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Updated: May 12, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
Published on: November 16, 2013
R Bastian Georg1, Alex N Halliday, Edwin A Schauble
1Department of Earth Sciences, University of Oxford, South Parks Road, Oxford OX1 3PR, UK.
Planetary silicate rocks show distinct silicon isotope differences. These variations suggest silicon was incorporated into Earth's core before the Moon formed, challenging evaporation theories.
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