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首页> 外文期刊>Earth and Planetary Science Letters: A Letter Journal Devoted to the Development in Time of the Earth and Planetary System >Remnants of a fossil alluvial fan landscape of Miocene age in the Atacama Desert of northern Chile using cosmogenic nuclide exposure age dating
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Remnants of a fossil alluvial fan landscape of Miocene age in the Atacama Desert of northern Chile using cosmogenic nuclide exposure age dating

机译:智利北部阿塔卡马沙漠中新世时代化石冲积扇化景观的残余物,利用宇宙成因核素暴露年龄定年

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We have used cosmogenic nuclides to estimate limits on the surface exposure durations and erosion rates of alluvial fans and bedrock surfaces in the Atacama Desert in Chile. The oldest landforms we studied are extensive alluvial fans referred to as "Atacama gravels". With the exception of samples collected in Antarctica, the cobbles collected on these alluvial surfaces have the lowest erosion rates of any samples, as determined by cosmogenic nuclides, analyzed to date. The oldest cobble has a model surface exposure age of 9 Myr, based on combined measurements of cosmogenic Be-10, Al-26, and Ne-21 concentrations. Cobbles from the alluvial fans are eroding slower than the surrounding steep mountainous bedrock surfaces. Maximum erosion rates for cobbles on alluvial surfaces are uniformly < 0.1 m/Myr. The survival of these gravels, specifically, and more generally, the stability of landform features in this geographic area is made possible by the attaimnent of hyperarid conditions in the Atacama Desert resulting from global climatic cooling about 15 Myr ago combined with the rain shadow effect caused by uplift of the Central Andes. The landform features observed presently in the Atacama Desert are remarkably stable and, despite the inevitable erosion that is detectable using cosmogenic nuclides, undoubtedly bear considerable resemblance to conditions as they existed in the Miocene. Over geologic time, the Atacama landscape is evolving in such a manner as to erode the higher bedrock ridges relative to the more stable, but stratigraphically lower depositional surfaces through which elastic detritus now travels occasionally along the floors of incised drainage systems leaving the older permeable alluvial fan surfaces largely intact as widespread remnants of a Miocene fossil landscape. (c) 2005 Elsevier B.V. All rights reserved.
机译:我们已使用宇宙成因核素来估计智利阿塔卡马沙漠中地表暴露持续时间以及冲积扇和基岩表面侵蚀速率的极限。我们研究过的最古老的地貌是被称为“阿塔卡马砾石”的大量冲积扇。迄今为止,除在南极洲收集的样品外,在这些冲积表面收集的卵石的腐蚀速率是所有样品中腐蚀率最低的,这是由宇宙成因核素确定的。根据对宇宙产生的Be-10,Al-26和Ne-21浓度的综合测量,最古老的鹅卵石的模型表面暴露年龄为9 Myr。冲积扇的卵石侵蚀的速度比周围陡峭的山区基岩表面要慢。冲积表面上鹅卵石的最大腐蚀速率一致地<0.1 m / Myr。这些砂砾的生存,尤其是更普遍的说,是由于大约15 Myr之前的全球气候变冷以及雨影效应造成的阿塔卡马沙漠中高干旱条件的存在,才使该地理区域的地貌特征得以稳定。通过安第斯山脉中部的隆升。目前在阿塔卡马沙漠中观察到的地貌特征非常稳定,尽管使用宇宙成因核素可以检测到不可避免的侵蚀,但毫无疑问,它们与中新世存在的条件十分相似。在地质时期内,阿塔卡马景观的演变方式是侵蚀较高的基岩山脊,而不是相对稳定但地层较低的沉积面,弹性碎屑现在偶尔会沿着切开的排水系统的底面行进,从而留下较旧的渗透性冲积层。扇面基本上完好无损,是中新世化石景观的广泛残留物。 (c)2005 Elsevier B.V.保留所有权利。

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