内蒙古达茂旗花岗岩类LA-ICP-MS 锆石U-Pb年龄及其地质意义   总被引：2，自引：1，他引：1  

冯丽霞  张志诚  韩宝福  任荣  李建锋  苏犁 《地质通报》2013,32(11):1737-1748

对内蒙古达茂旗北部构造单元的巴特敖包岛弧带2个花岗闪长岩岩体样品和南部构造单元一个花岗岩岩体的2件样品进行了LA-ICP-MS锆石U-Pb定年。北部构造单元采自2个花岗闪长岩岩体的样品锆石206Pb/238U年龄分别为468Ma±2Ma和452Ma±3Ma,代表了这2个岩体的侵位时间,表明古亚洲洋向华北克拉通之下俯冲不晚于468Ma±2Ma;南部构造单元采自同一花岗岩岩体的2件样品获得的锆石206Pb/238U年龄分别为268Ma±2Ma和264Ma±2Ma,和该单元西部岩体已有的锆石年龄相符。这为华北克拉通北缘岩浆作用研究提供了新的年代学证据。  相似文献   

北美内陆西部白垩纪脊椎动物生物年代学   总被引：1，自引：1，他引：0  

Spencer G.LUCAS  Robert M.SULLIVAN  Justin A.SPIELMANN 《地层学杂志》2012,(2):436-461

北美西部内陆白垩纪的脊椎动物生物年代学的研究始于19世纪90年代。前人建议的期,即陆生脊椎动物"期"或陆生哺乳动物"期"名已过十二个,但其中具有精确的定义者甚少,仅有少量的建议受到广泛认可和使用。本文定义或重新定义了10个陆生脊椎动物"期",包括了西部内陆从最老至最新的全部白垩纪—Comobluffian期(～提塘期至欧特里沃期)、Buffalogapian期(～巴列姆期至早阿普特期)、Cashenranchian期(～早阿普特期至晚阿尔布期)、Mussentuchian期(～晚阿尔布期至塞诺曼期)、Fencelakean期(土伦期至晚塞农期)、Aquilan期(～晚塞农期至早坎潘期)、Judithian期(～中坎潘期)、Kirtlandian期(～晚坎潘期)、Edmontonian期(～坎潘期末期至早马斯特里赫特期)以及Lancian期(～早马斯特里赫特期晚期)。每一个"期"的开始由一种恐龙或哺乳动物种类的首现来定义,而其结束由后续的"期"的开始来定义。这样定义的脊椎动物生物年代代表了完整的白垩纪时间表。但有些时间段(尤其是Neocomian(尼欧克姆期)的大部分以及部分"中"白垩世的一部分)缺乏足够的脊椎动物化石特征。这些白垩纪陆生脊椎动物"期"构成了一个能使北美西部内陆的脊椎动物的演化历史得以序和解释年代表。  相似文献   

东准噶尔北缘老山口铁铜金矿区侵入岩LA-ICP-MS锆石U-Pb定年及地质意义   总被引：13，自引：0，他引：13  

吕书君  杨富全  柴凤梅  张希兵  姜丽萍  刘锋  张志欣  耿新霞  欧阳刘进 《地质论评》2012,58(1):149-164

老山口铁铜金矿区位于准噶尔北缘的喀拉通克—卡拉先格尔成矿带南段,矿化与岩浆侵入活动有关。本文利用LA-ICP-MS锆石U-Pb定年方法对老山口铁铜金矿区的中粒闪长岩、正长岩、黑云母闪长岩和闪长玢岩进行了年代学研究,获得其年龄分别为353.8±1.9Ma、366.3±1.9Ma、3±2.3Ma和379.7±3Ma,表明矿区存在三期岩浆活动。其中黑云母闪长岩和闪长玢岩的年龄,在误差范围内一致,它们可能为中泥盆世同源岩浆演化的产物,且岩体侵入时代与准噶尔洋俯冲阶段花岗岩及卡拉先格尔斑岩铜矿带含矿斑岩年龄较一致,表明其可能是板块俯冲阶段的产物。闪长岩和正长岩的年龄分别为353.8±1.9Ma和366.3±1.9Ma,与东准噶尔北部青格里河下游一带后碰撞花岗岩类和布尔根一带后造山伸展A型花岗岩的年龄接近,而地球化学特征却存在差异,说明老山口正长岩和闪长岩体是俯冲晚期阶段的产物。根据地质特征,老山口铁铜金矿的形成与闪长岩及闪长玢岩侵入有关,因此岩体年龄也限定了矿区存在两期铁铜金矿化,即379Ma左右和354Ma左右。  相似文献   

