Planetary Migration

Planetary Migration is a dynamical process in planetary systems whereby a planet’s orbit—especially its semi-major axis—undergoes systematic change over time due to gravitational and tidal interactions with a protoplanetary disk, planetesimals, other planets, or the central star.

1K

Publications

79.7K

Citations

1.3K

Authors

532

Institutions

Publications per year

2017–2026

317

Authors

1.3K

  1. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    49 publications · 6.7K citations

    36

    h-index

  2. RP
    Richard P. Nelson

    Queen Mary University of London, United Kingdom

    36 publications · 3.5K citations

    29

    h-index

  3. BB
    Bertram Bitsch

    Max Planck Institute for Astronomy, Germany

    36 publications · 2.9K citations

    28

    h-index

  4. SN
    Sean N. Raymond

    Laboratoire d'Astrophysique de Bordeaux, France

    32 publications · 4.4K citations

    27

    h-index

  5. WK
    W. Kley

    University of Tübingen, Germany

    28 publications · 2.4K citations

    23

    h-index

1–5 of 1.3K

Venues

  1. The Astrophysical Journal

    ApJ · 223 publications · 23.9K citations

    91

    h-index

  2. Astronomy and Astrophysics

    158 publications · 12K citations

    63

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    224 publications · 12.9K citations

    59

    h-index

  4. The Astronomical Journal

    AJ · 67 publications · 5K citations

    38

    h-index

  5. The Astrophysical Journal Letters

    46 publications · 3.3K citations

    32

    h-index

1–5