# The Lissajous-Kustaanheimo-Stiefel transformation

**Authors:** Slawomir Breiter, Krzysztof Langner

arXiv: 1901.06876 · 2019-02-27

## TL;DR

This paper introduces the Lissajous-Kustaanheimo-Stiefel (LKS) transformation, a new method to analyze perturbed Kepler problems using action-angle variables that avoid singularities and do not depend on the orbital plane.

## Contribution

The LKS transformation provides a novel, singularity-free set of action-angle variables for the perturbed Kepler problem, enabling better analysis of orbital stability and dynamics.

## Key findings

- LKS transformation yields singularity-free action-angle variables.
- Allows analysis of stability for most orbital configurations.
- Enables reduction to lower degrees of freedom using bilinear invariant.

## Abstract

The Kustaanheimo-Stiefel transformation of the Kepler problem with a time-dependent perturbation converts it into a perturbed isotropic oscillator of 4-and-a-half degrees of freedom with additional constraint known as bilinear invariant. Appropriate action-angle variables for the constrained oscillator are required to apply canonical perturbation techniques in the perturbed problem. The Lissajous-Kustaanheimo-Stiefel (LKS) transformation is proposed, leading to the action-angle set which is free from singularities of the LCF variables earlier proposed by Zhao. One of the actions is the bilinear invariant, which allows the reduction back to the 3-and-a-half degrees of freedom. The transformation avoids any reference to the notion of the orbital plane, which allowed to obtain the angles properly defined not only for most of the circular or equatorial orbits, but also for the degenerate, rectilinear ellipses. The Lidov-Kozai problem is analyzed in terms of the LKS variables, which allow a direct study of stability for all equilibria except the circular equatorial and the polar radial orbits.

## Full text

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## Figures

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## References

30 references — full list in the complete paper: https://tomesphere.com/paper/1901.06876/full.md

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Source: https://tomesphere.com/paper/1901.06876