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The gravitational N-body simulation in the Solar system was performed usingdifferent parallel approaches with the comparisons in the computational timesand speed-up values being carried out under different model sizes and thenumber of processors. The numerical integration used is a second-order velocityVerlet approach which gives the acceptable accuracy in the orbits of majorbodies and asteroids with a time step size of 0.1 days.

N-body Simulations of the Solar System with CPU-based Parallel Methods