Improved Constraints on the Relative Timing of Metal Segregation in the Early Solar System Using Coupled W-Os Isotopes

Details Improved Constraints on the Relative Timing of Metal Segregation in the Early Solar System Using Coupled W-Os Isotopes Improved Constraints on the Relative Timing of Metal Segregation in the Early Solar System Using Coupled W-Os Isotopes

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1166w&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1166

Physics

Scientific paper

^1^8^2W has been used to place age constraints on early metal-silicate
segregation. New high-precision W measurements, coupled with Os-isotope
constraints on cosmic ray exposure history, allow small differences in
ages among iron groups to be resolved.

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