Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-26T05:53:44.052Z Has data issue: false hasContentIssue false
  • English
  • Français

The k:k+4 resonances in planetary systems

Published online by Cambridge University Press:  28 February 2005

Benoît Noyelles  and
Alain Vienne
Benoît Noyelles
Affiliation:
IMCCE - Laboratoire d'Astronomie de Lille, UMR 8028 du CNRS, 1 impasse de l'Observatoire, 59000 Lille, France e-mail : Benoit.Noyelles@imcce.fr
Alain Vienne
Affiliation:
IMCCE - Laboratoire d'Astronomie de Lille, UMR 8028 du CNRS, 1 impasse de l'Observatoire, 59000 Lille, France e-mail : Benoit.Noyelles@imcce.fr
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In this study we give a first description of De Haerdtl's 3:7 inequality between the Jovian satellites Ganymede and Callisto and 1:5 inequality between the Saturnian Titan and Iapetus and the resonant arguments associated. For each inequality, 19 arguments are associated. The overlapping of resonant zones induces stochasic layers that the system might have crossed in the past thanks to tidal dissipation.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Celestial mechanicsplanets and satellites: individual: Jupiter - Saturn
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUC197 , August 2004 , pp. 453 - 458
Copyright
© 2005 International Astronomical Union