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Clathrate hydrate

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254:. These natural gas hydrates are seen as a potentially vast energy resource and several countries have dedicated national programs to develop this energy resource. Clathrate hydrate has also been of great interest as technology enabler for many applications like seawater desalination, gas storage, carbon dioxide capture & storage, cooling medium for data centre and district cooling etc. Hydrocarbon clathrates cause problems for the petroleum industry, because they can form inside 946:, and it is mechanically more stable and has a larger lattice constant at low temperatures than the Ne-filled analogue. The existence of such a porous ice had been theoretically predicted before. From a theoretical perspective, empty hydrates can be probed using Molecular Dynamics or Monte Carlo techniques. Conde et al. used empty hydrates and a fully atomic description of the solid lattice to estimate the phase diagram of H 31: 3524: 3546: 291: 932:
renders theoretical and computer simulation methods the ideal choice to address their thermodynamic properties. Starting from very cold samples (110–145 K), Falenty et al. degassed Ne–sII clathrates for several hours using vacuum pumping to obtain a so-called ice XVI, while employing neutron diffraction to observe that (i) the empty sII hydrate structure decomposes at
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Kimble, R. A.; Lesser, M. P.; Martel, A. R.; Menanteau, F.; Meurer, G. R.; Miley, G. K.; Postman, M.; Rosati, P.; Sirianni, M.; Sparks, W. B.; Tran, H. D.; Tsvetanov, Z. I.; White, R. L.; Zheng, W. (2003). "Hubble Space Telescope ACS Coronagraphic Imaging of the Circumstellar Disk around HD 141569A".
919:, because they require much smaller concentrations than the conventional thermodynamic inhibitors. Kinetic inhibitors, which do not require water and hydrocarbon mixture to be effective, are usually polymers or copolymers and anti-agglomerants (requires water and hydrocarbon mixture) are polymers or 1944:
Clampin, M.; Krist, J. E.; Ardila, D. R.; Golimowski, D. A.; Hartig, G. F.; Ford, H. C.; Illingworth, G. D.; Bartko, F.; Bentez, N.; Blakeslee, J. P.; Bouwens, R. J.; Broadhurst, T. J.; Brown, R. A.; Burrows, C. J.; Cheng, E. S.; Cross, N. J. G.; Feldman, P. D.; Franx, M.; Gronwall, C.; Infante, L.;
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surface obtained was fitted by the universal form of the Parsafar and Mason equation of state with an accuracy of 99.7–99.9%. Framework deformation caused by applied temperature followed a parabolic law, and there is a critical temperature above which the isobaric thermal expansion becomes negative,
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Empty clathrate hydrates are thermodynamically unstable (guest molecules are of paramount importance to stabilize these structures) with respect to ice, and as such their study using experimental techniques is greatly limited to very specific formation conditions; however, their mechanical stability
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and anti-agglomerants in actual field operations is a new and evolving technology. It requires extensive tests and optimisation to the actual system. While kinetic inhibitors work by slowing down the kinetics of the nucleation, anti-agglomerants do not stop the nucleation, but stop the agglomeration
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The unit cell of Type H consists of 34 water molecules, forming three types of cages – two small ones of different types, and one "huge". In this case, the unit cell consists of three small cages of type 5, two small ones of type 456 and one huge of type 56. The formation of Type H requires the
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The unit cell of Type II consists of 136 water molecules, again forming two types of cages – small and large. In this case there are sixteen small cages and eight large ones in the unit cell. The small cage again has the shape of a pentagonal dodecahedron (5), but the large one is a
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are common structures in permafrost regions. Similar structures are found in deep water related to methane vents. Significantly, gas hydrates can even be formed in the absence of a liquid phase. Under that situation, water is dissolved in gas or in liquid hydrocarbon phase.
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When operating within a set of parameters where hydrates could be formed, there are still ways to avoid their formation. Altering the gas composition by adding chemicals can lower the hydrate formation temperature and/or delay their formation. Two options generally exist:
976:, respectively. Matsui et al. employed molecular dynamics to perform a thorough and systematic study of several ice polymorphs, namely space fullerene ices, zeolitic ices, and aeroices, and interpreted their relative stability in terms of geometrical considerations. 571:. The one at 43 μm is much weaker than the one at 60 μm, which means the water ice, is located in the outer parts of the disk at temperatures below 50 K. There is also another broad ice feature between 87 and 90 μm, which is very similar to the one in 903:. All may be recovered and recirculated, but the economics of methanol recovery is not favourable in most cases. MEG is preferred over DEG for applications where the temperature is expected to be −10 °C or lower due to high viscosity at low temperatures. 728:
deposits may be significant (10 to 10 cubic metres), which makes them of major interest as a potential energy resource. Catastrophic release of methane from the decomposition of such deposits may lead to a global climate change, referred to as the
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capture and sequestration. A nonstoichiometric compound, carbon dioxide hydrate, is composed of hydrogen-bonded water molecules arranged in ice-like frameworks that are occupied by molecules with appropriate sizes and regions. In structure I, the
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Hassanpouryouzband, Aliakbar; Joonaki, Edris; Vasheghani Farahani, Mehrdad; Takeya, Satoshi; Ruppel, Carolyn; Yang, Jinhai; J. English, Niall; M. Schicks, Judith; Edlmann, Katriona; Mehrabian, Hadi; M. Aman, Zachary; Tohidi, Bahman (2020).
489:), given the presence of other smaller help gases to fill and support the remaining cavities. Structure H hydrates were suggested to exist in the Gulf of Mexico. Thermogenically produced supplies of heavy hydrocarbons are common there. 835:
and to adhere to the pipe wall and thereby plug the pipeline. Once formed, they can be decomposed by increasing the temperature and/or decreasing the pressure. Even under these conditions, the clathrate dissociation is a slow process.
957:, and obtain the differences in chemical potentials between ice Ih and the empty hydrates, central to the van der Waals−Platteeuw theory. Jacobson et al. performed simulations using a monoatomic (coarse-grained) model developed for H 961:
O that is capable of capturing the tetrahedral symmetry of hydrates. Their calculations revealed that, under 1 atm pressure, sI and sII empty hydrates are metastable regarding the ice phases up to their melting temperatures,
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at suitable temperatures and pressures. Clathrate hydrates are not officially chemical compounds, as the enclathrated guest molecules are never bonded to the lattice. The formation and decomposition of clathrate hydrates are
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Choudhary, Nilesh; Chakrabarty, Suman; Roy, Sudip; Kumar, Rajnish (January 2019). "A comparison of different water models for melting point calculation of methane hydrate using molecular dynamics simulations".
