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- W2133281010 abstract "The settling trends of 318 lunar mare craters are compared with predictions of numerical finite-element models in order to determine the creep response of the upper lunar mare crust. No settling is evident in craters smaller than 5 km in diameter. Settling rates of larger craters increase as function of crater size in a manner suggesting a non-linear lunar creep response corresponding to the power law έ = 8.3 · 10 −34 σ2 where έ is the strain rate and σ is the differential stress. However, the observed nonlinearity is probably an apparent nonlinearity resulting from the temperature induced viscosity decrease with depth due to a lunar crustal temperature gradient of 3° C/km and a creep activation energy of 20 kcal/mole. It is concluded that creep in the lunar medium is essentially Newtonian, and that the effective viscosity of the upper lunar mare crust is (1.6 ± 0.3) · 1025 poise." @default.
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- W2133281010 date "1974-06-01" @default.
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- W2133281010 title "Creep response of the lunar crust in mare regions from an analysis of crater deformation" @default.
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- W2133281010 doi "https://doi.org/10.1016/0031-9201(74)90047-8" @default.
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