Accelerated particle irradiation parameters at different stages of the Solar system matter evolution

Consequences of accelerated particle interaction with matter at different stages of solar system evolution are considered. Calculations are made within the frames of a model based on a supposition that a burst of cosmic objects leads to detonation of H, He, C, O(Ne), particle acceleration at the shock wave front and their interaction with matter through which the shock wave passes at the same time. Three main irradiation stages: the common galactic nucleosynthesis, supernova flare and expanding supernova shell are studied. Significant differences in irradiation parameters of the solar system metter are observed at the main stages of its evolution