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Ussler, W.; Paull, C. K.; Lorenson, T.; Dallimore, S.; Medioli, B.; Blasco, S.; McLaughlin, F.; Nixon, F. M. (2005). "Methane Leakage from Pingo-like Features on the Arctic Shelf, Beaufort Sea, NWT, Canada".
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The unit cell of Type I consists of 46 water molecules, forming two types of cages – small and large. The unit cell contains two small cages and six large ones. The small cage has the shape of a pentagonal
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molecules occupying both large cavities (tetrakaidecahedral) and small cavities (pentagonal dodecahedral). Researchers believed that oceans and permafrost have immense potential to capture anthropogenic
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Prevent formation of hydrates by addition of chemicals that (a) shift the hydrate equilibrium conditions towards lower temperatures and higher pressures or (b) increase hydrate formation time (
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Therefore, preventing hydrate formation appears to be the key to the problem. A hydrate prevention philosophy could typically be based on three levels of security, listed in order of priority:
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Malfait, K.; Waelkens, C.; Waters, L.B.F.M.; Vandenbussche, B.; Huygen, E.; de Graauw, M.S. (1998). "The spectrum of the young star HD 100546 observed with the Infrared Space Observatory".
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suggest massive dust disks consisting of millimetre-sized grains, which disappear after several million years (e.g.,). A lot of work on detecting water ices in the Universe was done on the
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Babu, Ponnivalavan; Linga, Praveen; Kumar, Rajnish; Englezos, Peter (1 June 2015). "A review of the hydrate based gas separation (HBGS) process for carbon dioxide pre-combustion capture".
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Kamata, Shunichi; Nimmo, Francis; Sekine, Yasuhito; Kuramoto, Kiyoshi; Noguchi, Naoki; Kimura, Jun; Tani, Atsushi (June 2019). "Pluto's ocean is capped and insulated by gas hydrates".
203:, not chemical reactions. Their detailed formation and decomposition mechanisms on a molecular level are still not well understood. Clathrate hydrates were first documented in 1810 by 1024:) > (200 MPa, 200 K). The length of the hydrogen bonds responsible for framework integrity was insensitive to the thermodynamic conditions and its average value is 1445:
Chong, Zheng Rong; Yang, She Hern Bryan; Babu, Ponnivalavan; Linga, Praveen; Li, Xiao-Sen (2016). "Review of natural gas hydrates as an energy resource: Prospects and challenges".
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stars were fulfilled, despite the rapid grain growth to metre-scale. The key was to provide enough microscopic ice particles exposed to a gaseous environment. Observations of the
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Kieffer, Susan W.; Xinli Lu; Craig M. Bethke; John R. Spencer; Stephen Marshak; Alexandra Navrotsky (2006). "A Clathrate Reservoir Hypothesis for Enceladus' South Polar Plume".
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Iess, L.; Stevenson, D. J.; Parisi, M.; Hemingway, D.; Jacobson, R. A.; Lunine, Jonathan I.; Nimmo, F.; Armstrong, J. W.; Asmar, S. W.; Ducci, M.; Tortora, P. (April 4, 2014).
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Cruz, Fernando J. A. L.; Alavi, Saman; Mota, José P. B. (2019). "Low-Temperature Thermodynamic Study of the Metastable Empty Clathrate Hydrates Using Molecular Simulations".
1016:) field was analyzed in terms of angle and distance descriptors of a classical tetrahedral structure and observed to occur essentially by means of angular alteration for ( 654:" fractures found in that area. However, subsequent analysis of plume material makes it more likely that the geysers on Enceladus derive from a salty subsurface ocean. 417: 546: 1539: 1557:
Ghosh, Jyotirmoy; Methikkalam, Rabin Rajan J.; Bhuin, Radha Gobinda; Ragupathy, Gopi; Choudhary, Nilesh; Kumar, Rajnish; Pradeep, Thalappil (29 January 2019).
907:(TEG) has too low vapour pressure to be suited as an inhibitor injected into a gas stream. More methanol is lost in the gas phase when compared to MEG or DEG. 1086:
hydrate equilibrium curve in phase diagram towards higher temperature and lower pressures is still under scrutiny to make extensive large-scale storage of CO
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Cruz F.J.A.L.; Alavi S.; Mota J.P.B. (2019). "Low-Temperature Thermodynamic Study of the Metastable Empty Clathrate Hydrates Using Molecular Simulations".
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Youssef, Z.; Barreau, A.; Mougin, P.; Jose, J.; Mokbel, I. (15 April 2009). "Measurements of Hydrate Dissociation Temperature of Methane, Ethane, and CO
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cooperation of two guest gases (large and small) to be stable. It is the large cavity that allows structure H hydrates to fit in large molecules (e.g.
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The actual philosophy would depend on operational circumstances such as pressure, temperature, type of flow (gas, liquid, presences of water etc.).
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The 2020 Research Fronts report identified gas hydrate accumulation and mining technology as one of the top 10 research fronts in the geosciences.
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structure of hydrate clathrates would collapse into conventional ice crystal structure or liquid water. Most low molecular weight gases, including
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Zheng J.; Chong Z.R.; Qureshi M.F.; Linga P. (2020). "Carbon Dioxide Sequestration via Gas Hydrates: A Potential Pathway toward Decarbonization".
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originates from clathrate hydrates, where carbon dioxide, methane, and nitrogen are released when exposed to the vacuum of space through the "
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Kvenvolden, Keith A.; McMenamin, Mark A. (1980). "Hydrates of natural gas; a review of their geologic occurrence". Circular (Report).
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Natta, A.; Grinin, V.; Mannings, V. (2000). "Properties and Evolution of Disks around Pre-Main-Sequence Stars of Intermediate Mass".
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Falenty A.; Hansen T.C.; Kuhs F. (2014). "Formation and Properties of Ice XVI Obtained by Emptying a Type sII Clathrate Hydrate".
