Planetesimal-driven Migration

Planetesimal-Driven Migration is a theoretical mechanism of planetary orbital evolution in which gravitational interactions between a planet and a surrounding swarm of planetesimals gradually alter the planet's semi-major axis and eccentricity through cumulative angular momentum exchange.

51

Publications

4.8K

Citations

76

Authors

71

Institutions

Publications per year

2017–2026

7

Authors

76

  1. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    8 publications · 867 citations

    8

    h-index

  2. HF
    Harold F. Levison

    Southwest Research Institute, United States

    8 publications · 845 citations

    8

    h-index

  3. RS
    R. S. Gomes

    National Observatory, Brazil

    5 publications · 776 citations

    5

    h-index

  4. RB
    Ramon Brasser

    Tokyo Institute of Technology, Japan

    5 publications · 611 citations

    5

    h-index

  5. KT
    K. Tsiganis

    Aristotle University of Thessaloniki, Greece

    3 publications · 462 citations

    3

    h-index

1–5 of 76

Venues

  1. Icarus

    10 publications · 1.3K citations

    10

    h-index

  2. The Astrophysical Journal

    ApJ · 9 publications · 667 citations

    9

    h-index

  3. Astronomy and Astrophysics

    6 publications · 621 citations

    6

    h-index

  4. The Astronomical Journal

    AJ · 5 publications · 736 citations

    5

    h-index

  5. 4

    h-index

1–5