The polar spirals of Mars may be due to glacier surges deflected by Coriolis forces

Physics

Scientific paper

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Coriolis Effect, Glaciers, Mars Surface, Polar Regions, Ice, Planetary Rotation, Polar Caps, Spirals, Viscosity, Mars, Polar Regions, Ice, Coriolis Force, Patterns, Topography, Flow, Hypotheses, Ice Caps, Viscosity, Gravity Effects, Tectonics, Kinematics, Fractures, Velocity, Thermal Effects, Pressure, Layers, Deposits

Scientific paper

It is argued that the spiral patterns observed by the Mariner spacecraft in the layered ice deposits of the Martian polar regions are fractures which are formed perpendicularly to the gravitionally directed flow lines deflected by Coriolis forces. The minimum effective kinematic viscosity which is consistent with this hypothesis is 7 million sq m/s. It is shown that an occasional kinematic viscosity of 7 million sq m/s is sufficient to cause flow rates of 0.2 m/s along the slopes of the topographic highs. This flow rate would imply that glacier surges on the Martian poles are two orders of magnitude faster than those observed on earth.

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