Early Cretaceous A-type granites and Mo mineralization,Aershan area,eastern Inner Mongolia,Northeast China: geochemical and isotopic constraints     

《International Geology Review》2012,54(11):1357-1376

The Jiazishan porphyry-type molybdenum deposit is located in the eastern Inner Mongolia Autonomous Region in China. Mineralization occurs mainly as veins, lenses, and layers within the host porphyry. To better understand the link between mineralization and host igneous rocks, we studied samples from underground workings and report new SHRIMP II zircon U–Pb and Re–Os molybdenite ages, and geochemical data from both the molybdenites and the porphyry granites. Seven molybdenite samples yield a Re–Os isochron weighted mean age of 135.4 ± 2.1 Ma, whereas the porphyry granite samples yield crystallization ages of 139 ± 1.5 Ma (Jiazishan deposit) and 133 ± 1 Ma (Taolaituo deposit). The U–Pb and Re–Os ages are similar, suggesting that the mineralization is genetically related to Early Cretaceous porphyry emplacement. Re contents of the molybdenite range from 21.74 ppm to 52.08 ppm, with an average of 35.92 ppm, whereas δ³⁴ S values of the sulphide vary from 1.3‰ to 4.2‰. The ores have ²⁰⁶Pb/²⁰⁴Pb, ²⁰⁷Pb/²⁰⁴Pb, and ²⁰⁸Pb/²⁰⁴Pb ratios of 18.178–18.385, 15.503–15.613, and 37.979–38.382, respectively. We also obtained a weighted mean U–Pb zircon age of 294.2 ± 2.1 Ma for the oldest granite in Jiazishan area. All granites are A-type granites. These observations indicate that the molybdenites and the porphyry granites were derived from a mixed source involving young accretionary materials and enriched subcontinental lithospheric mantle. A synthesis of geochronological and geological data reveals that porphyry emplacement and Mo mineralization in the Jiazishan deposit occurred contemporaneously with Early Cretaceous tectonothermal events associated with lithospheric thinning, which was caused by delamination and subsequent upwelling of the asthenosphere associated with intra-continental extension in Northeast China.  相似文献   

Constraints on the onset age of the Sturtian glaciation from the Southeast Yangtze Block,South China     

《International Geology Review》2012,54(15):1876-1886

ABSTRACT

The Neoproterozoic glaciations represent a milestone in the Earth evolution due to their influence on atmosphere, biosphere and hydrosphere. Evidence for the Sturtian glaciation, the early stage of Cryogenian, has been recorded worldwide, but the precise timing and synchroneity of its counterpart, the Chang’an glaciation, in South China have been controversial. As such, new zircon U–Pb ages from the pre-Sturtian Gongdong Formation and the overlying the Chang’an Formation in southeastern Yangtze Block were reported. The youngest U–Pb zircon age from a tuff sample of the topmost Gongdong Formation was 716.8 ± 6.8 Ma, and that from a sandstone sample of the lower Chang’an Formation was 725.9 ± 4.4 Ma. The zircon weighted mean age of 716.8 ± 6.8 Ma was interpreted as the maximum depositional age of the termination of the Danzhou Group. This age, along with the ages reported from the bottom of the Danzhou Group, constrains deposition of the Danzhou Group to between ca. 820 Ma and ca. 715 Ma. The age of 716.8 ± 6.8 Ma from the top of the Gongdong Formation is consistent with the SIMS U-Pb age of 715.9 ± 2.8 Ma from the Sibao section, as well as ages from the Banxi Group, Liantuo Group, and Kaijianqiao Formation in the Yangtze Block, which further constrain the onset time of the Sturtian glaciation in South China at ca. 715 Ma. It is also, with uncertainties, consistent with ages from pre-Sturtian strata in Laurentia and Oman, which indicates a global synchroneity and extent for the Sturtian glaciation.  相似文献   

