Orbital Perturbations

Orbital Perturbations is a dynamical deviation in the trajectory of a celestial or artificial satellite from its ideal two-body Keplerian orbit, caused by external forces such as gravitational influences from third bodies, atmospheric drag, solar radiation pressure, or non-spherical mass distributions of the primary body.

2.3K

Publications

106.4K

Citations

3.5K

Authors

1.1K

Institutions

Publications per year

2017–2026

366

Authors

3.5K

  1. DJ
    Daniel J. Scheeres

    University of Colorado Boulder, United States

    43 publications · 2.4K citations

    25

    h-index

  2. LI
    Lorenzo Iorio

    Ministry of Education, Universities and Research, Italy

    21 publications · 642 citations

    15

    h-index

  3. KT
    Kyle T. Alfriend

    Texas A&M University, United States

    18 publications · 1.1K citations

    15

    h-index

  4. DG
    D. G. King‐Hele

    Electronics and Radar Development Establishment, India

    18 publications · 444 citations

    14

    h-index

  5. PG
    Pini GurŽfil

    Technion – Israel Institute of Technology, Israel

    17 publications · 457 citations

    14

    h-index

1–5 of 3.5K

Venues

  1. The Astrophysical Journal

    ApJ · 99 publications · 8K citations

    51

    h-index

  2. The Astronomical Journal

    AJ · 143 publications · 10.4K citations

    46

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    181 publications · 7.8K citations

    45

    h-index

  4. Celestial Mechanics and Dynamical Astronomy

    216 publications · 7.7K citations

    45

    h-index

  5. Icarus

    94 publications · 6.1K citations

    43

    h-index

1–5