Exploratory experiments of impact craters formed in viscous-liquid targets - Analogs for Martian rampart craters

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Models, Cratering, Mars Surface, Imaging Techniques, Planetary Evolution, Planetology, Viking Orbiter Spacecraft, Morphology, Water, Ice, Atmosphere, Gases, Flow, Fluidation, Rampart Craters, Cratering, Meteoroid Impacts, Artificial Impacts, Mars, Simulation Experiments, Craters, Ejecta, Regolith, Viking Orbiter

Scientific paper

An experimental study of impact cratering on a mudlike target has been conducted in order to develop a model for ejecta deposits which seem to have been emplaced by flow on the Martian surface. The study yields a possible scheme for the impact, ejection of material, ballistic transport of ejecta, and mode of secondary cratering by the fragments. Comparison of the experimental data with high-resolution Viking Orbiter imagery suggests that the deposits around such rampart craters as Arandes may have been formed by a flow of fluidized materials.

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