Migration Timescales

Migration Timescales is a theoretical construct in planetary science that denotes the characteristic duration over which a planet's orbital parameters evolve significantly due to gravitational interactions with a protoplanetary disk or other celestial bodies, distinguishing it from instantaneous orbital changes or secular perturbations by quantifying the rate of orbital migration.

34

Publications

2.5K

Citations

81

Authors

73

Institutions

Publications per year

2017–2026

7

Authors

81

  1. RS
    R. S. Gomes

    National Observatory, Brazil

    2 publications · 274 citations

    2

    h-index

  2. WH
    Weihao Huang

    Southern Marine Science and Engineering Guangdong Laboratory (Guangzhou), China

    1 publications · 19 citations

    1

    h-index

  3. KA
    Kazuhiro Akimoto

    Teikyo University, Japan

    1 publications · 14 citations

    1

    h-index

  4. PA
    Paul A. Sandery

    Bureau of Meteorology, Australia

    1 publications · 73 citations

    1

    h-index

  5. FG
    F. Goyache

    Servicio Regional de Investigación y Desarrollo Agroalimentario, Spain

    1 publications · 101 citations

    1

    h-index

1–5 of 81

Venues

  1. The Astrophysical Journal

    ApJ · 9 publications · 963 citations

    9

    h-index

  2. The Astronomical Journal

    AJ · 4 publications · 332 citations

    4

    h-index

  3. Astronomy and Astrophysics

    3 publications · 186 citations

    3

    h-index

  4. 2

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  5. Home Cultures

    1 publications · 19 citations

    1

    h-index

1–5