Meteoritic Isotopic Abundance Effects from R-Process Jets

Details Meteoritic Isotopic Abundance Effects from R-Process Jets Meteoritic Isotopic Abundance Effects from R-Process Jets

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1112c&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1112

Physics

1

Scientific paper

Supernovas of the kind that triggered the formation of the solar nebula,
through their r-process jets, appear to have provided distinct
meteoritic abundance signatures: r-process peaks at xenon and the rare
earth hump, and a p-process peak at Mo and Ru.

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