东天山四顶黑山层状岩体岩石地球化学特征

位于东天山黄山岩带最东端的四顶黑山镁铁质-超镁铁质层状杂岩体规模较大,呈北东向展布,可分为南、北2个岩体。主要岩石类型有单辉橄榄岩、橄榄辉石岩、橄榄苏长辉长岩、橄榄辉长岩、辉石角闪岩、辉长岩和角闪辉长岩,超镁铁岩相常与辉长岩相呈韵律互层。主量元素化学组成主要属拉斑玄武岩系列。岩石稀土元素配分曲线呈平坦型以及Eu的正异常,普遍富集大离子亲石元素(Rb、Ba、U),显示明显的Sr正异常以及Nb、Ta的亏损。通过橄榄石最高的Fo值(79.6)估算出母岩浆中MgO和FeO含量分别为6.23%和6.60%。岩浆在演化过程中发生了橄榄石、斜方辉石、单斜辉石、斜长石的分离结晶/堆晶作用以及较弱的上地壳同化混染作用。岩石高的(La/Yb)N值1.550和1.744值表明岩浆源区的深度可能大于90km;Th/U值特征以及Th/Yb-Nb/Yb和La/Ba-La/Nb图解表明,四顶黑山岩体的岩浆源区可能为受俯冲作用改造的岩石圈地幔。     

东天山黄山南镁铁-超镁铁岩体的岩浆演化过程:矿物学、Sr-Nd同位素特征的指示

黄山南镁铁-超镁铁质岩体位于东天山造山带觉罗塔格构造带内,属于土墩-黄山-图拉尔根镁铁-超镁铁质岩带。本文在前人研究的基础上,从橄榄石、辉石矿物学组成和全岩Sr、Nd同位素等方面对黄山南岩体进行了分析研究,并与黄山、黄山东、香山等典型含矿岩体作了对比,旨在进一步查明黄山南岩体的岩浆源区和母岩浆性质及其岩浆演化过程。Sr-Nd同位素特征表明黄山南岩体来自一个弱亏损的地幔源区,相较黄山、黄山东、香山等岩体的源区具有更加富集的特征。黄山南岩体中的橄榄石属于贵橄榄石,斜方辉石主要为古铜辉石,少数为紫苏辉石,单斜辉石主要为顽透辉石、普通辉石和少数的透辉石。单斜辉石和橄榄石的成分特征表明形成黄山南岩体的母岩浆为演化程度较低的拉斑玄武质岩浆,且母岩浆成分具有高Mg、高Ni的特点。计算得到黄山南岩体母岩浆的Fe O~T=13.20%、MgO=16.96%、Ni=377.2×10~(-6),且母岩浆在结晶分异过程中没有经历充分的硫化物熔离作用,这也是造成母岩浆中Ni含量较高以及岩体含矿性较差的主要因素。     

新疆东天山西段路北镁铁-超镁铁岩地球化学特征及构造意义

对新疆东天山西段路北岩体进行主量元素、微量元素研究,通过与东天山东段镁铁-超镁铁岩体及塔里木大火成岩省对比,探讨其岩体成因和区域构造演化。路北岩体随MgO含量升高,FeO~T升高,而A1_2O_3、CaO降低,表明其为以橄榄石、斜方辉石和单斜辉石为主的堆晶岩。路北岩体与东天山东段镁铁-超镁铁具相似的稀土和微量元素分布模式,与塔里木地区地幔柱成因的镁铁-超镁铁岩体相比,路北岩体亏损Nb,Ta,Ti等高场强元素,La,Ba,Th,U等不相容元素含量较低,较高的La/Nb和Ba/Nb比值和较低的Nb/U比值,表明其原始岩浆主要来源于受俯冲流体交代地幔的部分熔融,软流圈地幔的上涌可能为部分熔融提供热源。     

