Precession Of Orbits

Precession of Orbits is the gradual, secular rotation of the orbital ellipse of a celestial body around its primary focus, distinguished from other orbital perturbations by its long-term, cumulative change in the orientation of the orbit's pericenter within the orbital plane.

40

Publications

1.3K

Citations

61

Authors

47

Institutions

Publications per year

2017–2026

1

Authors

61

  1. JE
    John E. Cochran

    Auburn University, United States

    2 publications · 57 citations

    2

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  2. RG
    R. Greenberg

    University of Arizona, United States

    2 publications · 73 citations

    2

    h-index

  3. ME
    Michael Efroimsky

    United States Naval Observatory, United States

    2 publications · 54 citations

    2

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  4. GA
    G. Ares de Parga

    Instituto Politécnico Nacional, Mexico

    2 publications · 27 citations

    2

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  5. AA
    A. Avalos-Vargas

    Instituto Politécnico Nacional, Mexico

    2 publications · 27 citations

    2

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1–5 of 61

Venues

  1. American Journal of Physics

    7 publications · 168 citations

    7

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  2. Celestial Mechanics and Dynamical Astronomy

    7 publications · 215 citations

    7

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  3. 3

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  4. The Astrophysical Journal

    ApJ · 3 publications · 165 citations

    3

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  5. The Astronomical Journal

    AJ · 3 publications · 118 citations

    3

    h-index

1–5