Testing the Homogeneity of the Solar System for Iron (54, 56, 57, and 58) and Tungsten (182, 183, 184, and 186) Isotope Abundances

Details Testing the Homogeneity of the Solar System for Iron (54, 56, 57, and 58) and Tungsten (182, 183, 184, and 186) Isotope Abundances Testing the Homogeneity of the Solar System for Iron (54, 56, 57, and 58) and Tungsten (182, 183, 184, and 186) Isotope Abundances

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1498d&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1498

Computer Science

3

Scientific paper

The solar nebula was homogenized at a planetary scale at the 0.2 epsilon
and 0.5 epsilon level for iron-56 and iron-58, respectively. Preliminary
results seem to indicate the presence of a s-process tungsten component
in leaching experiments of primitive meteorites.

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