Combinations of processes responsible for Martian impact crater ``layered ejecta structures'' emplacement (original) (raw)

Journal of Geophysical Research, 2007

Abstract

We utilized images and stereo-derived topographic data acquired by the High Resolution Stereo Camera (HRSC) and Thermal Emission Imaging System (THEMIS) images together with other data in order to study the geology of “layered ejecta structures” associated with relatively pristine Martian impact craters. The geomorphology and morphometric properties indicate their origin as complex combinations of a variety of impact processes.

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