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Malfait, K.; Waelkens, C.; Bouwman, J.; De Koter, A.; Waters, L. B. F. M. (1999). "The ISO spectrum of the young star HD 142527".
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Beckwith, S. V. W.; Henning, T.; Nakagawa, Y. (2000). "Dust properties and assembly of large particles in protoplanetary disks".
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The thermodynamics of metastable empty sI clathrate hydrates have been probed over broad temperature and pressure ranges,
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Avoid operational conditions that might cause formation of hydrates by depressing the hydrate formation temperature using
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Conde M.M.; Vega C.; Tribello G.A.; Slater B. (2009). "The Phase Diagram of Water at Negative Pressures: Virtual Ices".
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of methane hydrates from under the seafloor were successful. However, commercial-scale production remains years away.
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HD 141569A, are dusty. Li & Lunine found water ice there. Knowing the ices usually exist at the outer parts of the
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Gao, Shuqiang (2008). "Investigation of Interactions between Gas Hydrates and Several Other Flow Assurance Elements".
231: 2725:"CO2 Hydrate: Synthesis, Composition, Structure, Dissociation Behavior, and a Comparison to Structure I CH4 Hydrate" 3575: 1410:
Buffett, B.; Archer, D. (2004). "Global inventory of methane clathrate: sensitivity to changes in the deep ocean".
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have proposed that a thin layer of clathrate hydrates thermally insulates the subsurface ocean of liquid water of
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Circone S.; Stern L.A.; Kirby S.H.; Durham W.B.; Chacoumakos B.C.; Rawn C.J.; Rondinone A.J.; Ishii Y. (2003).
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Li, Aigen; Lunine, Jonathan I.; Bendo, G. J. (2003). "Modeling the infrared emission from the ε-Eridani disk".
1109: 730: 657: 447: 259: 3083: 995:, by Cruz et al. using large-scale simulations and compared with experimental data at 100 kPa. The whole 823:
failure and damage valves and instrumentation. The results can range from flow reduction to equipment damage.
1217: 243: 2600:"Thermodynamic Stability and Growth of Guest-Free Clathrate Hydrates: A Low-Density Crystal Phase of Water" 819:. This is highly undesirable, because the clathrate crystals might agglomerate and plug the line and cause 3137: 1701: 1655:
Sloan, E. Dendy & Koh, Carolyn A. (2008) . "Chapter 2. Molecular Structures and Similarities to Ice".
1229: 851: 672: 588: 279: 1480: 923: – usually ammonium and COOH – surfactants being both attracted to hydrates and hydrocarbons. 584: 349: 313: 100:
and the guest molecule is typically a gas or liquid. Without the support of the trapped molecules, the
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Gao, Shuqiang; House, Waylon; Chapman, Walter (2005). "NMR/MRI Study of Clathrate Hydrate Mechanisms".
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in the Absence of Any Aqueous Phase and Prediction with the Cubic Plus Association Equation of State".
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Barlow, M.J., In the proceedings of 'ISO's view on stellar evolution', Noordwijkerhout, July 1–4, 1997
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ranging from 194.7 K at 100 kPa to 166.2 K at 500 MPa. Response to the applied (
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who found that water was a primary component of what was earlier thought to be solidified chlorine.
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Li, Aigen; Lunine, Jonathan I. (2003). "Modeling the infrared emission from the HD 141569A disk".
787: 3527: 2818: 2771: 2705: 2537: 2502: 2451: 2232: 2179: 2119: 2033: 2007: 1980: 1954: 1872: 1846: 1738: 1684:; Lunine, Jonathan I. (February 2003). "An interpretation of the nitrogen deficiency in comets". 1637: 1344: 1255: 1198: 904: 858: 844: 816: 661: 596: 564: 552: 521: 255: 93: 81: 1917:
Jaschek, C.; Jaschek, M. (1992). "A southern be star survey : Spectra and envelope radii".
1617: 2924: 2810: 2662: 2621: 2580: 2494: 2171: 2146: 2111: 1660: 1598: 1247: 1190: 915:(sticking together) of gas hydrate crystals. These two kinds of inhibitors are also known as 911: 896: 881: 725: 699: 458: 275: 223: 101: 77: 66: 3303: 2854: 2802: 2763: 2736: 2697: 2652: 2611: 2572: 2529: 2486: 2443: 2408: 2331: 2251: 2222: 2214: 2163: 2103: 2068: 2064: 2025: 1972: 1930: 1903: 1864: 1814: 1783: 1711: 1629: 1588: 1578: 1521: 1462: 1427: 1423: 1336: 1293: 1239: 1180: 1170: 1138: 772: 647: 385: 204: 200: 150: 89: 3538: 2831: 531: 2953: 2899: 2138: 892: 580: 428: 299: 251: 247: 2850: 2693: 2568: 2482: 2439: 2304: 2210: 2159: 2099: 2021: 1968: 1860: 1779: 1752: 1697: 1574: 1458: 1363: 1332: 210:
Clathrates have been found to occur naturally in large quantities. Around 6.4 trillion (
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Hersant, F (2004). "Enrichment in volatiles in the giant planets of the Solar System".
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Zeitschrift für Elektrochemie, Berichte der Bunsengesellschaft für physikalische Chemie
1593: 1558: 1388: 820: 780: 741: 560: 466: 440: 267: 263: 235: 132: 30: 2701: 2447: 1715: 587:. 90% of the ice in the latter was found crystalline at temperature around 50 K. 3564: 3323: 3275: 3260: 3128: 2981: 2976: 2971: 2775: 2709: 2455: 2349: 2236: 1348: 1202: 514: 85: 2822: 2767: 2541: 2183: 2123: 2037: 1876: 1641: 1259: 3580: 3333: 3245: 3240: 3235: 3133: 3103: 2917: 2506: 1540:"NUS, Keppel, SLNG in tie-up to develop better cooling technology for data centres" 1466: 1340: 681: 628: 616: 548: 424: 1984: 34:
Methane clathrate block embedded in the sediment of hydrate ridge, off Oregon, USA
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hydrates are more commonly used these days with its relevance in anthropogenic CO
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and, furthermore, (ii) the empty hydrate shows a negative thermal expansion at
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of water ice at 43 and 60 μm were found in the disk of the isolated
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Crystalline solid containing molecules caged in a lattice of frozen water
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Thermodynamic conditions favouring hydrate formation are often found in
3485: 3383: 3353: 3298: 3288: 3113: 3047: 3042: 3027: 3022: 3002: 2904:– Background knowledge about gas hydrates, their prevention and removal 1175: 1158: 764: 734: 721: 579:). Crystalline ices were also detected in the proto-planetary disks of 451: 219: 195: 167: 141: 54: 2806: 2740: 2657: 2640: 2616: 2599: 2576: 2520:
Kosyakov V.I. (2009). "Structure Formation Under Negative Pressures".
