Trojan Stability

Trojan Stability is a theoretical framework in celestial mechanics that characterizes the long-term orbital stability of small bodies gravitationally trapped near the Lagrangian points L4 and L5 of a two-body system, distinguished by its focus on resonant co-orbital dynamics that prevent ejection or collision despite perturbations.

43

Publications

2K

Citations

153

Authors

83

Institutions

Publications per year

2017–2026

4

Authors

153

  1. RD
    R. Dvořák

    University of Vienna, Austria

    8 publications · 305 citations

    8

    h-index

  2. RP
    Richard P. Schwarz

    Center for Astrophysics Harvard & Smithsonian, United States

    6 publications · 226 citations

    6

    h-index

  3. ÁS
    Á. Süli

    Eötvös Loránd University, Hungary

    5 publications · 169 citations

    5

    h-index

  4. SM
    Seppo Mikkola

    University of Turku, Finland

    4 publications · 130 citations

    4

    h-index

  5. FM
    F. Marzari

    University of Padua, Italy

    3 publications · 141 citations

    3

    h-index

1–5 of 153

Venues

  1. 10

    h-index

  2. The Astronomical Journal

    AJ · 7 publications · 238 citations

    7

    h-index

  3. Astronomy and Astrophysics

    7 publications · 290 citations

    7

    h-index

  4. Celestial Mechanics and Dynamical Astronomy

    4 publications · 188 citations

    4

    h-index

  5. The Astrophysical Journal

    ApJ · 3 publications · 214 citations

    3

    h-index

1–5