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Saturn's moon Iapetus has an equatorial ridge system, which may be as high as20 km, that may have formed by endogenic forces, such as tectonic andconvective forces, or exogenic processes such as debris infall. We usehigh-resolution topographic data to conduct a topographic analysis of theridge, which suggests a predominantly triangular morphology, with some ridgeface slopes reaching 40 degrees, allowing for an exogenic formation mechanism.

Topographic Constraints on the Origin of the Equatorial Ridge on Iapetus