2412: 2335: 2227: 1787: 1297: 1243: 1185: 427:(5) (which is not a regular dodecahedron) and the large one that of a 270:. Clathrates are suspected to occur in large quantities on some outer 3414: 3037: 900: 800:
In 2017, both Japan and China announced that attempts at large-scale
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Matsui T.; Hirata M.; Yagasaki T.; Matsumoto M.; Tanaka H. (2017).
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hydrate crystallizes as one of two cubic hydrates composed of 46 H
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is believed to play a major role in different processes on Mars.
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had been trapped in the form of hydrates and incorporated in the
3203: 3148: 3108: 1620:[Solid gas hydrates II. Structure and space chemistry]. 1389:"Clathrates: little known components of the global carbon cycle" 1104: 916: 2913: 2940: 2832:"Effect of gas hydrates melting on seafloor slope instability" 73: 62: 1481:"Drinkable water from cold energy | Engineers Australia" 509:, stated most of the conditions for hydrate formation in the 751:). The fast decomposition of such deposits is considered a 2830:
Sultan, N; Cochonat, P; Foucher, J.-P; Mienert, J (2004).
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is likely to form in condensation nebulae for gas giants.
258:, often resulting in obstructions. Deep sea deposition of 382:
respectively. A third hexagonal structure of space group
2139:"The Gravity Field and Interior Structure of Enceladus" 827:
Hydrate formation, prevention and mitigation philosophy
679:, the existence of which is suggested by data from the 2909: 1495:"Eco-friendly ways to harness natural gas efficiently" 1082:
hydrates. The utilization of additives to shift the CO
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The SUGAR Project (Submarine Gas Hydrate Reservoirs)
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Cages building the different gas hydrate structures
595:, as the one around the 5-million-year-old B9.5Ve 540: 411: 374: 338: 469:(56). Type II hydrates are formed by gases like O 1680:Iro, Nicolas; Gautier, Daniel; Hersant, Franck; 1559:"Clathrate hydrates in interstellar environment" 2324:Industrial & Engineering Chemistry Research 1563:Proceedings of the National Academy of Sciences 1131:Industrial & Engineering Chemistry Research 2641:"Hypothetical Ultralow-density Ice Polymorphs" 2350:"China claims breakthrough in 'flammable ice'" 1618:"Feste Gashydrate II. Struktur und Raumchemie" 1368:. Quarterly Journal of Science. pp. 81–84 1129:Englezos, Peter (1993). "Clathrate hydrates". 790:are frequently observed in polar ice samples. 2925: 2273:"Ice that burns could be a green fossil fuel" 887:The most common thermodynamic inhibitors are 439:. Typical guests forming Type I hydrates are 262:has been proposed as a method to remove this 8: 2598:Jacobson L.C.; Hujo W.; Molinero V. (2009). 1919:Astronomy and Astrophysics Supplement Series 435:(56). Together, they form a version of the 302:cubic structures: structure (Type) I (named 583:and the isolated Fe star HD 142527 in 282:, binding gas at fairly high temperatures. 3223: 2932: 2918: 2910: 2656: 2615: 2255: 2226: 2011: 1958: 1850: 1742: 1705: 1616:Stackelberg, M. v; Müller, H. R. (1954). 1592: 1582: 1233: 1218:"NMR MRI Study of Gas Hydrate Mechanisms" 1184: 1174: 533: 395: 387: 359: 351: 323: 315: 92:. In other words, clathrate hydrates are 882:Kinetic inhibitors and anti-agglomerants 182: 153: 144: 135: 127: 118: 109: 2906:(by manufacturer of hydrate autoclaves) 1159:"Gas hydrates in sustainable chemistry" 1121: 234:in the northern headwall flank of the 740:is a more potent greenhouse gas than 7: 3534: 2887:Leibniz Institute of Marine Sciences 2877:Leibniz Institute of Marine Sciences 854:in order to avoid hydrate formation; 230:. Such deposits can be found on the 2729:The Journal of Physical Chemistry B 2271:Marshall, Michael (26 March 2009). 1657:Clathrate hydrates of natural gases 1280:Gao S; Chapman WG; House W (2005). 1222:The Journal of Physical Chemistry B 1216:Gao S; House W; Chapman WG (2005). 1090:viable in shallower subsea depths. 