Collinear Lagrange Points is a theoretical construct in celestial mechanics denoting the set of three equilibrium points—L₁, L₂, and L₃—located along the line connecting two massive primary bodies in a restricted three-body system, distinguished by their linear alignment with the primaries and their dynamical instability.
60
Publications
2.4K
Citations
125
Authors
58
Institutions
Publications per year
2017–2026
10
Variants
Euler PointsL1, L2, And L3
Parents
Publications
60
1–5 of 60
Authors
125
- GM
3
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- CG
3
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- AA
3
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- DL
3
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- JS
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1–5 of 125
Institutions
58
University of Delhi
New Delhi, India
4 h-index
3 publications
53 citations
University of Pisa
Pisa, Italy
3 h-index
11 publications
361 citations
University of Patras
Pátrai, Greece
3 h-index
7 publications
150 citations
Ahmadu Bello University
Zaria, Nigeria
3 h-index
5 publications
129 citations
University of Colorado Boulder
Boulder, United States
2 h-index
3 publications
71 citations
Nanjing University
Nanjing, China
2 h-index
6 publications
96 citations
University of Cincinnati
Cincinnati, United States
2 h-index
2 publications
503 citations
Politecnico di Milano
Milan, Italy
2 h-index
2 publications
24 citations
1–8 of 58
Venues
- Celestial Mechanics and Dynamical Astronomy
9 publications · 660 citations
9
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- Astrophysics and Space Science
6 publications · 141 citations
6
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- Journal of Guidance Control and Dynamics
4 publications · 146 citations
5
h-index
- Acta Astronautica
4 publications · 77 citations
4
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- Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology
3 publications · 85 citations
3
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1–5