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

Authors

64

  1. ST
    Scott Tremaine

    Institute for Advanced Study, United States

    4 publications · 483 citations

    4

    h-index

  2. TE
    T. E. Simos

    University of Peloponnese, Greece

    3 publications · 232 citations

    3

    h-index

  3. HR
    Hanno Rein

    University of Toronto, Canada

    2 publications · 1.2K citations

    2

    h-index

  4. DK
    D. K. Yeomans

    Jet Propulsion Laboratory, United States

    2 publications · 151 citations

    2

    h-index

  5. MK
    M. Konacki

    Nicolaus Copernicus Astronomical Center, Poland

    2 publications · 41 citations

    2

    h-index

1–5 of 64

Venues

  1. The Astronomical Journal

    AJ · 12 publications · 803 citations

    11

    h-index

  2. 8

    h-index

  3. Celestial Mechanics and Dynamical Astronomy

    5 publications · 175 citations

    5

    h-index

  4. The Astrophysical Journal

    ApJ · 3 publications · 224 citations

    3

    h-index

  5. arXiv (Cornell University)

    Repository · 2 publications · 41 citations

    2

    h-index

1–5