1040:Clathrate hydrate, which encaged CO 831:Hydrates have a strong tendency to 755:, due to its potential to trigger 607:proposed an interpretation of the 375:{\displaystyle Fd{\overline {3}}m} 339:{\displaystyle Pm{\overline {3}}n} 25: 2702:10.1021/acsearthspacechem.9b00009 2448:10.1021/acsearthspacechem.9b00009 1044:as guest molecule is termed as CO 708:gas hydrates can be found on the 611:enrichment, observed in the four 591:demonstrated that relatively old 433:hexagonal truncated trapezohedron 306:) and structure (Type) II (named 80:molecules with large hydrophobic 3544: 3533: 3523: 3522: 575:(the Bug or Butterfly nebula in 266:from the atmosphere and control 2768:10.1021/acs.energyfuels.0c02309 899:(DEG), commonly referred to as 724:potentially trapped in natural 419:may also be observed (Type H). 238:. Clathrates can also exist as 1467:10.1016/j.apenergy.2014.12.061 1387:Ellen Thomas (November 2004). 1341:10.1016/j.chemphys.2018.08.036 298:Gas hydrates usually form two 96:in which the host molecule is 84:are trapped inside "cages" of 1: 2682:ACS Earth and Space Chemistry 2428:ACS Earth and Space Chemistry 1716:10.1016/S0019-1035(02)00038-6 917:low dosage hydrate inhibitors 201:first order phase transitions 2859:10.1016/j.margeo.2004.10.015 1526:10.1016/j.energy.2015.03.103 1105:Star formation and evolution 950:O at negative pressures and 619:, with respect to the Solar 364: 328: 2053:Planetary and Space Science 559:(ISO). For instance, broad 232:Norwegian continental shelf 3612: 2293:AGU Fall Meeting Abstracts 1892:Astronomy and Astrophysics 1803:Astronomy and Astrophysics 1682:Bockelée-Morvan, Dominique 1432:10.1016/j.epsl.2004.09.005 697: 557:Infrared Space Observatory 515:pre-main and main sequence 501:, trying to interpret the 222:is trapped in deposits of 3517: 3329:Short-track speed skating 3226: 2947: 2534:10.1007/s10947-009-0190-0 2219:10.1038/s41561-019-0369-8 2073:10.1016/j.pss.2003.12.011 1839:The Astrophysical Journal 1659:. CRC Press. p. 45. 811:Gas hydrates in pipelines 1947:The Astronomical Journal 1634:10.1002/bbpc.19540580105 1362:Michael Faraday (1859). 1163:Chemical Society Reviews 1110:Clathrate gun hypothesis 927:Empty clathrate hydrates 878:Thermodynamic inhibitors 731:clathrate gun hypothesis 658:Carbon dioxide clathrate 493:Hydrates in the universe 448:carbon dioxide clathrate 260:carbon dioxide clathrate 2168:10.1126/science.1250551 2108:10.1126/science.1133519 2065:2004P&SS...52..623H 1931:1992A&AS...95..535J 1904:1999A&A...345..181M 1815:1998A&A...332L..25M 1584:10.1073/pnas.1814293116 1424:2004E&PSL.227..185B 1412:Earth Planet. Sci. Lett 720:regions. The amount of 601:proto-planetary nebulae 437:Weaire–Phelan structure 280:trans-Neptunian objects 244:Mallik gas hydrate site 186:as well as some higher 1768:Protostars and Planets 1731:Protostars and Planets 1365:On Hydrate of Chlorine 1026:r(̅O H) = 0.25 nm 673:University of Hokkaido 542: 511:protoplanetary nebulae 413: 412:{\displaystyle P6/mmm} 376: 340: 295: 61:physically resembling 35: 2893:Gas hydrates in video 2000:Astrophysical Journal 1391:. Wesleyan University 716:), as well as in the 543: 541:{\displaystyle \tau } 414: 377: 341: 293: 33: 1048:hydrate. The term CO 852:operating conditions 694:Natural gas hydrates 532: 386: 350: 314: 3425:Iceman (occupation) 2889:, Kiel (IFM-GEOMAR) 2879:, Kiel (IFM-GEOMAR) 2851:2004MGeol.213..379S 2801:(41): 19090–19093. 2694:2019ESC.....3..789C 2610:(30): 10298–10307. 2569:2009JChPh.131c4510C 2491:10.1038/nature14014 2483:2014Natur.516..231F 2440:2019ESC.....3..789C 2305:2005AGUFM.C11A1069U 2211:2019NatGe..12..407K 2160:2014Sci...344...78I 2100:2006Sci...314.1764K 2094:(5806): 1764–1766. 2022:2003ApJ...594..987L 1969:2003AJ....126..385C 1861:2003ApJ...598L..51L 1780:2000prpl.conf..559N 1753:2000prpl.conf..533B 1698:2003Icar..161..511I 1575:2019PNAS..116.1526G 1459:2016ApEn..162.1633C 1333:2019CP....516....6C 1286:Ind. Eng. Chem. Res 1228:(41): 19090–19093. 1143:10.1021/ie00019a001 893:monoethylene glycol 850:Temporarily change 802:resource extraction 749:Atmospheric methane 623:. They assumed the 593:circumstellar disks 526:circumstellar discs 94:clathrate compounds 3571:Clathrate hydrates 2977:Crystalline phases 2898:2016-03-21 at the 2762:(9): 10529–10546. 2401:Energy & Fuels 1546:. 22 October 2019. 1176:10.1039/C8CS00989A 912:kinetic inhibitors 905:Triethylene glycol 869:Hydrate inhibitors 845:glycol dehydration 771:gases, as well as 662:Hydrogen clathrate 553:Herbig Ae/Be stars 538: 513:, surrounding the 409: 372: 336: 310:) of space groups 296: 39:Clathrate hydrates 36: 3576:Phase transitions 3558: 3557: 3539:Wikimedia Commons 3342: 3341: 2807:10.1021/jp052071w 2741:10.1021/jp027391j 2735:(23): 5529–5539. 