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On the Recycling of Amphibole-rich Ultramafic Intrusive Rocks in the Arc Crust: Evidence from Shikanoshima Island (Kyushu, Japan)

机译:弧形地壳中富含闪石的超镁铁质侵入岩的循环利用:来自鹿角岛(日本九州)的证据

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摘要

New insights into the role of amphibole in arc magma petrogenesis are provided by the mineral chemistry and U–Pb geochronology of Cretaceous amphibole-rich mafic rocks and associated granitoids from Shikanoshima Island (Kyushu, Japan). In the northeastern part of Shikanoshima Island a relatively large body (about 600 m in length) of amphibole-rich mafic rocks is found within granodiorite host-rocks. The core of the mafic body consists of amphibole-rich gabbrodiorite with a porphyritic texture. Towards the host granodiorite the porphyritic texture is progressively lost and a band of relatively homogeneous medium- to fine-grained mafic rock marks the boundary with the granitoid rocks. The amphibole-rich porphyritic gabbrodiorite consists of large amphibole grains (up to 60 vol. %) characterized by brown cores, occasional inclusions of clinopyroxene, and green rims. These large amphibole grains are dispersed in a fine-grained matrix consisting of green amphibole, clinopyroxene and plagioclase. Literature whole-rock data on the mafic rocks from Shikanoshima Island suggest that they are the intrusive counterparts of high-Mg andesite (HMA). Major and trace element mineral compositions reveal a marked chemical contrast between the brown amphibole (and its inclusions) and the matrix minerals, suggesting that they are not on the same liquid line of descent. The brown amphibole and its clinopyroxene inclusions were inherited from amphibole-rich ultramafic intrusive crustal rocks (e.g. hornblendites) crystallized from a melt with a chemical composition close to that of continental arc basalts. U–Pb geochronological data suggest that the xenocrystic material is about 20 Myr older than the matrix minerals. The matrix mineral crystallized from a parental liquid similar to sanukite-type HMA and with a trace element signature characterized by strong enrichment in elements with high crustal affinity and depletion in heavy rare earth elements. Green amphibole is a common mineral in all the studied lithologies; this allowed us to monitor the compositional variations in the liquid from which it crystallized moving from the core of the mafic complex to the host granodiorite. The data reveal that the interstitial melt had interacted with a melt enriched in elements with a high crustal affinity that, given the close association in the field, is inferred to be the host granitoid. These results favour an origin for sanukite-type HMA not from primary mantle melts but from mantle melts that have been affected by crustal processes and have been contaminated by crustal material. The major and trace element composition of the brown amphibole from the Shikanoshima Island mafic rocks is compared with that of brown amphibole from other amphibolite-rich intrusive rocks in orogenic settings worldwide (Alpine chain and Ross Orogen). The observed similarities suggest that the amphibole-rich mafic rocks are the expression of a magmatic process with a common geochemical affinity that is independent of the age and local geodynamic setting and thus related to a specific petrogenetic process. Amphibole-rich mafic and ultramafic intrusive rocks could be a common feature of all collisional systems and thus represent a ‘hidden’ amphibole reservoir in the arc crust. We show that amphibole plays a major role in the petrogenesis of sanukite-type HMA but is also expected to play a major role in the differentiation of many other arc magmas.
机译:来自鹿角岛(日本九州)的白垩纪富含闪石的镁铁质岩和相关的花岗岩类的矿物化学和U–Pb年代学提供了有关闪石在弧岩浆成岩作用中的作用的新见解。在鹿角岛岛的东北部,花岗闪长岩的母岩中发现了一个较大的长闪石质镁铁质岩体(长约600 m)。镁铁质体的核心是富含闪石的辉闪石辉闪石。朝向主体花岗闪长岩的斑状质地逐渐消失,相对均匀的中等粒度至细粒度的镁铁质岩带标志着花岗岩体的边界。富含闪石的斑状辉长辉石由大的闪石晶粒(最多60%(体积))组成,其特征为棕色核,偶尔夹有次氯环己烯和绿色边缘。这些大的角闪石颗粒分散在由绿色角闪石,斜向辉石和斜长石组成的细颗粒基质中。有关鹿角岛岛镁铁质岩石的全岩石文献资料表明,它们是高镁安山岩(HMA)的侵入性对应物。主要和微量元素矿物组成显示出棕色闪石(及其包裹体)与基质矿物之间存在明显的化学对比,表明它们不在同一下降液体线上。棕色闪石及其斜向辉石包裹体是从富含闪石的超镁铁质侵入性地壳岩石(例如角闪石)中继承的,该熔岩从化学成分接近大陆弧玄武岩的熔体中结晶出来。 U–Pb年代学数据表明,异相材料比基质矿物的年龄大20 Myr。母体矿物是从母液中结晶出来的,类似于色母矿型HMA,并具有痕量元素特征,其特征是具有高地壳亲和力的元素浓集和重稀土元素的耗尽。在所有研究的岩性中,绿色闪石是一种常见的矿物。这使我们能够监测从铁镁铁矿复合物核心到主体花岗闪石的结晶液体的组成变化。数据表明,间隙熔体已经与富含高地壳亲和力元素的熔体发生了相互作用,鉴于该领域的紧密联系,可以推断其为宿主花岗岩。这些结果有利于红宝石型HMA的起源,而不是来自原始地幔熔体,而是来自受地壳过程影响并被地壳物质污染的地幔熔体。在全球造山环境(高山链和罗斯造山带)中,比较了鹿角岛岛镁铁质岩石的棕色闪石的主要和微量元素组成与其他富角闪石侵入性岩石的棕色闪石的主要和微量元素组成。观察到的相似性表明,富含闪石的镁铁质岩体是岩浆过程的一种表现形式,具有共同的地球化学亲和力,与年龄和局部地球动力学环境无关,因此与特定的成岩过程有关。富含闪石的镁铁质和超镁铁质侵入岩可能是所有碰撞系统的共同特征,因此代表了地壳中“隐藏的”闪石储层。我们表明,闪石在Sanukite型HMA的岩石成因中起主要作用,但也有望在许多其他弧状岩浆的分化中起主要作用。

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    《Journal of Petrology》 |2012年第6期|p.1255-1285|共31页
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    1CNR–Istituto Di Geoscienze E Georisorse–Uos Di Pavia, Pavia, Italy 2CNR–Istituto Di Geoscienze E Georisorse–Pisa, Pisa, Italy 3Frontier Science Organisation, Kanazawa University, Kanazawa, Japan 4Department of Earth System Science, Fukuoka University, Fukuoka, Japan;

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