南阿尔金泥盆纪中基性杂岩体的成因及其地质意义研究     

张魁  刘良  王超  康磊  盖永升  廖小莹  马拓  赵国军 《岩石学报》2018,34(8):2481-2500

出露于南阿尔金西段的塔什萨依辉长岩和闪长岩及其内花岗质细脉是古生代多期岩浆活动的产物,它们构成了南阿尔金俯冲碰撞杂岩带的一部分,是深入探讨该地区构造演化过程的良好材料。本文通过对这些地质体野外地质特征、岩石学、地球化学特征、锆石U-Pb年代学和锆石Hf同位素特征的系统研究,以期确定其形成时代、源区性质和岩石成因,为深入探讨南阿尔金俯冲碰撞杂岩带的演化过程提供进一步约束。本文研究表明:辉长岩和闪长岩具相对较高的SiO_2含量(50.4%~53.5%)和Mg#(57~80),低的K_2O/Na_2O比值(0.17~0.67),为钙碱性系列岩石;辉长岩的∑REE偏低(36.9×10~(-6)~83.1×10~(-6)),Eu正异常(δEu=1.17~1.85);闪长岩∑REE稍高(182×10~(-6)~190×10~(-6)),Eu负异常(δEu=0.85~0.86);二者相对富集LREE和LILE,亏损HFSE。其主量元素特征、微量元素(高Nb、Zr含量,低Zr/Y比值)、锆石Hf同位素和Sr-Nd同位素组成表明二者应为大陆板内伸展背景下软流圈交代的岩石圈地幔部分熔融的产物,并在其岩浆演化过程中经历了地壳混染和分离结晶作用。花岗质细脉具高的Si O2含量(72.4%～75.5%)和K_2O/Na_2O比值(2.33～2.56),属于钾玄岩系列岩石;与闪长岩相比,两者微量元素蛛网图相似,但花岗质细脉轻重稀土分馏程度较大,Eu负异常(δEu=0.55～0.61)和P、Ti的亏损更加显著。锆石U-Pb定年结果显示,辉长岩形成时代约为400～420Ma;闪长岩和其内花岗质细脉的形成时代基本一致,约为400Ma,并具有相似的锆石Hf同位素组成和Sr-Nd同位素组成,结合地球化学特征及野外产状,推测花岗质细脉为闪长岩分异的产物。结合南阿尔金区域地质背景综合分析,塔什萨依辉长岩和闪长岩起源于造山后伸展背景下软流圈交代的岩石圈地幔的部分熔融,并经历了地壳混染和分离结晶作用;而闪长岩进一步分异形成花岗质细脉,并在其形成过程中可能伴随少量壳源熔融物质的加入。  相似文献   

柴达木盆地西北缘石英闪长岩的形成时代、岩石成因及地质意义     

辜平阳  陈锐明  查显锋  董增产  庄玉军  查方勇  李培庆 《岩石矿物学杂志》2018,37(1):19-33

柴达木盆地西北缘石英闪长岩Al2O3含量较高,全碱(Alk)含量较低,Na2OK2O,铝饱和指数A/CNK为0.87~0.91,属钙碱性准铝质岩石系列。球粒陨石标准化的稀土元素配分曲线表现为轻稀土元素富集型,轻、重稀土元素分馏明显,Eu弱负异常;微量元素地球化学特征显示,岩石富集Rb、Th、U等大离子亲石元素,亏损Nb、Ta、P、Ti等高场强元素,Nb/La和Rb/Nb比值较低,具有I型花岗岩的特征。石英闪长岩Ca O/Na2O比值较高(2.32~2.64),结合源岩判别图解综合推断其源于变玄武岩的部分熔融。全岩Zr饱和温度计算结果显示初始岩浆温度768℃;岩石地球化学特征表明岩浆源区压力1.5 Ga,源岩部分熔融的残留相可能为石榴子石+角闪石+金红石。经过锆石阴极发光分析和MC-LA-ICP-MS锆石U-Pb测年,获得206Pb/238Pb加权平均年龄为252±1 Ma,代表了柴达木盆地西北缘石英闪长岩的成岩年龄。结合区域地质演化特征,认为该岩体形成于与板块俯冲有关的火山弧构造环境,是晚二叠世末期宗务隆洋壳向柴北缘欧龙布鲁克地块俯冲,变玄武岩在相对较高的温压条件下发生部分熔融形成的。  相似文献   

Advances and Issues in Luminescence Dating of Loess Deposits in Arid Central Asia   总被引：1，自引：1，他引：0  

Leibin Wang  Haitao Wei  Jia Jia  Guoqiang Li  Fahu Chen 《地球科学进展》2018,33(1):93-102

