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Outer-core compositional stratification from observed core wave speed profiles

Author

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  • George Helffrich

    (Earthquake Research Institute, University of Tokyo, 1-1-1 Yayoi, Bunkyo-ku, Tokyo 113-0032, Japan
    Present address: Earth Sciences, University of Bristol, Wills Memorial Building, Queen’s Road, Bristol BS8 1RJ, UK.)

  • Satoshi Kaneshima

    (Earth and Planetary Sciences, University of Kyushu, 6-10-1 Hakozaki, Higashi-ku, Fukuoka 812-8581, Japan)

Abstract

Light elements must be present in the nearly pure iron core of the Earth to match the remotely observed properties of the outer and inner cores1,2. Crystallization of the inner core excludes light elements from the solid, concentrating them in liquid near the inner-core boundary that potentially rises and collects at the top of the core3, and this may have a seismically observable signal. Here we present array-based observations of seismic waves sensitive to this part of the core whose wave speeds require there to be radial compositional variation in the topmost 300 km of the outer core. The velocity profile significantly departs from that of compression of a homogeneous liquid. Total light-element enrichment is up to five weight per cent at the top of the core if modelled in the Fe–O–S system. The stratification suggests the existence of a subadiabatic temperature gradient at the top of the outer core.

Suggested Citation

  • George Helffrich & Satoshi Kaneshima, 2010. "Outer-core compositional stratification from observed core wave speed profiles," Nature, Nature, vol. 468(7325), pages 807-810, December.
    • Handle: RePEc:nat:nature:v:468:y:2010:i:7325:d:10.1038_nature09636
    DOI: 10.1038/nature09636
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