Post-accretion Core Evolution

Post-Accretion Core Evolution is a theoretical framework in planetary science that describes the ongoing physical and chemical differentiation processes within a planet's metallic core following the cessation of primary accretion, distinguishing it from earlier stages of core formation by focusing on solidification, convection, and compositional changes driven by cooling and inner core nucleation.

52

Publications

6.3K

Citations

216

Authors

149

Institutions

Publications per year

2017–2026

19

Authors

216

  1. CW
    Chris W. Ormel

    University of Amsterdam, Netherlands

    4 publications · 156 citations

    4

    h-index

  2. TK
    T. Kleine

    University of Münster, Germany

    4 publications · 1.4K citations

    4

    h-index

  3. MG
    Marc G. Brouwers

    University of Cambridge, United Kingdom

    4 publications · 156 citations

    4

    h-index

  4. AV
    Allona Vazan

    Open University of Israel, Israel

    3 publications · 101 citations

    3

    h-index

  5. AM
    Amelia M. Stutz

    Max Planck Institute for Astronomy, Germany

    2 publications · 91 citations

    2

    h-index

1–5 of 216

Venues

  1. The Astrophysical Journal

    ApJ · 8 publications · 1.1K citations

    8

    h-index

  2. Astronomy and Astrophysics

    6 publications · 329 citations

    6

    h-index

  3. Geochimica et Cosmochimica Acta

    5 publications · 941 citations

    5

    h-index

  4. Icarus

    4 publications · 577 citations

    4

    h-index

  5. The Astrophysical Journal Letters

    3 publications · 122 citations

    3

    h-index

1–5