Quaternions, introduced by Hamilton (Philos. Mag. 25, 489-495, 1844) as a generalization of complex numbers, lead to a remarkably simple representation of the perturbed three-dimensional Kepler problem as a perturbed harmonic oscillator. The paper gives an overview of this technique, including an outlook to applications in perturbation theories. © Springer Science+Business Media B.V. 2006.
CITATION STYLE
Waldvogel, J. (2006). Quaternions and the perturbed Kepler problem. In Celestial Mechanics and Dynamical Astronomy (Vol. 95, pp. 201–212). https://doi.org/10.1007/s10569-005-5663-7
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