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地球内核中的隐匿碳通过密集 Fe7C3 的切变软化而显现。

Hidden carbon in Earth's inner core revealed by shear softening in dense Fe7C3.

机构信息

Department of Earth and Environmental Sciences, University of Michigan, Ann Arbor, MI 48109; Department of Geology, University of Illinois at Urbana-Champaign, Urbana, IL 61801; Hawaii Institute of Geophysics and Planetology, University of Hawaii at Manoa, Honolulu, HI 96822;

Department of Earth and Environmental Sciences, University of Michigan, Ann Arbor, MI 48109;

出版信息

Proc Natl Acad Sci U S A. 2014 Dec 16;111(50):17755-8. doi: 10.1073/pnas.1411154111. Epub 2014 Dec 1.

Abstract

Earth's inner core is known to consist of crystalline iron alloyed with a small amount of nickel and lighter elements, but the shear wave (S wave) travels through the inner core at about half the speed expected for most iron-rich alloys under relevant pressures. The anomalously low S-wave velocity (vS) has been attributed to the presence of liquid, hence questioning the solidity of the inner core. Here we report new experimental data up to core pressures on iron carbide Fe7C3, a candidate component of the inner core, showing that its sound velocities dropped significantly near the end of a pressure-induced spin-pairing transition, which took place gradually between 10 GPa and 53 GPa. Following the transition, the sound velocities increased with density at an exceptionally low rate. Extrapolating the data to the inner core pressure and accounting for the temperature effect, we found that low-spin Fe7C3 can reproduce the observed vS of the inner core, thus eliminating the need to invoke partial melting or a postulated large temperature effect. The model of a carbon-rich inner core may be consistent with existing constraints on the Earth's carbon budget and would imply that as much as two thirds of the planet's carbon is hidden in its center sphere.

摘要

地球的内核已知由结晶铁与少量镍和较轻元素组成,但横波(S 波)在内核中的传播速度约为相关压力下大多数富铁合金预期速度的一半。异常低的 S 波速度(vS)归因于液体的存在,因此对内核的固态性提出了质疑。在这里,我们报告了新的实验数据,直至碳化铁 Fe7C3 的内核压力,Fe7C3 是内核的候选成分,表明其声速在压力诱导的自旋配对转变结束时显著下降,该转变在 10 GPa 至 53 GPa 之间逐渐发生。转变后,声速随密度以异常低的速率增加。将数据外推到内核压力并考虑温度效应,我们发现低自旋 Fe7C3 可以再现观测到的内核 vS,从而消除了部分熔融或假定的大温度效应的需要。富含碳的内核模型可能与地球碳预算的现有限制一致,并意味着多达三分之二的行星碳隐藏在其中心球体内。

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