2658:10.1063/1.4994757 2617:10.1021/jp903439a 2577:10.1063/1.3182727 2477:(7530): 231–234. 2413:10.1021/ef800189k 2336:10.1021/ie801351e 2199:Nature Geoscience 1666:978-0-8493-9078-4 1544:The Straits Times 1499:The Straits Times 1298:10.1021/ie050464b 1292:(19): 7373–7379. 1244:10.1021/jp052071w 1169:(15): 5225–5309. 1065:O molecules (or D 897:diethylene glycol 700:Methane clathrate 689:Hydrates on Earth 635:' feeding zones. 597:Herbig Ae/Be star 565:Herbig Ae/Be star 459:methane clathrate 431:, specifically a 367: 331: 224:methane clathrate 65:, in which small 16:(Redirected from 3603: 3591:Industrial gases 3548: 3537: 3536: 3526: 3525: 3224: 2934: 2927: 2920: 2911: 2862: 2845:(1–4): 379–401. 2836: 2826: 2795:J. Phys. Chem. B 2780: 2779: 2751: 2745: 2744: 2720: 2714: 2713: 2677: 2671: 2670: 2660: 2636: 2630: 2629: 2619: 2604:J. Phys. Chem. B 2595: 2589: 2588: 2552: 2546: 2545: 2517: 2511: 2510: 2466: 2460: 2459: 2423: 2417: 2416: 2407:(5): 3150–3153. 2396: 2390: 2389: 2386:"Web of Science" 2382: 2376: 2375: 2364: 2358: 2357: 2346: 2340: 2339: 2330:(8): 4045–4050. 2315: 2309: 2308: 2287: 2281: 2280: 2268: 2262: 2261: 2259: 2247: 2241: 2240: 2230: 2194: 2188: 2187: 2143: 2134: 2128: 2127: 2083: 2077: 2076: 2048: 2042: 2041: 2015: 2013:astro-ph/0311070 1995: 1989: 1988: 1962: 1960:astro-ph/0303605 1941: 1935: 1934: 1914: 1908: 1907: 1887: 1881: 1880: 1854: 1852:astro-ph/0311069 1834: 1828: 1825: 1819: 1818: 1798: 1792: 1791: 1763: 1757: 1756: 1746: 1744:astro-ph/9902241 1726: 1720: 1719: 1709: 1677: 1671: 1670: 1652: 1646: 1645: 1613: 1607: 1606: 1596: 1586: 1569:(5): 1526–1531. 1554: 1548: 1547: 1536: 1530: 1529: 1509: 1503: 1502: 1491: 1485: 1484: 1477: 1471: 1470: 1442: 1436: 1435: 1418:(3–4): 185–199. 1407: 1401: 1400: 1398: 1396: 1384: 1378: 1377: 1375: 1373: 1359: 1353: 1352: 1321:Chemical Physics 1315: 1309: 1308: 1306: 1304: 1277: 1271: 1270: 1268: 1266: 1237: 1213: 1207: 1206: 1188: 1178: 1153: 1147: 1146: 1137:(7): 1251–1274. 1126: 1027: 994: 986: 975: 974:= 252 ± 2 K 968: 967:= 245 ± 2 K 956: 945: 938: 547: 545: 544: 539: 418: 416: 415: 410: 399: 381: 379: 378: 373: 368: 360: 345: 343: 342: 337: 332: 324: 300:crystallographic 250:of northwestern 217: 215: 205:Sir Humphry Davy 185: 176: 170: 164: 157: 147: 138: 130: 121: 112: 21: 3611: 3610: 3606: 3605: 3604: 3602: 3601: 3600: 3561: 3560: 3559: 3554: 3513: 3480: 3444: 3398: 3338: 3270: 3219: 3213: 3084:Albedo feedback 3072: 2986: 2972:Amorphous solid 2960: 2943: 2938: 2900:Wayback Machine 2869: 2834: 2829: 2792: 2789: 2787:Further reading 2784: 2783: 2753: 2752: 2748: 2722: 2721: 2717: 2679: 2678: 2674: 2638: 2637: 2633: 2597: 2596: 2592: 2554: 2553: 2549: 2522:J. Struct. Chem 2519: 2518: 2514: 2468: 2467: 2463: 2425: 2424: 2420: 2398: 2397: 2393: 2384: 2383: 2379: 2366: 2365: 2361: 2348: 2347: 2343: 2321: 2317: 2316: 2312: 2289: 2288: 2284: 2270: 2269: 2265: 2249: 2248: 2244: 2196: 2195: 2191: 2154:(6179): 78–80. 2141: 2136: 2135: 2131: 2085: 2084: 2080: 2050: 2049: 2045: 2006:(2): 987–1010. 1997: 1996: 1992: 1943: 1942: 1938: 1916: 1915: 1911: 1889: 1888: 1884: 1836: 1835: 1831: 1826: 1822: 1800: 1799: 1795: 1765: 1764: 1760: 1728: 1727: 1723: 1679: 1678: 1674: 1667: 1654: 1653: 1649: 1615: 1614: 1610: 1556: 1555: 1551: 1538: 1537: 1533: 1511: 1510: 1506: 1501:. 30 June 2017. 1493: 1492: 1488: 1479: 1478: 1474: 1444: 1443: 1439: 1409: 1408: 1404: 1394: 1392: 1386: 1385: 1381: 1371: 1369: 1361: 1360: 1356: 1317: 1316: 1312: 1302: 1300: 1279: 1278: 1274: 1264: 1262: 1235:10.1.1.175.9193 1215: 1214: 1210: 1155: 1154: 1150: 1128: 1127: 1123: 1118: 1096: 1089: 1085: 1081: 1077: 1072: 1069:O) and eight CO 1068: 1064: 1060: 1055: 1051: 1047: 1043: 1038: 1035: 1025: 989:100 kPa ≤ 988: 980: 970: 963: 960: 951: 949: 940: 933: 929: 871: 829: 813: 784: 776: 746: 739: 726:methane hydrate 702: 696: 691: 530: 529: 495: 476: 472: 455: 444: 429:tetradecahedron 384: 383: 348: 347: 312: 311: 288: 252:Canadian Arctic 248:Mackenzie Delta 213: 211: 184: 178: 172: 166: 160: 155: 151: 146: 142: 137: 133: 129: 123: 120: 114: 111: 105: 90:water molecules 86:hydrogen bonded 28: 23: 22: 15: 12: 11: 5: 3609: 3607: 3599: 3598: 3593: 3588: 3583: 3578: 3573: 3563: 3562: 3556: 3555: 3553: 3552: 3541: 3530: 3518: 3515: 3514: 3512: 3511: 3509:Snowball Earth 3506: 3501: 3499:Little Ice Age 3496: 3490: 3488: 3482: 3481: 3479: 3478: 3473: 3468: 3463: 3458: 3452: 3450: 3446: 3445: 3443: 