新疆圪塔山口含铜镍岩体锆石SHRIMPU-Pb年龄、岩石地球化学特征及其地质意义

圪塔山口含铜镍镁铁-超镁铁质岩体位于东天山黄山–镜儿泉–图拉尔根铜镍矿带东段。岩体由I-1,I-2,I-3,I-4四个小岩体组成,主要岩石类型为辉石橄榄岩、橄榄辉石岩、辉长岩和闪长岩,主要赋矿岩相为辉石橄榄岩。I-2号含矿岩体锆石SHRIMP U-Pb年龄为275.0±3.6 Ma,与东天山地区含铜镍矿镁铁–超镁铁岩体形成时代相近,I-4号不含矿岩体锆石SHRIMP U-Pb年龄为364.2±3.9 Ma,明显早于含矿岩体。样品的主量元素组成显示岩浆演化过程主要发生了橄榄石和少量辉石的分离结晶/堆晶作用;稀土元素球粒陨石标准化配分曲线呈轻稀土略富集的右倾型,Eu异常不明显;微量元素特征显示相对富集大离子亲石元素(Cs、Sr、Ba),适度亏损高场强元素(Nb、Ta、Ti)。岩石地球化学特征表明岩浆演化过程中遭受了较弱的中–下地壳物质混染。U/Th-Th/Zr、Ba/Th-Th/Yb图解,La/Nb、La/Ba和Ba/Nb比值表明岩浆源区遭受了明显的俯冲流体交代作用。综合含矿岩体年代学、岩石地球化学特征及区域演化历史,认为圪塔山口含矿岩体形成于碰撞后伸展背景,可能同时叠加了塔里木地幔柱活动的影响。     

桂北元宝山宝坛地区约825Ma镁铁-超镁铁岩的地球化学及其地质意义

镁铁－超镁铁岩的岩石学和地球化学特征表明，元宝山超镁铁岩中橄榄石的Fo为78－83，岩石具有明显的包橄结构，具有LREE亏损，低Th/Nb和La/Nb比值以及高（t)值（约＋5），是来源于亏损地幔低程度部分熔融的岩浆堆晶的产物；宝坛地区镁铁－超镁铁岩富集LREE，具有高的Th/Nb,La/Nb比值和低的（t)值（－0．45－7．01），是镁铁质岩浆上升，结晶过程中与地壳物质混染（AFC）的结果，超镁铁岩与澳大利亚Garidner岩脉群具有相似的不相容元素分布型式和Nd(t) 值，是导致新元古代Rodinia超大陆裂解的地幔柱熔融的产物。     

甘肃北山地区骆驼山镁铁--超镁铁岩体岩石成因

骆驼山镁铁--超镁铁岩体主要岩石类型有单辉橄长岩、橄榄辉长苏长岩、橄长岩、辉长苏长岩、辉长岩。橄榄石Fo为76~83,为贵橄榄石。辉石化学特征以及主量元素特征表明其属拉斑玄武岩系列,稀土元素配分曲线总体表现为轻稀土稍富集、重稀土微分异的特征。微量元素具有大离子亲石元素(Rb、Ba、Sr)相对富集,高场强元素Ta、Hf、Th相对亏损的特征。岩浆演化过程中分离结晶作用主要受单斜辉石控制。Nb/U、Ce/Pb值更接近于地壳值以及敏感元素比值协变关系表明岩浆演化过程发生了同化混染作用。Th/Yb-Nb/Yb、La/Ba-La/Nb之间的关系指示岩浆源区可能为流体交代改造的富集型岩石圈地幔。     

新疆中天山白石泉含铜镍矿镁铁-超镁铁岩体地球化学特征与岩石成因

白石泉含Cu-Ni硫化物镁铁-超镁铁侵入体位于中天山地块,其主要岩石类型有辉石橄榄岩、橄榄辉石岩、橄长岩、辉长岩及角闪辉长岩等,具有明显的堆晶结构.对岩体的主要、微量及稀土元素地球化学特征研究表明,岩体属铁质镁铁-超镁铁岩,具有拉斑玄武质岩浆的分异趋势;并相对富集大离子亲石元素(Rb、Ba、Sr等)、亏损高场强元素(Nb、Ta、Zr、Hf),以及具有LREE富集((La/Yb)n=1.27～9.95)的右倾型稀土元素分布模式.Pb同位特征表明母岩浆与软流圈地幔和EM Ⅱ地幔物质有关.综合地球化学特征表明,母岩浆为来源于受早期俯冲物质混染的软流圈地幔的高镟拉斑玄武岩浆.岩浆在上升过程中,没有受到上地壳及围岩的混染.原生岩浆形成后,经过了橄榄石、辉石、斜长石及铬铁矿的分离结晶作用和硫化物的熔离作用.目前出露的岩体为富含橄榄石及硫化物的“晶粥“在高位岩浆房中演化的产物.     

