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It is generally recognized that main-belt asteroids (MBAs) and nuclei ofextinct comets are the two main sources for the Near-Earth-Asteroids (NEAs).Theoretical studies of NEAs dynamics and numerical modelling of their orbitalmotions showed that the resonance mechanism for supplying NEAs is quitesufficient to sustain this population. Asteroid 1983 SA, also known as 3552 DonQuixote, is one of Near Earth Asteroids (NEAs) and the most probable candidatesfor NEAs of the cometary origin. In this work, an investigation on theevolution of the orbit is done by using the SWIFT subroutine package, where thegravitational perturbations of eight planets: Mercury, Venus, Earth, Mars,Jupiter, Saturn, Uranus, and Neptune are considered. Migration of asteroid 3552Don Quixote from Near Earth Asteroids (NEAs) to Jovian-crosser asteroid isfound.

Migration of Near Earth Asteroid to Jovian-Crosser Asteroid:Case Study 3552 Don Quixote