Hf/W Isotopic Evolution from N-Body Accretion Simulations: Constraints on Equilibration Processes During Large Impacts

Details Hf/W Isotopic Evolution from N-Body Accretion Simulations: Constraints on Equilibration Processes During Large Impacts Hf/W Isotopic Evolution from N-Body Accretion Simulations: Constraints on Equilibration Processes During Large Impacts

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1390n&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1390

Physics

Scientific paper

We incorporate Hf/W isotopic evolution calculations into an N-body
accretion code. Matching the observations requires that even the largest
impactors undergo re-equilibration with the target mantle.

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