Non-keplerian Orbits

Non-Keplerian Orbits is a theoretical construct in orbital dynamics that denotes a satellite orbit trajectory that deviates from the classical two-body gravitational solution due to continuous propulsion or persistent perturbative forces, thereby maintaining a non-Keplerian path unlike natural or impulsive maneuver-based orbits.

88

Publications

3.2K

Citations

253

Authors

147

Institutions

Publications per year

2017–2026

15

Authors

253

  1. CR
    Colin R. McInnes

    University of Strathclyde, United Kingdom

    15 publications · 569 citations

    14

    h-index

  2. FV
    F. V. Hessman

    University of Göttingen, Germany

    5 publications · 259 citations

    5

    h-index

  3. KB
    K. Beuermann

    University of Göttingen, Germany

    5 publications · 259 citations

    5

    h-index

  4. JS
    Jules Simo

    University of Strathclyde, United Kingdom

    4 publications · 68 citations

    4

    h-index

  5. GM
    Giovanni Mengali

    University of Pisa, Italy

    4 publications · 154 citations

    4

    h-index

1–5 of 253

Venues

  1. 12

    h-index

  2. Journal of Guidance Control and Dynamics

    11 publications · 489 citations

    11

    h-index

  3. Astronomy and Astrophysics

    11 publications · 454 citations

    10

    h-index

  4. The Astrophysical Journal

    ApJ · 7 publications · 454 citations

    7

    h-index

  5. 4

    h-index

1–5