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Glacial and gully erosion on Mars: A terrestrial perspective

Conway, Susan J.; Butcher, Frances E. G.; de Haas, Tjalling; Deijns, Axel J.; Grindrod, Peter M. and Davis, Joel M. (2018). Glacial and gully erosion on Mars: A terrestrial perspective. Geomorphology, 318 pp. 26–57.

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DOI (Digital Object Identifier) Link: https://doi.org/10.1016/j.geomorph.2018.05.019
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Abstract

The mid- to high latitudes of Mars host assemblages of landforms consistent with a receding glacial landscape on Earth. These landforms are postulated to have formed N5 Ma under a different climate regime when Mars' orbital obliquity was on average 10° higher than today. Here, we investigate the spatiotemporal relationship betweengullies and glacial landforms, both common in the mid-latitudes. Gullies are kilometre-scale landforms with asource alcove, transportation channel, and depositional apron. The glacial landforms comprise (1) extant viscous flow features (VFF) that extend from the base of crater walls into the interior of crater floors and are widely interpreted as debris-covered glaciers containing extant ice, and (2) landforms such as arcuate ridges at the base of crater walls that have been interpreted as relicts of more recent, less extensive glacial advances focussed on crater walls. We measure headwall retreat associated with glacial landforms and date their host-craters to constrain minimum headwall retreat rates. We record headwall retreat rates up to ~102m My−1 for the youngest suite of glacial landforms, equivalent to erosion rates of wet-based glaciers on Earth and to headwall retreat rates associated with martian bedrock gully systems. We find extensive evidence for a single erosional episode dating 5–10 Ma, which postdates emplacement of the majority of VFF but seems to predate formation of the gullies. We propose that the wet-based glacial episode was associated with glaciation focussed on the crater walls rather than melting of the glacial ice deposits on the crater floors (VFF). This is consistent with our observations of crater wall morphologies, including the presence of arcuate ridges consistent with terrestrial glaciotectonic features that require liquid water to form, textural alteration of the eroded bedrock surface consistent with ice-segregation and frost-shattering, and the presence of downslope pasted-on terrain, tentatively interpreted here as glacial till deposits sourced from glacial erosion of the crater wall. The pasted-on terrain is usually interpreted as a thicker, latitude-dependant mantle located on sloping terrain formed from airfall of ice nucleated on dust, but we suggest that it has been reworked by glaciation and is predominantly glacial in origin. Although our results cannot substantiate that gullies are produced by meltwater, the discovery of this wet glacial event does provide evidence for widespread meltwater generation in Mars' recent history.

Item Type: Journal Item
Copyright Holders: 2018 Elsevier B.V.
ISSN: 0169-555X
Project Funding Details:
Funded Project NameProject IDFunding Body
Not SetNot SetFrench Space Agency, CNES
STFC DTG 2015 - 2016 (2015 Intake)ST/N50421X/1STFC (Science & Technology Facilities Council)
Rubicon grant019.153LW.002Netherlands Organization for Scientific Research (NWO)
Not SetST/R002355/1UK Space Agency (UK SA)
Not SetST/L00254X/1UK Space Agency (UK SA)
Keywords: Mars; water; gullies; glaciers; glaciers on Mars; water on Mars; geomorphology; remote sensing; glacial meltwater
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Research Group: Space
Item ID: 55269
Depositing User: Frances Butcher
Date Deposited: 30 May 2018 13:28
Last Modified: 13 Sep 2018 11:13
URI: http://oro.open.ac.uk/id/eprint/55269
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