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Stability of Asteroidal Motion in the Hecuba Gap

Published online by Cambridge University Press:  14 August 2015

H. Scholl  and
R. Giffen
H. Scholl
Affiliation:
Astronomisches Rechen-Institut, Heidelberg, Germany
R. Giffen
Affiliation:
Astronomisches Rechen-Institut, Heidelberg, Germany

Extract

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There exist gaps in the frequency distribution of the osculating mean motions of the asteroids. In these gaps, the mean motions of the asteroids are commensurable to Jupiter's mean motion.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 62: The Stability of the Solar System , 1974 , pp. 77 - 79
Copyright
Copyright © Reidel 1974 

References

Froeschlé, C. and Scheidecker, J.-P.: 1974, this volume, p. 297.CrossRefGoogle Scholar
Giffen, R. B.: 1973, Astron. Astrophys. 23, 387–403.Google Scholar