Obliquity Variations

Obliquity Variations is a geophysical construct that quantifies the temporal changes in the axial tilt of a planet relative to its orbital plane, distinguishing it from static obliquity by characterizing the dynamic evolution of rotational orientation over astronomical timescales.

135

Publications

8.1K

Citations

423

Authors

253

Institutions

Publications per year

2017–2026

34

Authors

423

  1. FH
    F.J. Hilgen

    Utrecht University, Netherlands

    5 publications · 355 citations

    5

    h-index

  2. LJ
    Lucas Joost Lourens

    Utrecht University, Netherlands

    5 publications · 355 citations

    5

    h-index

  3. ET
    E. Tuenter

    Utrecht University, Netherlands

    5 publications · 438 citations

    5

    h-index

  4. BG
    B. G. Bills

    Jet Propulsion Laboratory, United States

    4 publications · 146 citations

    4

    h-index

  5. JL
    J. Laskar

    Institut de Mécanique Céleste et de Calcul des Éphémérides, France

    4 publications · 373 citations

    4

    h-index

1–5 of 423

Venues

  1. The Astronomical Journal

    AJ · 15 publications · 776 citations

    15

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 11 publications · 1.2K citations

    11

    h-index

  3. The Astrophysical Journal

    ApJ · 8 publications · 571 citations

    8

    h-index

  4. Icarus

    8 publications · 431 citations

    8

    h-index

  5. Climate of the past

    6 publications · 374 citations

    6

    h-index

1–5