Long-term Orbital Integration
Long-Term Orbital Integration is a computational method in celestial mechanics that distinguishes itself by numerically propagating the trajectories of celestial bodies over extended timescales to accurately model the evolution of their orbits under the influence of gravitational and non-gravitational perturbations.
40
Publications
3.2K
Citations
64
Authors
54
Institutions
Publications per year
2017–2026
5
Parents
40
A three million year integration of the earth's orbit
Thomas Quinn, Scott Tremaine, Martin J. Duncan · The Astronomical Journal · 1991 · 277 citations
Natural Sciences, Astronomy, Physics +16
1–5 of 40
64
4
h-index
3
h-index
2
h-index
2
h-index
2
h-index
1–5 of 64
54

University of Toronto
Toronto, Canada
5 h-index
7 publications
1.9K citations
Canadian Institute for Theoretical Astrophysics
Toronto, Canada
4 h-index
4 publications
770 citations
Jet Propulsion Laboratory
Pasadena, United States
3 h-index
5 publications
238 citations
University of Peloponnese
Tripoli, Greece
3 h-index
3 publications
265 citations
The University of Texas at Austin
Austin, United States
2 h-index
3 publications
54 citations

University of Hawaiʻi at Mānoa
Honolulu, United States
2 h-index
2 publications
66 citations
University of California, Los Angeles
Los Angeles, United States
2 h-index
4 publications
431 citations
ETH Zurich
Zurich, Switzerland
2 h-index
2 publications
79 citations
1–8 of 54
AJ · 12 publications · 803 citations
11
h-index
8 publications · 1.4K citations
8
h-index
5 publications · 175 citations
5
h-index
ApJ · 3 publications · 224 citations
3
h-index
Repository · 2 publications · 41 citations
2
h-index
1–5