RHEOLOGICAL PROPERTIES OF WATER ICE—APPLICATIONS TO SATELLITES OF THE OUTER PLANETS 1

By W. Durham. 2001

203 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/49935d7a7a0f734a6f16ef58a4874e36585f1868

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Citations in the corpus

Europa: Tidal heating of upwelling thermal plumes and the origin of lenticulae and chaos melting (2002, background): “Values of Q range between 40 and 60 kJ/mole [Durham and Stern, 2001; Goldsby and Kohlstedt, 2001].”
Subsurface oceans and deep interiors of medium-sized outer planet satellites and large trans-neptunian objects (2006, background): “Laboratory-derived flow laws for pure, polycrystalline ice suggest that both dislocation (n 3) and grain-size-sensitive creep are appropriate flow mechanisms for ice I, whereas dislocation creep is the dominant mechanism for high-pressure ice phases (Weertman, 1983; Durham et al., 1998; Durham and S”
A new family of planets? Ocean-Planets (2003, methodology): “Their phase at high pressure is Perovskite (P > 23 MPa; Anderson, 1997) with the ρ(P ) relation as measured by Duffy and Arhens (1995); – the phase diagram of H2O is complex, with 10 ice phases (Durham and Stern, 2001).”
Ice structures, patterns, and processes: A view across the icefields (2012, background): “An interesting related question to that of astrophysical ice phases, around which work is ongoing (Durham and Stern, 2001; Greve, 2006), is about the rheology or glaciology of ices in a planetary context; e.g., are there glaciers on Pluto?”
Modeling climate diversity, tidal dynamics and the fate of volatiles on TRAPPIST-1 planets (2017, unknown): “At the same temperature and stress conditions, water ice has a viscosity ≤ 1016 Pa s, for grain size lower than 1 mm, based on experimental data (Durham et al. 2001; Durham & Stern 2001; Goldsby & Kohlstedt 2001).”
Interior composition, structure and dynamics of the Galilean satellites (2004, methodology): “A major complication in the thermal modeling of the water ice-liquid outer layer on Europa is the rheology of ice (Durham and Stern 2001, Durham et al. 1997, 1998, 2001, Goldsby and Kohlstedt 1997, 2001, Stern et al. 1997) both in its control of convection and dissipation.”