Obliquity Evolution

Obliquity Evolution is a theoretical construct in celestial mechanics that models the long-term variations in the axial tilt of a planet due to gravitational interactions with other bodies, distinguishing it from other orbital element changes by specifically characterizing the temporal dynamics of rotational axis orientation in the context of secular perturbations.

43

Publications

3.5K

Citations

97

Authors

70

Institutions

Publications per year

2017–2026

10

Authors

97

  1. BG
    B. G. Bills

    Jet Propulsion Laboratory, United States

    3 publications · 133 citations

    3

    h-index

  2. JN
    Joshua N. Winn

    Massachusetts Institute of Technology, United States

    2 publications · 136 citations

    2

    h-index

  3. SA
    Simon Albrecht

    Aarhus University, Denmark

    2 publications · 136 citations

    2

    h-index

  4. WR
    William R. Ward

    Jet Propulsion Laboratory, United States

    2 publications · 343 citations

    2

    h-index

  5. JW
    Jack Wisdom

    Massachusetts Institute of Technology, United States

    2 publications · 311 citations

    2

    h-index

1–5 of 97

Venues

  1. Icarus

    5 publications · 315 citations

    5

    h-index

  2. The Astrophysical Journal Letters

    4 publications · 266 citations

    4

    h-index

  3. Science

    3 publications · 576 citations

    3

    h-index

  4. Journal of Geophysical Research Atmospheres

    JGR · 3 publications · 203 citations

    3

    h-index

  5. Astronomy and Astrophysics

    2 publications · 147 citations

    2

    h-index

1–5