3442: 3437: 3432: 3427: 3422: 3417: 3412: 3406: 3404: 3400: 3399: 3397: 3396: 3391: 3386: 3381: 3376: 3371: 3366: 3361: 3356: 3350: 3348: 3344: 3343: 3340: 3339: 3337: 3336: 3331: 3326: 3321: 3316: 3311: 3309:Figure skating 3306: 3301: 3296: 3291: 3286: 3280: 3278: 3272: 3271: 3269: 3268: 3263: 3258: 3253: 3248: 3243: 3238: 3233: 3227: 3221: 3215: 3214: 3212: 3211: 3206: 3201: 3196: 3191: 3186: 3181: 3176: 3171: 3166: 3161: 3156: 3151: 3146: 3141: 3131: 3126: 3121: 3116: 3111: 3106: 3101: 3096: 3094:Circle or disc 3091: 3086: 3080: 3078: 3074: 3073: 3071: 3070: 3065: 3060: 3055: 3050: 3045: 3040: 3035: 3025: 3020: 3015: 3010: 3005: 3000: 2994: 2992: 2988: 2987: 2985: 2984: 2979: 2974: 2968: 2966: 2962: 2961: 2948: 2945: 2944: 2939: 2937: 2936: 2929: 2922: 2914: 2908: 2907: 2890: 2880: 2868: 2867:External links 2865: 2864: 2863: 2839:Marine Geology 2827: 2788: 2785: 2782: 2781: 2746: 2715: 2688:(5): 789–799. 2672: 2631: 2590: 2547: 2512: 2461: 2434:(5): 789–799. 2418: 2391: 2377: 2374:. 19 May 2017. 2359: 2356:. 19 May 2017. 2341: 2319: 2310: 2282: 2263: 2257:10.3133/cir825 2242: 2205:(6): 407–410. 2189: 2129: 2078: 2059:(7): 623–641. 2043: 2030:10.1086/376939 1990: 1977:10.1086/375460 1953:(1): 385–392. 1936: 1909: 1882: 1869:10.1086/380495 1845:(1): L51–L54. 1829: 1820: 1793: 1758: 1721: 1707:10.1.1.487.722 1692:(2): 511–532. 1672: 1665: 1647: 1608: 1549: 1531: 1504: 1486: 1472: 1447:Applied Energy 1437: 1402: 1379: 1354: 1310: 1272: 1208: 1148: 1120: 1119: 1117: 1114: 1113: 1112: 1107: 1102: 1095: 1092: 1087: 1083: 1079: 1078:in the form CO 1075: 1070: 1066: 1062: 1058: 1053: 1049: 1045: 1041: 1037: 1033: 1030: 993:≤ 500 MPa 958: 947: 944:< 55 K 928: 925: 885: 884: 879: 870: 867: 863: 862: 855: 848: 828: 825: 821:flow assurance 812: 809: 782: 774: 744: 737: 698:Main article: 695: 692: 690: 687: 671:(2019) of the 631:flying in the 561:emission bands 537: 505:deficiency in 494: 491: 474: 470: 467:hexadecahedron 453: 442: 408: 405: 402: 398: 394: 391: 371: 366: 363: 358: 355: 335: 330: 327: 322: 319: 287: 284: 268:climate change 264:greenhouse gas 236:Storegga Slide 26: 24: 14: 13: 10: 9: 6: 4: 3: 2: 3608: 3597: 3594: 3592: 3589: 3587: 3584: 3582: 3579: 3577: 3574: 3572: 3569: 3568: 3566: 3551: 3547: 3542: 3540: 3531: 3529: 3520: 3519: 3516: 3510: 3507: 3505: 3502: 3500: 3497: 3495: 3492: 3491: 3489: 3487: 3483: 3477: 3474: 3472: 3469: 3467: 3464: 3462: 3459: 3457: 3454: 3453: 3451: 3447: 3441: 3438: 3436: 3433: 3431: 3428: 3426: 3423: 3421: 3418: 3416: 3413: 3411: 3408: 3407: 3405: 3401: 3395: 3392: 3390: 3387: 3385: 3382: 3380: 3377: 3375: 3372: 3370: 3367: 3365: 3362: 3360: 3357: 3355: 3352: 3351: 3349: 3347:Constructions 3345: 3335: 3332: 3330: 3327: 3325: 3324:Speed skating 3322: 3320: 3317: 3315: 3312: 3310: 3307: 3305: 3302: 3300: 3297: 3295: 3292: 3290: 3287: 3285: 3282: 3281: 3279: 3277: 3273: 3267: 3264: 3262: 3259: 3257: 3254: 3252: 3249: 3247: 3244: 3242: 3239: 3237: 3234: 3232: 3229: 3228: 3225: 3222: 3216: 3210: 3207: 3205: 3202: 3200: 3197: 3195: 3192: 3190: 3187: 3185: 3182: 3180: 3177: 3175: 3172: 3170: 3167: 3165: 3162: 3160: 3157: 3155: 3152: 3150: 3147: 3145: 3142: 3139: 3135: 3132: 3130: 3127: 3125: 3122: 3120: 3117: 3115: 3112: 3110: 3107: 3105: 3102: 3100: 3097: 3095: 3092: 3090: 3087: 3085: 3082: 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Chem. Phys 2642: 2635: 2632: 2627: 2623: 2618: 2613: 2609: 2605: 2601: 2594: 2591: 2586: 2582: 2578: 2574: 2570: 2566: 2563:(3): 034510. 2562: 2558: 2557:J. Chem. Phys 2551: 2548: 2543: 2539: 2535: 2531: 2527: 2523: 2516: 2513: 2508: 2504: 2500: 2496: 2492: 2488: 2484: 2480: 2476: 2472: 2465: 2462: 2457: 2453: 2449: 2445: 2441: 2437: 2433: 2429: 2422: 2419: 2414: 2410: 2406: 2402: 2395: 2392: 2387: 2381: 2378: 2373: 2372:National Post 2369: 2363: 2360: 2355: 2351: 2345: 2342: 2337: 2333: 2329: 2325: 2314: 2311: 2306: 2302: 2299:: C11A–1069. 2298: 2294: 2286: 2283: 2278: 2277:New Scientist 2274: 2267: 2264: 2258: 2253: 2246: 2243: 2238: 2234: 2229: 2224: 2220: 2216: 2212: 2208: 2204: 2200: 2193: 2190: 2185: 2181: 2177: 2173: 2169: 2165: 2161: 2157: 2153: 2149: 2148: 2140: 2133: 2130: 2125: 2121: 2117: 2113: 2109: 2105: 2101: 2097: 2093: 2089: 2082: 2079: 2074: 2070: 2066: 2062: 2058: 2054: 2047: 2044: 2039: 2035: 2031: 2027: 2023: 2019: 2014: 2009: 2005: 2001: 1994: 1991: 1986: 1982: 1978: 1974: 1970: 1966: 1961: 1956: 1952: 1948: 1940: 1937: 1932: 1928: 1924: 1920: 1913: 1910: 1905: 1901: 1897: 1893: 1886: 1883: 1878: 1874: 1870: 1866: 1862: 1858: 1853: 1848: 1844: 1840: 1833: 1830: 1824: 1821: 1816: 1812: 1808: 1804: 1797: 1794: 1789: 1785: 1781: 1777: 1773: 1769: 1762: 1759: 1754: 1750: 1745: 1740: 1736: 1732: 1725: 1722: 1717: 1713: 1708: 1703: 1699: 1695: 1691: 1687: 1683: 1676: 1673: 1668: 1662: 1658: 1651: 1648: 1643: 1639: 1635: 1631: 1627: 1624:(in German). 