D. L. Blaney, R. T. Pappalardo, H. Hussman, G. C. Collins, R. M. Mastrapa, J. F. Cooper, R. Greeley, J. B. Dalton, T. A. Hurford, E. B. Bierhaus, F. Nimmo, D. A. Williams, D. A. Senske , D. Grinspoon, R. E. Johnson, S. Kattenhorn, P. Hayne, B. Betts, W. B. McKinnon, L. M. Prockter, A. P. Showman, J. H. Shirley, K. Khurana, S. Grasby, B. G. Bills, L. Friedman, J. Castillo, C. Sotin, G. Hansen, K. Klaus, B. J. Buratti, S. W. Asmar, M. J. S. Belton, E. Heggy, L. Sklar, A. R. Hendrix, J. R. Spear, S. Ulamec, L. Bruzzone, F. Tosi, R. Jaumann, G. Strazzulla, A. Coates, J. Emery, L. Allamandola, A. Coustenis, R. W. Carlson, W. Grundy, S. D. Vance, G. Branduardi-Raymont, M. Barmatz, P. M. Beauchamp, A. D. Anbar, C. A. Raymond, K. P. Hand, E. Shock, K. Stephan, D. L. Goldsby, D. D. Blankenship, M. Choukroun, W. Moore, E. P. Turtle, T. Pierson, S. Neuer, M. Zolotov
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets.
Europa''s icy surface may hide an ocean of liquid water. We summarize the unanswered questions pertaining to Europa following the Galileo mission, and address how those questions will be answered by suggested missions such as EJSM and a lander, as well as new telescopic and laboratory measurements.