鲁西中生代高Mg闪长岩的成因:年代学与岩石地球化学证据

鲁西高Mg闪长岩分布较为广泛, 莱芜铁铜沟岩体和淄博金岭岩体是其典型代表.铁铜沟岩体早期苏长辉长岩和晚期辉石闪长岩、金岭黑云母闪长岩的LA-ICPMS U-Pb谐和加权平均年龄分别为(131.4±4.9)Ma(n=15)、(134.5±2.3) Ma(n=13)和(132.8±4.2)Ma(n=12), 它们代表了岩体的侵位结晶年龄——早白垩世.铁铜沟岩体晚期辉石闪长岩中浑圆状锆石的LA-ICPMS U-Pb谐和年龄为(2 513±54)Ma(n=8), 代表了华北克拉通基底的存在.该类岩石以高Mg# (> 60)、富钠、富含轻稀土元素、贫重稀土元素以及高场强元素(Nb、Ta、Zr、Hf)的明显亏损为特征, 显示埃达克岩(adakite) 的特征.该类岩石中地幔橄榄岩包体的广泛存在以及高Mg的特征表明原始岩浆的地幔成因, 而Sr-Nd同位素组成(I_sr为0.704 75-0.707 72和ε_Nd(t)值为-3.95--13.30)和高场强元素(Nb、Ta、Zr、Hf)的亏损以及太古代继承锆石的存在均暗示岩浆源区应有陆壳物质的涉入.铁铜沟岩体和金岭岩体闪长岩成分的差异应归因于岩浆源区性质的差异和部分熔融程度的不同.基于该类岩石的地球化学和所含包体, 同时结合华北克拉通东部中生代早期岩石圈演化历史, 可以认为鲁西中生代早白垩世高Mg闪长岩的形成应为拆沉的岩石圈(地幔+下地壳)与软流圈混熔的产物.      

内蒙古林西早中生代O型高镁埃达克质安山岩的发现及其意义

对内蒙古林西地区火山岩样品的地球化学研究表明,其具有大洋型(O型)高镁埃达克质安山岩的地球化学特征[w(SiO2)=57.89%～63.97%、w(Al2O3)=15.39%～16.17%、w(Na2O)/w(K2O)=1.5～2.2(除一个为0.9)、A/CNK=0.83～0.97、Mg#=49～64、w(Cr)=91～209μg/g、w(Ni)=52.2～111.4μg/g、w(Sr)=551～1018μg/g、w(Yb)=1.18～1.71μg/g、w(Y)=12.6～17.7μg/g、δ(Eu)=0.86～0.94]。利用LA-ICP-MS对其锆石进行了U-Pb定年,得到206Pb/238U加权平均年龄为(244±2)Ma(MSWD=0.36)。此时,区域内古亚洲洋已闭合,综合地球化学特征和区域地质环境说明,林西高镁埃达克质安山岩是由残余洋壳部分熔融并随后与地幔橄榄岩相互作用形成的。内蒙古林西早中生代高镁埃达克质安山岩的产出表明,洋壳来源的埃达克岩(O型埃达克岩)不仅可以随俯冲同时产生,而且也可以在非俯冲环境下由保存在古俯冲带地幔中的残余洋壳部分熔融产生。     

鲁西中生代高镁闪长岩的地球化学特征及其成因探讨

鲁西中生代侵入岩包括辉长岩,闪长岩,花岗闪长岩和花岗岩,以闪长岩最为常见。莱芜和沂南等地的闪长岩具有高Mg#(0.45～0.69),Cr(<278μg/g)的特点,并富集大离子亲石元素(LILE)和亏损高场强元素(HFSE),其总体成分特点类似于北美苏必利尔省的太古代高镁闪长岩和产于现代俯冲带的高镁安山岩。不过鲁西高镁闪长岩的HREE含量相对较高(Yb=1.1～1.9μg/g),La/Yb比值相对较低(6.7～20),其成分更接近于Piip型高镁安山岩。鲁西高镁闪长岩代表了华北地台早期拉张环境下的岩浆活动,可能是受深俯冲扬子大陆下地壳释放的埃达克质熔体交代的岩石圈地幔直接熔融的产物。     

