Planetary Obliquity

Planetary Obliquity is the angular deviation between a planet's rotational axis and the perpendicular to its orbital plane, serving as a key astronomical parameter that governs the distribution and seasonality of stellar insolation across its surface.

158

Publications

10.7K

Citations

483

Authors

229

Institutions

Publications per year

2017–2026

50

Authors

483

  1. JN
    Joshua N. Winn

    Massachusetts Institute of Technology, United States

    12 publications · 2.6K citations

    12

    h-index

  2. SA
    Simon Albrecht

    Aarhus University, Denmark

    7 publications · 1.8K citations

    7

    h-index

  3. GW
    Geoffrey W. Marcy

    University of California, Berkeley, United States

    6 publications · 1.2K citations

    6

    h-index

  4. AW
    Andrew W. Howard

    University of California, Berkeley, United States

    5 publications · 1K citations

    5

    h-index

  5. JA
    John Asher Johnson

    University of California, Berkeley, United States

    5 publications · 1.8K citations

    5

    h-index

1–5 of 483

Venues

  1. The Astrophysical Journal

    ApJ · 31 publications · 2.9K citations

    26

    h-index

  2. The Astronomical Journal

    AJ · 25 publications · 1.2K citations

    18

    h-index

  3. The Astrophysical Journal Letters

    15 publications · 1.5K citations

    15

    h-index

  4. Icarus

    13 publications · 931 citations

    12

    h-index

  5. Astronomy and Astrophysics

    11 publications · 1K citations

    11

    h-index

1–5