首页> 外文期刊>Journal of Volcanology and Geothermal Research >The Late Miocene-Quaternary Antofalla volcanic complex, southern Puna, NW Argentina: Protracted history, diverse petrology, and economic potential
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The Late Miocene-Quaternary Antofalla volcanic complex, southern Puna, NW Argentina: Protracted history, diverse petrology, and economic potential

机译:阿根廷西北部普纳南部中新世-第四纪晚安托法拉火山综合体:悠久的历史,多样的岩石学和经济潜力

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The Antofalla volcanic complex (AVC) is located on the southern Puna plateau of NW Argentina, ~100 km east of the main axis of the Cordillera Occidental volcanic arc. It lies on the NW-SE Archibarca lineament, one of several transverse structures that cut across the Andes from Chile, and divert arc magmatism in SE-trending fingers across the Puna. ~(40)Ar/~(39)Ar dating of volcanic products from the AVC reveals a protracted magmatic history from 10.9 to ≤ 1.6 Ma. Initial volcanism was characterized by eruption of voluminous rhyolitic ignimbrites, deposited directly onto exposed crystalline basement and supracrustal sedimentary rocks. These rhyolites record significant geochemical evidence for crustal contamination, or derivation by crustal melting, which decreases upwards through the pyroclastic sequence. They were followed by extrusion of potassic lavas of the shoshonite-latite-trachydacite suite from 10.1 to 9.5 Ma. Subsequent magmatism (9.1-1.6 Ma) was of basaltic andesite-andesite-dacite composition, with localized, smaller volume, dacitic and rhyolitic ignimbrites. Monogenetic basaltic andesite cinder cones and lava flows were erupted in the Quaternary in response to a change to transtensional tectonics in the Puna. The volcanic sequence is interpreted to record the early development of a lower crustal MASH zone at ~11 Ma, where mantle-derived arc magmas interacted extensively with felsic lower crustal rocks to produce evolved shoshonitic compositions, and crustal melts that erupted to form rhyolitic ignimbrites (common at this time throughout the Puna). After establishment of a steady-state MASH zone by ~9 Ma, subsequent basaltic andesite-andesite magmas show less evidence of felsic crustal contamination, and may have developed largely by interaction with previous ultramafic-mafic fractionates of early magmas in the lower crust. More felsic dacitic magmas appear to have evolved largely by fractional crystallization from basaltic andesites and andesites, with widespread evidence of mixing and mingling between magmas of different degrees of differentiation. Some contamination by upper crustal components is also evident in these dacites, but is shown more clearly by small-volume rhyolites, some of which may again represent predominantly crustal melts. Epithermal deposits of Au and Pb-Zn-Ag occur within the AVC, apparently associated with the formation of rhyolite domes. The mineralization style is typical of other Andean volcanic centres, and may be underlain by deeper-seated porphyry-styles of mineralization. Extensive blanketing by younger lavas and limited erosiori restricts exposure of these altered and mineralized sequences, however, although the potential for further discoveries beneath cover or at depth in this system appears high.
机译:安托法拉火山综合体(AVC)位于阿根廷西北部南部的普纳高原,距离科迪勒拉西部火山弧主轴线以东约100公里。它位于NW-SE Archibarca上,这是从智利横穿安第斯山脉的几种横向结构之一,并且将SE趋势手指上的弧岩浆转移到了Puna上。 AVC火山产物的〜(40)Ar /〜(39)Ar年代测定揭示了从10.9到≤1.6 Ma的长期岩浆历史。最初的火山作用的特征是大量流纹岩火成岩的喷发,直接沉积在裸露的结晶基底和上壳沉积岩上。这些流纹岩记录了重要的地球化学证据,表明地壳受到污染,或因地壳融化而衍生,在整个火山碎屑序列中逐渐降低。他们之后是从10.1到9.5 Ma的钾长石-latite-次长晶石套件的钾熔岩挤出。随后的岩浆活动(9.1-1.6 Ma)为玄武质安山岩-安山岩-针铁矿组成,局部,体积较小,为高铁和流纹岩的火成岩。第四纪的第四纪爆发了单相玄武质安山岩煤渣锥和熔岩流,这是由于Puna的张性构造变化所致。火山序列被解释为记录了约11 Ma的下地壳MASH带的早期发育,其中地幔衍生的弧形岩浆与长英质下地壳岩石广泛相互作用,产生了演化的钾钾铁质成分,地壳熔体喷出形成流纹岩火成岩(目前在整个Puna中都很常见)。在约9 Ma建立一个稳态MASH区后,随后的玄武质安山岩-安山岩岩浆显示出长笛质壳污染的证据较少,并且可能主要是与下地壳中早期岩浆的早期超镁铁质-镁铁质组分相互作用而形成的。越来越多的长英质岩浆岩似乎是通过玄武质安山岩和安山岩的分步结晶演化而来的,广泛证据表明不同分化程度的岩浆之间混合混合。在这些数据中,上地壳成分也有一些污染,但小体积流纹岩则更清楚地表明,其中一些可能再次代表了地壳熔体。 Au和Pb-Zn-Ag的超热沉积发生在AVC内,显然与流纹岩穹顶的形成有关。矿化风格是其他安第斯火山中心的典型特征,并且可能是深层斑岩型矿化的基础。较年轻的熔岩广泛覆盖和有限的埃罗索雷伊限制了这些变化和矿化的层序的暴露,尽管在该系统的掩盖下或深处进一步发现的可能性很高。

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