Faulting of ILD Deposits on Ceti Mensa, Western Candor Chasma, Mars

Physics

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Scientific paper

Active normal faulting within Ceti Mensa continued until at least 1.4 km
of ILD material was deposited. Only a thin layer of ILD material
postdates fault motion. The domal topography of Ceti Mensa may reflect
the inward tilt of two fault blocks.

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