High-resolution loess deposits are widely distributed in Arid Central Asia (ACA) and provide important records associated with dust transportation, paleoenvironmental and paleoclimatic evolution. The chronology is the foundation of the research into loess deposits as an environmental archive. In recent decades, the gradually developed optical dating method has been increasingly matured and become an important approach to establishing the loess-paleosol sequences. Here, we summarized and discussed previous work on loess chronology mainly based on optical dating approach in ACA. The following understandings have been listed: ① In comparison with optical dating method, the suitable material for ¹⁴C dating is uncommon in ACA. However, the dating range of luminescence dating is more extensive, and the dating materials are accessible. Thus, the optical dating is widely applicable in the establishment of loess framework in this area. ② Until now, the quartz Single Aliquot Regeneration (SAR) method can be applied to the establishment of loess-paleosol sequence since last glacial period. But several issues remain unaddressed. For example, the Optically Stimulated Luminescence (OSL) signal sensitivity of quartz grains are low in some areas. Furthermore, the results of OSL dating of different grain sizes within a single sample are inconsistent in some areas. The solution of these problems still requires more methodological research. ③ The post-IR IRSL (pIRIR) and multiple elevated temperature stimulation (MET-pIRIR) protoCols of feldspar have basically overcome the anomalous fading issue in the traditional IRSL dating process. In ACA, the framework since MIS 7 can be established with K-feldspar luminescence dating method. Compared with quartz luminescence characteristics, the K-feldspar luminescence signals are more sensitive and exhibit a high saturation level. In specific applications, it is necessary to establish the age frame according to the luminescence sensitivity, the age of samples or other factors.  相似文献   

安徽茶亭铜金矿床赋矿石英闪长玢岩黑云母成分特征及成岩成矿指示意义     

肖庆玲  周涛发  袁峰  王世伟  谢祖军  刘静 《矿床地质》2018,37(6):1179-1194

安徽宣城茶亭矿床位于长江中下游成矿带东南缘的南陵-宣城盆地内,是近年来该盆地内新发现的大型斑岩型Cu-Au矿床。石英闪长玢岩是茶亭矿床主要的赋矿岩石,文章从石英闪长玢岩的造岩矿物黑云母入手,利用EMPA及LA-ICP-MS等原位微区分析方法,对黑云母进行了详细的矿物化学分析,旨在查明赋矿石英闪长玢岩形成的物理化学条件,并探讨其成岩成矿意义。分析结果表明:茶亭赋矿石英闪长玢岩中黑云母具有高w(TiO_2)、低w(Al_2O_3)的特征,整体富Mg、贫Fe。黑云母温压计算结果表明,在不同深度上,石英闪长玢岩具有相似的结晶温度及压力,其结晶温度为746～773℃,压力为44～85 MPa,对应深度为1.7～3.3 km,平均为2.47 km,显示石英闪长玢岩侵位深度相对较浅。黑云母中高的氧化系数(0.613～0.864)、高Mg#(0.557～0.864),以及w(MgO)介于14.73%～15.86%,均显示石英闪长玢岩为壳幔混源,并且以幔源为主。黑云母成分显示石英闪长玢岩形成于较高氧逸度条件下。浅部岩体具有较高的X_(Mg)值,表明浅部岩体氧逸度较高,可能指示随着岩浆的不断演化,残余岩浆的氧逸度不断降低。同时,石英闪长玢岩黑云母相对一般斑岩型铜矿具有较高的w(Cu),并且高Cl、低F。这些特征均有利于茶亭Cu-Au矿床的形成。  相似文献   

