Locations and Properties of Ice-Exposing Scarps and New Impact Craters in the Mid-Latitudes of Mars
Although ice in the Martian mid-latitudes is typically covered by a layer of dust or
regolith, it is exposed in some locations by fresh impact craters or in erosional scarps. In
both cases, the exposed ice is massive or excess ice with a low lithic content. We find that
erosional scarps occur between 50–61 north and …