Origin of Nucleosynthetic Isotope Heterogeneity in the Solar Nebula Inferred from Mo and W Isotopes in Acid Leachates from Murchison

Details Origin of Nucleosynthetic Isotope Heterogeneity in the Solar Nebula Inferred from Mo and W Isotopes in Acid Leachates from Murchison Origin of Nucleosynthetic Isotope Heterogeneity in the Solar Nebula Inferred from Mo and W Isotopes in Acid Leachates from Murchison

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2405b&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2405

Physics

1

Scientific paper

The first W-isotopic data of chondrite leachates are presented.
Implications for the distribution of nucleosynthetic carriers, the
origin of planetary-scale nucleosynthetic anomalies, and the solar
system initial ɛ^1^8^2W are discussed.

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