Discovery of new ice may change understanding of water

The newly discovered ice is amorphous - that is, its molecules are in a disorganised form, not neatly ordered as they are in ordinary, crystalline ice. Amorphous ice, although rare on Earth, is the main type of ice found in space. That is because in the colder environment of space, ice does not have enough thermal energy to form crystals.

For the study, published in the journal Science, the research team used a process called ball milling, vigorously shaking ordinary ice together with steel balls in a jar cooled to -200 degrees Centigrade.

They found that, rather than ending up with small bits of ordinary ice, the process yielded a novel amorphous form of ice that, unlike all other known ices, had the same density as liquid water and whose state resembled water in solid form. They named the new ice medium-density amorphous ice (MDA).

The team suggested that MDA (which looks like a fine white powder) may exist inside ice moons of the outer solar system, as tidal forces from gas giants such as Jupiter and Saturn may exert similar shear forces on ordinary ice as those created by ball milling. In addition, the team found that when MDA was warmed up and recrystallised, it released an extraordinary amount of heat, meaning it could trigger tectonic motions and “icequakes” in the kilometres-thick covering of ice on moons such as Jupiter’s Ganymede (pictured below). 

Senior author Professor Christoph Salzmann (UCL Chemistry) said: “Water is the foundation of all life. Our existence depends on it, we launch space missions searching for it, yet from a scientific point of view it is poorly understood.

“We know of 20 crystalline forms of ice, but only two main types of amorphous ice have previously been discovered, known as high-density and low-density amorphous ices. There is a huge density gap between them and the accepted wisdom has been that no ice exists within that density gap. Our study shows that the density of MDA is precisely within this density gap and this finding may have far-reaching consequences for our understanding of liquid water and its many anomalies.”

The density gap between the known amorphous ices has led scientists to suggest water in fact exists as two liquids at very cold temperatures and that theoretically, at a certain temperature, both of these liquids could co-exist, with one type floating above the other, as when mixing oil and water. This hypothesis has been demonstrated in a computer simulation, but not confirmed by experiment. The researchers say that their new study may raise questions about the validity of this idea.

Professor Salzmann said: “Existing models of water should be re-tested. They need to be able to explain the existence of medium-density amorphous ice. This could be the starting point for finally explaining liquid water.”

The researchers proposed that the newly discovered ice may be the true glassy state of liquid water – that is, a precise replica of liquid water in solid form, in the same way that glass in windows is the solid form of liquid silicon dioxide. However, another scenario is that MDA is not glassy at all, but is in a heavily sheared crystalline state.

Co-author Professor Andrea Sella (UCL Chemistry) said: “We have shown it is possible to create what looks like a stop-motion kind of water. This is an unexpected and quite amazing finding.”

Lead author Dr Alexander Rosu-Finsen, who carried out the experimental work while at UCL Chemistry, said: “We shook the ice like crazy for a long time and destroyed the crystal structure. Rather than ending up with smaller pieces of ice, we realised that we had come up with an entirely new kind of thing, with some remarkable properties.”

By mimicking the ball-milling procedure via repeated random shearing of crystalline ice, the team also created a computational model of MDA. Dr Michael Davies, who carried out the computational modelling whilst a PhD student in the ICE (interfaces, catalytic & environmental) lab at UCL and the University of Cambridge, said: “Our discovery of MDA raises many questions on the nature of liquid water and so understanding MDA’s precise atomic structure is very important.” 

Ordinary crystalline ice (left) and MDA (right) at the atomic-scale. Credit: Michael Davies

Water has many anomalies that have long baffled scientists. For instance, water is at its most dense at 4 degrees Centigrade and becomes less dense as it freezes (hence why ice floats). Also, the more you squeeze liquid water, the easier it gets to compress, deviating from principles true for most other substances. 

Amorphous ice was first discovered in its low-density form in the 1930s when scientists condensed water vapour on a metal surface cooled to -110 degrees Centigrade. Its high-density state was discovered in the 1980s when ordinary ice was compressed at nearly -200 degrees Centigrade. While common in space, on Earth, amorphous ice is thought only to occur in the cold upper reaches of the atmosphere.

Screenshot from video (below) showing the jar with medium-density amorphous ice inside, with steel balls and liquid nitrogen.

Ball milling is a technique used in several industries to grind or blend materials, but had not before been applied to ice. In the study, liquid nitrogen was used to cool a grinding jar to -200 degrees Centigrade and the density of the ball-milled ice was determined from its buoyancy in liquid nitrogen. The researchers used a number of other techniques to analyse the structure and properties of MDA, including X-ray diffraction (looking at the pattern of X-rays reflected off the ice) and Raman spectroscopy (looking at how the ice scatters light) at UCL Chemistry as well as small-angle diffraction at the UCL Centre for Nature Inspired Engineering to explore its long-range structure.

Furthermore, they used calorimetry to investigate the heat released when the medium-density ice recrystallised at warmer temperatures. They found that, if they compressed the MDA and then warmed it up, it released a surprisingly large amount of energy as it recrystallised showing that H₂O can be a high-energy geophysical material that may drive tectonic motions in the ice moons of the solar system.

Links

• The paper in Science
• Professor Christoph Salzmann’s academic profile
• Professor Andrea Sella’s academic profile
• UCL Chemistry
• UCL Mathematical & Physical Sciences
• ICE lab
• UCL Centre for Nature Inspired Engineering

Images

• From top: Part of the set-up for creating medium-density amorphous ice: ordinary ice and steel balls in a jar. Credit: Christoph Salzmann.
• Composite image of Jupiter’s moon Ganymede, taken by the NASA Juno spacecraft on its 34^th flyby of the gas giant. Credit: NASA/JPL-Caltech/SwRI/MSSS/Kevin M. Gill
• Ice to MDA computational image: Ordinary crystalline ice (left) and MDA (right) at the atomic-scale. Credit: Michael Davies
• Screenshot from video (below) showing the jar with medium-density amorphous ice inside, with steel balls and liquid nitrogen.

Videos

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