Abstract
A recently developed iterative technique for solving the perturbed Kepler problem is explained, in a step-by-step detail, using the simple example of oblateness perturbations. The results are then extended to deal with higher-degree zonal harmonics.
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Vrbik, J. Zonal-Harmonics Perturbations. Celestial Mech Dyn Astr 91, 217–237 (2005). https://doi.org/10.1007/s10569-004-2294-3
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DOI: https://doi.org/10.1007/s10569-004-2294-3