Perchuk A L, Gerya T V, Zakharov V S, Griffin W L
Faculty of Geology, Lomonosov Moscow State University, Moscow, 119234, Russia.
Korzhinskii Institute of Experimental Mineralogy, Russian Academy of Sciences, Chernogolovka, 142432, Russia.
Sci Rep. 2021 Nov 2;11(1):21489. doi: 10.1038/s41598-021-00837-y.
Partial melting of mantle peridotites at spreading ridges is a continuous global process that forms the oceanic crust and refractory, positively buoyant residues (melt-depleted mantle peridotites). In the modern Earth, these rocks enter subduction zones as part of the oceanic lithosphere. However, in the early Earth, the melt-depleted peridotites were 2-3 times more voluminous and their role in controlling subduction regimes and the composition of the upper mantle remains poorly constrained. Here, we investigate styles of lithospheric tectonics, and related dynamics of the depleted mantle, using 2-D geodynamic models of converging oceanic plates over the range of mantle potential temperatures (T = 1300-1550 °C, ∆T = T - T = 0-250 °C) from the Archean to the present. Numerical modeling using prescribed plate convergence rates reveals that oceanic subduction can operate over this whole range of temperatures but changes from a two-sided regime at ∆T = 250 °C to one-sided at lower mantle temperatures. Two-sided subduction creates V-shaped accretionary terrains up to 180 km thick, composed mainly of highly hydrated metabasic rocks of the subducted oceanic crust, decoupled from the mantle. Partial melting of the metabasic rocks and related formation of sodic granitoids (Tonalite-Trondhjemite-Granodiorite suites, TTGs) does not occur until subduction ceases. In contrast, one sided-subduction leads to volcanic arcs with or without back-arc basins. Both subduction regimes produce over-thickened depleted upper mantle that cannot subduct and thus delaminates from the slab and accumulates under the oceanic lithosphere. The higher the mantle temperature, the larger the volume of depleted peridotites stored in the upper mantle. Extrapolation of the modeling results reveals that oceanic plate convergence at ∆T = 200-250 °C might create depleted peridotites (melt extraction of > 20%) constituting more than half of the upper mantle over relatively short geological times (~ 100-200 million years). This contrasts with the modeling results at modern mantle temperatures, where the amount of depleted peridotites in the upper mantle does not increase significantly with time. We therefore suggest that the bulk chemical composition of upper mantle in the Archean was much more depleted than the present mantle, which is consistent with the composition of the most ancient lithospheric mantle preserved in cratonic keels.
在扩张脊处地幔橄榄岩的部分熔融是一个持续的全球过程,它形成了洋壳以及难熔的、具有正浮力的残余物(熔体亏损的地幔橄榄岩)。在现代地球,这些岩石作为大洋岩石圈的一部分进入俯冲带。然而,在早期地球,熔体亏损的橄榄岩体积要大2至3倍,它们在控制俯冲机制和上地幔成分方面的作用仍然不太明确。在这里,我们使用从太古宙到现代的一系列地幔势温度(T = 1300 - 1550°C,∆T = T - T = 0 - 250°C)范围内汇聚大洋板块的二维地球动力学模型,研究岩石圈构造样式以及亏损地幔的相关动力学。使用规定板块汇聚速率的数值模拟表明,大洋俯冲在这个整个温度范围内都能发生,但在∆T = 250°C时从双侧俯冲模式转变为下地幔温度较低时的单侧俯冲模式。双侧俯冲形成了厚度达180千米的V形增生地形,主要由俯冲洋壳高度水化的变质基性岩组成,与地幔解耦。直到俯冲停止,变质基性岩才会发生部分熔融以及相关的钠质花岗岩类(英云闪长岩 - 奥长花岗岩 - 花岗闪长岩组合,TTGs)的形成。相比之下,单侧俯冲会导致有或没有弧后盆地的火山弧。两种俯冲模式都会产生过度增厚的亏损上地幔,其无法俯冲,因此从板块上脱离并堆积在大洋岩石圈之下。地幔温度越高,上地幔中储存的亏损橄榄岩体积就越大。对模拟结果的外推表明,在∆T = 200 - 250°C时大洋板块汇聚可能会在相对较短的地质时间(约一亿至两亿年)内形成构成上地幔一半以上的亏损橄榄岩(熔体提取率> 20%)。这与现代地幔温度下的模拟结果形成对比,在现代地幔温度下,上地幔中亏损橄榄岩的数量不会随时间显著增加。因此,我们认为太古宙上地幔的总体化学成分比现代地幔贫化得多,这与克拉通地幔龙骨中保存的最古老岩石圈地幔的成分一致。