首页> 外文期刊>Journal of South American earth sciences >Calc-alkaline rear-arc magmatism in the Fuegian Andes: Implications for the mid-cretaceous tectonomagmatic evolution of southernmost South America
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Calc-alkaline rear-arc magmatism in the Fuegian Andes: Implications for the mid-cretaceous tectonomagmatic evolution of southernmost South America

机译:福伊第斯安第斯山脉中的钙碱性后岩浆作用:对南美洲最南端的中白垩纪构造岩性演化的启示

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摘要

The magmatic arc of the Fuegian Ancles is composed mostly of Upper Mesozoic to Cenozoic calc-alkaline plutons and subordinated lavas. To the rear arc, however, isolated mid-Cretaceous monzonitic plutons and small calc-alkaline dykes and sills crop out. This calc-alkaline unit (the Ushuaia Peninsula Andesites, UPA) includes hornblende-rich, porphyritic quartz meladiorites, granodiorites, andesites, dacites and lamprophyres. Radiometric dating and cross-cutting relationships indicate that UPA is younger than the monzonitic suite. The geochemistry of UPA is medium to high K, with high LILE (Ba 500-2000 ppm, Sr 800-1400 ppm), HFSE (Th 7-23 ppm, Nb 7-13 ppm, Ta 0.5-1.1 ppm) and LREE (La 16-51 ppm) contents, along with relatively low HREE (Yb 1.7-1.3 ppm) and Y (9-19 ppm). The similar mineralogy and geochemistry of all UPA rocks suggest they evolved from a common parental rnagma, by low pressure crystal fractionation, without significant crustal assimilation. A pure Rayleigh fractionation model indicates that 60-65% of crystal fractionation of 60% hornblende + 34% plagioclase + 4% clino-pyroxene +1% Fe-Ti oxide, apatite and sphene (a paragenesis similar of UPA mafic rocks) can explain evolution from lamprophyres to dacites. The UPA has higher LILE, HFSE and LREE, and lower HREE and Y than the calc-alkaline plutons and lavas of the volcanic front. The HREE and Y are lower than in the potassic plutons as well. High concentrations of Th, Nb, Ta, Zr, Hf, LREE and Ce/Pb, and low U/Th, Ba/Th ratios in UPA, even in the least differentiated samples, suggest contributions from subducted sediments to the mantle source. On the other hand, relatively low HREE and Y, high LREE/HREE (La/Yb 11-38) ratios and Nb-Ta contents can be interpreted as mantle metasomatism by partial melts of either subducted garnetiferous oceanic sediment or basalt as well. Additionally, high LILE content in UPA, similar to the potassic plutons, suggests also a mantle wedge previously metasomatized by potassic parental magmas in their route to crustal levels. Therefore, UPA represents a unique suite in the Fuegian arc generated in a multiple hybridized source. UPA generation is related to a transition from normal to flat subduction which additionally caused the widening and landward migration of the magmatic arc, as well as crustal deformation. Rear-arc magmatism endured ca. 22 m.y.; afterwards, calc-alkaline magmatism remained at the volcanic front.
机译:伏安阶角的岩浆弧主要由上中生代至新生代钙碱性岩体和次级熔岩组成。然而,到后弧,出现了孤立的白垩纪中部单晶系小行星和小的钙碱性堤坝和窗台。这个钙碱性单位(乌斯怀亚半岛安山岩,UPA)包括富含角闪石的斑状石英黑闪长岩,花岗闪长岩,安山岩,菊苣和煌斑岩。辐射定年和跨领域关系表明,UPA比单星套房还年轻。 UPA的地球化学为中高K,LILE(Ba 500-2000 ppm,Sr 800-1400 ppm),HFSE(Th 7-23 ppm,Nb 7-13 ppm,Ta 0.5-1.1 ppm)和LREE( La 16-51 ppm)含量,以及相对较低的HREE(Yb 1.7-1.3 ppm)和Y(9-19 ppm)。所有UPA岩石的相似的矿物学和地球化学表明,它们是通过低压晶体分级从普通的母体岩浆演化而来的,没有明显的地壳同化作用。纯瑞利分馏模型表明,60%角闪石+ 34%斜长石+ 4%斜向辉石+ 1%Fe-Ti氧化物,磷灰石和石的晶体分级的60-65%可以解释(类似于UPA基性岩石)从萤火虫演变为菊苣。与火山岩前缘的碱性钙质岩浆和熔岩相比,UPA的LILE,HFSE和LREE较高,而HREE和Y较低。 HREE和Y也低于钾离子体。即使在分化程度最低的样品中,UPA中高浓度的Th,Nb,Ta,Zr,Hf,LREE和Ce / Pb以及较低的U / Th,Ba / Th比也表明,俯冲沉积物对地幔源的贡献。另一方面,相对较低的HREE和Y,较高的LREE / HREE(La / Yb 11-38)比和Nb-Ta含量也可以通过俯冲的花岗石海洋沉积物或玄武岩的部分熔体解释为地幔交代作用。另外,UPA中的高LILE含量类似于钾盐岩体,也暗示了先前由钾盐父母岩浆在地壳水平过程中被交代的地幔楔。因此,UPA在多重混合源中生成的Fuegian弧中代表了唯一的套件。 UPA的产生与从正常俯冲到平坦俯冲的转变有关,这进一步导致了岩浆弧的扩大和向陆迁移以及地壳变形。后弧岩浆作用持续约下午22点;此后,钙碱性岩浆作用仍留在火山前沿。

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