Planetary Secular Theory

Planetary Secular Theory is a theoretical framework in celestial mechanics that models the long-term, averaged gravitational interactions among planets to predict their orbital evolution, excluding short-periodic variations.

46

Publications

2.4K

Citations

72

Authors

54

Institutions

Publications per year

2017–2026

8

Authors

72

  1. JL
    J. Laskar

    Institut de Mécanique Céleste et de Calcul des Éphémérides, France

    5 publications · 689 citations

    5

    h-index

  2. KV
    Kathryn Volk

    University of Arizona, United States

    3 publications · 113 citations

    3

    h-index

  3. CB
    C. Beaugé

    Universidad Nacional de Córdoba, Argentina

    3 publications · 116 citations

    3

    h-index

  4. GF
    G. Francou

    Centre National de la Recherche Scientifique, France

    3 publications · 335 citations

    3

    h-index

  5. TA
    T. A. Michtchenko

    Universidade de São Paulo, Brazil

    2 publications · 87 citations

    2

    h-index

1–5 of 72

Venues

  1. The Astrophysical Journal

    ApJ · 7 publications · 529 citations

    7

    h-index

  2. The Astronomical Journal

    AJ · 7 publications · 351 citations

    7

    h-index

  3. Celestial Mechanics and Dynamical Astronomy

    6 publications · 136 citations

    6

    h-index

  4. 6

    h-index

  5. Astronomy and Astrophysics

    3 publications · 139 citations

    3

    h-index

1–5