东昆仑石头坑德镁铁-超镁铁质岩体矿物学特征及成矿指示

石头坑德镁铁-超镁铁质岩体位于东昆仑造山带东段五龙沟地区,邻近昆中大断裂,主要岩性为辉石岩、橄辉岩、橄榄岩、辉长岩等,铜镍矿体主要赋存于Ⅰ号岩体的辉石岩、橄辉岩和橄榄岩中。岩石地球化学特征表明,其镁铁比值(m/f)变化范围在2.77~6.01之间,属铁质系列的镁铁-超镁铁岩,有利于成铜镍矿。稀土总量总体较低,轻稀土元素之间分馏强,重稀土元素之间分馏弱。岩石总体富集LILE(Rb、Ba、Th、U),贫HFSE(Nb、Ta、Zr、Y),具有明显的Rb、U正异常及Nb、Ta的负异常。超镁铁岩类橄榄石中的Ni普遍亏损,指示深部存在硫化物的熔离作用,在橄榄石结晶之前,大量的Ni进入到硫化物中,极有利于形成富矿岩浆或矿浆。可见,伴随同化混染作用的发生,岩浆中S达到过饱和,进而硫化物发生不混溶作用,富含硫化物的岩浆运移至东昆仑造山带邻近昆中断裂构造薄弱的部位成岩成矿。铜镍矿体多赋存在含橄榄石的超镁铁质岩体内,指示石头坑德岩体深部存在高度富集铜镍的部位,是下一步的找矿方向。     

新疆黄山铜镍硫化物矿床成矿岩浆作用过程

黄山铜镍硫化物矿床镁铁．超镁铁质岩体岩相发育良好,主要包括橄榄岩、辉石岩、辉长岩和闪长岩,橄榄岩中部分橄榄石包含有硫化物珠滴。对该岩体不同岩相进行了主元素、微量元素、铂族元素和单矿物的分析,结果表明,不同类型岩石的化学组成受橄榄石、辉石和斜长石结晶分异作用的控制。微量元素和稀土元素具有相似的分布模式,（La／Yb）N介于1．14—3．65之间,明显亏损Nb和Ta,富集Sr。含矿岩石Cu／Pd和Ti／Pd比值大于原生地幔岩浆。上述结果揭示黄山镁铁-超镁铁质岩体不同岩性的岩石具有不同的主元素和微量元素特征,但母岩浆来自同一源区。根据橄榄石的F0值和全岩的主要氧化物组成估算出母岩浆为高镁（MgO约为15％）玄武岩岩浆,在岩浆作用过程中地壳富硅组分的混染是导致硫化物熔离的主要机制。     

东天山二叠纪镁铁-超镁铁质成矿岩体造岩矿物特征及其成因意义

东天山造山带与镁铁-超镁铁质岩体有关的铜镍硫化物矿床数量多,分布集中,是我国重要的铜镍成矿带之一。成矿岩体多以小岩体群形式产出,由西向东分布有白鑫滩、黄山和图拉尔根3个岩体群,大型矿床主要赋存在黄山岩体群内。本文对3个岩体群内成矿岩体的主要造岩矿物进行了系统的对比研究。成矿岩体的主要造岩矿物为贵橄榄石、古铜辉石、单斜辉石、斜长石和角闪石以及少量的铬尖晶石和金云母。橄榄石Al温度计计算结果表明,黄山岩体群内成矿岩体的母岩浆结晶温度介于1 143~1 257℃之间,略低于白鑫滩和图拉尔根岩体群(1 283~1 301℃)。单斜辉石压力计算表明成矿岩体的结晶压力相似,介于0.31~0.33 GPa之间。成矿岩体中均富含含水矿物,且单斜辉石结晶早于斜长石,指示成矿岩体的原始岩浆形成于富水环境。成矿岩体的单斜辉石具有较高的Al/Ti值,铬尖晶石和橄榄石具有与岛弧火山岩相似的矿物学特征,结合区域构造演化,认为东天山镁铁-超镁铁质成矿岩体的原始岩浆是被消减板片交代过的地幔部分熔融的产物。矿物学特征对比显示了黄山岩体群内成矿岩体更富斜方辉石和中性斜长石,且具有较低的铬尖晶石Cr~#值和橄榄石Ca含量。结合前人研究成果和相关地球化学数据,认为相对高的混染程度导致了黄山岩体群的母岩浆富SiO_2和Al_2O_3,同时降低了岩浆的结晶温度。     

