首页> 外文期刊>Journal of South American earth sciences >The U-Pb and Hf isotope evidence of detrital zircons of the Ordovician Ollantaytambo Formation, southern Peru, and the Ordovician provenance and paleogeography of southern Peru and northern Bolivia
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The U-Pb and Hf isotope evidence of detrital zircons of the Ordovician Ollantaytambo Formation, southern Peru, and the Ordovician provenance and paleogeography of southern Peru and northern Bolivia

机译:秘鲁南部奥陶纪Ollantaytambo组碎屑锆石的U-Pb和Hf同位素证据,以及秘鲁南部和玻利维亚北部的奥陶纪物源和古地理

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The Ordovician Ollantaytambo Formation represents one of only two known occurrences of Lower Paleozoic volcanic rocks in southern Peru and northern Bolivia. Its lower part consists of mafic lapilli tuffs, shales and mature sandstones form the upper part. We present LA-ICP-MS U-Pb ages and Hf isotope data of detrital zircons from one of the upper member sandstones in order to determine both the duration of volcanism and the provenance of the mature detritus, and to use the data to further define the paleogeography of the Ordovician basin in the northern Central Andes. The detrital zircon ages of the Ollantaytambo Formation range from 2013 Ma to 445 Ma. They are grouped mainly between 1400 and 1100 Ma (35%), 1100 and 900 Ma (14%), 770 and 650 Ma (14%), and from 500 Ma to 440 Ma (30%). Within these groups the main peaks are at 1249 Ma, 1052 Ma, 741 Ma and 459 Ma. The older groups correspond to major orogenic cycles recorded on the southwestern Amazonia craton, the Rondonia-San Ignacio, Sunsas, and Brasiliano orogenies. The younger one reflects the activity of the Early Paleozoic Famatinian magmatic arc known mainly from the southern Central Andes, but also recognized on the Arequipa Massif and in northern Peru. The provenance of the grains with ages between 770 Ma and 650 Ma is enigmatic as there are no known sources in southwestern Amazonia or the Central Andes. The εHf(t) values of selected Ollantaytambo Formation zircons are between -22 and +3 and considered to be moderately juvenile to evolved. Truely juvenile zircons with a composition similar to the depleted mantle were not identified. Together with additional literature data from Ordovician formations in southern Peru, the Hf-isotope data indicate production of juvenile crust mainly in the Mesoproterozoic, and increasing recycling of this crust during the Neoproterozoic and Early Paleozoic orogenic events.
机译:奥陶纪的Ollantaytambo组是秘鲁南部和玻利维亚北部仅两个已知的下古生界火山岩之一。它的下部由镁铁矿凝灰岩,上部的页岩和成熟的砂岩组成。为了确定火山活动的持续时间和成熟碎屑物的来源,我们提供了来自上层成员砂岩之一的碎屑锆石的LA-ICP-MS U-Pb年龄和Hf同位素数据,并使用这些数据进一步定义安第斯中部北部奥陶纪盆地的古地理。 Ollantaytambo组的碎屑锆石年龄从2013 Ma到445 Ma。它们主要分为1400至1100 Ma(35%),1100至900 Ma(14%),770至650 Ma(14%)和500 Ma至440 Ma(30%)。在这些组中,主要峰位于1249 Ma,1052 Ma,741 Ma和459 Ma。年龄较大的组对应于西南亚马孙克拉通,朗多尼亚-圣伊格纳西奥,桑萨斯和巴西利亚诺造山运动中记录的主要造山运动周期。较年轻的一个反映了早古生代的法马提尼岩浆弧的活动,该弧主要从安第斯中部南部已知,但在阿雷基帕断层块和秘鲁北部也得到认可。年龄在770 Ma至650 Ma之间的谷物的起源是神秘的,因为在西南亚马逊地区或安第斯中部尚无已知来源。选定的Ollantaytambo组锆石的εHf(t)值在-22和+3之间,被认为是适中的幼稚动物。并未鉴定出组成与枯竭地幔相似的真正锆石。 Hf同位素数据与秘鲁南部奥陶纪地层的其他文献数据一起显示,幼壳主要在中元古代生产,并且在新元古代和早古生代造山活动中这种壳的循环利用不断增加。

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