The orbital evolution of the near-Earth asteroids.

Computer Science

Scientific paper

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Near-Earth Objects: Orbital Evolution

Scientific paper

Based on the property that the motions of NEAs in the solar system can be described by the model of a perturbed two-body problem. The authors use a composition of an algorithm to construct and improve explicit symplectic algorithm with higher efficiency for a non-autonomous Hamiltonian system. The orbital evolutions of 86 NEAs for a time span of 103 ≡ 104 years were computed.

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