青海省刚察地区高镁安山岩锆石U-Pb LA-ICP-MS年代学及构造意义

基于青海省刚察地区1：5万电泵站等4幅区调项目,在拉脊山蛇绿构造混杂岩带药水泉组中识别一套玄武岩、玄武安山岩、安山岩类岩石组合,其岩相学、岩石地球化学特征与高镁安山岩相类似.岩石斑晶以斜长石和辉石为主,不含橄榄石,基质也含有大量的斜长石.岩石地球化学特征表现为K2O+Na2O含量2.55%~5.15%,Na2O > K2O,K2O含量0.22%~0.82%,为低钾;CaO含量5.31%~11.41%,TiO2含量0.27%~0.55%,变化范围较小;MgO含量为5.78%~11.06%,变化范围不大.总体具有低硅、钛、钾,高钙、镁,富钠之特征.稀土配分曲线为右倾斜状,多呈铕正异常,为轻稀土富集型.微量元素Rb、Ba、Th、Cr、Ni等变化幅度大,反映岩浆生成和演化过程复杂,但演变仍以部分熔融为主.选取玄武岩样品,通过LA-ICP-MS U-Pb锆石微区定年,获得了451.7±1.8 Ma年龄值,其时代为晚奥陶世.总体特征表明,刚察地区火山岩为埃达克型高镁安山岩,其构造环境为活动大陆边缘的岛弧.     

Petrogenesis and tectonic implications of ultrapotassic microgranitoid enclaves in Late Triassic arc granitoids,Qinling orogen,central China

The origin of microgranitoid enclaves in granitic plutons has long been debated (hybrid magma blobs vs. refractory restites or cognate fragments). This article presents detailed petrography, SHRIMP zircon U–Pb chronology, bulk-rock major and trace element analyses, and Sr–Nd isotope and in situ zircon Hf isotopic geochemistry for microgranitoid enclaves within two Late Triassic granitic plutons in the Qinling orogen. Zircon U–Pb dating shows that the enclaves formed during the Carnian (222.5 ± 2.1 to 220.7 ± 1.9 Ma) coeval with their host granitoids (220.0 ± 2.0 to 218.7 ± 2.4 Ma). Field and petrological observations (e.g. double enclaves, xenocrysts, acicular apatite, and poikilitic K-feldspar or quartz) suggest that the enclaves are globules of a mantle-derived more mafic magma that was injected into and mingled with the host magma. The enclaves are mainly ultrapotassic, distinct from the host granitoids that have high-K calc-alkaline bulk-rock compositions. Although the enclaves have closely similar bulk-rock Sr–Nd isotope [initial ⁸⁷Sr/⁸⁶Sr?=?0.7046–0.7056, ?_Nd (T)?=?–0.3 to –5.0] and in situ zircon Hf isotope [?_Hf (T)?=?–1.5 to?+2.9] ratios as the granitoids [initial ⁸⁷Sr/⁸⁶Sr?=?0.7042–0.7059, ?_Nd (T)?=?–0.6 to –6.3, ?_Hf (T)?=?–2.2 to?+1.6], chemical relationships including very different bulk-rock compositions at a given SiO₂ content lead us to interpret the isotopic similarities as reflecting similar but separate isotopic source rocks. Detailed elemental and isotopic data suggest that the enclaves and the host granitoids were emplaced in a continental arc environment coupled with northward subduction of the Palaeo-Tethyan oceanic crust. Partial melting of subducted sediments triggered by dehydration of the underlying igneous oceanic crust, with melts interacting with the overlying mantle wedge, formed high-K calc-alkaline granitic magmas, whereas partial melting of diapiric phlogopite-pyroxenites, solidified products of the same subducting sediment-derived melts, generated ultrapotassic magmas of the microgranitoid enclaves. Our new data further confirm that in the Late Triassic time the Qinling terrane was an active continental margin rather than a post-collisional regime, giving new insights into the tectonic evolution of this orogen.     

