Geomorphological characterisation and interpretation of a mid-latitude glacier-like form: Hellas Planitia, Mars

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Type Article
Original languageEnglish
Pages (from-to)330-346
Number of pages17
JournalIcarus
Volume211
Issue number1
Early online date10 Nov 2010
DOI
Publication statusPublished - 01 Jan 2011
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Abstract

We describe and interpret the surface terrain types associated with a widely-reported not, vert, similar4 km long, mid-latitude martian viscous flow feature (VFF). The feature is located in the southern hemisphere, on the poleward-facing rim of a not, vert, similar60 km-diameter crater in eastern Hellas Planitia. High Resolution Imaging Science Experiment (HiRISE) images, analysed in both 2D and 3D, reveal that the upper margin of the feature is bounded by steep (not, vert, similar30°) headwalls, typically some tens of metres high, that are formed from unconsolidated material and characterised by a series of slope–parallel linear incisions. Below these incised headwalls, the feature flows at a general angle of not, vert, similar10° from a broad upper basin to a confined lower tongue that is bounded by a nested sequence of elongate raised ridges. These characteristics are typical of several VFFs in the region and are strikingly similar to moraine-bounded valley glaciers on Earth, and we sub-classify this feature as a ‘glacier-like form’ (GLF)1. The GLF comprises five distinctive surface terrain types that contrast sharply with surface characteristics outside its bounding moraines. Four of these terrains (scaly terrain, polygonized terrain, linear terrain and mound-and-tail terrain) are located within the GLF’s innermost bounding moraine, while the fifth (rectilinear-ridge terrain) is located between its frontal moraines. These terrains are mapped, characterised and associated with possible mechanisms of formation to draw inferences about the GLF’s glaciology and glacial history. This analysis suggests that the GLF reached its maximal extent in the geologically-recent past, and that it may have been partially wet-based at that time. Subsequent to this phase, the GLF experienced an extended period of general recession that has been punctuated by several episodes of still-stand or advance. Currently, the GLF’s basin appears to be composed of a lower zone that is dominated by an exposed former glacier bed and an upper zone that may still contain a now-degraded and dust-mantled viscous mass, similar to many partially-glacierized basins on Earth.

Keywords

  • Mars, Mars, Surface, Mars, Polar caps