Planetary Migration Models

Planetary Migration Models is a theoretical framework in planetary science that explains the orbital evolution of planets through interactions with protoplanetary disks or other gravitational mechanisms, distinguishing it from static planetary formation models by emphasizing dynamic orbital changes during early system development.

247

Publications

20.1K

Citations

483

Authors

276

Institutions

Publications per year

2017–2026

67

Authors

483

  1. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    14 publications · 2.2K citations

    13

    h-index

  2. DN
    David Nesvorný

    Southwest Research Institute, United States

    12 publications · 1.1K citations

    12

    h-index

  3. SU
    S. Udry

    University of Geneva, Switzerland

    12 publications · 2.2K citations

    12

    h-index

  4. SN
    Sean N. Raymond

    Laboratoire d'Astrophysique de Bordeaux, France

    10 publications · 2.1K citations

    10

    h-index

  5. BB
    Bertram Bitsch

    Max Planck Institute for Astronomy, Germany

    9 publications · 442 citations

    9

    h-index

1–5 of 483

Venues

  1. The Astrophysical Journal

    ApJ · 47 publications · 4.5K citations

    36

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    51 publications · 2.8K citations

    28

    h-index

  3. Astronomy and Astrophysics

    34 publications · 3.3K citations

    26

    h-index

  4. The Astronomical Journal

    AJ · 25 publications · 1.7K citations

    19

    h-index

  5. The Astrophysical Journal Letters

    13 publications · 929 citations

    13

    h-index

1–5