Teshima pyroclastics: Onset of characteristic Setouchi magmatism induced by slab melting at 14.8 Ma

Ar-Ar ages, and petrographical and geochemical characteristics of pyroclastics and an overlying lava from Teshima Island, southwest Japan are presented. Although previous geological and age data suggested Teshima pyroclastics were products of magmatism > 3 my prior to lava flows of Setouchi volcanic rocks generated in association with southward migration of the southwest Japan arc sliver during opening of the Sea of Japan backarc basin at ~ 15 Ma, the present results led to the conclusion that a sequence of Setouchi volcanism, induced by slab melting and subsequent melt-mantle reactions, produced both pyroclastics and lava at 14.6–14.8 Ma. This age is oldest among those reported so far and may represent the timing of onset of characteristic Setouchi magmatism immediately posterior to and hence as a result of the mega-tectonic event including rotation of the southwest Japan arc sliver.     

Post-collisional, Potassic and Ultrapotassic Magmatism of the Northern Tibetan Plateau: Constraints on Characteristics of the Mantle Source, Geodynamic Setting and Uplift Mechanisms

Cenozoic, post-collisional, potassic and ultrapotassic igneousrocks in the North Qiangtang, Songpan–Ganzi and NorthKunlun terranes of the northern Tibetan Plateau are distributedalong a semi-continuous, east–west-trending, volcanicbelt, which is over 1200 km in length. Spatially, there is aclose association with major strike-slip faults, thrust faultsand pull-apart basins. The ages of these magmatic rocks rangefrom 45 Ma to the present (the youngest known eruption occurredin 1951); they are shoshonitic, compositionally similar to K-richsubduction-related magmas, and range in SiO₂ from 44 to 66 wt%. There is a relative enrichment of large ion lithophile elements(LILE) and light rare earth elements (LREE) in the most primitivemagmatic rocks (MgO >6 wt %) in the North Qiangtang terranecompared with those in the Songpan–Ganzi and North Kunlunterranes; correspondingly, the primitive magmas have higher⁸⁷Sr/⁸⁶Sr and ²⁰⁶Pb/²⁰⁴Pb, and lower ¹⁴³Nd/¹⁴⁴Nd ratios in theNorth Qiangtang terrane than in the Songpan–Ganzi andNorth Kunlun terranes. The dominant factors that control thegeochemical characteristics of the magmas are an enriched asthenosphericmantle source composition, the degree of partial melting ofthis source, and the combined processes of crustal assimilationand fractional crystallization (AFC). Enrichment of the asthenosphereis considered to have occurred by incorporation of subductedsediments into the mantle wedge above a subducted slab of Indianlithosphere during India–Asia convergence. Continentallithospheric mantle, metasomatically enriched during earlierepisodes of subduction, may have also contributed a source componentto the magmas. Trace element modelling indicates that the mantlesource of the most primitive magmas in the North Qiangtang terranecontained higher amounts of subducted sediment (0·5–10%)compared with those in the Songpan–Ganzi and North Kunlunterranes (<2%). The degrees of partial melting required togenerate the primitive potassic and ultrapotassic magmas fromthe enriched mantle sources range from <0·1% to 15%in the three major basement terranes. Energy-constrained AFCmodel calculations show that the more evolved magmatic rocks(MgO <6 wt %) are the results of AFC processes in the middlecrust in the North Qiangtang terrane and the upper crust inthe Songpan–Ganzi and North Kunlun terranes. We proposethat the ultimate driving force for the generation of the post-collisionalpotassium-rich magmatism in north Tibet is the continuous northwardunderthrusting of the Indian continental lithosphere followingIndia–Asia collision. This underthrusting resulted inupwelling of hot asthenosphere beneath north Tibet, squeezedup between the advancing Indian lithosphere and the backstopof the rigid Asian continental lithosphere. Asthenospheric upwellingmay have also contributed to uplift of the northern TibetanPlateau. KEY WORDS: Tibetan Plateau; potassic and ultrapotassic magmatism; enriched asthenospheric mantle source; EC-AFC modelling; geodynamics     

