Resonant Secular Dynamics

Resonant Secular Dynamics is a theoretical framework within celestial mechanics that describes the long-term evolution of orbital systems under the combined influence of secular gravitational interactions and mean-motion resonances, distinguished by its integration of resonant angle dynamics into secular perturbation analysis.

85

Publications

4K

Citations

133

Authors

91

Institutions

Publications per year

2017–2026

15

Authors

133

  1. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    6 publications · 571 citations

    6

    h-index

  2. JH
    Jacques Henrard

    University of Namur, Belgium

    4 publications · 250 citations

    4

    h-index

  3. JF
    Jean-Baptiste Fouvry

    Centre National de la Recherche Scientifique, France

    3 publications · 94 citations

    3

    h-index

  4. VC
    V. Carruba

    Universidade Estadual Paulista (Unesp), Brazil

    3 publications · 114 citations

    3

    h-index

  5. AC
    Alessandra Celletti

    University of Rome Tor Vergata, Italy

    3 publications · 106 citations

    3

    h-index

1–5 of 133

Venues

  1. Icarus

    14 publications · 1K citations

    14

    h-index

  2. Celestial Mechanics and Dynamical Astronomy

    15 publications · 579 citations

    14

    h-index

  3. 11

    h-index

  4. The Astronomical Journal

    AJ · 9 publications · 406 citations

    9

    h-index

  5. Astronomy and Astrophysics

    6 publications · 240 citations

    6

    h-index

1–5