Abstract
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.
Original language | English |
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Title of host publication | Dynamics of Populations of Planetary Systems |
Subtitle of host publication | Proceedings of IAU Colloquium #197, held 31 August - 4 Spetember, 2004 in Belgrade, Serbia and Montenegro |
Editors | Z Knezevic, A Milani |
Publisher | Cambridge University Press |
Pages | 453-458 |
Number of pages | 6 |
Publication status | Published - 2005 |
Keywords
- Celestial mechanics
- planets and satellites: individual: Jupiter - Saturn