Constraining the composition, core sizes and thermal state of the Moon for the models of the magma ocean

Details Constraining the composition, core sizes and thermal state of the Moon for the models of the magma ocean Constraining the composition, core sizes and thermal state of the Moon for the models of the magma ocean

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf...16k&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.16

Mathematics

Scientific paper

In the present work, we suggest a new model of constitution and internal
structure of the Moon. This model is based on the hypothesis of chemical
differentiation of the Moon as a result of partial melting of initially
homogeneous material (hypothetical magma ocean); it involves modern
mathematical processing of the P - and S-velocities [1, 6].

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