Equinoctial Elements

Equinoctial Elements is a set of orbital elements that parameterize the shape, size, and orientation of an orbit using a singularity-free formulation at zero inclination, distinguished from classical orbital elements by employing the longitude of the ascending node, the argument of perigee, and the mean longitude at epoch in a way that avoids numerical instabilities near equatorial orbits.

36

Publications

1.8K

Citations

66

Authors

31

Institutions

Publications per year

2017–2026

6

Variants

Equinoctial Orbital Elements

Authors

66

  1. JA
    Jean Albert Kéchichian

    The Aerospace Corporation, United States

    5 publications · 112 citations

    5

    h-index

  2. PC
    Paul Cefola

    Draper Laboratory, United States

    3 publications · 306 citations

    3

    h-index

  3. MV
    Massimiliano Vasile

    University of Strathclyde, United Kingdom

    3 publications · 170 citations

    3

    h-index

  4. KT
    Kyle T. Alfriend

    Texas A&M University, United States

    3 publications · 119 citations

    3

    h-index

  5. MW
    Martin Walker

    University of Manchester, United Kingdom

    2 publications · 360 citations

    2

    h-index

1–5 of 66

Venues

  1. Journal of Guidance Control and Dynamics

    11 publications · 615 citations

    11

    h-index

  2. Celestial Mechanics and Dynamical Astronomy

    5 publications · 682 citations

    5

    h-index

  3. Acta Astronautica

    3 publications · 105 citations

    3

    h-index

  4. Astrodynamics Conference

    Conference · 2 publications · 64 citations

    2

    h-index

  5. Chinese Journal of Aeronautics

    CJA · 2 publications · 58 citations

    2

    h-index

1–5