Barycentric Motion

Barycentric Motion is the orbital motion of two bodies in a gravitational system relative to their common center of mass, distinguished from absolute or geocentric motion by its reference frame being fixed at the system’s barycenter.

44

Publications

2.3K

Citations

113

Authors

89

Institutions

Publications per year

2017–2026

8

Authors

113

  1. AM
    A. Mérand

    Centre National de la Recherche Scientifique, France

    3 publications · 106 citations

    3

    h-index

  2. PK
    P. Kervella

    Laboratoire d’études spatiales et d’instrumentation en astrophysique, France

    3 publications · 106 citations

    3

    h-index

  3. GW
    G. W. Null

    Jet Propulsion Laboratory, United States

    2 publications · 57 citations

    2

    h-index

  4. MA
    M. A. C. Perryman

    European Space Research and Technology Centre, Netherlands

    2 publications · 28 citations

    2

    h-index

  5. FM
    F. Mignard

    Observatoire de la Côte d’Azur, France

    2 publications · 80 citations

    2

    h-index

1–5 of 113

Venues

  1. The Astronomical Journal

    AJ · 5 publications · 597 citations

    5

    h-index

  2. Astronomy and Astrophysics

    5 publications · 266 citations

    5

    h-index

  3. arXiv (Cornell University)

    Repository · 3 publications · 73 citations

    3

    h-index

  4. The Astrophysical Journal

    ApJ · 2 publications · 49 citations

    2

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 2 publications · 210 citations

    2

    h-index

1–5