Terrestrial Planet Migration

Terrestrial Planet Migration is a theoretical construct in planetary science that denotes the orbital displacement of rocky, Earth-like planets within protoplanetary disks due to gravitational interactions with disk material or other celestial bodies, distinguishing it from migration mechanisms affecting giant or gaseous planets.

35

Publications

2.3K

Citations

62

Authors

51

Institutions

Publications per year

2017–2026

4

Authors

62

  1. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    4 publications · 337 citations

    4

    h-index

  2. SN
    Sean N. Raymond

    Laboratoire d'Astrophysique de Bordeaux, France

    4 publications · 425 citations

    4

    h-index

  3. MJ
    Martyn J. Fogg

    Queen Mary University of London, United Kingdom

    4 publications · 207 citations

    4

    h-index

  4. RP
    Richard P. Nelson

    Queen Mary University of London, United Kingdom

    3 publications · 172 citations

    3

    h-index

  5. KJ
    K. J. Walsh

    Southwest Research Institute, United States

    2 publications · 95 citations

    2

    h-index

1–5 of 62

Venues

  1. The Astrophysical Journal

    ApJ · 8 publications · 565 citations

    8

    h-index

  2. Astronomy and Astrophysics

    5 publications · 369 citations

    5

    h-index

  3. 5

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 3 publications · 134 citations

    3

    h-index

  5. Astrobiology

    2 publications · 267 citations

    2

    h-index

1–5