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101.
内蒙古中部四子王旗地区晚二叠-早三叠世过铝花岗岩定年及成因 总被引:4,自引:1,他引:3
研究区位于华北板块北缘中段,紧邻兴蒙造山带,是研究古生代—中生代地壳增生演化的重要地区。本文对区内三个花岗岩体进行了锆石LA-ICP-MSU-Pb定年及岩石地球化学研究。结果表明阿玛乌苏花岗闪长岩形成于267±9Ma(MSWD=9.7);布龙二长花岗岩和格尔图白云母正长花岗岩分别侵位于239±4Ma和238±6Ma(MSWD=0.91);而侵入格尔图白云母正长花岗岩的白云母二长花岗岩脉则获得了224±8Ma(MSWD=5.7)的侵位年龄。岩石地球化学特征显示阿玛乌苏花岗闪长岩为岩浆混合成因,暗示大规模岩浆底侵作用的存在;格尔图白云母正长花岗岩具明显的稀土元素"四分组"效应,是分异岩浆与流体作用的结果,可能经历一定程度的地壳混染,非真正意义上的S型花岗岩,属于造山后岩浆热事件,应代表造山的结束。格尔图白云母正长花岗岩及白云母二长花岗岩脉均受到热液流体作用,说明在中三叠世(224~238Ma),区内一直存在有大量的热液流体活动,且热液流体可能富含F和Cl,区内产出的大规模的萤石矿是否为该期流体活动的产物尚需进一步工作。 相似文献
102.
新疆贝勒库都克A型花岗岩锆石U-Pb年龄、地球化学及锡成矿 总被引:1,自引:0,他引:1
新疆东准噶尔卡拉麦里地区是一个重要的锡成矿带,分布有多种类型花岗岩。贝勒库都克岩体位于锡成矿带中部,由黑云母正长花岗岩和黑云母二长花岗岩组成。本文通过精确的LA-ICP-MS锆石U-Pb测年获得贝勒库都克含锡黑云母正长花岗岩年龄为283±2Ma,MSWD=0.14(95%置信度),时代属于早二叠世,这与东准噶尔后碰撞深成岩浆活动的范围(330~265Ma)相吻合。岩石地球化学研究表明,贝勒库都克岩体富硅(SiO2=75.25%~76.67%),低铝(Al2O3=11.91%~12.86%),贫镁(MgO=0.02%~0.18%)和钙(CaO=0.39%~0.89%),富碱(Na2O+K2O=8.08%~8.97%),K2O>Na2O,NK/A=0.86~0.95(平均0.92),A/NCK=0.97~1.02,富集Rb、K等大离子亲石元素及Zr、Hf等高场强元素,Ba,Nb,Sr强烈亏损,δEu=0.01~0.11,其FeOt/MgO(12.71~84.51,平均34.55)和10000Ga/A1(2.97~4.20)值大,HFSE元素(Zr+Nb+Ce+Y=191.8×10-6~353.3×10-6)含量高,明显不同于典型的I型和S型花岗岩,基本属于典型的铝质A型花岗岩。年代学和地球化学综合研究表明,贝勒库都克铝质A型花岗岩是壳幔混合成因,是准噶尔地区后碰撞幔源岩浆底侵作用导致大陆地壳垂向生长过程的记录者。贝勒库都克铝质A型花岗岩Sn的含量高(6.0×10-6~19.5×10-6,个别为80.0×10-6),铝质A型花岗岩是成矿热液的直接母体,而富Sn的流体相最终形成了贝勒库都克锡矿床,锡矿与铝质A型花岗岩是同期地质事件的产物。 相似文献
103.
