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Detailed studies have been done of ice creep as related to the icy satellites, Ganymede and Callisto. Included were: (1) the flow of high-pressure water ices II, III, and V, and (2) frictional sliding of ice I sub h. Work was also begun on the study of the effects of impurities on the flow of ice. Test results are summarized.

Frictional sliding experiments conducted to study crustal behavior on the icy Galilean satellites are described as well as the microstructural aspects of ice flow. An improved heat exchanger and computer control of temperature are being used to explore the lower regimes of strain rate. A preliminary measurement of the strengths of some of the higher pressure polymorphs of ice was obtained and is considered.