Co-accretion Processes

Co-Accretion Processes is a theoretical framework in planetary science that explains the concurrent formation of a planetary satellite and its host planet from a shared circumplanetary disk, distinguishing it from alternative satellite origin models by emphasizing synchronized condensation and accumulation of mass within a gravitationally bound co-orbital environment.

16

Publications

3.8K

Citations

42

Authors

33

Institutions

Publications per year

2017–2026

9

Authors

42

  1. RM
    R. M. Canup

    Southwest Research Institute, United States

    2 publications · 31 citations

    2

    h-index

  2. RR
    Raluca Rufu

    Southwest Research Institute, United States

    1 publications · 17 citations

    1

    h-index

  3. AI
    André Izidoro

    Centre National de la Recherche Scientifique, France

    1 publications · 12 citations

    1

    h-index

  4. SH
    S. Hotzel

    University of Helsinki, Finland

    1 publications · 38 citations

    1

    h-index

  5. CT
    Claudia Toci

    University of Milan, Italy

    1 publications · 16 citations

    1

    h-index

1–5 of 42

Venues

  1. Astronomy and Astrophysics

    3 publications · 71 citations

    3

    h-index

  2. Icarus

    3 publications · 3.3K citations

    3

    h-index

  3. The Astrophysical Journal

    ApJ · 2 publications · 31 citations

    2

    h-index

  4. Nature Astronomy

    2 publications · 143 citations

    2

    h-index

  5. Geology

    1 publications · 193 citations

    1

    h-index

1–5