1623: 1619: 1612: 1609: 1604: 1600: 1595: 1590: 1585: 1580: 1576: 1572: 1568: 1564: 1560: 1553: 1550: 1545: 1541: 1535: 1532: 1527: 1523: 1519: 1515: 1508: 1505: 1500: 1496: 1490: 1487: 1482: 1476: 1473: 1468: 1464: 1460: 1456: 1453:: 1633–1652. 1452: 1448: 1441: 1438: 1433: 1429: 1425: 1421: 1417: 1413: 1406: 1403: 1390: 1383: 1380: 1367: 1366: 1358: 1355: 1350: 1346: 1342: 1338: 1334: 1330: 1326: 1322: 1314: 1311: 1299: 1295: 1291: 1287: 1283: 1276: 1273: 1261: 1257: 1253: 1249: 1245: 1241: 1236: 1231: 1227: 1223: 1219: 1212: 1209: 1204: 1200: 1196: 1192: 1187: 1182: 1177: 1172: 1168: 1164: 1160: 1152: 1149: 1144: 1140: 1136: 1132: 1125: 1122: 1115: 1111: 1108: 1106: 1103: 1101: 1098: 1097: 1093: 1091: 1031: 1029: 1023: 1019: 1015: 1011: 1006: 1002: 998: 992: 984: 981:100 K ≤ 977: 973: 966: 954: 943: 936: 926: 924: 922: 918: 913: 908: 906: 902: 898: 894: 890: 883: 880: 877: 876: 875: 868: 866: 860: 856: 853: 849: 846: 842: 841: 840: 837: 834: 826: 824: 822: 818: 810: 808: 805: 803: 798: 795: 791: 789: 785: 778: 770: 766: 762: 758: 754: 750: 743: 736: 732: 727: 723: 719: 715: 711: 707: 704:Naturally on 701: 693: 688: 686: 684: 683: 678: 674: 670: 665: 663: 659: 655: 653: 649: 645: 641: 636: 634: 630: 629:planetesimals 626: 622: 618: 614: 613:giant planets 610: 606: 602: 598: 594: 590: 586: 582: 578: 574: 570: 567:HD 100546 in 566: 562: 558: 554: 550: 535: 527: 523: 520: 516: 512: 508: 504: 500: 492: 490: 488: 484: 478: 468: 462: 460: 456: 449: 445: 438: 434: 430: 426: 420: 406: 403: 400: 396: 392: 389: 369: 361: 356: 353: 333: 325: 320: 317: 309: 305: 301: 292: 285: 283: 281: 277: 273: 269: 265: 261: 257: 256:gas pipelines 253: 249: 245: 241: 237: 233: 229: 225: 221: 208: 206: 202: 197: 193: 189: 181: 175: 169: 163: 158: 148: 139: 126: 117: 108: 103: 99: 95: 91: 87: 83: 79: 75: 71: 68: 64: 60: 56: 52: 48: 44: 40: 32: 19: 3334:Tour skating 3134:Frost flower 2965:Major phases 2873:Gas hydrates 2842: 2838: 2798: 2794: 2759: 2756:Energy Fuels 2755: 2749: 2732: 2728: 2718: 2685: 2681: 2675: 2648: 2644: 2634: 2607: 2603: 2593: 2560: 2556: 2550: 2525: 2521: 2515: 2474: 2470: 2464: 2431: 2427: 2421: 2404: 2400: 2394: 2380: 2371: 2362: 2353: 2344: 2327: 2323: 2313: 2296: 2292: 2285: 2276: 2266: 2245: 2202: 2198: 2192: 2151: 2145: 2132: 2091: 2087: 2081: 2056: 2052: 2046: 2003: 1999: 1993: 1950: 1946: 1939: 1922: 1918: 1912: 1895: 1891: 1885: 1842: 1838: 1832: 1823: 1806: 1802: 1796: 1771: 1767: 1761: 1734: 1730: 1724: 1689: 1685: 1675: 1656: 1650: 1628:(1): 25–39. 1625: 1621: 1611: 1566: 1562: 1552: 1543: 1534: 1517: 1513: 1507: 1498: 1489: 1475: 1450: 1446: 1440: 1415: 1411: 1405: 1393:. 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3314:Ice hockey 3289:Iceboating 3220:activities 2991:Formations 2982:Superionic 2228:2115/76168 1788:2014/17884 1186:1912/26136 1116:References 859:inhibitors 757:landslides 718:permafrost 621:abundances 603:, Hersant 240:permafrost 47:clathrates 3261:Sculpture 3077:Phenomena 2776:225428567 2710:140362440 2528:: 60–65. 2456:140362440 2237:182346067 1702:CiteSeerX 1349:106222519 1303:August 3, 1265:August 3, 1230:CiteSeerX 1203:219971360 1100:Clathrate 817:pipelines 753:geohazard 648:Enceladus 625:volatiles 581:ε-Eridani 536:τ 522:continuum 365:¯ 329:¯ 286:Structure 88:, frozen 70:molecules 67:non-polar 3528:Category 3486:Ice ages 3440:Yakhchāl 3420:Icehouse 3246:Climbing 3241:Blocking 3236:Blasting 3154:Hair ice 3104:Crystals 2896:Archived 2823:18762205 2815:16853461 2667:28886658 2626:19585976 2585:19624212 2542:97767359 2499:25503235 2354:BBC News 2184:28990283 2176:24700854 2124:41743663 2116:17170301 2038:14852254 1877:16191976 1642:93862670 1603:30630945 1327:: 6–14. 1260:18762205 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Index

Gas hydrates

crystalline
solids
ice
non-polar
molecules
gases
polar
moieties
hydrogen bonded
water molecules
clathrate compounds
water
lattice
O
H
N
CO2
CH4
H2S
Ar
Kr
Xe
Cl
hydrocarbons
freons
hydrates
first order phase transitions
Sir Humphry Davy

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