西天山东塔尔别克金矿区安山岩LA-ICP-MS锆石U-Pb年代学、元素地球化学与岩石成因

东塔尔别克金矿区位于西天山吐拉苏盆地内阿希金矿区南侧,构造上属于伊犁-中天山微板块与准噶尔板块之间的博罗科努早古生代岛弧带西段。东塔尔别克矿区出露有一些安山岩,这些岩石具有典型高镁安山岩特征,如高硅（SiO₂=58.94%~63.85%),具有较高的MgO含量(3.75%~6.59%)和Mg^#(58~69)、高的Cr（94.2×10^-6~241×10^-6）、和Ni（54.5×10^-6~126 ×10^-6）含量,以及低的FeO^T/MgO比值。除了Sr含量略微偏低（235×10^-6~696×10^-6）之外,这些岩石基本显示了埃达克岩的地球化学特征：高的Al₂O₃（15.39%~16.65%）,低Y（9.86×10^-6~14.9×10^-6）含量,以及高的Sr/Y比值(23.8~48.1),无Eu异常,Nb、Ta、Ti亏损等。LA-ICP-MS锆石U-Pb测年结果显示安山岩的年龄为347.2±1.6Ma,为早石炭世。安山岩富集Rb、Th、U 等大离子亲石元素,相对亏损Nb、Ta、Ti等高场强元素,轻重稀土元素分馏明显,具有俯冲带岛弧岩浆的特征。东塔尔别克安山岩可能形成于岛弧环境中,并可能由俯冲的晚古生代北天山洋洋壳以及少量上覆沉积物熔融形成,产生的熔体在上升过程中与地幔橄榄岩发生了相互作用. 熔体-地幔相互作用对区内金矿的形成具有重要意义。     

天山北部石炭纪埃达克岩-高镁安山岩-富Nb岛弧玄武质岩：对中亚造山带显生宙地壳增生与铜金成矿的意义

新疆天山北部地区存在有石炭纪的埃达克岩-高镁安山岩-富Nb玄武质岩组合，并且其中许多岩石与铜（金）矿床伴生（如达巴特、阿希、土屋-延东、赤湖，等等）。埃达克岩富钠、高Sr但亏损Y与Yb，无明显Eu-正Eu异常以及正Sr异常与Nb、Ti亏损。高镁安山（闪长）岩是本次研究首次报道的，这些岩石无明显Eu-正Eu异常以及Nb、Ti亏损，普遍具有高的MgO和Cr、Ni含量，其中阿希金矿区一些样品类似于日本西南新生代Setouchi弧火山岩带中的赞岐岩类。富Nb玄武质岩富钠贫钾，具有微弱负．正Ba、Nb和Ti异常以及高的Nb／La比值，不同于大多数正常岛弧玄武岩。天山北部地区石炭纪埃达克岩具有高的8Nd（t）（＋3．4-＋9．0）和低的（^87Sr／^86Sr）i（0．7032—0．7043）。富Nb玄武质岩具有变化的εNd（t）（＋3．6-＋11．6）和（^87Sr／^86Sr）；（0．7007—0．7067）。我们的研究表明，天山北部地区石炭纪埃达克岩-高镁安山岩-富Nb玄武质岩组合可能是“埃达克岩交代的岛弧岩浆岩系列”。埃达克岩最有可能由石炭纪北天山洋的年轻洋壳在俯冲过程中熔融形成。另外，俯冲板片产生的熔体以及所释放的少量流体在上升过程中可能交代地幔楔橄榄岩或与其发生反应：一方面，触发地幔楔橄榄岩发生熔融形成富Nb岛弧玄武质岩；另一方面，地幔组分迅速进入到板片熔体中，导致其地幔组分增加，乃至形成高镁安山岩。因此，天山北部地区石炭纪埃达克岩-高镁安山岩-富Nb玄武质岩组合表明：（1）天山北部地区石炭纪可能为岛弧环境而非裂谷环境；（2）天山地区石炭纪的地壳生长可能以侧向增生为主；（3）除了亏损地幔之外，俯冲洋壳的熔融可能也在地壳的生长中发挥了重要的作用；（4）俯冲板片产生的埃达克质岩浆具有高的氧逸度，而其与地幔楔橄榄岩的强烈相互作用将导致地幔中的金属硫化物分解，成矿金属元素进入到岩浆中。这可能是新疆北部铜金矿化与一些埃达克岩、高镁安山（闪长）岩或富Nb岛弧玄武质岩密切共生的基本原因。     

