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We observe similar structures in the orbital radii of satellite and ringsystems of Uranus, Jupiter and Neptune. This stimulates an investigation thatthe evolution of these systems and Saturn's system is initiated by a commonmechanism that involves the interaction of radiation with their subnebulae(protosatellite disks). A model is presented that is characterized by resonancecreated through stimulated radiative molecular association (SRMA) reactions. Inthis model thermal energy is extracted from a protoplanetary disk at specificdistances from the protoplanet wherever there is a match between the localthermal energy of the disk and the energy of photons impinging on the disk.Radiation is supplied by a portion of the hydrogen molecule's spectrum for theUranian, Jovian and Neptunian disks and a portion of the hydrogen atom'sspectrum for the Saturnian disk. Findings shed light on the early evolution andstructure of satellite systems including the complicated ring system of Saturn.They also link satellite orbital radii size distributions to shapes oftemperature distributions (TD's) in protosatellite disks. Theoreticallydetermined TD's in the protosatellite disks of Uranus (Mousis 2004) and Saturn(Mousis Gautier and Bockelee-Moran, 2002) are essential to the presentinvestigation.

Temperature Distributions in the Protosatellite Disks of Uranus, Jupiter, Neptune and Saturn and Common Structure in Their Satellite Systems