造山带铜镍硫化物矿床的岩浆起源:以东天山黄山南铜镍矿床为例

位于中亚造山带南缘的新疆东天山地区因其出露大量的二叠纪镁铁质-超镁铁质岩体并产出一系列铜镍硫化物矿床而成为近年来地质学界关注的焦点.选择新疆东天山地区黄山南含铜镍矿镁铁质-超镁铁质岩体为研究对象,对其开展了系统的岩石学、矿物学和地球化学研究,以探讨造山带铜镍硫化物矿床的岩浆起源与性质.黄山南岩体主要由方辉橄榄岩、二辉橄榄岩、橄榄二辉岩、（橄榄）辉长苏长岩和闪长岩组成.各岩相显示富集大离子亲石元素和轻稀土元素、强烈亏损Nb-Ta、Ti,类似于典型岛弧火山岩特征.黄山南镁铁质-超镁铁质岩具有较大变化范围的ε_Nd（t=282.5 Ma）值（-1.31~4.22）和（87Sr/86Sr）_i比值（0.703 2~0.706 9）以及高的（206Pb/204Pb）_i比值（17.67~18.90）,暗示其来源于一个适度富集的亏损地幔并经历了5%~20%新生地壳物质混染和~5%上地壳物质混染.根据橄榄石最高Fo牌号（摩尔含量为86.6%）计算的黄山南母岩浆为苦橄质岩浆（MgO=12.11%、FeO_Total=11.14%、Ni=306×10-6）,指示其岩浆源区应为软流圈和交代地幔楔共同熔融的源区.黄山南橄榄石低的Ca（< 725×10-6）和100×Mn/Fe（1.18~1.38）、高的Ni（1 451×10-6~2 813×10-6）和Mn/Zn（11.09~23.53）,暗示黄山南母岩浆来源于含有辉石岩的不均一橄榄岩地幔源区.因此,我们推测黄山南岩体的原始岩浆来源于早期经历过俯冲流体改造的含有辉石岩的交代岩石圈地幔源区.      

东昆仑希望沟橄榄辉石岩LA-ICP-MS锆石U-Pb定年及岩石地球化学特征

东昆仑古特提斯域镁铁-超镁铁质岩石的研究极为薄弱,对青海东昆仑东段希望沟镁铁-超镁铁质杂岩体中橄榄辉石岩进行岩相学、地球化学及年代学分析,以期为东昆仑晚古生代-早中生代构造岩浆演化提供新的约束。利用LA-ICP-MS锆石U-Pb定年,获得希望沟橄榄辉石岩加权平均年龄为（262.4±1.6）Ma,表明岩体侵位于中二叠世。岩石地球化学研究显示,希望沟橄榄辉石岩具有较高的Mg#值（85.31~86.27）,m/f比值介于5.50~6.18,属于铁质超基性岩类;具有低TiO₂（0.41%~0.52%）和低Al₂O₃（3.04%~4.57%）,属钙碱性系列。岩石富集大离子亲石元素（Rb、Th、U）和Pb,相对亏损高场强元素（Nb、Ta、P、Ti）,ΣREE为29.79×10-6~38.96×10-6,（La/Yb）_N为1.71~2.51,平均2.15,δEu=0.73~0.86,具有弱的Eu负异常。岩石成因分析表明,岩石源区为被俯冲改造的岩石圈地幔,岩浆在演化过程中遭受了上地壳物质的同化混染作用。结合东昆仑区域构造演化,认为希望沟橄榄辉石岩为阿尼玛卿古特提斯洋俯冲阶段的岩浆记录。      