柴北缘达达肯乌拉山地区闪长岩锆石LA-ICP-MSU-Pb年龄、岩石地球化学特征及其构造意义   总被引：1，自引：0，他引：1  

刘永乐  刘智刚  张爱奎  何书跃  张大明  毛生元  李兴良  奎明娟 《矿床地质》2018,37(5):1079-1090

达达肯乌拉山位于柴达木盆地北缘中东部,区内发育闪长岩体,以小岩株形式产出。通过对达达肯乌拉山闪长岩岩石LA-ICP-MS锆石U-Pb定年和地球化学特征的研究,获得闪长岩体的年龄为(240.5±1.7) Ma,属早印支期。闪长岩体的w(K_2O)较高,为2.03%～2.30%,w(Na2O)含量较低,为3.2%～3.44%,为一套准铝质及弱过铝质高K、低Na的高钾钙碱性型I型花岗岩。岩石稀土元素总量为158.35×10~(-6)～200.41×10~(-6),球粒陨石标准化曲线向右倾斜,重稀土元素曲线呈水平状,轻稀土元素富集,但负铕异常不明显,岩浆分异程度不高。岩石的La/Ta(54.32～68.51)、Sm/Nd(0.18～0.19)及Rb/Sr(0.11～0.19)比值特征反映该岩体岩浆具有壳幔混合的特点。通过构造判别,反映达达肯乌拉山岩体可能形成于俯冲陆壳断离、幔源岩浆底侵的地球动力学背景,在中央造山带早中生代统一的板块碰撞与挤压构造体制下,以滩间山蛇绿岩带为基础,发生陆壳俯冲和断离作用,并诱发幔源岩浆的底侵和下地壳物质的部分熔融,沿火山机构侵位形成达达肯乌拉山岩体。  相似文献   

大兴安岭扎兰屯地区晚奥陶世石英闪长岩体岩石地球化学特征及其地质意义   总被引：2，自引：0，他引：2  

马庆  刘建峰  迟效国 《地质通报》2018,37(5):853-862

扎兰屯音河岩体被音河水系分为南、北两部分,研究发现南、北岩体形成年代不同,选取南部岩体(称为二村岩体)进行研究。二村岩体主要由石英闪长岩-英云闪长岩组成,石英闪长岩的LA-ICP-MS锆石U-Pb年龄为444.0±4.6Ma,时代为晚奥陶世。岩石化学组成相对富钠、贫钾,Na2O/K2O值大于1(1.73~3.17),属中钾钙碱性系列。岩石富含轻稀土元素、亏损重稀土元素,富集大离子亲石元素Rb、Ba、K,显著亏损Nb、Ta、P、Ti等高场强元素。矿物组成及岩石地球化学特征指示其为I型花岗岩。岩体的形成时代、构造背景与多宝山岛弧火成岩相似,为区域多宝山岛弧西南向延伸提供了新的制约。  相似文献   

差应力与岩石熔融性状关系的实验研究   总被引：1，自引：0，他引：1  

董春艳  马瑞  迟效国  刘建峰  黎广荣 《吉林大学学报(地球科学版)》2006,36(2):177-182

为考察不同应力状态下岩石应变与岩石熔融作用的关系,利用英国Instron公司生产的电液伺服实验系统,配以围压和加温系统设计了动、静态不同条件下细粒闪长岩的对比熔融实验,力图找到差应力与岩石熔融程度及其熔体成分的关系.通过岩石动、静态熔融实验结果的对比得出:差应力的存在能够导致细粒闪长岩的熔融,随着差应力(应变速率)的增加,熔体的量增加,熔体成分向富Si、Al方向转变.  相似文献   

Luminescence and ESR dating of the sedimentary infill from the multi-level cave system of Alkerdi-Zelaieta (Navarre,N Spain)     

《Quaternary Geochronology》2022

The finding of Upper Paleolithic engravings in 2016 triggered a multidisciplinary investigation of the Alkerdi cave system (Urdazubi, N Spain). The study of the speleogenetic processes led to the identification of at least 6 paragenetic cave levels with associated sedimentary infill. In order to unravel the timing of changes in the karst dynamics and to get some insights about sediment origin, two sediment samples were collected from cave levels 4 and 1 for numerical dating purpose, using both Optically Stimulated Luminescence (OSL) and Electron Spin Resonance (ESR) methods. One additional modern-age sample was also taken from the entrance of the karst to evaluate the magnitude of the optical bleaching achieved by the quartz grains before entering the cave system. Last, one sample was collected from a flowstone for U-series dating, providing independent age control.OSL measurements were carried out using small quartz multi-grain (MG) and single-grain (SG) Single Aliquot Regenerative-dose (SAR) protocol. Initial Equivalent Dose (D_e) results show evidence of saturated OSL signal for the sample of the higher level (with ∼60% of saturated aliquots). Unlike SA data, SG analyses do not meet the usual quality criteria (e.g., relatively high recuperation ratios, only a few grains with useable signal), suggesting that corresponding dating results should be treated with caution.Hence, both MG and SG TT-OSL and MG ESR methods were subsequently employed, as the corresponding signals are known to have higher saturation levels than OSL ones. ESR analyses were based on the Multiple Centre (MC) approach using the standard multi-grain multi-aliquot additive (MAA) dose method, while TT-OSL measurements were performed following Demuro et al. (2020). The latter, however, did not return any useful results for both samples. MC ESR data show the usual D_e pattern (D_e(Al)>D_e(Ti op. D)>D_e(Ti–H)) indicating that among the three ESR signals analyzed, the Ti–H most likely provides the closest estimate to the true burial age. However, low measurement repeatability and goodness-of-of fit indicate that the reliability of the ESR results may be reasonably questioned.Results derived from this multi-technique dating approach provide the first chronological constraints for the sedimentary infill of the Alkerdi cave system. In particular, they suggest that sediment deposition in Cave Level 4 (ALK-OSL01) occurred around 130 ka, which is in good agreement with the minimum age constraint given by the speleothem (80.5 ± 9.0 ka). In comparison, the young age obtained for sample ALK-OSL02 (5.0 ± 0.9 ka) suggests recent Holocene formation of the lowest cave level 1.Finally, the MG De value obtained for the modern sample is close to zero (<1 Gy), indicating that the OSL signal is almost fully reset at a multi-grain level before entering the cave. Additionally, despite the large De overdispersion measured in this modern sample, the De values are one to two order of magnitude lower than those obtained with the same model in the other two samples. Therefore, the large OSL D_e overdispersion (OD) values of up to 64% obtained for the two samples from Cave Level 4 and 1 are most likely related to re-sedimentation processes inside the cave system.  相似文献   