Late Palaeozoic 40Ar/39Ar ages of the HP-LT metamorphic rocks from the Kekesu Valley,Chinese southwestern Tianshan: new constraints on exhumation tectonics     

《International Geology Review》2012,54(4):389-404

abstract

Although numerous ages have been obtained for the Chinese southwestern Tianshan high pressure/ultrahigh pressure-low temperature (HP/UHP-LT) metamorphic belt in the past two decades, its exhumation history is still controversial. The poor age constraint was related to the appealing low metamorphic temperatures and excess Ar commonly present under HP/UHP conditions. This study aims to provide new age constraints on the orogen’s exhumation by obtaining ⁴⁰Ar/³⁹Ar mica ages using the conventional step-heating technique, with emphasis on the avoidance of excess Ar contamination. From a cross section along the Kekesu Valley, four samples, three from the HP-LT metamorphic belt (TK050, TK051, and TK081) and one from the southern margin of the low pressure metamorphic belt (TK097), were selected for ⁴⁰Ar/³⁹Ar dating. Phengites from garnet glaucophane schist TK050 and the surrounding rock garnet phengite schist TK051 yield comparable plateau ages of 321.4 ± 1.6 and 318.6 ± 1.6 Ma, respectively, while epidote mica schist TK081 gives a younger plateau age of 293.3 ± 1.5 Ma. Considering the chemical compositions of phengites, mineral assemblages, and microstructures in the thin slices, we suppose that the former represents the time the HP rocks retrograded from the peak stage (eclogite facies) to the (epidote)-blueschist facies, whereas the latter reflects greenschist facies overprinting. Biotite and muscovite from two-mica quartzite TK097 give similar plateau ages of 253.0 ± 1.3 and 247.1 ± 1.2 Ma, interpreted to date movement on the post collisional transcrustal South Nalati ductile shear zone. By combining our new ages with published data, a two-stage exhumation model is suggested for the Chinese southwestern Tianshan HP/UHP-LT metamorphic belt: initial fast exhumation to a depth of about 30–35 km by ~320 Ma was followed by relatively slow (~1 mm year^–1) uplift to ~10 km by ~293 Ma.  相似文献   

麻山杂岩的两种变质作用及其与花岗岩的关系   总被引：2，自引：1，他引：1  

任留东  王彦斌  杨崇辉  赵子然  郭进京  高洪林 《岩石学报》2012,28(9):2855-2865

在黑龙江佳木斯地块麻山杂岩中识别出麻山杂岩中具有两种类型的变质作用:早期局部的麻粒岩相变质作用(M1)和伴随的无水深熔作用(>530Ma),即狭义的麻山群高级变质作用,变质岩多以残留块体形式散布于后期混合岩或花岗岩之中;麻粒岩相变质之后由于广泛的岩浆活动,造成了强烈的混合岩化作用(500Ma)和相应大范围的晚期角闪岩相变质作用(M2)。角闪岩相和麻粒岩相变质并非带状递进变化,而是在时空上均有差异的两种变质作用。混合岩化过程中的富水流体对早期"干"岩石进行了明显的退变质改造,从而造成高级变质岩变质结构的复杂性。此外,含水花岗岩的侵位对先期麻粒岩相变质成因锆石同位素体系有重置作用,使得早期的变质年龄难以测定。麻山杂岩的变质-花岗岩关系与东南极普里兹带有类似之处,在变形-变质之后迅速发生了构造体系的转换,出现了新的岩浆活动,只是花岗岩发育强度有所不同,反映了两地构造演化细节上的差异。西伯利亚古陆南缘及中亚造山带内部的一些微陆块发生了与冈瓦纳陆块内泛非事件类似的构造-热-岩浆事件,因此,中亚造山带内部的佳木斯地块及其他类似的微陆块与冈瓦纳古陆边缘活动带具有相似的构造性质。  相似文献   

