Early Planetary Differentiation

Early Planetary Differentiation is a geological process paradigm in planetary science denoting the initial large-scale separation of a planet's constituent materials into chemically distinct layers—such as core, mantle, and crust—driven primarily by density contrasts and convective instabilities during the early stages of planetary formation.

79

Publications

10K

Citations

247

Authors

143

Institutions

Publications per year

2017–2026

16

Authors

247

  1. KM
    Klaus Mezger

    University of Münster, Germany

    6 publications · 2.7K citations

    6

    h-index

  2. LE
    L. E. Borg

    Lawrence Livermore National Laboratory, United States

    5 publications · 570 citations

    5

    h-index

  3. SS
    S. Sahijpal

    Panjab University, India

    4 publications · 76 citations

    4

    h-index

  4. CM
    Carsten Münker

    University of Cologne, Germany

    4 publications · 2.6K citations

    4

    h-index

  5. GK
    Gurpreet Kaur Bhatia

    Panjab University, India

    3 publications · 43 citations

    3

    h-index

1–5 of 247

Venues

  1. Earth and Planetary Science Letters

    13 publications · 988 citations

    13

    h-index

  2. Geochimica et Cosmochimica Acta

    11 publications · 892 citations

    11

    h-index

  3. Meteoritics and Planetary Science

    10 publications · 666 citations

    10

    h-index

  4. Science

    5 publications · 3.2K citations

    5

    h-index

  5. Proceedings of the National Academy of Sciences

    PNAS · 5 publications · 261 citations

    5

    h-index

1–5