Trojan Asteroid Dynamics

Trojan Asteroid Dynamics is a theoretical framework within celestial mechanics that specifically models the orbital behavior and stability of asteroids co-orbiting with a planet in its Lagrangian points, thereby distinguishing itself from general asteroid dynamics through its focus on resonant gravitational configurations.

61

Publications

3.1K

Citations

126

Authors

91

Institutions

Publications per year

2017–2026

10

Authors

126

  1. RD
    R. Dvořák

    University of Vienna, Austria

    4 publications · 125 citations

    4

    h-index

  2. BG
    Boris Garfinkel

    Yale University, United States

    4 publications · 131 citations

    4

    h-index

  3. RP
    Richard P. Schwarz

    Center for Astrophysics Harvard & Smithsonian, United States

    4 publications · 125 citations

    4

    h-index

  4. B�
    B�lint �rdi

    Eötvös Loránd University, Hungary

    3 publications · 97 citations

    3

    h-index

  5. HF
    Harold F. Levison

    Southwest Research Institute, United States

    3 publications · 1.1K citations

    3

    h-index

1–5 of 126

Venues

  1. Celestial Mechanics and Dynamical Astronomy

    14 publications · 479 citations

    13

    h-index

  2. Icarus

    12 publications · 412 citations

    12

    h-index

  3. 8

    h-index

  4. The Astronomical Journal

    AJ · 4 publications · 269 citations

    4

    h-index

  5. Astronomy and Astrophysics

    3 publications · 78 citations

    3

    h-index

1–5