Secular and Periodic Motions of the Node of an Artificial Earth-Satellite

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Scientific paper

IN a recent paper on the effect of the Earth's oblateness on the orbit of a near satellite, King-Hele1 mars an otherwise commendable presentation by abundant criticism of some earlier papers on this subject by myself and collaborators2,3. Although King-Hele's remarks were not so intended, his statements have had the effect of raising serious doubts about the validity of my early solutions and in particular about the usefulness of my approach to the problem of satellite orbit perturbations.

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