Planetary System Stability

Planetary System Stability is a theoretical construct in astrophysics that characterizes the long-term dynamical persistence of orbital configurations within a planetary system, distinguishing it from transient or chaotic arrangements by its reliance on gravitational interactions that maintain bounded, non-colliding trajectories over astronomical timescales.

325

Publications

19.3K

Citations

732

Authors

353

Institutions

Publications per year

2017–2026

71

Authors

732

  1. KG
    Krzysztof Goździewski

    Nicolaus Copernicus University, Poland

    17 publications · 746 citations

    16

    h-index

  2. JJ
    Jack J. Lissauer

    Ames Research Center, United States

    12 publications · 2.3K citations

    12

    h-index

  3. JH
    Jonathan Horner

    UNSW Sydney, Australia

    12 publications · 628 citations

    12

    h-index

  4. SN
    Sean N. Raymond

    Laboratoire d'Astrophysique de Bordeaux, France

    11 publications · 621 citations

    11

    h-index

  5. RA
    Robert A. Wittenmyer

    UNSW Sydney, Australia

    11 publications · 759 citations

    11

    h-index

1–5 of 732

Venues

  1. The Astrophysical Journal

    ApJ · 63 publications · 5.4K citations

    46

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    65 publications · 2.9K citations

    36

    h-index

  3. Astronomy and Astrophysics

    36 publications · 1.9K citations

    25

    h-index

  4. The Astronomical Journal

    AJ · 25 publications · 1.7K citations

    18

    h-index

  5. Icarus

    17 publications · 1.4K citations

    16

    h-index

1–5