The rocky bodies from which the Earth formed may have already separated into a metal core and silicate shell. Innovative experiments exploring the behaviour of molten metal trapped between silicate grains suggest how.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
References
Yoshino, T., Walter, M. J. & Katsura, T. Nature 422, 154–157 (2003).
Yin, Q. et al. Nature 418, 949–952 (2002).
Kleine T., Münker, C., Mezger, K. & Palme, H. Nature 418, 952–955 (2002).
von Bargen, N. & Waff, H. S. J. Geophys. Res. 91, 9261–9276 (1986).
Ghosh, A. & McSween, H. Y. Icarus 134, 187–206 (1998).
Bruhn, D., Growbner, N. & Kohlstedt, D. L. Nature 403, 883–886 (2000).
Roberts, J. J., Tyburczy, J. A., Locke, D., Minarik, W. & Kinney, J. Eos 83, F400 (2002).
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Minarik, B. The core of planet formation. Nature 422, 126–127 (2003). https://doi.org/10.1038/422126a
Issue Date:
DOI: https://doi.org/10.1038/422126a