Obliquity Determination

Obliquity Determination is a methodological framework in planetary science that quantifies the axial tilt of a celestial body relative to its orbital plane by analyzing rotational dynamics and gravitational interactions, distinguishing it from other geophysical inversion techniques through its specific focus on spin-axis orientation and its constraints on interior mass distribution.

104

Publications

10.4K

Citations

339

Authors

223

Institutions

Publications per year

2017–2026

29

Authors

339

  1. SA
    Simon Albrecht

    Aarhus University, Denmark

    5 publications · 460 citations

    5

    h-index

  2. HI
    Howard Isaacson

    University of California, Berkeley, United States

    4 publications · 470 citations

    4

    h-index

  3. JN
    Joshua N. Winn

    Massachusetts Institute of Technology, United States

    4 publications · 483 citations

    4

    h-index

  4. MN
    Mikkel N. Lund

    Aarhus University, Denmark

    3 publications · 339 citations

    3

    h-index

  5. SG
    Sander Goossens

    Goddard Space Flight Center, United States

    3 publications · 276 citations

    3

    h-index

1–5 of 339

Venues

  1. The Astronomical Journal

    AJ · 18 publications · 606 citations

    16

    h-index

  2. The Astrophysical Journal

    ApJ · 10 publications · 1K citations

    10

    h-index

  3. Astronomy and Astrophysics

    8 publications · 4.5K citations

    8

    h-index

  4. Icarus

    5 publications · 309 citations

    5

    h-index

  5. The Astrophysical Journal Letters

    5 publications · 235 citations

    5

    h-index

1–5