Trojan Stability
Trojan Stability is a theoretical framework in celestial mechanics that characterizes the long-term orbital stability of small bodies gravitationally trapped near the Lagrangian points L4 and L5 of a two-body system, distinguished by its focus on resonant co-orbital dynamics that prevent ejection or collision despite perturbations.
43
Publications
2K
Citations
153
Authors
83
Institutions
Publications per year
2017–2026
4
Parents
43
Collision probability with the planets and the distribution of planetary matter
E. Öpik · 1951 · 269 citations
Natural Sciences, Astronomy, Physics +14
Extrasolar Trojan planets close to habitable zones
Astronomy and Astrophysics · 2004 · 81 citations · Full text
Natural Sciences, Astronomy, Physics +13
On the stability of the Trojan asteroids.
Antonio Giorgilli, Ch. Skokos · 1997 · 58 citations
1–5 of 43
153
8
h-index
Center for Astrophysics Harvard & Smithsonian, United States
6 publications · 226 citations
6
h-index
5
h-index
4
h-index
3
h-index
1–5 of 153
83
University of Vienna
Vienna, Austria
8 h-index
13 publications
540 citations

Eötvös Loránd University
Budapest, Hungary
4 h-index
10 publications
320 citations
Observatoire de la Côte d’Azur
Nice, France
4 h-index
4 publications
189 citations

York University
Toronto, Canada
3 h-index
5 publications
163 citations
Nanjing University
Nanjing, China
3 h-index
7 publications
229 citations

Centre National de la Recherche Scientifique
Paris, France
3 h-index
3 publications
100 citations

University of Padua
Padua, Italy
3 h-index
5 publications
235 citations
Valongo Observatory
Rio de Janeiro, Brazil
2 h-index
6 publications
181 citations
1–8 of 83
9 publications · 335 citations
10
h-index
AJ · 7 publications · 238 citations
7
h-index
7 publications · 290 citations
7
h-index
4 publications · 188 citations
4
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ApJ · 3 publications · 214 citations
3
h-index
1–5