Mean-motion Resonance Width

Mean-Motion Resonance Width is a theoretical metric in celestial mechanics that quantifies the extent in semi-major axis space over which a mean-motion resonance significantly influences orbital evolution, distinguishing it from other dynamical indicators by its specific association with the libration zone of resonant arguments in Hamiltonian systems of planetary perturbations.

62

Publications

3.6K

Citations

147

Authors

114

Institutions

Publications per year

2017–2026

14

Authors

147

  1. TG
    Tabaré Gallardo

    Universidad de la República de Uruguay, Uruguay

    4 publications · 262 citations

    4

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  2. NM
    Norman Murray

    Canadian Institute for Theoretical Astrophysics, Canada

    3 publications · 202 citations

    3

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  3. EB
    Eric B. Ford

    University of Florida, United States

    3 publications · 868 citations

    3

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  4. MJ
    Matthew J. Holman

    Center for Astrophysics Harvard & Smithsonian, United States

    3 publications · 977 citations

    3

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  5. DR
    David R. Ciardi

    California Institute of Technology, United States

    3 publications · 850 citations

    3

    h-index

1–5 of 147

Venues

  1. Icarus

    13 publications · 763 citations

    13

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  2. 9

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  3. The Astronomical Journal

    AJ · 8 publications · 518 citations

    8

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  4. Celestial Mechanics and Dynamical Astronomy

    7 publications · 177 citations

    7

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  5. The Astrophysical Journal

    ApJ · 6 publications · 326 citations

    6

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1–5