Roche Limits

Roche Limits is a theoretical threshold in orbital dynamics defining the minimum distance at which a celestial body, held together primarily by self-gravitation, can approach a more massive body without being torn apart by tidal forces induced by the latter's gravitational gradient.

96

Publications

6.2K

Citations

412

Authors

214

Institutions

Publications per year

2017–2026

29

Authors

412

  1. FA
    Frederic A. Rasio

    Northwestern University, United States

    5 publications · 574 citations

    5

    h-index

  2. JS
    Julien Salmon

    Southwest Research Institute, United States

    3 publications · 171 citations

    3

    h-index

  3. DV
    Dimitri Veras

    University of Warwick, United Kingdom

    3 publications · 278 citations

    3

    h-index

  4. LA
    Leslie A. Rogers

    California Institute of Technology, United States

    3 publications · 241 citations

    3

    h-index

  5. RM
    R. M. Canup

    Southwest Research Institute, United States

    3 publications · 171 citations

    3

    h-index

1–5 of 412

Venues

  1. The Astrophysical Journal

    ApJ · 34 publications · 2.6K citations

    23

    h-index

  2. 10

    h-index

  3. The Astrophysical Journal Letters

    9 publications · 594 citations

    8

    h-index

  4. Astronomy and Astrophysics

    6 publications · 264 citations

    6

    h-index

  5. 4

    h-index

1–5