柴达木北缘东段呼德生镁铁-超镁铁质岩体锆石U-Pb年代学、地球化学及成岩成矿分析

呼德生岩体位于柴北缘造山带欧龙布鲁克微陆块东南缘,侵位于古元古代金水口变质岩群中。该岩体从中心到边缘依次出现橄榄岩→辉石岩→辉长岩的岩相分带特征,岩石主要类型有纯橄岩、橄榄二辉岩和辉长岩,各岩石之间多为过渡接触关系,镍铜矿化主要赋存于辉石岩中。锆石LAICP-MS U-Pb年代学研究表明,岩体形成年龄为425.2±5.8Ma,为柴北缘晚志留世-晚泥盆世后造山伸展阶段岩浆作用的产物。岩石镁铁比值(m/f)为2.51~5.37,属于铁质系列基性-超基性岩。各类岩石富集轻稀土元素(LREE)和大离子亲石元素(Ba、Sr、Rb),而亏损高场强元素(Zr、Hf、Nb、Ta)。岩相学、矿物学及岩石地球化学研究表明岩浆在演化过程中发生了一定程度的结晶分异作用和同化混染作用。结合岩体形成年代及区域地质资料,呼德生岩体应形成于大陆边缘伸展阶段,原始岩浆在演化过程中经历了地幔流体的交代作用。通过对岩浆结晶分异程度及同化混染情况等方面的综合评价,认为呼德生岩体具有良好的铜镍硫化物矿床形成条件。     

Petrogenesis of the ~740 Korab Kansi mafic-ultramafic intrusion,South Eastern Desert of Egypt: Evidence of Ti-rich ferropicritic magmatism

The Neoproterozoic Korab Kansi mafic-ultramafic intrusion is one of the largest (100 km²) intrusions in the Southern Eastern Desert of Egypt. The intrusion consists of Fe-Ti-bearing dunite layers, amphibole peridotites, pyroxenites, troctolites, olivine gabbros, gabbronorites, pyroxene gabbros and pyroxene-hornblende gabbros, and also hosts significant Fe-Ti deposits, mainly as titanomagnetite-ilmenite. These lithologies show rhythmic layers and intrusive contacts against the surrounding granites and ophiolitic-island arc assemblages. The wide ranges of olivine forsterite contents (Fo_67.9-85.7), clinopyroxene Mg# (0.57–0.95), amphibole Mg# (0.47–0.88), and plagioclase compositions (An_85.8-40.9) indicate the role of fractional crystallization in the evolution from ultramafic to mafic rock types. Clinopyroxene (Cpx) has high REE contents (2–30 times chondrite) with depleted LREE relative to HREE, like those crystallized from ferropicritic melts generated in an island-arc setting. Melts in equilibrium with Cpx also resemble ferropicrites crystallized from olivine-rich mantle melts. Cpx chemistry and its host rock compositions have affinities to tholeiitic and calc-alkaline magma types. Compositions of mafic-ultramafic rocks are depleted in HFSE (e.g. Nb, Ta, Zr, Th and U) relative to LILE (e.g. Li, Rb, Ba, Pb and Sr) due to the addition of subduction-related hydrous fluids (rich in LILE) to the mantle source, suggesting an island-arc setting. Fine-grained olivine gabbros may represent quenched melts approximating the primary magma compositions because they are typically similar in assemblage and chemistry as well as in whole-rock chemistry to ferropicrites. We suggest that the Korab Kansi intrusion crystallized at temperatures ranging from ~700 to 1100 °C from ferropicritic magma derived from melting of metasomatized mantle at <5 Kbar. These hydrous ferropicritic melts were generated in the deep mantle and evolved by fractional crystallization under high ƒO₂ at relatively shallow depth. Fractionation formed calc-alkaline magmas during the maturation of an island arc system, reflecting the role of subduction-related fluids. The interaction of metasomatized lithosphere with upwelling asthenospheric melts produced the Fe and Ti-rich ferropicritic parental melts that are responsible for precipitating large quantities of Fe-Ti oxide layers in the Korab Kansi mafic-ultramafic intrusion. The other factors controlling these economic Fe-Ti deposits beside parental melts are high oxygen fugacity, water content and increasing degrees of mantle partial melting. The generation of Ti-rich melts and formation of Fe-Ti deposits in few layered intrusions in Egypt possibly reflect the Neoproterozoic mantle heterogeneity in the Nubian Shield. We suggest that Cryogenian-Tonian mafic intrusions in SE Egypt can be subdivided into Alaskan-type intrusions that are enriched in PGEs whereas Korab Kansi-type layered intrusions are enriched in Fe-Ti-V deposits.     

