger zircon grains are mainly euhedral to subhedral crystals, whereas older zircon grains are predominantly rounded grains. A comparison of the ages and Hf isotopic compositions of the zircon grains with those of nearby exposed crustal terranes suggest that chromitite zircon grains are similar to those reported from terranes of Mexico and northern South America. Hence, chromitite zircon grains are interpreted as sedimentary-derived xenocrystic grains that were delivered into the mantle wedge beneath the Greater Antilles intra-oceanic volcanic arc by metasomatic fluids/melts during subduction processes. Thus, continental crust recycling by subduction could explain all populations of old xenocrystic zircon in Cretaceous mantle-hosted chromitites from eastern Cuba ophiolite. We integrate the results of this study with petrological-thermomechanical modeling and existing geodynamic models to propose that ancient zircon xenocrysts, with a wide spectrum of ages and Hf isotopic compositions, can be transferred to the mantle wedge above subducting slabs by cold plumes.  相似文献   

20.
Hf‐isotope data of >1100 detrital zircon grains from the Palaeozoic, south‐central Andean Gondwana margin record the complete crustal evolution of South America, which was the predominant source. The oldest grains, with crustal residence ages of 3.8–4.0 Ga, are consistent with complete recycling of existing continental crust around 4 Ga. We confirm three major Archaean, Palaeoproterozoic (Transamazonian) and late Mesoproterozoic to early Neoproterozoic crust‐addition phases as well as six igneous phases during Proterozoic to Palaeozoic time involving mixing of juvenile and crustally reworked material. A late Mesoproterozoic to early Neoproterozoic, Grenville‐age igneous belt can be postulated along the palaeo‐margin of South America. This belt was the basement for later magmatic arcs and accreted allochthonous microcontinents as recorded by similar crustal residence ages. Crustal reworking likely dominated over juvenile addition during the Palaeozoic era, and Proterozoic and Archaean zircon was mainly crustally reworked from the eroding, thickened Ordovician Famatinian arc.  相似文献   

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