地球地核形成中的金属-硅酸盐平衡。

E. Ohtani
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引用次数: 0

摘要

岩浆海中分离的金属液滴半径小于1cm,在岩浆海中分离大约需要106秒。积聚在岩浆海底部的金属液体,当金属液滴生长到半径约1km时,开始落入下地幔。本文的理论分析表明,落入熔融岩浆海的小金属液滴与硅酸盐岩浆海在热化学上处于平衡状态,而落入下地幔的大金属液滴则与周围的硅酸盐岩浆海处于不平衡状态。因此,从金属-硅酸盐平衡的条件估计岩浆海的深度是可能的。地幔中镍和钴的丰度可以用金属和硅酸盐在40 GPa和2500℃的化学平衡来解释,表明存在深度为1200 km的原始陆相岩浆海洋。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Metal-Silicate Equilibrium in the Core Formation of the Earth.
Metal droplets separating in the magma ocean have the radius less than 1cm, and it takes about 106 seconds to separate in the magma ocean. Metallic liquid accumulated in the bottom of the magma ocean starts to fall into the lower mantle when the metal drops grow into the radius of about 1km. The present theoretical analysis implies that the small metal droplets falling into the molten magma ocean are thermally and chemically in equilibrium with the silicate magma ocean, whereas the large metal pools falling in the lower mantle are disequilibrium with the surrounding silicates. Therefore it may be possible to estimate the depth of the magma ocean from the conditions of the metal-silicate equilibrium. Abundances of Ni and Co in the mantle may be accounted for by the chemical equilibrium between metal and silicate at 40 GPa and 2500°C, suggesting existence of the primordial terrestrial magma ocean with the depth of 1200 km.
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