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Constraints on Core Composition from Shock-Wave Data

Ahrens, T. J. (1982) Constraints on Core Composition from Shock-Wave Data. Philosophical Transactions A: Mathematical, Physical and Engineering Sciences, 306 (1492). pp. 37-47. ISSN 1364-503X. https://resolver.caltech.edu/CaltechAUTHORS:20141103-142818323

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Abstract

Seismic data demonstrate that the density of the liquid core is some 8-10 % less than pure iron. Equations of state of Fe-Si, C, FeS_2, FeS, KFeS_2 and FeO, over the pressure interval 133-364 GPa and a range of possible core temperatures (3500-5000 K), can be used to place constraints on the cosmochemically plausible light element constituents of the core (Si, C, S, K and O). The seismically derived density profile allows from 14 to 20 % Si (by mass) in the outer core. The inclusion of Si, or possibly C (up to 11 %), in the core is possible if the Earth accreted inhomogeneously within a region of the solar nebulae in which a C:O (atomic) ratio of about 1 existed, compared with a C:O ratio of 0.6 for the present solar photosphere. In contrast, homogeneous accretion permits Si, but not C, to enter the core by means of reduction of silicates to metallic Fe-Si core material during the late stages of the accumulation of the Earth. The data from the equation of state for the iron sulphides allow up to 9-13 % S in the core. This composition would provide the entire Earth with a S:Si ratio in the range 0.14-0.3, comparable with meteoritic and cosmic abundances. Shock-wave data for KFeS_2 give little evidence for an electronic phase change from 4s to 3d orbitals, which has been suggested to occur in K, and allow the Earth to store a cosmic abundance of K in the metallic core.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1098/rsta.1982.0064 DOIArticle
http://rsta.royalsocietypublishing.org/content/306/1492/37PublisherArticle
Additional Information:© 1982 Royal Society of London. Published 20 August 1982. I appreciated the opportunity to present this material to a critical audience. The work was supported by N.S.F. grant no. EAR-79-26384. Contribution number 3753, Division of Geological and Planetary Sciences, California Institute of Technology.
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Funding AgencyGrant Number
NSFEAR-79-26384
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Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences3753
Issue or Number:1492
Record Number:CaltechAUTHORS:20141103-142818323
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20141103-142818323
Official Citation:T. J. Ahrens Constraints on Core Composition from Shock-Wave Data Phil. Trans. R. Soc. Lond. A August 20, 1982 306 1492 37-47; doi:10.1098/rsta.1982.0064
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:51191
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:03 Nov 2014 22:37
Last Modified:03 Oct 2019 07:30

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