Fractured Craters in Southern Syrtis Major, Mars

Physics

Scientific paper

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Scientific paper

Craters around the south-eastern edge of Syrtis Major are eroded and/or refilled. Additionally the crater floors are shaped by wind and fluvial activity generating highly weathered morphologies. Young basaltic deposits originating from nearby Syrtis Major predominately cover the floor of these impact craters. We investigated the correlation between basaltic crater deposits and Syrtis Major volcanic activities.

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