Impact-driven Core Formation

Impact-Driven Core Formation is a theoretical framework within planetary science that explains the differentiation of metallic cores in terrestrial planets through high-energy impact events as the primary mechanism driving mass segregation and core accretion.

203

Publications

15.4K

Citations

582

Authors

263

Institutions

Publications per year

2017–2026

47

Authors

582

  1. CA
    C. A. Raymond

    Jet Propulsion Laboratory, United States

    6 publications · 576 citations

    6

    h-index

  2. DP
    D. P. O’Brien

    Planetary Science Institute, United States

    6 publications · 588 citations

    6

    h-index

  3. WF
    W. F. Bottke

    Southwest Research Institute, United States

    6 publications · 996 citations

    6

    h-index

  4. RM
    R. M. Canup

    Southwest Research Institute, United States

    6 publications · 1.2K citations

    6

    h-index

  5. DL
    D. L. Buczkowski

    Johns Hopkins University Applied Physics Laboratory, United States

    5 publications · 397 citations

    5

    h-index

1–5 of 582

Venues

  1. Icarus

    36 publications · 2.9K citations

    27

    h-index

  2. Nature

    13 publications · 2.3K citations

    13

    h-index

  3. The Astrophysical Journal

    ApJ · 12 publications · 666 citations

    12

    h-index

  4. Earth and Planetary Science Letters

    12 publications · 469 citations

    12

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 11 publications · 1K citations

    11

    h-index

1–5