Nodal Precession

Nodal Precession is a type of secular perturbation in orbital mechanics characterized by the gradual, continuous rotation of the orbital plane of a celestial body about the symmetry axis of the central body, due to non-spherical gravitational forces, specifically manifesting as the precession of the line of nodes.

63

Publications

2.9K

Citations

216

Authors

141

Institutions

Publications per year

2017–2026

23

Variants

Precession Of The Nodes

Authors

216

  1. DL
    Dong Lai

    Cornell University, United States

    4 publications · 236 citations

    4

    h-index

  2. JP
    J. Patterson

    Columbia University, United States

    4 publications · 215 citations

    4

    h-index

  3. DR
    David R. Skillman

    Columbia University, United States

    3 publications · 188 citations

    3

    h-index

  4. DJ
    David J. Harvey

    University of Oxford, United Kingdom

    2 publications · 174 citations

    2

    h-index

  5. MC
    Marshall C. Johnson

    The Ohio State University, United States

    2 publications · 97 citations

    2

    h-index

1–5 of 216

Venues

  1. 15

    h-index

  2. The Astrophysical Journal

    ApJ · 7 publications · 455 citations

    7

    h-index

  3. The Astronomical Journal

    AJ · 3 publications · 122 citations

    3

    h-index

  4. Astronomy and Astrophysics

    3 publications · 124 citations

    3

    h-index

  5. arXiv (Cornell University)

    Repository · 2 publications · 30 citations

    2

    h-index

1–5