Hill Regions

Hill Regions is a dynamical construct in celestial mechanics that delineates the volume of space within which a massless particle can remain gravitationally bound under the influence of two primary bodies in the Restricted Three-Body Problem, as determined by the Jacobi constant's energy constraints.

222

Publications

7.5K

Citations

504

Authors

215

Institutions

Publications per year

2017–2026

23

Variants

Hill's RegionsZero-velocity Surfaces

Authors

504

  1. GK
    G. K. Hight

    AgResearch, New Zealand

    6 publications · 181 citations

    6

    h-index

  2. JR
    J. R. Donnison

    Queen Mary University of London, United Kingdom

    6 publications · 183 citations

    6

    h-index

  3. KE
    K. E. Jury

    AgResearch, New Zealand

    6 publications · 181 citations

    6

    h-index

  4. GW
    G. W. Sheath

    AgResearch, New Zealand

    6 publications · 119 citations

    6

    h-index

  5. MG
    M. G. Lambert

    AgResearch, New Zealand

    5 publications · 196 citations

    5

    h-index

1–5 of 504

Venues

  1. 13

    h-index

  2. New Zealand Journal of Agricultural Research

    NZJA · 15 publications · 590 citations

    12

    h-index

  3. Celestial Mechanics and Dynamical Astronomy

    7 publications · 459 citations

    7

    h-index

  4. The Astrophysical Journal

    ApJ · 5 publications · 349 citations

    5

    h-index

  5. Bulletin of the American Schools of Oriental Research

    BASOR · 5 publications · 148 citations

    5

    h-index

1–5