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Chaotic motions of prometheus and pandora |
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| Authors: | Peter Goldreich Nicole Rappaport |
| Institution: | a California Institute of Technology, Pasadena, CA 91125, USA b Institute for Advanced Study, Princeton, NJ 08540, USA c Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA |
| Abstract: | Recent HST images of the saturnian satellites Prometheus and Pandora show that their longitudes deviate from predictions of ephemerides based on Voyager images. Currently Prometheus is lagging and Pandora leading these predictions by somewhat more than 20°. We show that these discrepancies are fully accounted for by gravitational interactions between the two satellites. These peak every 24.8 days at conjunctions and excite chaotic perturbations. The Lyapunov exponent for the Prometheus-Pandora system is of order 0.3 year−1 for satellite masses based on a nominal density of 0.63 g cm−3. Interactions are strongest when the orbits come closest together. This happens at intervals of 6.2 years when their apses are antialigned. In this context, we note the sudden changes of opposite signs in the mean motions of Prometheus and Pandora at the end of 2000 occurred around the time their apsidal lines were antialigned. |
| Keywords: | Satellites of Saturn Orbits Chaos |
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