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| Paper: |
The Orbital Evolution of Near-Earth Asteroids in the 3:1 Mean Motion Resonance |
| Volume: |
316, Order and Chaos in Stellar and Planetary Systems |
| Page: |
118 |
| Authors: |
Timoshkova, E.I. |
| Abstract: |
The paper examines the orbital evolution of a group of 12 near-Earth asteroids with the mean motions being in resonance 3:1 with Jupiter, by the numerical integration over 100,000 years. The computation of six osculating elements has been done by forward integration taking into account the perturbations from all 9 major planets. The behaviour of the osculating semi-major axis, eccentricity and inclination has been analysed for all time of integration. |
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