Classical Orbital Elements

Classical Orbital Elements is a set of six parameters consisting of semi-major axis, eccentricity, inclination, longitude of the ascending node, argument of periapsis, and true anomaly at epoch that uniquely define the size, shape, and orientation of a Keplerian orbit in three-dimensional space relative to a central body.

54

Publications

2.1K

Citations

211

Authors

129

Institutions

Publications per year

2017–2026

4

Authors

211

  1. LB
    L. Binnendijk

    University of Pennsylvania, United States

    4 publications · 64 citations

    4

    h-index

  2. NR
    Nancy Remage Evans

    Smithsonian Astrophysical Observatory, United States

    3 publications · 39 citations

    3

    h-index

  3. HA
    Harold A. McAlister

    Georgia State University, United States

    2 publications · 72 citations

    2

    h-index

  4. PG
    Pini GurŽfil

    Technion – Israel Institute of Technology, Israel

    2 publications · 102 citations

    2

    h-index

  5. JJ
    J. J. Kavelaars

    Herzberg Institute of Astrophysics, Canada

    2 publications · 318 citations

    2

    h-index

1–5 of 211

Venues

  1. The Astronomical Journal

    AJ · 9 publications · 552 citations

    9

    h-index

  2. Journal of Guidance Control and Dynamics

    6 publications · 331 citations

    6

    h-index

  3. The Astrophysical Journal

    ApJ · 5 publications · 134 citations

    5

    h-index

  4. 3

    h-index

  5. Icarus

    2 publications · 62 citations

    2

    h-index

1–5