Multistage Core Formation in Planetesimals Revealed by Numerical Modeling and Hf-W Chronometry of Iron Meteorites

Author:

Neumann W.12ORCID,Kruijer T. S.13,Breuer D.2ORCID,Kleine T.1

Affiliation:

1. Institut für Planetologie; University of Münster; Münster Germany

2. Institut für Planetenforschung; Deutsches Zentrum für Luft- und Raumfahrt (DLR); Berlin Germany

3. Nuclear and Chemical Sciences Division; Lawrence Livermore National Laboratory; Livermore CA USA

Funder

U.S. DOE by Lawrence Livermore National Laboratory

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference75 articles.

1. Reference data for the density and viscosity of liquid aluminum and liquid iron;Assael;Journal of Physical and Chemical Reference Data,2006

2. Pyroxenes from non-carbonaceous chondritic meteorites;Binns;Mineralogical Magazine,1970

3. The impact of nebular evolution on volatile depletion trends observed in differentiated objects;Bland;41st Lunar and Planetary Science Conference, Abstract 1817,2010

4. Iron meteorites as remnants of planetesimals formed in the terrestrial planet region;Bottke;Nature,2006

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