Evolution of Orbits in the Outer Part of the Asteroidal Belt and in the Kirkwood Gaps as Influenced by the Mass Effects of Saturn and Jupiter

Author:

Froeschlé C.,Scholl H.

Publisher

Springer Netherlands

Reference8 articles.

1. Franklin, F.A., Marsden, B.G., Williams, J.G., Bardwell, C.M. (1975), Astron. J. 80, p. 729.

2. Froeschlé, C. and Scholl, H. (1978), Astron. and Astrophys., to be published.

3. Lecar, M. and Franklin, F.A. (1973), Icarus 20, p. 422.

4. Nacozy, P.E. (1976), Astron. J. 81, p. 787.

5. Scholl, H. and Froeschlé, C. (1975), Astron. and Astrophys. 42, p. 457.

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1. Irregular behaviour and eccentricity increase in the trajectories of a dynamical system modelling asteroidal motions;Earth, Moon and Planets;1991-09

2. A hyperbolic twist mapping model for the study of asteroid orbits near the 3?1 resonance;ZAMP Zeitschrift f#x00FC;r angewandte Mathematik und Physik;1986-09

3. On the Stability of Resonant Asteroid Orbits;International Astronomical Union Colloquium;1983

4. On the Stability of Resonant Asteroid Orbits;Astrophysics and Space Science Library;1983

5. A Qualitative Study of Stabilizing and Destabilizing Factors in Planetary and Asteroidal Orbits;Applications of Modern Dynamics to Celestial Mechanics and Astrodynamics;1982

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