Secular Orbital Evolution

Secular Orbital Evolution is a long-term, non-periodic alteration in the orbital elements of a celestial body or artificial satellite caused by cumulative gravitational and nongravitational forces, particularly solar radiation pressure, that distinguishes it from short-term periodic orbital perturbations.

145

Publications

9.2K

Citations

283

Authors

186

Institutions

Publications per year

2017–2026

27

Authors

283

  1. FA
    Frederic A. Rasio

    Northwestern University, United States

    5 publications · 971 citations

    5

    h-index

  2. SN
    Smadar Naoz

    University of California, Los Angeles, United States

    4 publications · 665 citations

    4

    h-index

  3. JF
    Jean-Baptiste Fouvry

    Centre National de la Recherche Scientifique, France

    4 publications · 110 citations

    4

    h-index

  4. AM
    Alessandro Morbidelli

    Observatoire de la Côte d’Azur, France

    4 publications · 230 citations

    4

    h-index

  5. HR
    H. Rickman

    Uppsala University, Sweden

    4 publications · 91 citations

    4

    h-index

1–5 of 283

Venues

  1. Monthly Notices of the Royal Astronomical Society

    39 publications · 1.9K citations

    24

    h-index

  2. The Astrophysical Journal

    ApJ · 27 publications · 3.1K citations

    23

    h-index

  3. Astronomy and Astrophysics

    11 publications · 478 citations

    11

    h-index

  4. Icarus

    8 publications · 402 citations

    8

    h-index

  5. 5

    h-index

1–5