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Shock compression of Fe-Ni-Si system to 280 GPa: Implications for the composition of the Earth's outer core

机译:Fe-Ni-Si系统的冲击压缩至280 GPa:对地球外核成分的影响

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The shock Hugoniot of an Fe-9 wt %Ni-10 wt %Si system as a model of the Earth's core has been measured up to -280 GPa using a two-stage light-gas gun. The samples had an average density of 6.853 (±0.036) g/cm~3. The relationship between shock velocity (U_s) and particle velocity (u_p) can be described by U_s (km/s) = 3.95 (±0.15) + 1.53 (±0.05) u_p (km/s). The calculated Hugoniot temperatures and the melting curve indicate that the model composition melts above a shock pressure of ~168GPa, which is significantly lower than the shock-melting pressure of iron (-225 GPa). A comparison of the pressure-density (P-p) profiles between the model composition and the preliminary reference Earth model gives a silicon content close to 10wt %, necessary to compensate the density deficit in the Earth's outer core from seismological observations, if silicon is present as a major light element in the Fe-Ni core system.
机译:Fe-9wt%Ni-10wt%Si系统作为地球核心的模型的冲击休格尼奥特已经使用两级轻气枪测量了高达-280 GPa的压力。样品的平均密度为6.853(±0.036)g / cm〜3。冲击速度(U_s)和质点速度(u_p)之间的关系可以用U_s(km / s)= 3.95(±0.15)+ 1.53(±0.05)u_p(km / s)来描述。计算出的Hugoniot温度和熔化曲线表明,模型成分在〜168GPa的冲击压力以上熔化,该压力明显低于铁的冲击熔化压力(-225 GPa)。比较模型组成和初步参考地球模型之间的压力密度(Pp)曲线,可以得出硅含量接近10wt%,这是补偿地震观测中地球外核密度不足的必要条件(如果存在硅) Fe-Ni芯系统中的主要轻元素。

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