Ideal frames for perturbed Keplerian motions

Details Ideal frames for perturbed Keplerian motions Ideal frames for perturbed Keplerian motions

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976cemec..13..253d&link_type=abstract

Celestial Mechanics, vol. 13, Mar. 1976, p. 253-263.

Computer Science

Cartan Space, Celestial Mechanics, Euler Equations Of Motion, Kepler Laws, Orbit Perturbation, Hamiltonian Functions, Orbital Mechanics, Pfaff Equation

Scientific paper

Cartan's exterior calculus is used to refer a perturbed Keplerian motion
to an ideal frame by means of either the Eulerian parameters or the
Eulerian angles, in which case the equations are given a Hamiltonian
form. The results are compared with the corresponding systems in the
orbital and nodal frames.

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