Lagrange Point Stability
Lagrange Point Stability is a theoretical construct in celestial mechanics that characterizes the resilience of equilibrium points in a rotating three-body system to small perturbations, distinguishing itself by its dependence on the gravitational and centrifugal potential landscape and its sensitivity to non-ideal forces such as solar radiation pressure.
20
Publications
631
Citations
39
Authors
28
Institutions
Publications per year
2017–2026
4
20
Edward Belbruno, J. Richard Gott · The Astronomical Journal · 2005 · 79 citations · Full text
Natural Sciences, Astronomy, Physics +14
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39
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28

York University
Toronto, Canada
3 h-index
6 publications
84 citations

University of Strathclyde
Glasgow, United Kingdom
2 h-index
5 publications
95 citations

Johns Hopkins University
Baltimore, United States
2 h-index
2 publications
57 citations
University of Vienna
Vienna, Austria
1 h-index
1 publications
30 citations
Laboratoire d’études spatiales et d’instrumentation en astrophysique
Meudon, France
1 h-index
1 publications
26 citations
Nanjing University
Nanjing, China
1 h-index
2 publications
60 citations

Beijing Institute of Technology
Beijing, China
1 h-index
3 publications
75 citations

University of Glasgow
Glasgow, United Kingdom
1 h-index
1 publications
65 citations
1–8 of 28
AJ · 5 publications · 164 citations
5
h-index
3 publications · 60 citations
3
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3 publications · 84 citations
3
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1 publications · 75 citations
1
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ApJ · 1 publications · 36 citations
1
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1–5