Archean Shoshonitic Lamprophyres of the Abitibi Subprovince, Canada: Petrogenesis, Age, and Tectonic Setting

Archean shoshonitic lamprophyre dikes are prevalent along majortranslithospheric structures that demark tectonostratigraphicterranes in the Abitibi greenstone belt of the Superior Province.The lamprophyres post-date volcanism, tonalitic batholiths,deformation, and metamorphism of the terranes, and are mostprominently developed in trans-tensional graben, where theyare associated with molasse sediments and an alkaline suiteof plutons, stocks, and trachytes. Mineralogically, the dikesare characterized by zoned phiogopite or hornblende phenocrystsand/or diopsidic pyroxene, restriction of feldspar to the groundmass,globular segregations of K-feldspar and calcite, olivine ‘pilite’,and accessory Ti-magnetite, Cr-spinel, apatite, titanite, andSr-rich calcite; crustal xenoliths are sporadically present. Compositionally, weakly altered primititive dikes have contentsof SiO₂ (41–48 wt.%), TiO₂ (06–11 wt.%), P₂O₅(041–076 wt.%), Cr (258–915 ppm), Co (36–84ppm), Ni (159–368 ppm), and Sc (15–32 ppm), mg-numbers(72–79), and K₂O/Na₂O ratios (10–43) similar tothose of Phanerozoic shoshonitic lamprophyres. The primitivedikes are also characterized by extreme enrichments of K, Rb,Ba, Cs, U, and Th, enhanced light rare earth elements (REE),and fractionated REE patterns [La_n=33–274; (La/Yb)_n=16–87].On mid-ocean ridge basalt (MORB) normalized plots the dikesshow coherent patterns, with (1)enrichment of K, Rb, and Barelative to Sr and LREE, (2) variable enrichments of Rb andBa relative to K, (3) troughs at Ta–Nb and Ti, and (4)variable negative P and positive Sm anomalies. Compositionalvariations of lamprophyre suites within restricted areas areinterpreted to reflect melting of compositionally heterogeneoussources, variable degrees of assimilation–fractional crystallization,and mixing of distinct batches of lamprophyric magmas. Primary¹⁸O values of the magmas are close to 63 as given by resistantpyroxene; these are ¹⁸O-relative to MORB, but comparable withPhanerozoic alkali basalts and lamprophyres. Mica, clinopyroxene,hornblende, and feldspar do not retain magmatic equilibriumfractionations for oxygen isotopes. A concordant U–Pbage of 26742 Ma was obtained from titanite, similar to theages of shoshonitic plutons in the same area. The lamprophyredikes possess a total range of _Nd between 041 and 211(1),and define a distinct field in common with other late Archeanshoshonites on an f^(Sm/Nd) vs. _Nd plot. Pyroxenes yield a low⁸⁷Sr/⁸⁶Sr(0701102), whereas whole-rock Rb-Sr isotope systematicsare disturbed. Lamprophyres are not known from pre-27-Ga terranes. Their compositionand inferred geodynamic setting is consistent with an originin a depleted mantle wedge, enriched in large ion lithophileelements (LILE) and LREE during subduction by slab and sediment(low Sr/Nd) dehydration. Partial melting may have been triggeredby rebound and decompression that followed accretional collisionof two allochthonous greenstone terranes at a plate margin.The onset of shoshonitic magmatism at 27 Ga coincides withthe transition from tonalite–trondhjemite–granodiorite(TTG) dominated magmatism with high (La/Yb)_n and low Yb (slabmelting) to mantle-wedge derived granites featuring lower (La/Yb)_nand higher Yb (slab dehydration), owing to decreasing heat flow.Accretion of greenstone belts, and their buoyant harzburgiticroots, consolidated a thick subcontinental mantle lithosphereby 27 Ga, which was subsequently the source of Jurassic kimberlitesthat intruded the persistently reactivated Archean translithosphericstructures.     

西藏冈底斯南缘冲木达约30Ma埃达克质侵入岩的成因:向北俯冲的印度陆壳的熔融?

40～25 Ma之间通常被认为是拉萨地块特别是藏南冈底斯带岩浆活动的间歇期,与新特提斯洋板片断离后印度-亚洲大陆的硬碰撞有关.对出露于冈底斯东段南缘的冲木达石英二长岩-花岗闪长岩及相关的闪长质包体进行了锆石LA-ICPMS U-Pb定年和主微量元素、Sr-Nd同位素和锆石原位Hf同位素研究.年代学分析显示,侵入岩及其包...