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Investigations were carried out on the stability of the two gas giant systemHD 60532 itself including additional, smaller bodies. The methods used werenumerical simulations with the Lie Series integration method, and secularperturbation theory. The aims were to find stable regions for potentialEarth-like planets within the system, and confirming the stability of thedetected planets. As results, the given configuration can be considered stablefor a period of at least 65 million years. The two planets create a largeunstable section between 0.25 and 3.6 AU, where no additional body is able toremain stable. Variations in the mutual inclination between test bodies and therest of the system of up to 20{\deg} have little effects on the size of thezone of instability.

Stability Analysis of Possible Terrestrial Planets in the HD 60532 System