Lack of relationship between Al ages of chondrules and their mineralogical and chemical compositions     

Johan Villeneuve  Marc Chaussidon  Guy Libourel 《Comptes Rendus Geoscience》2012,344(9):423-431

Previous studies have suggested the existence of a correlation between ²⁶Al relative crystallisation ages and mineralogical and bulk chemical compositions of ferromagnesian chondrules from the Bishunpur and Semarkona unequilibrated ordinary (0120 and 0150). However, because the precision in ²⁶Al ages was moderate, these correlations are questionable. Here, we report mineralogical and chemical compositions of 14 ferromagnesian chondrules from Semarkona for which precise ²⁶Al ages were previously obtained (Villeneuve et al., 2009). We find global correlation of ²⁶Al ages neither with bulk chemical composition of chondrules, nor with the different types of ferromagnesian chondrules, i.e. PO, POP and PP. This indicates that if some kind of correlations between chemical compositions of chondrules and their ages of formation exists, they do not exist at timescales that can be measured with the ²⁶Al-²⁶Mg systematics but presumably at much shorter timescales.  相似文献   

西秦岭造山带北缘大草滩群物源研究——LA-ICP-MS碎屑锆石U-Pb年龄证据     

吴树宽  裴先治  李佐臣  李瑞保  裴磊  陈有炘  高景民  刘成军  魏方辉  王银川 《地质通报》2012,31(9):1469-1481

选取甘肃东部西秦岭造山带北缘晚泥盆世大草滩群碎屑岩为研究对象,运用LA-ICP-MS锆石U-Pb同位素年代学方法,探讨大草滩群的物质来源。结果表明,大草滩群碎屑锆石年龄谱明显分为4组:422～518Ma、756～887Ma、1100～1231Ma和2417～2736Ma。其中,422～518Ma的年龄数据约占总体的67%,所占比例最大,年龄相对集中,且呈现出最强烈的峰值,其余年龄段所占比例则较少。422～518Ma年龄组分指示其物源可能以邻近地区的西秦岭北缘构造带和北祁连造山带为主,该组分年龄是加里东期中南祁连和西秦岭微地块分别向北俯冲、碰撞产生的一系列火成岩在造山剥蚀后的沉积响应。碎屑锆石同位素年龄中756～887Ma年龄组分反映其物源可能来自祁连造山带和西秦岭北缘构造带。1100～1231Ma年龄组分反映其物源可能主要来自祁连造山带。2417～2736Ma年龄组分反映了物源来自北祁连造山带和西秦岭北缘构造带的结晶基底,部分物源也有可能来自于华北板块基底。综合分析显示,大草滩群碎屑沉积物质来源较为复杂,具有明显的多元性,存在西秦岭北缘构造带、祁连造山带和华北板块基底3个物源区,祁连造山带和西秦岭北缘构造带对大草滩群的沉积有重大的物源贡献。两者相比较,祁连造山带应为大草滩群最主要的物源区。  相似文献   

On the Characteristic and Dynamic Ages of Pulsars     

T. G. Mdzinarishvili  G. I. Melikidze  R. M. Dzigvashvili 《Astrophysics》2004,47(1):29-36

A method that is independent of the model for the distribution of free electrons in the galaxy is proposed for revealing possible oscillations of pulsars in the direction perpendicular to the galactic plane. Oscillations of pulsars in this direction with a half period of approximately 10⁸ years on the scale of characteristic ages are found by this method, which is independent of the distance scale.  相似文献