There are four systems of a massive central body with a regularily str
uctured satellite system in the Solar system: the planetary system and
the satellite systems of Jupiter, Saturn and Uranus. Comparable struc
tures in these four systems can be understood as indications for compa
rable processes of origin and formation. It is the aim of this paper t
o describe comparable properties, and to discuss possible physical pro
cesses in pre-satellite disks which can be the cause for this comparab
ility.