Metanhydrater er en type is som inneholder fanget metan. Forskere har fått mer innsikt i hvordan dette uvanlige stoffet reagerer på ytre belastning. Foto: Geir Mogen
Methane hydrates, sometimes called clathrates, are a kind of ice that contains trapped methane. Researchers are beginning to unlock key properties of this unusual substance. Photo: Geir Mogen

Uncovering secrets of ice that burns

Methane hydrates can be seen as a potential energy source or as a dangerous source of methane – a greenhouse gas that is 20 times more potent than CO2. With the help of a supercomputer and an interdisciplinary team, scientists have uncovered important details about their stability if they are disturbed by human-induced or natural forces.

Methane hydrates are a kind of ice that contains methane, and that form at certain depths under the sea or buried in permafrost. They can also form in pipelines that transport oil and gas, leading to clogging. Yet methane hydrates are nearly impossible to study because it is very hard to get samples, and the samples themselves are highly unstable in the laboratory.

A team of scientists from Norway, China and the Netherlands has now shown how the size of grains of the molecules that make up the natural structure of methane hydrates determines how they behave if they are loaded with weight or disturbed.

That could have important implications for everything from climate science to their use as a future energy source, said Zhiliang Zhang, a professor at the Norwegian University of Science and Technology and founder of the university’s Nanomechanical Lab.

“If we have basic knowledge about the mechanical properties of methane hydrates, we can use this information so that we manage them properly,” Zhang said. “How methane hydrates behave can have a big impact on safety, environmental issues and climate change.”

Poorly understood and unstable


Methane hydrates are thought to be found on Mars’s polar ice caps. If so, it might be possible to mine them to provide power to possible manned missions to Mars. Here, the unmanned Curiosity Mars rover takes a selfie on the “Big Sky” site on Mount Sharp, on Mars. Photo credit: NASA/JPL-Caltech/MSSS

Methane hydrates have been known since the 1930s, when natural gas companies found that their pipelines were sometimes clogged by a kind of ice composed of water and methane. Methane hydrates were later found in permafrost in the 1960s, and in the oceans, commonly on the edges of the continental shelves, but only at certain ocean pressures and temperatures. They are also thought to be found on other planets, including Mars.

When methane hydrates “melt”, they release the methane trapped inside the ice, but because the methane was first trapped under pressure when the hydrate was formed, one cubic metre of solid methane hydrate will release 160 cubic metres of methane gas. That makes them either a potent energy source, or if they melt as the permafrost melts, a potent source of methane, which will act as a greenhouse gas.

But mining methane hydrates as an energy source, an option that is being explored by Japan among others, is technically difficult. Their location on the soft, sediment-loaded edges of the continental shelves makes them difficult to mine, and when they are disturbed, their crystal structure may suddenly dissociate and release the methane trapped inside.

This mechanism has been suggested as one reason why the largest landslide known to humankind, the Storegga Slide, was so destructive. The Storegga Slide took place about 8000 years ago, from an underwater location off the west coast of southern Norway.

The slides – there were three in total­– sent a wall of water roaring out across the North Sea and Norwegian Sea. The evidence of the passage of the tsunami wave in Scotland that shows the wave reached heights of 3-6 metres in that region. One hypothesis for the slide was that an earthquake caused the methane hydrates in the region to become unstable and to explosively release their gas.

Computer simulations show surprising behaviour

Researchers at NTNU’s Nanomechanical Lab and from the university’s Department of Chemistry and their collaborators in China and the Netherlands are interested in understanding the relation between molecular structures and the mechanical stability of materials. Methane hydrates, with their ice lattice structure containing trapped molecules of methane, pose an intriguing three-dimensional and practical problem from this perspective.

Bjørn Skallerud, Zhiliang Zhang, Signe Kjelstrup, Jianying He from NTNU

From left, Bjørn Skallerud and Zhiliang Zhang, both professors in NTNU’s Department of Structural Engineering; Signe Kjelstrup, professor in NTNU’s Department of Chemistry and Jianying He, an associate professor in NTNU’s Department of Structural Engineering were involved in a cross-disciplinary effort to study the mechanical properties of methane hydrates. They were joined by colleagues from Xiamen University and the China University of Geosciences and Delft University of Technology in the Netherlands in a publication in Nature Communications. Photo: Nancy Bazilchuk, NTNU

In a paper published in the 2 November edition of Nature Communications, corresponding author Zhang and his colleagues describe how they used a computer simulation of two types of methane hydrates, monocrystalline hydrates and polycrystalline hydrates, to see what would happen if they were compressed or if pressures on the hydrates were suddenly released.

The researchers built their computer models using common molecular models for ice/water and methane, arranged as either monocrystalline or polycrystalline grains, and simulated the effect of applying forces to the collection of grains.

Maximum capacity found

The simulated hydrate structures were subjected to two different kinds of stress: tensile stress, or the forces they would experience as they were pulled apart, and compressive stress, or the forces they would experience if they were squashed by weight.

The simulations showed that the size of the crystals—what researchers call the grain size—that made up the hydrate structure had a great deal to say in terms of how the structure reacted to both kinds of stresses.

In both tensile and compression stress simulations, the surprising finding was that as the grain size got smaller, the hydrates first got stronger, able to tolerate both compression and tensile stress—but only until they reached a certain grain size. If the researchers conducted simulations on grain sizes smaller than those identified as the turning point, the hydrate actually got weaker.

The maximum capacity of the hydrates appears when the grain size is around 15 to 20 nm. This resembles the behaviour of polycrystalline metals, such as copper. However, this is the first time that researchers have seen this type of behaviour in methane hydrates as a material. The grain size-dependent strength and maximum capacity that the researchers found can be used in predicting and preventing the failure of hydrates in the future.

Instability can be triggered

This unexpected rapid weakening of the crystal structure as the grain size gets smaller has important implications for any work in areas where hydrates are found.

The researchers reported that the dissociation of methane hydrates can be triggered by the ground deformation caused by “earthquakes, storms, sea-level fluctuations or man-made disturbances (including well drilling and gas production from hydrate reservoirs).”

“This has an impact on these big issues,” Zhang said. “Here we have taken one step forward, but of course there is a lot more work to be done.”

Zhang said the researchers plan to continue their collaboration and are currently at work on a centre of excellence application to the Research Council of Norway.

Reference: Jianyang Wu, Fulong Ning, Thuat T. Trinh, Signe Kjelstrup, Thijs J.H. Vlugt, Jianying He, Bjørn H. Skallerud and Zhiliang Zhang. Mechanical instability of monocrystalline and polycrystalline methane hydrates. Nature Communications. DOI:10.1038/NCOMMS9743