A W-Isotope Evolution Model with a Deep Magma Ocean and a Solid Lower Mantle: Application to Mars and Earth

Details A W-Isotope Evolution Model with a Deep Magma Ocean and a Solid Lower Mantle: Application to Mars and Earth A W-Isotope Evolution Model with a Deep Magma Ocean and a Solid Lower Mantle: Application to Mars and Earth

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1847y&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

1

Scientific paper

A core-formation model with a deep magma ocean and a solid lower mantle
has been formulated for the Hf-W system. Based on this model, W isotope
data of martian meteorites imply that the mean age of Mars is 0.3-1.6
m.y. after the formation of the solar system.

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