asteroidal motion
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1984 ◽  
Vol 34 (1-4) ◽  
pp. 443-452 ◽  
Author(s):  
J. Schubart ◽  
R. Bien
Keyword(s):  

1983 ◽  
Vol 74 ◽  
pp. 163-163
Author(s):  
H. Scholl ◽  
C. Froeschle

AbstractResonant asteroidal motion is investigated over 17 000 years in a three-dimensional elliptical model Sun-Jupiter-Asteroid averaged by Schubart's method à la Poincarè. Orbits remain trapped in the resonance over this period. The various stability mechanisms are discussed. With respect to their behaviour of ω and ῶ, our resulting orbits reveal 5 distinct classes. These 5 classes can be described in Schubart's topology for the planar problem. As compared to the planar case, eccentricities of orbits in the three-dimensional model vary more strongly. This is an important result for the problem of the delivery of meteorites.


1979 ◽  
Vol 81 ◽  
pp. 207-215 ◽  
Author(s):  
Joachim Schubart

This paper consists of a review about work done on three-dimensional motion at commensurabilities of either the mean motions, or of secular periods, and of a report on the author's recent results on some special cases. Real and fictitious asteroidal orbits and the corresponding long-period effects are the main subject of interest. At first, methods are listed.


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