Metal-silicate Segregation
Metal-Silicate Segregation is a geophysical process in planetary differentiation whereby molten metallic components, primarily iron and nickel, separate from silicate minerals due to density differences and gravitational settling, leading to the formation of a metallic core and a silicate mantle during the early accretion and heating phases of terrestrial planet formation.
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2017–2026
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Metal/silicate fractionation in the solar system
John S. Lewis · Earth and Planetary Science Letters · 1972 · 342 citations
G. Budde, Christoph Burkhardt, G. A. Brennecka et al. · Earth and Planetary Science Letters · 2016 · 285 citations · Full text
K. Righter, M. J. Drake, Gregory M. Yaxley · Physics of The Earth and Planetary Interiors · 1997 · 247 citations
Natural Sciences, Materials Engineering, Materials Science +15
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Centre National de la Recherche Scientifique
Paris, France
21 h-index
69 publications
4.9K citations
Planetary Science Institute
Tucson, United States
13 h-index
21 publications
1.7K citations

Carnegie Institution for Science
Washington, United States
12 h-index
19 publications
1.7K citations
University of Bayreuth
Bayreuth, Germany
12 h-index
28 publications
2.4K citations

Institut de physique du globe de Paris
Paris, France
11 h-index
25 publications
1.6K citations
University of Arizona
Tucson, United States
11 h-index
20 publications
1.7K citations
Johnson Space Center
Houston, United States
8 h-index
17 publications
998 citations
University of Oxford
Oxford, United Kingdom
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22 publications
1.3K citations
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