Spin-orbit Resonance

Spin-Orbit Resonance is a dynamical state in which the rotational period of a celestial body exhibits a simple integer ratio with its orbital period around a primary, resulting in a gravitational interaction that stabilizes the system's long-term evolution.

327

Publications

20.2K

Citations

1K

Authors

416

Institutions

Publications per year

2017–2026

59

Authors

1K

  1. AC
    A. C. M. Correia

    Institut de Mécanique Céleste et de Calcul des Éphémérides, France

    8 publications · 455 citations

    8

    h-index

  2. DL
    Daniel Loss

    University of Basel, Switzerland

    7 publications · 608 citations

    7

    h-index

  3. NR
    Nicolas Rambaux

    Institut de Mécanique Céleste et de Calcul des Éphémérides, France

    7 publications · 313 citations

    7

    h-index

  4. JL
    J. Laskar

    Institut de Mécanique Céleste et de Calcul des Éphémérides, France

    5 publications · 397 citations

    5

    h-index

  5. GA
    G. Anglada‐Escudé

    Institute of Space Sciences, Spain

    4 publications · 628 citations

    4

    h-index

1–5 of 1K

Venues

  1. Physical Review Letters

    PRL · 27 publications · 3.4K citations

    18

    h-index

  2. The Journal of Chemical Physics

    17 publications · 1.1K citations

    15

    h-index

  3. Physical Review B

    PRB · 19 publications · 730 citations

    15

    h-index

  4. Physical review. B./Physical review. B

    PRB · 15 publications · 654 citations

    14

    h-index

  5. The Astrophysical Journal

    ApJ · 14 publications · 696 citations

    14

    h-index

1–5