Variations in the sensitivity of the optically stimulated luminescence from quartz in the Xifeng section: A spatiotemporal comparison across the Chinese Loess Plateau since the last interglaciation     

《Quaternary Geochronology》2022

The sensitivity of the optically stimulated luminescence (OSL) from quartz is thought to be mainly influenced by source rock (crystallization temperature and quartz defect types) and depositional history (irradiation/bleaching cycles). In this study, the OSL sensitivity of quartz of different grain sizes from loess (L1) and paleosol (S1) layers at the Xifeng section of the Chinese Loess Plateau was analyzed. The OSL sensitivity of the samples from the Xifeng section shows a distinct difference between glacial and interglacial cycles, which is consistent with the patterns observed from magnetic susceptibility (MS) and grain sizes. The highest OSL sensitivity is observed in S1, which is twelve times the lowest sensitivity observed in L1. Moreover, the contribution of the fast component of quartz OSL from the paleosol accounts for more than 90% of the total OSL signal. In contrast, the middle and slow components contribute more in loess, and a significant variation among different aliquots was observed.Comparison of the data obtained from loess sections from different regions, including Xifeng, Luochuan, Jingyuan and Shimao, show significant differences in the magnitudes of OSL sensitivity but a similar pattern between glacial and interglacial periods. The results of this study suggest that, except for the wildfire model proposed to interpret the high OSL sensitivity in paleosol (Zhang, 2018), the shift of wind pattern of westerly wind (i.e., transporting “dim” source from North Tibetan Plateau and northwesterly wind (i.e., transporting “bright” source from Alxa Arid Lands and the subsequent mixture from the different sources may partially contribute to the different OSL sensitivities observed for Xifeng and Luochuan. In contrast, the OSL sensitivity of Shimao samples from L1 was affected by the input from the Mu Us Desert, and those of Jingyuan may affected by the contribution from the Yellow River.  相似文献   

Revisiting natural and laboratory electron spin resonance (ESR) dose response curves of quartz from Chinese loess     

《Quaternary Geochronology》2022

Natural and laboratory ESR dose response curves (DRCs) of [AlO₄/h]⁰ and [TiO₄/M⁺]⁰ were investigated for samples of quartz from the Luochuan loess-palaeosol master section, Chinese Loess Plateau. The natural and laboratory DRCs show a clear divergence above ∼1000 Gy, with much lower D₀ values and saturation levels observed for the natural DRCs, which is in agreement with the previous study by Tsukamoto et al. (2018). Young (<15 ka) samples from Luochuan and Jingbian – another site of the Chinese Loess Plateau, together with two modern samples of Chinese loess, were used to investigate the residual signals of [AlO₄/h]⁰ and [TiO₄/M⁺]⁰ centres. Our results are in line with published studies and show that the significant residual signals corresponding to several tens to hundreds of Gy are present in both Al and Ti centres. These need to be taken into account before laboratory DRC construction. ESR pulse annealing experiments performed on samples irradiated with different doses show an apparent dose-dependent thermal instability of [AlO₄/h]⁰ and [TiO₄/M⁺]⁰, with the signals for higher doses decaying faster with increasing temperature. We attribute the change in D₀ with preheat reported in Tsukamoto et al.2018, as well as the difference between laboratory and natural DRCs, to this apparent dose-dependent thermal instability of the signals. The saturation level of the natural DRC, being the result of reaching the equilibrium between filling of the traps and emptying them due to thermal decay, is therefore additionally affected at higher doses, due to the increased thermal instability. The inability to recreate in the laboratory the same response to irradiation as the one observed in nature questions the accuracy of dating samples beyond ∼1000 Gy.  相似文献