Mean-motion Resonance Width
Mean-Motion Resonance Width is a theoretical metric in celestial mechanics that quantifies the extent in semi-major axis space over which a mean-motion resonance significantly influences orbital evolution, distinguishing it from other dynamical indicators by its specific association with the libration zone of resonant arguments in Hamiltonian systems of planetary perturbations.
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3.6K
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147
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114
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2017–2026
14
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The Mauna Kea-Cerro-Tololo (MKCT) Kuiper Belt and Centaur Survey
David Jewitt, Jane Luu, Jun Chen · The Astronomical Journal · 1996 · 157 citations
Natural Sciences, Astronomy, Physics +12
1–5 of 62
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Center for Astrophysics Harvard & Smithsonian, United States
3 publications · 977 citations
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3
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114
California Institute of Technology
Pasadena, United States
6 h-index
9 publications
1.3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
6 h-index
9 publications
3.4K citations
University of Arizona
Tucson, United States
6 h-index
6 publications
235 citations
Aristotle University of Thessaloniki
Thessaloniki, Greece
4 h-index
9 publications
205 citations
Jet Propulsion Laboratory
Pasadena, United States
4 h-index
5 publications
1.1K citations

University of Rochester
Rochester, United States
3 h-index
6 publications
322 citations
University of Florida
Gainesville, United States
3 h-index
4 publications
1K citations
Institute of Astronomy
Moscow, Russia
3 h-index
5 publications
289 citations
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13 publications · 763 citations
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9 publications · 279 citations
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AJ · 8 publications · 518 citations
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7 publications · 177 citations
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ApJ · 6 publications · 326 citations
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