Cassini States

Cassini State is a stable equilibrium configuration in the rotational dynamics of a celestial body, defined by a specific alignment between the body's spin axis, its orbit normal, and the normal to the plane of precession, where the spin axis and orbit normal precess synchronously under gravitational torques.

47

Publications

2.9K

Citations

145

Authors

94

Institutions

Publications per year

2017–2026

9

Variants

Cassini State

Authors

145

  1. PD
    P. D. Nicholson

    Cornell University, United States

    6 publications · 469 citations

    6

    h-index

  2. SJ
    S. J. Peale

    University of California, Santa Barbara, United States

    6 publications · 770 citations

    6

    h-index

  3. JN
    Jeffrey N. Cuzzi

    Ames Research Center, United States

    4 publications · 219 citations

    4

    h-index

  4. SC
    Sean C. Solomon

    Carnegie Institution for Science, United States

    3 publications · 391 citations

    3

    h-index

  5. MM
    Matthew M. Hedman

    Cornell University, United States

    3 publications · 249 citations

    3

    h-index

1–5 of 145

Venues

  1. Icarus

    16 publications · 1K citations

    15

    h-index

  2. Astronomy and Astrophysics

    5 publications · 183 citations

    5

    h-index

  3. Journal of Geophysical Research Planets

    4 publications · 72 citations

    4

    h-index

  4. The Astrophysical Journal

    ApJ · 3 publications · 251 citations

    3

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 2 publications · 178 citations

    2

    h-index

1–5