Cooling of the Earth and core formation after the giant impact
Bernard J. Wood () and
Alex N. Halliday
Additional contact information
Bernard J. Wood: University of Bristol
Alex N. Halliday: University of Oxford
Nature, 2005, vol. 437, issue 7063, 1345-1348
Abstract:
Beat the clock One aspect of early Earth evolution that remains puzzling is the discrepancy between the more rapid formation time of the core given by the decay of hafnium to tungsten than by the clock based on the decay of uranium to lead. Wood and Halliday suggest that the explanation may be that the Hf–W clock represents the principal phase of core formation before the giant impact that formed the Moon. The upheaval introduced oxidation and the formation of a sulphur-rich metal in to which lead would have dissolved preferentially, in effect resetting the U–Pb clock to a younger date.
Date: 2005
References: Add references at CitEc
Citations: View citations in EconPapers (1)
Downloads: (external link)
https://www.nature.com/articles/nature04129 Abstract (text/html)
Access to the full text of the articles in this series is restricted.
Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.
Export reference: BibTeX
RIS (EndNote, ProCite, RefMan)
HTML/Text
Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:437:y:2005:i:7063:d:10.1038_nature04129
Ordering information: This journal article can be ordered from
https://www.nature.com/
DOI: 10.1038/nature04129
Access Statistics for this article
Nature is currently edited by Magdalena Skipper
More articles in Nature from Nature
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().