Orbital Resonance

Orbital Resonance is a dynamical state in celestial and orbital mechanics wherein the orbital periods of two gravitationally interacting bodies are related by a ratio of small integers, leading to periodic gravitational perturbations that distinguish it from non-resonant or secular orbital interactions.

630

Publications

34.7K

Citations

882

Authors

426

Institutions

Publications per year

2017–2026

106

Authors

882

  1. TA
    T. A. Michtchenko

    Universidade de São Paulo, Brazil

    16 publications · 875 citations

    14

    h-index

  2. SF
    S. Ferraz‐Mello

    Universidade de São Paulo, Brazil

    15 publications · 802 citations

    14

    h-index

  3. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    14 publications · 1.6K citations

    14

    h-index

  4. AC
    A. C. M. Correia

    Institut de Mécanique Céleste et de Calcul des Éphémérides, France

    11 publications · 516 citations

    11

    h-index

  5. DN
    David Nesvorný

    Southwest Research Institute, United States

    10 publications · 688 citations

    10

    h-index

1–5 of 882

Venues

  1. The Astrophysical Journal

    ApJ · 60 publications · 6.4K citations

    40

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    96 publications · 4.2K citations

    36

    h-index

  3. The Astronomical Journal

    AJ · 60 publications · 3.6K citations

    33

    h-index

  4. Icarus

    43 publications · 2.4K citations

    29

    h-index

  5. Celestial Mechanics and Dynamical Astronomy

    49 publications · 1.8K citations

    28

    h-index

1–5