The strength and rheology of methane clathrate hydrate

Methane clathrate hydrate (structure I) is found to be very strong, based on laboratory triaxial deformation experiments we have carried out on samples of synthetic, high‐purity, polycrystalline material. Samples were deformed in compressional creep tests (i.e., constant applied stress, σ), at condi...

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Published in:Journal of Geophysical Research: Solid Earth
Main Authors: Durham, William B., Kirby, Stephen H., Stern, Laura A., Zhang, Wu
Format: Article in Journal/Newspaper
Language:English
Published: AGU (American Geophysical Union) 2003
Subjects:
Online Access:https://oceanrep.geomar.de/id/eprint/42634/
https://oceanrep.geomar.de/id/eprint/42634/1/Durham_et_al-2003-Journal_of_Geophysical_Research.pdf
https://doi.org/10.1029/2002JB001872
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spelling ftoceanrep:oai:oceanrep.geomar.de:42634 2023-05-15T17:11:41+02:00 The strength and rheology of methane clathrate hydrate Durham, William B. Kirby, Stephen H. Stern, Laura A. Zhang, Wu 2003 text https://oceanrep.geomar.de/id/eprint/42634/ https://oceanrep.geomar.de/id/eprint/42634/1/Durham_et_al-2003-Journal_of_Geophysical_Research.pdf https://doi.org/10.1029/2002JB001872 en eng AGU (American Geophysical Union) https://oceanrep.geomar.de/id/eprint/42634/1/Durham_et_al-2003-Journal_of_Geophysical_Research.pdf Durham, W. B., Kirby, S. H., Stern, L. A. and Zhang, W. (2003) The strength and rheology of methane clathrate hydrate. Journal of Geophysical Research: Solid Earth, 108 (B4). p. 2182. DOI 10.1029/2002JB001872 <https://doi.org/10.1029/2002JB001872>. doi:10.1029/2002JB001872 info:eu-repo/semantics/restrictedAccess Article PeerReviewed 2003 ftoceanrep https://doi.org/10.1029/2002JB001872 2023-04-07T15:39:14Z Methane clathrate hydrate (structure I) is found to be very strong, based on laboratory triaxial deformation experiments we have carried out on samples of synthetic, high‐purity, polycrystalline material. Samples were deformed in compressional creep tests (i.e., constant applied stress, σ), at conditions of confining pressure P = 50 and 100 MPa, strain rate 4.5 × 10−8 ≤ equation image ≤ 4.3 × 10−4 s−1, temperature 260 ≤ T ≤ 287 K, and internal methane pressure 10 ≤ PCH4 ≤ 15 MPa. At steady state, typically reached in a few percent strain, methane hydrate exhibited strength that was far higher than expected on the basis of published work. In terms of the standard high‐temperature creep law, equation image = Aσne−(E*+PV*)/RT the rheology is described by the constants A = 108.55 MPa−n s−1, n = 2.2, E* = 90,000 J mol−1, and V* = 19 cm3 mol−1. For comparison, at temperatures just below the ice point, methane hydrate at a given strain rate is over 20 times stronger than ice, and the contrast increases at lower temperatures. The possible occurrence of syntectonic dissociation of methane hydrate to methane plus free water in these experiments suggests that the high strength measured here may be only a lower bound. On Earth, high strength in hydrate‐bearing formations implies higher energy release upon decomposition and subsequent failure. In the outer solar system, if Titan has a 100‐km‐thick near‐surface layer of high‐strength, low‐thermal conductivity methane hydrate as has been suggested, its interior is likely to be considerably warmer than previously expected. Article in Journal/Newspaper Methane hydrate OceanRep (GEOMAR Helmholtz Centre für Ocean Research Kiel) Ice Point ENVELOPE(-56.781,-56.781,51.217,51.217) Journal of Geophysical Research: Solid Earth 108 B4
institution Open Polar
collection OceanRep (GEOMAR Helmholtz Centre für Ocean Research Kiel)
op_collection_id ftoceanrep
language English
description Methane clathrate hydrate (structure I) is found to be very strong, based on laboratory triaxial deformation experiments we have carried out on samples of synthetic, high‐purity, polycrystalline material. Samples were deformed in compressional creep tests (i.e., constant applied stress, σ), at conditions of confining pressure P = 50 and 100 MPa, strain rate 4.5 × 10−8 ≤ equation image ≤ 4.3 × 10−4 s−1, temperature 260 ≤ T ≤ 287 K, and internal methane pressure 10 ≤ PCH4 ≤ 15 MPa. At steady state, typically reached in a few percent strain, methane hydrate exhibited strength that was far higher than expected on the basis of published work. In terms of the standard high‐temperature creep law, equation image = Aσne−(E*+PV*)/RT the rheology is described by the constants A = 108.55 MPa−n s−1, n = 2.2, E* = 90,000 J mol−1, and V* = 19 cm3 mol−1. For comparison, at temperatures just below the ice point, methane hydrate at a given strain rate is over 20 times stronger than ice, and the contrast increases at lower temperatures. The possible occurrence of syntectonic dissociation of methane hydrate to methane plus free water in these experiments suggests that the high strength measured here may be only a lower bound. On Earth, high strength in hydrate‐bearing formations implies higher energy release upon decomposition and subsequent failure. In the outer solar system, if Titan has a 100‐km‐thick near‐surface layer of high‐strength, low‐thermal conductivity methane hydrate as has been suggested, its interior is likely to be considerably warmer than previously expected.
format Article in Journal/Newspaper
author Durham, William B.
Kirby, Stephen H.
Stern, Laura A.
Zhang, Wu
spellingShingle Durham, William B.
Kirby, Stephen H.
Stern, Laura A.
Zhang, Wu
The strength and rheology of methane clathrate hydrate
author_facet Durham, William B.
Kirby, Stephen H.
Stern, Laura A.
Zhang, Wu
author_sort Durham, William B.
title The strength and rheology of methane clathrate hydrate
title_short The strength and rheology of methane clathrate hydrate
title_full The strength and rheology of methane clathrate hydrate
title_fullStr The strength and rheology of methane clathrate hydrate
title_full_unstemmed The strength and rheology of methane clathrate hydrate
title_sort strength and rheology of methane clathrate hydrate
publisher AGU (American Geophysical Union)
publishDate 2003
url https://oceanrep.geomar.de/id/eprint/42634/
https://oceanrep.geomar.de/id/eprint/42634/1/Durham_et_al-2003-Journal_of_Geophysical_Research.pdf
https://doi.org/10.1029/2002JB001872
long_lat ENVELOPE(-56.781,-56.781,51.217,51.217)
geographic Ice Point
geographic_facet Ice Point
genre Methane hydrate
genre_facet Methane hydrate
op_relation https://oceanrep.geomar.de/id/eprint/42634/1/Durham_et_al-2003-Journal_of_Geophysical_Research.pdf
Durham, W. B., Kirby, S. H., Stern, L. A. and Zhang, W. (2003) The strength and rheology of methane clathrate hydrate. Journal of Geophysical Research: Solid Earth, 108 (B4). p. 2182. DOI 10.1029/2002JB001872 <https://doi.org/10.1029/2002JB001872>.
doi:10.1029/2002JB001872
op_rights info:eu-repo/semantics/restrictedAccess
op_doi https://doi.org/10.1029/2002JB001872
container_title Journal of Geophysical Research: Solid Earth
container_volume 108
container_issue B4
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