Precession Models

Precession Models is a theoretical framework in astrometry that describes the gradual, long-term changes in the orientation of a celestial body's rotational axis due to gravitational perturbations, distinguishing it from other astronomical reference corrections by specifically accounting for the slow conical motion of the Earth's polar axis over millennia within the context of reference frame and ephemeris computations.

138

Publications

6.1K

Citations

1.3K

Authors

333

Institutions

Publications per year

2017–2026

26

Authors

1.3K

  1. NC
    N. Capitaine

    Centre National de la Recherche Scientifique, France

    10 publications · 496 citations

    10

    h-index

  2. PT
    P. T. Wallace

    Rutherford Appleton Laboratory, United Kingdom

    7 publications · 422 citations

    7

    h-index

  3. JC
    J. Chapront

    Centre National de la Recherche Scientifique, France

    4 publications · 326 citations

    4

    h-index

  4. VD
    V. Dehant

    Royal Observatory of Belgium, Belgium

    4 publications · 212 citations

    4

    h-index

  5. JG
    J. G. Williams

    Imperial College London, United Kingdom

    3 publications · 317 citations

    3

    h-index

1–5 of 1.3K

Venues

  1. Astronomy and Astrophysics

    11 publications · 418 citations

    11

    h-index

  2. 10

    h-index

  3. Celestial Mechanics and Dynamical Astronomy

    9 publications · 282 citations

    9

    h-index

  4. The Astronomical Journal

    AJ · 8 publications · 424 citations

    8

    h-index

  5. Physical review. D/Physical review. D.

    PRD · 5 publications · 329 citations

    6

    h-index

1–5