Trojan Asteroid Dynamics
Trojan Asteroid Dynamics is a theoretical framework within celestial mechanics that specifically models the orbital behavior and stability of asteroids co-orbiting with a planet in its Lagrangian points, thereby distinguishing itself from general asteroid dynamics through its focus on resonant gravitational configurations.
61
Publications
3.1K
Citations
126
Authors
91
Institutions
Publications per year
2017–2026
10
Parents
61
Chaotic capture of Jupiter's Trojan asteroids in the early Solar System
Alessandro Morbidelli, Harold F. Levison, K. Tsiganis et al. · Nature · 2005 · 905 citations
Natural Sciences, Astronomy, Physics +16
Dynamical evolution of Jupiter's Trojan asteroids
Harold F. Levison, Eugene M. Shoemaker, C. S. Shoemaker · Nature · 1997 · 159 citations
Natural Sciences, Astronomy, Physics +14
1–5 of 61
126
4
h-index
4
h-index
Center for Astrophysics Harvard & Smithsonian, United States
4 publications · 125 citations
4
h-index
3
h-index
3
h-index
1–5 of 126
91

Eötvös Loránd University
Budapest, Hungary
6 h-index
8 publications
197 citations

Southwest Research Institute
San Antonio, United States
4 h-index
9 publications
1.3K citations
University of Vienna
Vienna, Austria
4 h-index
8 publications
204 citations
Kindai University
Osaka, Japan
4 h-index
4 publications
151 citations
Yale University
New Haven, United States
4 h-index
4 publications
131 citations
Observatoire de la Côte d’Azur
Nice, France
3 h-index
7 publications
3.7K citations

University of Hawaii System
Honolulu, United States
3 h-index
6 publications
130 citations

Centre National de la Recherche Scientifique
Paris, France
3 h-index
4 publications
136 citations
1–8 of 91
14 publications · 479 citations
13
h-index
12 publications · 412 citations
12
h-index
8 publications · 391 citations
8
h-index
AJ · 4 publications · 269 citations
4
h-index
3 publications · 78 citations
3
h-index
1–5