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Detailed Reference Information |
Beeman, M., Durham, W.B. and Kirby, S.H. (1988). Friction of ice. Journal of Geophysical Research 93: doi: 10.1029/88JB01435. issn: 0148-0227. |
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The frictional strength of ice seems to be well below that for all other rocks. Triaxial testing of cylinders of pure water ice containing a 45¿ inclined sawcut, at temperatures of 77≤T≤115 K and confining pressures 0.1≤P≤250 MPa, reveals the frictional laws &tgr;=0.20 &sgr;n+8.3 MPa for P≥10 MPa and &tgr;=0.55 &sgr;n+1.0 MPa for P≤5 MPa, where &tgr; and &sgr;n are the shear and normal stresses on the sawcut surface. Friction is independent of T and, over the one order of magnitude tested, of average sliding velocity. The sliding behavior is invariably stick slip. Examination of sliding surfaces shows only minor gouge development. A curious arrangement of densely packed short vertical fractures occurs primarily in samples with anomalously low strength. These results apply to models of near-surface tectonic activity on Jupiter's three large icy moons, Europa, Callisto, and Ganymede. They indicate, for example, that a global expansion on Ganymede of 3 linear percent will cause extensional movement on preexisting faults at depths to 7¿3 km. ¿ American Geophysical Union 1988 |
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Abstract |
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Keywords
Planetology, Solid Surface Planets, Surface materials and properties, Planetology, Solid Surface Planets, Physical properties of materials, Physical Properties of Rocks, Fracture and flow, Tectonophysics, Rheology—general |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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