  Investigations were carried out on the stability of the two gas giant system
HD 60532 itself including additional, smaller bodies. The methods used were
numerical simulations with the Lie Series integration method, and secular
perturbation theory. The aims were to find stable regions for potential
Earth-like planets within the system, and confirming the stability of the
detected planets. As results, the given configuration can be considered stable
for a period of at least 65 million years. The two planets create a large
unstable section between 0.25 and 3.6 AU, where no additional body is able to
remain stable. Variations in the mutual inclination between test bodies and the
rest of the system of up to 20{\deg} have little effects on the size of the
zone of instability.
