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Titanium isotopes constrain a magmatic transition at the Hadean-Archean boundary in the Acasta Gneiss Complex

机译:钛同位素限制了Acasta Gneiss复合物的HAREAN-Archean边界的岩浆过渡

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Plate subduction greatly influences the physical and chemical characteristics of Earth’s surface and deep interior, yet the timing of its initiation is debated because of the paucity of exposed rocks from Earth’s early history. We show that the titanium isotopic composition of orthogneisses from the Acasta Gneiss Complex spanning the Hadean to Eoarchean transition falls on two distinct magmatic differentiation trends. Hadean tonalitic gneisses show titanium isotopic compositions comparable to modern evolved tholeiitic magmas, formed by differentiation of dry parental magmas in plume settings. Younger Eoarchean granitoid gneisses have titanium isotopic compositions comparable to modern calc-alkaline magmas produced in convergent arcs. Our data therefore document a shift from tholeiitic- to calc-alkaline–style magmatism between 4.02 and 3.75 billion years (Ga) in the Slave craton.
机译:板削架极大地影响了地球表面和深层内部的物理和化学特征,但其启动的时间是由于地球早期历史上暴露的岩石缺乏的争论。 我们表明,来自Acasta Gneiss复杂的正交性的钛同位素组成遍布HAREAN到EOACHEAN过渡的两种不同的岩石分化趋势。 HARALONITITALESES显示与现代进化的烟草岩浆相当的钛同位素组合物,通过在羽流环境中的干父母岩浆的分化形成。 较年轻的Eoarchean Granitoid片状物具有与在会聚弧中产生的现代钙碱磁带相当的钛同位素组合物。 因此,我们的数据文件记录了从奴隶Craton的4.02和375亿年(GA)之间的山金族 - 钙碱式岩浆岩。

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