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Équipe de Minéralogie, Institut de Minéralogie et de
Physique
des Milieux Condensés, Institut de Physique du Globe de
Paris
UMR CNRS 7590, Université Pierre et Marie
Curie
Université Denis Diderot, 4 Place Jussieu, 75252 Paris,
France
E-mail:
guillaume.fiquet{at}impmc.jussieu.fr
Équipe de Minéralogie, Institut de Minéralogie et de
Physique
des Milieux Condensés, Institut de Physique du Globe de
Paris
UMR CNRS 7590, Université Pierre et Marie
Curie
Université Denis Diderot, 4 Place Jussieu, 75252 Paris,
France
More than 90 percent of the Earth's mass is composed of iron, oxygen, silicon and magnesium, distributed among a metal-rich core, a silicate-rich mantle and more highly fractionated crustal rocks (less than 1% of the total). Mantle and core compositions can be approximated quite easily provided the bulk-Earth composition is assumed to be the same as that of appropriate meteorites. Critical mineral-physics data, some of which are reviewed in this article, are then needed to develop viable compositional and thermal Earth models, thus leading to a better knowledge of the deepest rocks in the Earth.
KEYWORDS: mantle, core, differentiation, chondrites
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