Three-body Problem Stability
Three-Body Problem Stability is a theoretical construct in celestial mechanics that characterizes the qualitative persistence of bounded orbital configurations among three gravitationally interacting bodies, distinguishing it from general dynamical stability by addressing the inherent chaos and lack of general analytical solutions in three-body systems.
377
Publications
15.2K
Citations
484
Authors
265
Institutions
Publications per year
2017–2026
44
Parents
377
Dynamics of Systems of Two Close Planets
Brett Gladman · Icarus · 1993 · 639 citations
Natural Sciences, Astronomy, Physics +16
Equivalence Principle for Massive Bodies. I. Phenomenology
Kenneth Nordtvedt · Physical Review · 1968 · 242 citations
Natural Sciences, Astronomy, Physics +13
1–5 of 377
484
20
h-index
9
h-index
National Research Institute of Astronomy and Geophysics, Egypt
8 publications · 515 citations
8
h-index
8
h-index
7
h-index
1–5 of 484
265

Ahmadu Bello University
Zaria, Nigeria
17 h-index
39 publications
1.2K citations
University of Patras
Pátrai, Greece
14 h-index
36 publications
1.3K citations

University of Delhi
New Delhi, India
13 h-index
27 publications
630 citations
Jet Propulsion Laboratory
Pasadena, United States
9 h-index
11 publications
802 citations
Universitat de Barcelona
Barcelona, Spain
9 h-index
12 publications
1.1K citations
Aristotle University of Thessaloniki
Thessaloniki, Greece
9 h-index
9 publications
588 citations
Universitat Politècnica de Catalunya
Barcelona, Spain
8 h-index
14 publications
723 citations

Centre National de la Recherche Scientifique
Paris, France
8 h-index
16 publications
886 citations
1–8 of 265
81 publications · 3.3K citations
31
h-index
44 publications · 1.4K citations
23
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15 publications · 727 citations
14
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AJ · 16 publications · 740 citations
12
h-index
12 publications · 611 citations
11
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1–5