Co-orbital Moons

Co-Orbital Moons is a dynamical configuration in which two or more planetary moons share similar orbital paths around a planet, distinguished by their persistent gravitational interactions that maintain stable leading and trailing positions relative to each other within the same or adjacent Lagrange points.

4

Publications

97

Citations

10

Authors

7

Institutions

Publications per year

2017–2026

0

Authors

10

  1. NJ
    N. J. Cooper

    Queen Mary University of London, United Kingdom

    1 publications · 24 citations

    1

    h-index

  2. MT
    M. Tsuchida

    Universidade Estadual Paulista (Unesp), Brazil

    1 publications · 12 citations

    1

    h-index

  3. AI
    André Izidoro

    Centre National de la Recherche Scientifique, France

    1 publications · 12 citations

    1

    h-index

  4. CA
    C. A. Giuppone

    Argentine National Observatory, Argentina

    1 publications · 42 citations

    1

    h-index

  5. CD
    C. D. Murray

    Queen Mary University of London, United Kingdom

    1 publications · 24 citations

    1

    h-index

1–5 of 10

Venues

  1. Celestial Mechanics and Dynamical Astronomy

    1 publications · 42 citations

    1

    h-index

  2. The Astronomical Journal

    AJ · 1 publications · 24 citations

    1

    h-index

  3. NASA STI/Recon Technical Report N

    1 publications · 19 citations

    1

    h-index

  4. 1

    h-index

  5. Icarus

    1 publications · 10 citations

1–5