Stability Of Orbits

Stability of Orbits is the property of an orbital trajectory in which small perturbations do not lead to unbounded deviation over time, ensuring long-term confinement of the orbiting body within a bounded region relative to the primary gravitational source.

2K

Publications

96K

Citations

3.2K

Authors

1.2K

Institutions

Publications per year

2017–2026

254

Authors

3.2K

  1. GC
    G. Contopoulos

    Academy of Athens, Greece

    24 publications · 969 citations

    17

    h-index

  2. DJ
    Daniel J. Scheeres

    University of Colorado Boulder, United States

    18 publications · 1.1K citations

    16

    h-index

  3. RD
    R. Dvořák

    University of Vienna, Austria

    20 publications · 834 citations

    16

    h-index

  4. OC
    O. C. Winter

    Universidade Estadual Paulista (Unesp), Brazil

    11 publications · 476 citations

    11

    h-index

  5. SM
    Seppo Mikkola

    University of Turku, Finland

    11 publications · 690 citations

    11

    h-index

1–5 of 3.2K

Venues

  1. Celestial Mechanics and Dynamical Astronomy

    112 publications · 4.4K citations

    39

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    104 publications · 4.4K citations

    36

    h-index

  3. The Astrophysical Journal

    ApJ · 46 publications · 3.4K citations

    32

    h-index

  4. The Astronomical Journal

    AJ · 64 publications · 4.8K citations

    31

    h-index

  5. Journal of Guidance Control and Dynamics

    55 publications · 2.1K citations

    28

    h-index

1–5