The Petrology and Geochemistry of Oto-Zan Composite Lava Flow on Shodo-Shima Island, SW Japan: Remelting of a Solidified High-Mg Andesite Magma

The Oto-Zan lava in the Setouchi volcanic belt is composed ofphenocryst-poor, sparsely plagioclase-phyric andesites (sanukitoids)and forms a composite lava flow. The phenocryst assemblagesand element abundances change but Sr–Nd–Pb isotopiccompositions are constant throughout the lava flow. The sanukitoidat the base is a high-Mg andesite (HMA) and contains Mg- andNi-rich olivine and Cr-rich chromite, suggesting the emplacementof a mantle-derived hydrous (7 wt % H₂O) HMA magma. However,Oto-Zan sanukitoids contain little H₂O and are phenocryst-poor.The liquid lines of descent obtained for an Oto-Zan HMA at 0·3GPa in the presence of 0·7–2·1 wt % H₂Osuggest that mixing of an HMA magma with a differentiated felsicmelt can reasonably explain the petrographical and chemicalcharacteristics of Oto-Zan sanukitoids. We propose a model wherebya hydrous HMA magma crystallizes extensively within the crust,resulting in the formation of an HMA pluton and causing liberationof H₂O from the magma system. The HMA pluton, in which interstitialrhyolitic melts still remain, is then heated from the base byintrusion of a high-T basalt magma, forming an H₂O-deficientHMA magma at the base of the pluton. During ascent, this secondaryHMA magma entrains the overlying interstitial rhyolitic melt,resulting in variable self-mixing and formation of a zoned magmareservoir, comprising more felsic magmas upwards. More effectiveupwelling of more mafic, and hence less viscous, magmas througha propagated vent finally results in the emplacement of thecomposite lava flow. KEY WORDS: high-Mg andesite; sanukitoid; composite lava; solidification; remelting     

高镁安山岩/闪长岩类(HMA)和镁安山岩/闪长岩类(MA):与洋俯冲作用相关的两类典型的火成岩类

本文主要基于对实验岩石学成果的简要评述,讨论与洋俯冲作用有关的两类典型的火成岩类:楔形地幔在含水条件下橄榄岩局部熔融产生的高镁安山岩/闪长岩类(HMA)和俯冲洋壳局部熔融岩浆与地幔楔相互作用产生的镁安山岩/闪长岩类(MA)。提出:(1)识别HMA和MA必须同时运用两套参数系统:SiO2-MgO系统和SiO2-FeO/MgO系统;(2)区别HMA和MA是在它们均符合LF-CA(低Fe钙碱趋势)特征条件下,再用SiO2-MgO系统进一步加以鉴别;(3)识别HMA和MA的方法,或用在给定SiO2时,MgO和FeO/MgO的具体数值,或用图解法。     

Stratigraphy and paleomagnetism of a 2.9-km composite lava section in Eyjafjördur,Northern Iceland: a reconnaissance study

Eight mountainside profiles in lava flows south of the fjord Eyjafjördur, Northern Iceland, were sampled for paleomagnetic studies. The sampling was concurrent with pilot stratigraphic mapping of the lava sequences in these and several supplementary profiles. The eight profiles are correlated with minor overlaps so that they form a composite section of 2.9 km thickness, estimated to cover the age range between about 9 and 5 million years ago (Hardarson et al. 1999). Paleomagnetic measurements made on 319 lavas generally yield primary remanence directions of high stability and within-unit consistency. Evidence for at least 17 reversals of the geomagnetic field is seen, as well as numerous field excursions. Frequent clustering of directions in successive lavas indicates that the volcanism was episodic.