Geochemistry of an Alaskan-type mafic-ultramafic complex in Eastern Desert,Egypt:New insights and constraints on the Neoproterozoic island arc magmatism

Mikbi intrusion(MI) is a part of the Neoproterozoic Nubian Shield located along the NE-SW trending major fracture zones prevailing southern Eastern Desert of Egypt. In this study, we present for the first time detailed mineralogical and bulk-rock geochemical data to infer some constraints on the parental magma genesis and to understand the tectonic processes contributed to MI formation. Lithologically, it is composed of fresh peridotite, clinopyroxenite, hornblendite, anorthosite, gabbronorite, pyroxene amphibole gabbro, amphibole gabbro and diorite. All rocks have low Th/La ratios(mostly <0.2) and lack positive Zr and Th anomalies excluding significant crustal contamination. They show very low concentrations of Nb, Ta, Zr and Hf together with sub-chondritic ratios of Nb/Ta(2-15) and Zr/Hf(19-35),suggesting that their mantle source was depleted by earlier melting extraction event. The oxygen fugacity(logfO_2) estimated from diorite biotite is around the nickel-nickel oxide buffer(NNO) indicating crystallization from a relatively oxidized magma. Amphiboles in the studied mafic-ultramafic rocks indicate relative oxygen fugacity(i.e. ΔNNO; nickel-nickel oxide) of 0.28-3 and were in equilibrium mostly with 3.77-8.24 wt.% H_2 O_melt(i.e. water content in the melt), consistent with the typical values of subduction-related magmas. Moreover, pressure estimates(0.53-6.79 kbar) indicate polybaric crystallization and suggest that the magma chamber(s) was located at relatively shallow crustal levels. The enrichment in LILE(e.g., Cs, Ba, K and Sr) and the depletion in HFSE(e.g., Th and Nb) relative to primitive mantle are consistent with island arc signature. The olivine, pyroxene and amphibole compositions also reflect arc affinity. These inferences suggest that their primary magma was derived from partial melting of a mantle source that formerly metasomatized in a subduction zone setting. Clinopyroxene and bulkrock data are consistent with orogenic tholeiitic affinity. Consequently, the mineral and bulk-rock chemistry strongly indicate crystallization from hydrous tholeiitic magma. Moreover, their trace element patterns are subparallel indicating that the various rock types possibly result from differentiation of the same primary magma. These petrological, mineralogical and geochemical characteristics show that the MI is a typical Alaskan-type complex.     

Geochemical and Petrological Studies on the Early Carboniferous Sidingheishan Mafic–Ultramafic Iintrusion in the Southern Margin of the Central Asian Orogenic Belt, NW China

