Trojan Dynamics

Trojan Dynamics is a theoretical framework in celestial mechanics that models the stability and orbital evolution of small bodies trapped in the Lagrangian points of a resonant orbit, distinguishing itself by analyzing the long-term gravitational interactions between co-orbital objects in 1:1 mean-motion resonance with a secondary mass.

49

Publications

1.4K

Citations

87

Authors

70

Institutions

Publications per year

2017–2026

10

Authors

87

  1. RD
    R. Dvořák

    University of Vienna, Austria

    4 publications · 125 citations

    4

    h-index

  2. ÀJ
    Àngel Jorba

    Universitat de Barcelona, Spain

    3 publications · 81 citations

    3

    h-index

  3. JH
    Jonathan Horner

    UNSW Sydney, Australia

    3 publications · 128 citations

    3

    h-index

  4. FG
    Frederic Gabern

    Universitat de Barcelona, Spain

    3 publications · 166 citations

    3

    h-index

  5. FM
    F. Marzari

    University of Padua, Italy

    3 publications · 103 citations

    3

    h-index

1–5 of 87

Venues

  1. 10

    h-index

  2. Icarus

    7 publications · 247 citations

    7

    h-index

  3. Celestial Mechanics and Dynamical Astronomy

    7 publications · 232 citations

    7

    h-index

  4. Astronomy and Astrophysics

    3 publications · 84 citations

    3

    h-index

  5. Solar System Research

    2 publications · 30 citations

    2

    h-index

1–5