Mathematics
Scientific paper
Feb 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975cemec..11...39s&link_type=abstract
Celestial Mechanics, vol. 11, Feb. 1975, p. 39-41.
Mathematics
6
Equations Of Motion, Orbit Perturbation, Perturbation Theory, Two Body Problem, Angular Momentum, Eccentricity, Harmonic Oscillators, Transformations (Mathematics)
Scientific paper
The equations of motion for the perturbed two-body problem are transformed into a perturbed harmonic oscillator by means of a time transformation and by using the perturbed and unperturbed forms for angular momentum, the Laplace or eccentricity vector, and energy. The motion is then completely determined by a set of equations which is of order 11.
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