Ice XII

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The crystal structure of ice XII Icexii-ru.jpg
The crystal structure of ice XII

Ice XII is a metastable, dense, crystalline phase of solid water, a type of ice. Ice XII was first reported in 1996 by C. Lobban, J.L. Finney and W.F. Kuhs and, after initial caution, was properly identified in 1998.

Contents

It was first obtained by cooling liquid water to 260  K (−13 °C; 8 °F) at a pressure of 0.55 gigapascals (5,400 atm). Ice XII was discovered existing within the phase stability region of ice V. Later research showed that ice XII could be created outside that range. Pure ice XII can be created from ice Ih at 77 K (−196.2 °C; −321.1 °F) by rapid compression (0.81-1.00 GPa/min) or by warming high density amorphous ice at pressures between 0.8 to 1.6 gigapascals (7,900 to 15,800 atm).

While it is similar in density (1.29 g/cm3 at 127 K (−146 °C; −231 °F)) to ice IV (also found in the ice V space) it exists as a tetragonal crystal. Topologically it is a mix of seven- and eight-membered rings, a 4-connected net (4-coordinate sphere packing)—the densest possible arrangement without hydrogen bond interpenetration.

Ordinary water ice is known as ice Ih, (in the Bridgman nomenclature). Different types of ice, from ice II to ice XVI, have been created in the laboratory at different temperatures and pressures.

Ice XIV

When hydrochloric-acid-doped ice XII is cooled down to about 110 K, it undergoes a phase transition into a partially hydrogen-ordered phase, namely ice XIV. [1] The transition entropy from ice XIV to ice XII is estimated to be 60% of Pauling entropy based on DSC measurements. [2] The formation of ice XIV from ice XII is more favoured at high pressure. [3]

See also

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<span class="mw-page-title-main">Ice XI</span> Alternative state of water ice

Ice XI is the hydrogen-ordered form of Ih, the ordinary form of ice. Different phases of ice, from ice II to ice XIX, have been created in the laboratory at different temperatures and pressures. The total internal energy of ice XI is about one sixth lower than ice Ih, so in principle it should naturally form when ice Ih is cooled to below 72 K. The low temperature required to achieve this transition is correlated with the relatively low energy difference between the two structures. Water molecules in ice Ih are surrounded by four semi-randomly directed hydrogen bonds. Such arrangements should change to the more ordered arrangement of hydrogen bonds found in ice XI at low temperatures, so long as localized proton hopping is sufficiently enabled; a process that becomes easier with increasing pressure. Correspondingly, ice XI is believed to have a triple point with hexagonal ice and gaseous water at.

<span class="mw-page-title-main">Ice VII</span> Alternative state of water ice

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Ice II is a rhombohedral crystalline form of ice with a highly ordered structure. It is formed from ice Ih by compressing it at a temperature of 198 K at 300 MPa or by decompressing ice V. When heated it undergoes transformation to ice III. Ordinary water ice is known as ice Ih,. Different types of ice, from ice II to ice XIX, have been created in the laboratory at different temperatures and pressures. It is thought that the cores of icy moons like Jupiter's Ganymede may be made of ice II.

<span class="mw-page-title-main">Ice VI</span> Alternative state of water ice

Ice VI is a form of ice that exists at high pressure at the order of about 1 GPa and temperatures ranging from 130 up to 355 Kelvin ; see also the phase diagram of water. Its discovery and the discovery of other high-pressure forms of water were published by P.W. Bridgman in January 1912.

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<span class="mw-page-title-main">Ice XVI</span> Alternative state of water ice

Ice XVI is the least dense experimentally obtained crystalline form of ice. It is topologically equivalent to the empty structure of sII clathrate hydrates. It was first obtained in 2014 by removing gas molecules from a neon clathrate under vacuum at temperatures below 147 K. The resulting empty water frame, ice XVI, is thermodynamically unstable at the experimental conditions, yet it can be preserved at cryogenic temperatures. Above 145–147 K at positive pressures ice XVI transforms into the stacking-faulty ice Ic and further into ordinary ice Ih. Theoretical studies predict ice XVI to be thermodynamically stable at negative pressures.

Ice XIX is a proposed crystalline phase of water. Along with ice XV, it is one of two phases of ice directly related to ice VI. Ice XIX is prepared by cooling HCl-doped ice VI at a pressure above 1.6 GPa down to about 100 K. As of 2022, its crystal structure has not been elucidated.

Ice IV is a metastable high-pressure phase of ice. It is formed when liquid water is compressed with an immense force.

<span class="mw-page-title-main">Ice XVII</span> Alternative state of water ice

Ice XVII is a metastable form of ice with a hexagonal structure and helical channels that was discovered in 2016. It can be formed by freezing water with hydrogen molecules at high pressure to form a filled ice, and then removing the hydrogen molecules from the structure. The form has potential for being used in hydrogen storage. Ice XVII made from heavy water can also be reduced to pure cubic ice.

<span class="mw-page-title-main">Thomas Loerting</span> Austrian chemist

Thomas Loerting is an Austrian chemist and associate professor at the University of Innsbruck. His research focuses on amorphous systems, the physics and chemistry of ice and chemistry at low temperatures.

References

  1. Salzmann CG, Radaelli PG, Hallbrucker A, Mayer E, Finney JL (2006). "The preparation and structures of hydrogen ordered phases of ice". Science. 311 (5768): 1758–61. Bibcode:2006Sci...311.1758S. doi:10.1126/science.1123896. PMID   16556840. S2CID   44522271.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  2. Köster KW, Fuentes-Landete V, Raidt A, Seidl M, Gainaru C, Loerting T; et al. (2018). "Author Correction: Dynamics enhanced by HCl doping triggers 60% Pauling entropy release at the ice XII-XIV transition". Nat Commun. 9: 16189. Bibcode:2018NatCo...916189K. doi:10.1038/ncomms16189. PMC   6026910 . PMID   29923547.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  3. Fuentes-Landete V; Köster KW; Böhmer R; Loerting T (2018). "Thermodynamic and kinetic isotope effects on the order-disorder transition of ice XIV to ice XII". Phys Chem Chem Phys. 20 (33): 21607–21616. Bibcode:2018PCCP...2021607F. doi: 10.1039/c8cp03786h . PMID   30101255. S2CID   51969440.