为了弄清楚勉略构造带中三岔子岛弧火山岩的形成时代及源区特征,对南秦岭勉略缝合带三岔子岛弧蛇绿混杂岩中的辉绿岩墙样品进行了锆石U—PB年代学、锆石Hf同位素组成及微量元素组成研究。结果表明,三岔子辉绿岩中的锆石主要包括2个年龄区间:有8颗锆石记录古生代年龄信息,其n(205Pb)/n(238u)年龄为264~487Ma,Ⅷ(Th)/w(U)为0.4~0.8,其中有6颗锆石的N(176Hf)/N(177Hf)初始值为0.281934~0.282292,埘应的EHf(f)值为9.4~-16.4,为典型的壳源岩浆锆石,另外2个测点(BQG-014,BQG-021)的N(176Hf)/N(177Hf)为0.282722~0.282798,对应的εHf(f)值为4.5~6.3,为典型的幔源岩浆锆石;有15颗锆石记录厂元古代-太古代的年龄信息,N(207Pb)/N(206Pb)年龄主要为1713~2559Ma,N(176Hf)/N(177Hf)初始值为0.281288~0.282263,对应的εHf(t)值为-1.3~8.7,绝大部分锆石的εHf(t)值大于2,显示出幔源岩浆锆行的特征。根据锆石Hf同位素组成,BQG-014和BQG-021样品为典型的幔源岩浆锆石,因此,其形成年龄(264~295Ma)应代表了勉略洋消减过程中一次重要的大陆弧岩浆作用时间。 相似文献
104.
The Epupa Metamorphic Complex constitutes the southwestern margin of the Congo Craton and is exposed in a hilly to mountainous terrain of northwestern Namibia, bordering the Kunene River and extending into southern Angola. It consists predominantly of granitoid gneisses which are migmatized over large areas. This migmatization locally led to anatexis and produced crustal-melt granites such as the Otjitanda Granite. We have undertaken reconnaissance geochemical studies and single zircon U–Pb SHRIMP and Pb–Pb evaporation dating of rocks of the Epupa Complex. The granitoid gneisses, migmatites and anatectic melts are similar in composition and constitute a suite of metaluminous to peraluminous, calc-alkaline granitoids, predominantly with volcanic arc geochemical signatures. The zircon protolith ages for the orthogneisses range from 1861 ± 3 to 1758 ± 3 Ma. Anatexis in the migmatitic Epupa gneisses was dated from a melt patch at 1762 ± 4 Ma, and the anatectic Otjitanda Granite has a zircon age of 1757 ± 4 Ma. Migmatization and anatexis therefore occurred almost immediately after granitoid emplacement and date a widespread high-temperature Palaeoproterozoic event at ∼1760 Ma which has not been recorded elswhere in northern Namibia. The Nd isotopic systematics of all dated samples are surprisingly similar and suggest formation of the protolith from a source region that probably separated from the depleted mantle about 2.4–2.0 Ga ago. A major Archaean component in the source area is unlikely. 相似文献
105.
In 1973 Bill Compston advocated the building of an ion microprobe at the Research School of Earth Sciences (RSES) at the Australian National University (ANU). The commercial ion probes available at this time were too small to have sufficient sensitivity for trace element analysis and too low in mass resolution to avoid molecular interferences. The project commenced in 1974 with the appointment of a former ANU PhD student Steve Clement who had expertise in beam transport theory. To achieve high sensitivity and high mass resolution, beam transport theory indicated that a much larger magnet than in any commercially available mass spectrometer would be required. Clement chose an ion optical design, by Professor Matsuda of Osaka University in 1974, which had the required combination of high mass resolution and high transmission. Clement's job was to produce the detailed scientific designs and machine drawings for the new instrument as well as testing the completed instrument. Clement coined the term SHRIMP-Sensitive High Resolution Ion MicroProbe. By the end of 1977 nearly all the components had been manufactured and the big electromagnet had been successfully tested. In the following year the secondary mass analyzer was assembled and tested using a thermal ionization source and showed great promise with flat-topped peaks at 5000 resolution and 50% transmission with 50 V energy spread. At this stage the machine had far exceeded the specifications for the available commercial ion probes. Continued development during 1981 to the point where the original design specifications were fully realized was time consuming since learning how to use the entirely novel instrument was no simple task; no one else had an instrument like SHRIMP. The application of the instrument to zircon U–Pb geochronology established the necessary operating conditions for measuring Pb isotopic compositions and the elemental ratios Pb/U and U/Zr from 20 μm diameter spots on single zircon grains. Application of this in the early 1980s started a revolution in Precambrian geology by the ability to produce rapidly accurate and precise age determinations on structurally complex zircon samples. 相似文献
106.
