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.

147

Publications

10.4K

Citations

403

Authors

187

Institutions

Publications per year

2017–2026

39

Authors

403

  1. KR
    K. Righter

    Johnson Space Center, United States

    9 publications · 856 citations

    9

    h-index

  2. MJ
    M. J. Drake

    University of Arizona, United States

    9 publications · 888 citations

    9

    h-index

  3. BJ
    Bernard J. Wood

    University of Bristol, United Kingdom

    8 publications · 771 citations

    8

    h-index

  4. DC
    D. C. Rubie

    University of Bayreuth, Germany

    8 publications · 793 citations

    8

    h-index

  5. WV
    W. van Westrenen

    Vrije Universiteit Amsterdam, Netherlands

    7 publications · 334 citations

    7

    h-index

1–5 of 403

Venues

  1. Geochimica et Cosmochimica Acta

    44 publications · 3.6K citations

    35

    h-index

  2. Earth and Planetary Science Letters

    31 publications · 2.7K citations

    26

    h-index

  3. Science

    8 publications · 757 citations

    8

    h-index

  4. Meteoritics and Planetary Science

    6 publications · 173 citations

    6

    h-index

  5. Geophysical Research Letters

    5 publications · 217 citations

    5

    h-index

1–5