Trojan Dynamics
Trojan Dynamics is a theoretical framework in celestial mechanics that models the stability and orbital evolution of small bodies trapped in the Lagrangian points of a resonant orbit, distinguishing itself by analyzing the long-term gravitational interactions between co-orbital objects in 1:1 mean-motion resonance with a secondary mass.
49
Publications
1.4K
Citations
87
Authors
70
Institutions
Publications per year
2017–2026
10
Parents
49
1–5 of 49
87
4
h-index
3
h-index
3
h-index
3
h-index
3
h-index
1–5 of 87
70
University of Vienna
Vienna, Austria
4 h-index
5 publications
139 citations
Observatoire de la Côte d’Azur
Nice, France
4 h-index
5 publications
196 citations
Kindai University
Osaka, Japan
3 h-index
3 publications
101 citations

UNSW Sydney
Sydney, Australia
3 h-index
3 publications
101 citations

Consejo Nacional de Investigaciones Científicas y Técnicas
Buenos Aires, Argentina
3 h-index
4 publications
94 citations
Nanjing University
Nanjing, China
3 h-index
6 publications
122 citations

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

Eötvös Loránd University
Budapest, Hungary
2 h-index
3 publications
80 citations
1–8 of 70
11 publications · 381 citations
10
h-index
7 publications · 247 citations
7
h-index
7 publications · 232 citations
7
h-index
3 publications · 84 citations
3
h-index
2 publications · 30 citations
2
h-index
1–5