Hill Sphere Dynamics is a theoretical framework in celestial mechanics that models the gravitational influence domain of a celestial body within which its gravitational pull dominates over perturbations from more distant, massive bodies, thereby determining the stability regions for orbital capture and motion of nearby satellites.
19
Publications
731
Citations
89
Authors
66
Institutions
Publications per year
2017–2026
5
Parents
Publications
19
Liberating exomoons in white dwarf planetary systems
Matthew J. Payne, Dimitri Veras, Matthew J. Holman et al. · Monthly Notices of the Royal Astronomical Society · 2016 · 68 citations · Full text
Natural Sciences, Astronomy, Physics +16
1–5 of 19
Authors
89
- SC
2
h-index
- MR
1
h-index
- DF
1
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- VD
1
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- CG
1
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1–5 of 89
Institutions
66
University of Exeter
Exeter, United Kingdom
3 h-index
10 publications
299 citations
Centre National de la Recherche Scientifique
Paris, France
2 h-index
7 publications
167 citations
The Open University
Milton Keynes, United Kingdom
2 h-index
4 publications
124 citations
Leiden University
Leiden, The Netherlands
2 h-index
2 publications
188 citations
University of Kent
Canterbury, United Kingdom
2 h-index
3 publications
91 citations
University of Michigan
Ann Arbor, United States
2 h-index
3 publications
44 citations
Michigan United
Kalamazoo, United States
2 h-index
3 publications
44 citations
Observatoire de Paris
Paris, France
1 h-index
2 publications
50 citations
1–8 of 66
Venues
- Monthly Notices of the Royal Astronomical Society
6 publications · 286 citations
6
h-index
- Astronomy and Astrophysics
2 publications · 58 citations
2
h-index
- The Astrophysical Journal
ApJ · 2 publications · 169 citations
2
h-index
- Dépôt institutionnel de l'Université libre de Bruxelles (Université Libre de Bruxelles)
Repository · 1 publications · 10 citations
1
h-index
- Communications in Nonlinear Science and Numerical Simulation
1 publications · 19 citations
1
h-index
1–5