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The interiors and exteriors of the >25 km diameter Batson, Nako, Salkhad, and Jori craters (and McCauley crater to a lesser degree) on the northeastern rim of Hellas basin, Mars, were extensively modified by glacio-fluvial and glacio-lacustrine activity during the Middle and Late Amazonian, from some time before 1.4 Ga to the present as revealed by CTX, HiRISE, and CaSSIS observations. This work presents extensive descriptions and discussions of individual candidate glacial and glaciofluvial landforms associated with cratered landscapes, as well as their spatial association. We also present absolute age dates and a relative sequence of events, followed by a possible environmental reconstruction, involving a regional ice cover, subglacial meltwater, and ice-covered lakes. On crater interiors, inferred glacial modification included dissection of interior rims, emplacement of depositional aprons with basinward scarps, remnant glaciers and associated fresh shallow valleys, supraglacial debris, and candidate moraines. On crater exterior rims and on the plateaus surrounding Batson crater we describe moderate incision and sedimentation, subglacial meltwater runoff through Navua A Valles, candidate eskers, valleys discordant with topography but concordant with inferred ice flow direction, and hummocky material, among others. Wet-based glaciation and subglacial runoff may have been favored due to a locally enhanced geothermal heating or strain heating on steep crater slopes. This work presents a comprehensive and detailed characterization of landforms interpreted as glacial in origin, which could be used to guide identifications of glacial landforms in other cratered regions of Mars.
Galofre et al. (Fri,) studied this question.