Two-body Stability

Two-Body Stability is a theoretical construct in orbital mechanics that characterizes the stability of the mutual gravitational interaction between two celestial bodies in a closed system, distinguishing it from multi-body stability phenomena by isolating the dynamical evolution of their relative motion under Newtonian gravitation.

130

Publications

5.6K

Citations

222

Authors

152

Institutions

Publications per year

2017–2026

10

Authors

222

  1. DJ
    Daniel J. Scheeres

    University of Colorado Boulder, United States

    4 publications · 319 citations

    4

    h-index

  2. FI
    F. I. Cooperstock

    University of Victoria, Canada

    3 publications · 162 citations

    3

    h-index

  3. GA
    Gustavo Alonso

    Universidad Politécnica de Madrid, Spain

    3 publications · 183 citations

    3

    h-index

  4. JM
    José Meseguer

    Universidad Politécnica de Madrid, Spain

    3 publications · 183 citations

    3

    h-index

  5. CR
    Colin R. McInnes

    University of Strathclyde, United Kingdom

    3 publications · 219 citations

    3

    h-index

1–5 of 222

Venues

  1. Celestial Mechanics and Dynamical Astronomy

    16 publications · 687 citations

    15

    h-index

  2. Journal of Guidance Control and Dynamics

    10 publications · 634 citations

    10

    h-index

  3. Astrophysics and Space Science

    5 publications · 88 citations

    5

    h-index

  4. 4

    h-index

  5. Icarus

    4 publications · 825 citations

    4

    h-index

1–5