Axial Precession

Axial Precession is the gradual, cyclical wobble in the orientation of a planet's rotational axis, caused by gravitational torques from the Sun and Moon acting on the planet's equatorial bulge, which distinguishes it from other forms of planetary motion by altering the timing of seasonal alignment over long periods without changing the axial tilt magnitude.

26

Publications

920

Citations

66

Authors

40

Institutions

Publications per year

2017–2026

7

Authors

66

  1. BG
    B. G. Bills

    Jet Propulsion Laboratory, United States

    2 publications · 83 citations

    2

    h-index

  2. SR
    Stephen R. Meyers

    University of Wisconsin–Madison, United States

    1 publications · 14 citations

    2

    h-index

  3. AM
    Alberto Malinverno

    Lamont-Doherty Earth Observatory, United States

    1 publications · 14 citations

    2

    h-index

  4. RS
    R. S. Fishman

    Oak Ridge National Laboratory, United States

    1 publications · 24 citations

    1

    h-index

  5. BP
    Branislav Pongrác

    Comenius University Bratislava, Slovakia

    1 publications · 14 citations

    1

    h-index

1–5 of 66

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 4 publications · 139 citations

    4

    h-index

  2. Nature

    2 publications · 170 citations

    2

    h-index

  3. Physical Review Letters

    PRL · 2 publications · 60 citations

    2

    h-index

  4. Journal of Applied Physics

    1 publications · 17 citations

    1

    h-index

  5. Geophysical Research Letters

    1 publications · 26 citations

    1

    h-index

1–5