Long-term Orbit Evolution
Long-Term Orbit Evolution is a theoretical framework in orbital mechanics that models the gradual, cumulative changes in celestial bodies' trajectories over extended periods due to secular perturbations, distinguishing it from short-term or periodic orbital variations.
113
Publications
5K
Citations
241
Authors
150
Institutions
Publications per year
2017–2026
20
Parents
113
Secular evolution of the solar system over 10 million years
J. Laskar · 1988 · 219 citations
Natural Sciences, Astronomy, Physics +16
1–5 of 113
241
7
h-index
Istituto di Scienza e Tecnologie dell'Informazione "Alessandro Faedo", Italy
6 publications · 186 citations
6
h-index
Istituto di Scienza e Tecnologie dell'Informazione "Alessandro Faedo", Italy
6 publications · 186 citations
6
h-index
4
h-index
4
h-index
1–5 of 241
150
Observatoire de la Côte d’Azur
Nice, France
9 h-index
15 publications
794 citations

Centre National de la Recherche Scientifique
Paris, France
8 h-index
14 publications
324 citations
Institut de Mécanique Céleste et de Calcul des Éphémérides
Paris, France
5 h-index
5 publications
121 citations

University of Namur
Namur, Belgium
5 h-index
7 publications
209 citations
Politecnico di Milano
Milan, Italy
5 h-index
8 publications
171 citations
Charles University
Prague, Czechia
5 h-index
7 publications
164 citations

Czech Academy of Sciences, Astronomical Institute
Ondřejov, Czechia
5 h-index
6 publications
128 citations

Sorbonne Université
Paris, France
5 h-index
6 publications
133 citations
1–8 of 150
19 publications · 943 citations
16
h-index
10 publications · 365 citations
10
h-index
9 publications · 230 citations
9
h-index
ApJ · 10 publications · 1.1K citations
9
h-index
8 publications · 207 citations
8
h-index
1–5