Orbital Elements

Orbital Elements is a set of six canonical parameters—semi-major axis, eccentricity, inclination, longitude of the ascending node, argument of periapsis, and true anomaly—that uniquely define the size, shape, and orientation of a celestial or artificial body’s orbit in three-dimensional space relative to a central gravitating body.

2K

Publications

111.4K

Citations

4.5K

Authors

1.1K

Institutions

Publications per year

2017–2026

237

Authors

4.5K

  1. DJ
    Daniel J. Scheeres

    University of Colorado Boulder, United States

    18 publications · 1.7K citations

    17

    h-index

  2. SU
    S. Udry

    University of Geneva, Switzerland

    16 publications · 1.7K citations

    16

    h-index

  3. DQ
    D. Queloz

    University of Geneva, Switzerland

    15 publications · 1.7K citations

    15

    h-index

  4. RA
    Robert A. Jacobson

    Iowa State University, United States

    18 publications · 723 citations

    14

    h-index

  5. FP
    F. Pepe

    University of Geneva, Switzerland

    14 publications · 1.7K citations

    14

    h-index

1–5 of 4.5K

Venues

  1. Icarus

    222 publications · 12.8K citations

    61

    h-index

  2. The Astrophysical Journal

    ApJ · 115 publications · 7.7K citations

    48

    h-index

  3. The Astronomical Journal

    AJ · 137 publications · 7.4K citations

    44

    h-index

  4. Celestial Mechanics and Dynamical Astronomy

    117 publications · 6.8K citations

    42

    h-index

  5. Nature

    48 publications · 8.2K citations

    34

    h-index

1–5