Ice II is a rhombohedralcrystalline form of ice with a highly ordered structure. It is formed from ice Ih by compressing it at a temperature of 198K at 300 MPa or by decompressing ice V. When heated it undergoes transformation to ice III. Ordinarywater ice is known as ice Ih, . Different types of ice, from ice II to ice XVIII, have been created in the laboratory at different temperatures and pressures. It is thought that the cores of icy moons like Jupiter'sGanymede may be made of ice II.
History
The properties of ice II were first described and recorded by Gustav Heinrich Johann Apollon Tammann in 1900 during his experiments with ice under high pressure and low temperatures. Having produced ice III, Tammann then tried condensing the ice at a temperature between under of pressure. Tammann noted that in this state ice II was denser than he had observed ice III to be. He also found that both types of ice can be kept at normal atmospheric pressure in a stable condition so long as the temperature is kept at that of liquid air, which slows the change in conformation back to ice Ih. In later experiments by Bridgman in 1912, it was shown that the difference in volume between ice II and ice III was in the range of. This difference hadn't been discovered by Tammann due to the small change and was why he had been unable to determine an equilibrium curve between the two. The curve showed that the structural change from ice III to ice II was more likely to happen if the medium had previously been in the structural conformation of ice II. However, if a sample of ice III that had never been in the ice II state was obtained, it could be supercooled even below −70 °C without it changing into ice II. Conversely, however, any superheating of ice II was not possible in regards to retaining the same form. Bridgman found that the equilibrium curve between ice II and ice IV was much the same as with ice III, having the same stability properties and small volume change. The curve between ice II and ice V was extremely different, however, with the curve's bubble being essentially a straight line and the volume difference being almost always.
