Keplerian Motion

Keplerian Motion is the idealized two-body orbital motion of a celestial object governed solely by Newtonian gravitation, where the trajectory follows one of Kepler’s laws of planetary motion.

1K

Publications

60.1K

Citations

1.8K

Authors

783

Institutions

Publications per year

2017–2026

107

Authors

1.8K

  1. RF
    R. F. Díaz

    Centre National de la Recherche Scientifique, France

    20 publications · 1.3K citations

    18

    h-index

  2. MD
    M. Deleuil

    Centre National de la Recherche Scientifique, France

    19 publications · 1.2K citations

    18

    h-index

  3. AS
    A. Santerne

    Centre National de la Recherche Scientifique, France

    20 publications · 1.3K citations

    18

    h-index

  4. FB
    F. Bouchy

    University of Geneva, Switzerland

    20 publications · 1.6K citations

    18

    h-index

  5. AS
    A. S. Bonomo

    Osservatorio Astrofisico di Torino, Italy

    17 publications · 1.2K citations

    17

    h-index

1–5 of 1.8K

Venues

  1. The Astrophysical Journal

    ApJ · 57 publications · 6.3K citations

    40

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    57 publications · 3.1K citations

    32

    h-index

  3. Celestial Mechanics and Dynamical Astronomy

    84 publications · 2.7K citations

    29

    h-index

  4. Astronomy and Astrophysics

    34 publications · 2.6K citations

    28

    h-index

  5. Journal of Guidance Control and Dynamics

    51 publications · 3.5K citations

    26

    h-index

1–5