
doi: 10.1007/bf01230890
The osculating orbit of a planetary satellite moving in the equatorial plane of the central body under the influence of a rotational symmetric perturbation force is elliptical in first order approximation even if the true orbit is always circular. The satellite motion is influenced by a resonance effect due to this perturbing force. An inclined true satellite orbit cannot be circular.
equatorial plane, osculating orbit, circular orbit, Orbital mechanics, planetary satellite, rotational symmetric perturbation
equatorial plane, osculating orbit, circular orbit, Orbital mechanics, planetary satellite, rotational symmetric perturbation
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