Remarks on the numerical integration of near-parabolic orbits

Details Remarks on the numerical integration of near-parabolic orbits Remarks on the numerical integration of near-parabolic orbits

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976cemec..14...85s&link_type=abstract

(Conference on Mathematical Methods in Celestial Mechanics, 5th, Oberwolfach, West Germany, Aug. 24-30, 1975.) Celestial Mechani

Mathematics

1

Astrodynamics, Numerical Integration, Orbital Mechanics, Satellite Perturbation, Transformations (Mathematics), Eccentric Orbits, Equations Of Motion, Motion Stability, Orbital Elements, Satellite Drag

Scientific paper

For near-parabolic orbits the distinction between coordinates and
elements disappears provided the KS-technique is used. In KS-variables a
pure parabolic motion is described by linear functions. Advantage is
taken of that fact for establishing numerical procedures in perturbed
near-parabolic cases.

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