Lagrange Point Stability

Lagrange Point Stability is a theoretical construct in celestial mechanics that characterizes the resilience of equilibrium points in a rotating three-body system to small perturbations, distinguishing itself by its dependence on the gravitational and centrifugal potential landscape and its sensitivity to non-ideal forces such as solar radiation pressure.

20

Publications

631

Citations

39

Authors

28

Institutions

Publications per year

2017–2026

4

Authors

39

  1. CR
    Colin R. McInnes

    University of Strathclyde, United Kingdom

    3 publications · 105 citations

    3

    h-index

  2. KA
    K. A. Innanen

    University of Calgary, Canada

    3 publications · 42 citations

    3

    h-index

  3. SZ
    S.-P. Zhang

    York University, Canada

    2 publications · 28 citations

    2

    h-index

  4. KR
    Kenneth R. Meyer

    University of Cincinnati, United States

    1 publications · 75 citations

    1

    h-index

  5. RB
    R. Broucke

    The University of Texas at Austin, United States

    1 publications · 36 citations

    1

    h-index

1–5 of 39

Venues

  1. The Astronomical Journal

    AJ · 5 publications · 164 citations

    5

    h-index

  2. Advances in Space Research

    3 publications · 60 citations

    3

    h-index

  3. Celestial Mechanics and Dynamical Astronomy

    3 publications · 84 citations

    3

    h-index

  4. Journal of Differential Equations

    1 publications · 75 citations

    1

    h-index

  5. The Astrophysical Journal

    ApJ · 1 publications · 36 citations

    1

    h-index

1–5