Space Sci Rev DOI 10.1007/s11214-010-9635-1 Evolution of Icy Satellites G. Schubert · H. Hussmann · V. L a i n e y · D.L. Matson · W.B. McKinnon · F. Sohl · C. Sotin · G. Tobie · D. Turrini · T. Van Hoolst Received: 10 July 2009 / Accepted: 8 February 2010 © The Author(s) 2010 Abstract Evolutionary scenarios for the major satellites of Jupiter, Saturn, Neptune, and Pluto-Charon are discussed. In the Jovian system the challenge is to understand how the G. Schubert () Department of Earth and Space Sciences and Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095, USA e-mail:
[email protected] H. Hussmann · F. Sohl German Aerospace Center (DLR), Institute of Planetary Research, 12489 Berlin, Germany H. Hussmann e-mail:
[email protected] F. Sohl e-mail:
[email protected] V. Lainey IMCCE-Observatoire de Paris, UMR 8028 du CNRS, 77 Avenue Denfert-Rochereau, 75014 Paris, France e-mail:
[email protected] D.L. Matson JPL 183-335, 4800 Oak Grove Drive, Pasadena, CA 91109, USA e-mail:
[email protected] W.B. McKinnon Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, One Brookings Drive, Saint Louis, MO 63130, USA e-mail:
[email protected] C. Sotin JPL/Caltech, 4800 Oak Grove Drive, Pasadena, CA 91109, USA e-mail:
[email protected] G. Tobie University of Nante, Nantes, France e-mail:
[email protected] G. Schubert et al. present Laplace resonance of Io, Europa, and Ganymede was established and to determine whether the heat being radiated by Io is in balance with the present tidal dissipation in the moon.