The Sidingheishan mafic-ultramafic intrusion is located in the eastern part of the Northern Tianshan Mountain, along the southern margin of the Central Asian Orogenic Belt in northern Xinjiang autonomous region of China. The Sidingheishan intrusion is mainly composed of wehrlite, olivine websterite, olivine gabbro, gabbro and hornblende gabbro. At least two pulses of magma were involved in the formation of the intrusion. The first pulse of magma produced an olivine-free unit and the second pulse produced an olivine-bearing unit. The magmas intruded the Devonian granites and granodiorites.An age of 351.4±5.8 Ma(Early Carboniferous) for the Sidingheishan intrusion has been determined by U-Pb SHRIMP analysis of zircon grains separated from the olivine gabbro unit. A U-Pb age of 359.2±6.4 Ma from the gabbro unit has been obtained by LA-ICP-MS. Olivine of the Sidingheishan intrusion reaches 82.52 mole% Fo and 1414 ppm Ni. On the basis of olivine-liquid equilibria, it has been calculated that the MgO and FeO included in the parental magma of a wehrlite sample were approximately10.43 wt% and 13.14 wt%, respectively. The Sidingheishan intrusive rocks are characterized by moderate enrichments in Th and Sm, slight enrichments in light REE, and depletions in Nb, Ta, Zr and Hf. The ε_(Nd)(t) values in the rock units vary from +6.70 to +9.64, and initial ~(87)Sr/~(86)Sr ratios range between 0.7035 and0.7042. Initial ~(206)Pb/~(204)Pb, ~(207)Pb/~(204)Pb and ~(208)Pb/~(204)Pb values fall in the ranges of 17.23-17.91,15.45-15.54 and 37.54-38.09 respectively. These characteristics are collectively similar to the Heishan intrusion and the Early Carboniferous subduction related volcanic rocks in the Santanghu Basin, North Tianshan and Beishan area. The low(La/Gd)_(PM) values between 0.26 and 1.77 indicate that the magma of the Sidingheishan intrusion was most likely derived from a depleted spinel-peridotite mantle.(Th/Nb)_(PM)ratios from 0.59 to 20.25 indicate contamination of the parental magma in the upper crust.Crystallization modeling methods suggest that the parental magma of the Sidingheishan intrusion was generated by flush melting of the asthenosphere and subsequently there was about 10 vol%contamination from a granitic melt. This was followed by about 5 vol% assimilation of upper crustal rocks. Thus, the high-Mg basaltic parental magma of Sidingheishan intrusion is interpreted to have formed from partial melting of the asthenosphere during the break-off of a subducted slab.     

攀西地区大板山岩体的年代学、元素地球化学及其对铜镍硫化物矿床成因的约束

大板山镁铁-超镁铁质杂岩体位于攀西地区西北部,受金河-菁河断裂带控制,主要岩石类型有辉长岩、苏长辉长岩和二辉橄榄岩。本次研究集中于苏长辉长岩和二辉橄榄岩,其中,二辉橄榄岩具有明显的堆晶结构,橄榄石Fo值最高可达81.4。二辉橄榄岩SiO₂含量为42.93%~44.18%,苏长辉长岩SiO₂含量为44.89%~52.76%,稀土总量(∑REE)相对较低(23.2×10^-6~61.7×10^-6),并均呈现出近平行的、相对平缓的右倾稀土元素配分模式,说明其为同源岩浆演化的关系。此外,大部分样品相对富集大离子亲石元素(LILE;如Rb、Sr、Ba等),适度亏损高场强元素(HFSE;如Nb、Ta、Ti等)。结合其较低的SiO₂含量和微量元素比值(如Th/Ta和La/Nb等),表明岩浆未遭受大量的地壳混染。岩相学和岩石地球化学特征均显示了非常明显的分离结晶作用。根据(Tb/Yb)_PM-(Yb/Sm)_PM图解,大板山岩体的原始岩浆主要来源于岩石圈地幔轻度富集不相容元素的尖晶石相二辉橄榄岩。二辉橄榄岩样品中橄榄石Fo-NiO图解中多数点落在硫化物未熔离的范围,且样品全岩Cu/Zr比值为7.04~103,而苏长辉长岩中Cu/Zr比值为0.88~5.56,反映了二辉橄榄岩-苏长辉长岩可能经历了由S不饱和到过饱和的过程。推测硫化物的熔离可能是岩浆在上地壳岩浆房中发生了以橄榄石和辉石为主的分离结晶作用,造成硫化物达到过饱和。锆石LA-ICP-MS测年表明,岩体年龄为259.69±0.61Ma,与峨眉山大火成岩省其它镁铁-超镁铁质岩体的形成时间基本一致。