Fluid Lava Flows in Gusev Crater, Mars

Physics

Scientific paper

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Scientific paper

Basaltic rocks in Gusev are modeled to have viscosities of 2.3 to 50
Pa•s at the time of eruption and thus were emplaced as very fluid
flood lavas, consistent with the morphologies seen in orbiter data, at
3.65 by based on crater counts.

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