Tracing the 850-Ma continental flood basalts from a piece of subducted continental crust in the North Qaidam UHPM belt,NW China 总被引:10,自引:0,他引:10
A Paleozoic ultrahigh-pressure metamorphic (UHPM) belt extends along the northern margin of the Qaidam Basin, North Tibetan Plateau. Eclogites in the Yuka eclogite terrane, northwest part of this UHPM belt, occur as blocks or layers of varying size intercalated with granitic and pelitic gneisses. These eclogites have protoliths geochemically similar to enriched-type mid-ocean ridge basalts (E-MORB) and oceanic island basalts (OIB). On the basis of Ti/Y ratios, they can be divided into low-Ti and high-Ti groups. The low-Ti group (LTG) eclogites exhibit relatively low TiO2 (most <2.5 wt%) and Ti/Y (<500) but comparatively high Mg# (48–55), whereas the high-Ti group (HTG) eclogites have high TiO2 (most >2.5 wt%) and Ti/Y (>500) but lower Mg# (46–52). Zircons from two eclogite samples gave a magmatic crystallization (protolith) age of ∼850 Ma and a UHPM age of ∼433 Ma. The occurrence, geochemical features and age data of the Yuka eclogites suggest that their protoliths are segments of continental flood basalts (CFBs) with a mantle plume origin, similar to most typical CFBs. Our observation, together with the tectonic history and regional geologic context, lend support for the large scale onset of mantle plume within the Rodinia supercontinent at ∼850 Ma. The Qaidam block is probably one of the fragments of the Rodinia supercontinent with a volcanic-rifted passive margin. The latter may have been dragged to mantle depths by its subducting leading edge of the oceanic lithosphere in the Early Paleozoic. 相似文献
107.
Combined U–Pb and Lu–Hf isotope analyses of detrital zircon grains from the auriferous Eldorado Reef conglomerate, upper Central Rand Group, reveal new insights into the provenance of the sediments and thus, by implication, possibly also into that of the gold. Most of the detrital zircon grains, which are of magmatic origin, yielded Mesoarchaean ages clustering around 2.94 and 3.06 Ga. A subordinate zircon population gave ages with maxima at 3.28 and 3.44 Ga. The Mesoarchaean zircon grains mostly show super-chondritic ?Hft of up to +5.2, whereas the Palaeoarchaean zircon grains have nearly chondritic composition with ?Hft between −1.3 and +2.0. The new dataset of the Mesoarchaean zircon populations provides the first unambiguous evidence of the formation of juvenile crust not only at 3.06 but also at 2.94 Ga. As the analysed zircon grains are from the ruditic fraction, they must be derived from a comparatively proximal source in close vicinity to the Central Rand Basin. Based on currently available data, this source was most likely a magmatic arc that existed at the northern edge of the Witwatersrand Block at 3.06 Ga. An additional source might be the 2.94 Ga magmatic rocks of the Kraaipan Greenstone Belt that occurs to the west of the Witwatersrand Block. The minor fraction of Palaeoarchaean zircon grains in the Eldorado Reef perhaps stem from sources that are isotopically similar to the Barberton Greenstone Belt and the Limpopo Belt but were more proximal to the Central Rand Basin. 相似文献
108.
