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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 >Long-term preservation of early formed mantle heterogeneity by mobile lid convection: Importance of grainsize evolution
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Long-term preservation of early formed mantle heterogeneity by mobile lid convection: Importance of grainsize evolution

机译:移动盖对流的长期保存早期形成的地幔异质性:谷物进化的重要性

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The style of tectonics on the Hadean and Archean Earth, particularly whether plate tectonics was in operation or not, is debated. One important, albeit indirect, constraint on early Earth tectonics comes from observations of early-formed geochemical heterogeneities: Nd-142 and W-182 anomalies recorded in Hadean to Phanerozoic rocks from different localities indicate that chemically heterogeneous reservoirs, formed during the first similar to 500 Myrs of Earth's history, survived their remixing into the mantle for over 1 Gyrs. Such a long mixing time is difficult to explain because hotter mantle temperatures, expected for the early Earth, act to lower mantle viscosity and increase convective vigor. Previous studies found that mobile lid convection typically erases heterogeneity within similar to 100 Myrs under such conditions, leading to the hypothesis that stagnant lid convection on the early Earth was responsible for the observed long mixing times. However, using two-dimensional Cartesian convection models that include grainsize evolution, we find that mobile lid convection can preserve heterogeneity at high mantle temperature conditions for much longer than previously thought, because higher mantle temperatures lead to larger grainsizes in the lithosphere. These larger grainsizes result in stronger plate boundaries that act to slow down surface and interior convective motions, in competition with the direct effect temperature has on mantle viscosity. Our models indicate that mobile lid convection can preserve heterogeneity for approximate to 0.4-1 Gyrs at early Earth mantle temperatures when the initial heterogeneity has the same viscosity as the background mantle, and approximate to 1-4 Gyrs when the heterogeneity is ten times more viscous than the background mantle. Thus, stagnant lid convection is not required to explain long-term survival of early formed geochemical heterogeneities, though these heterogeneities having an elevated viscosity compared to the surrounding mantle may be essential for their preservation. (C) 2017 Elsevier B.V. All rights reserved.
机译:在冥古宙和地球构造运动的风格,板块尤其是是否在运行与否,辩论。在早期的地球构造学的一个重要的,虽然是间接的,约束来自于早期形成的地球化学非均质性意见:钕142,并记录在冥古以显生宙岩石W-182的异常从不同的地方表明,化学非均质储层,在第一近似形成地球历史的500米儿丝,克服了它们混音到地幔超过1 Gyrs。这么长的混合时间是难以解释的,因为较热的地幔温度,预计早期地球,作用于下地幔粘性,增加对流活力。先前的研究发现,移动盖子对流通常擦除内这样的条件下类似于100米儿丝异质性,导致假设,即早期地球停滞盖对流负责观察到的长的混合时间。然而,使用二维笛卡尔对流模型,包括粒度大小演变,我们发现移动的盖子对流可以保持在较高的地幔温度条件下异质性比以前认为的要长得多,因为较高的温度地幔导致岩石圈大grainsizes。这些较大的grainsizes导致在作用于表面和内部对流运动减速,与直接的影响温度的竞争已经上地幔粘性较强板的边界。我们的模型表明,移动盖子对流可在早期地球地幔的温度保持为近似的异质性,以0.4-1 Gyrs当初始异质具有相同的粘度为背景套和近似至1-4 Gyrs当异质性是十倍更粘稠比背景地幔。因此,不需要停滞盖对流解释早期形成地球化学非均质的长期存活,虽然具有提高粘度比周围的地幔可以是用于它们的保存必要这些异质性。 (c)2017年Elsevier B.V.保留所有权利。

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