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- W2043794902 abstract "[1] We apply steady state boundary layer theory to single phase, dike-driven hydrothermal systems beneath the surface of Mars to provide estimates of the heat and liquid water outputs over a range of crustal permeabilities and dike dimensions. Model results yielded a heat output of ∼1.8 × 1019 J/yr and a volumetric fluid flow rate of ∼15 km3/yr for a 1000 km long, 1 km tall dike-like intrusion injected into crust with a permeability of 10−11 m2. A similar, 10 km tall dike could generate a heat output of ∼5.6 × 1019 J/yr and ∼46 km3/yr of fluid flow. For dike half-widths of 10 and 100 m, total volume production of fluid ranged between ∼45 and ∼13,800 km3 along one side of the dike over the respective 3 and 300 year half-dike lifetimes. The calculated fluid flow rates are much less than those estimated for production of the outflow channel system, Athabasca Valles; yet, the total fluid volume produced is of the required magnitude. If fluid could be stored in a near surface reservoir until later episodic release(s), the water volume supplied by one side of a single, 100 m half-width, 200 km long, and 10 km tall dike emplaced into a region with permeability equal to 10−11 m2 could form the outflow channel. Hydrothermally generated meltwater from an overlying, near surface ice layer was found to contribute significantly to the fluid flow volume for this system." @default.
- W2043794902 created "2016-06-24" @default.
- W2043794902 creator A5042003069 @default.
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- W2043794902 date "2012-05-01" @default.
- W2043794902 modified "2023-10-11" @default.
- W2043794902 title "Boundary layer models of hydrothermal circulation on Mars and its relationship to geomorphic features" @default.
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- W2043794902 doi "https://doi.org/10.1029/2012je004049" @default.
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