东天山星星峡缝合带早古生代强过铝质花岗岩的研究及其地质意义 总被引:1,自引:0,他引:1
铅炉子过铝质花岗岩带发育于中天山岛弧带南缘的星星峡缝合带内,为一长条形的二云母花岗岩。岩体地球化学特征是高Si、Al和K,低Mg、Fe的组份,全碱含量中等,σ=1.74~1.9,K_2ONa_2O,A/CNK1.1,属于高钾钙碱性过铝质花岗岩类(SP)。岩体的CaO/Na_2O和Al_2O_3/TiO_2比值都相对较低,分别为(0.06~0.07)和(48.9~55.3);REE、Nb、Y含量和Rb/Sr、Rb/Ba比值相对较高;Rb、Th和LREE相对富集,Ba、Si、Eu、Ti、P和HREE相对亏损;ε_(HF)(t)=-2.3~+1.6表明岩体还具有较高的锆石同位素特征,T_(2DM)变化范围为1573~1329 Ma。这些地质学和地球化学研究表明铅炉子二云母花岗岩形成于后碰撞的伸展环境中,是在高温、中低压条件下发生重熔形成的,其源岩为古老的地壳物质和年轻的增生物质通过物理风化作用形成泥质岩。本文通过测年获得二云母花岗岩锆石LA-ICPMS年龄为444.5±2.2 Ma,表明铅炉子过铝质花岗岩形成于晚奥陶世,是中天山岛弧带和公婆泉岛弧带的碰撞时间的上限,它也是中天山岛弧带与公婆泉岛弧带碰撞造山作用的产物,是中亚增生造山带的增生方式之一。 相似文献
109.
宁芜盆地火山-次火山岩的锆石U-Pb年龄、Hf同位素组成及其地质意义 总被引:40,自引:23,他引:17
宁芜火山盆地是长江中下游重要的火山盆地之一,在盆地内自下而上依次发育龙王山组、大王山组、姑山组和娘娘山组火山岩和若干个同源次火山岩或小侵入岩体。本文对宁芜盆地火山-次火山岩进行了详细的锆石U-Pb年龄和Hf同位素地球化学研究。研究结果表明,大王山组粗安岩锆石U-Pb年龄为130.3±0.9Ma,姑山组两个粗安岩锆石U-Pb年龄分别为128.2±1.3Ma和128.5±1.8Ma,另外三个侵入岩年龄分别为127.1±1.2Ma、128.3±0.6Ma和128.2±1.0Ma,均为早白垩纪。综合前人成果,认为长江中下游地区火山盆地内火山活动的时限在135~124Ma之间,不存在侏罗纪岩浆活动。宁芜盆地火山岩和侵入岩的锆石176Hf/177Hf值在0.282502~0.282673范围内,εHf(t)变化为-6.9~-0.7,显示岩浆源自于岩石圈富集地幔部分熔融并在上升过程中受地壳物质的混染,为岩石圈伸展环境的产物。 相似文献
110.
赣南地区石雷石英闪长岩的成因:岩石化学、副矿物微量元素、锆石U-Pb年代学与Sr-Nd-Hf同位素制约 总被引:5,自引:2,他引:3
石雷石英闪长岩是赣南崇-余-犹地区比较特殊的闪长质侵入体。锆石的原位U-Pb定年表明,该岩体侵位于433.5±3.4Ma。全岩主量元素特征上显示出中偏酸性(SiO2=56.92%~64.70%),富Al(Al2O3=14.10%~14.83%),富碱(Alk=6.41%~7.40%)特别是富钾(K2O=3.86%~4.85%),镁、铁含量较高,MgO:3.47%~5.95%,FeOT:5.23%~8.14%以及低磷(P2O5=0.27%~0.4%)的特点;微量元素上主要富集K、Rb、Cs等大离子亲石元素和轻稀土元素,亏损Nb、Ta、Ti、P等高场强元素。磷灰石微量元素特征上显示高度富集稀土元素特别是轻稀土元素的特征;具有Eu的负异常(δEu=0.37~0.45)。ISr位于0.7073~0.7132之间,εNd(t)变化于-8.41~-4.97之间,两阶段钕模式年龄介于1.58~1.86Ga之间,Hf同位素组成相对均一,εHf(t)主要集中变化于-8~-2之间,两阶段Hf模式年龄加权平均为1.77±0.09Ga,这些特征都暗示了该石英闪长质岩体的形成是强烈壳幔相互作用的产物,区内加里东晚期可能发生了局部的岩石圈的减薄。 相似文献