Concepedia

Hill Stability

Hill Stability is a theoretical framework in orbital mechanics that defines the dynamical regime in which a celestial body remains gravitationally bound within the influence sphere of a primary mass under the perturbative effects of a third, more distant body, thereby distinguishing it from other orbital stability criteria by its reliance on the relative energy and angular momentum thresholds in the restricted three-body problem.

47

Publications

2.2K

Citations

77

Authors

60

Institutions

Publications per year

2017–2026

5

Variants

Hill's Stability

Parents

Publications

47

Transit timing effects due to an exomoon

David Kipping · Monthly Notices of the Royal Astronomical Society · 2008 · 273 citations · Full text

, , +14

Hill stability and distance curves for the general three-body problem

Christian Marchal, George Bozis · Celestial Mechanics and Dynamical Astronomy · 1982 · 233 citations

, , +13

Stability Limits in Extrasolar Planetary Systems

Rory Barnes, R. Greenberg · The Astrophysical Journal · 2006 · 139 citations · Full text

, , +16

PLANET-PLANET SCATTERING LEADS TO TIGHTLY PACKED PLANETARY SYSTEMS

Sean N. Raymond, Rory Barnes, Dimitri Veras et al. · The Astrophysical Journal · 2009 · 108 citations · Full text

, , +13

Geometrical aspects of stability theory for Hill's equations

Henk Broer, Mark Levi · Archive for Rational Mechanics and Analysis · 1995 · 95 citations

, , +9

1–5 of 47

Authors

77

  1. JR
    J. R. Donnison

    Queen Mary University of London, United Kingdom

    7 publications · 236 citations

    7

    h-index

  2. DV
    Dimitri Veras

    University of Warwick, United Kingdom

    3 publications · 186 citations

    3

    h-index

  3. SG
    Shengping Gong

    Tsinghua University, China

    3 publications · 62 citations

    3

    h-index

  4. RB
    Rory Barnes

    University of Washington, United States

    2 publications · 247 citations

    2

    h-index

  5. PD
    Plamen Djakov

    The Ohio State University, United States

    2 publications · 47 citations

    2

    h-index

1–5 of 77

Institutions

60

  1. Queen Mary University of London

    London, United Kingdom

    7 h-index

    7 publications

    236 citations

  2. Tsinghua University

    Beijing, China

    3 h-index

    7 publications

    117 citations

  3. University of Arizona

    Tucson, United States

    3 h-index

    5 publications

    538 citations

  4. University of Glasgow

    Glasgow, United Kingdom

    2 h-index

    3 publications

    64 citations

  5. The Ohio State University

    Columbus, United States

    2 h-index

    2 publications

    47 citations

  6. Planetary Science Institute

    Tucson, United States

    2 h-index

    5 publications

    602 citations

  7. Sofia University "St. Kliment Ohridski"

    Sofia, Bulgaria

    2 h-index

    2 publications

    47 citations

  8. Sapientia Hungarian University of Transylvania

    Cluj-Napoca, Romania

    2 h-index

    2 publications

    73 citations

1–8 of 60

Venues

  1. 9

    h-index

  2. Celestial Mechanics and Dynamical Astronomy

    7 publications · 414 citations

    7

    h-index

  3. The Astrophysical Journal

    ApJ · 5 publications · 376 citations

    5

    h-index

  4. Astrophysics and Space Science

    3 publications · 67 citations

    3

    h-index

  5. Planetary and Space Science

    3 publications · 98 citations

    3

    h-index

1–5