Objectives | The ENCELADE Team: Constraining the Dynamical Timescale and Internal Processes of the Saturn and Jupiter Systems from Astrometry

Astrometric reduction of the remaining ISS-Cassini data,
New astrometric reduction of the USNO photographic plates for Saturn,
Dynamical fit to astrometric data of Saturnian physical parameters (including tides in Saturn at different frequencies and Enceladus),
Interpretation of the results in terms of the orbital and interior evolution of the satellites,
Interpretation of ring evolution and formation scenarios,
New astrometric reduction of the USNO photographic plates of Jupiter,
Dynamical fit to astrometric data of Jovian physical parameters (including tides in Jupiter and Io)