The Open UniversitySkip to content

Wet-Based Glaciation on Mars

Butcher, Frances E. G. (2019). Wet-Based Glaciation on Mars. PhD thesis. The Open University.

Full text available as:
PDF (Version of Record) - Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
Download (32MB) | Preview
Google Scholar: Look up in Google Scholar


Mars is a glacial planet. It hosts water ice in large polar ice caps, and in thousands of ‘viscous flow features’ in its mid latitudes that are thought to be debris-covered water ice glaciers. These ice deposits range between a few million to ~1 billion years in age and formed during Mars’ most recent epoch, the late Amazonian. The late Amazonian was characterised by extremely cold and arid climate conditions that are not conducive to melting of ice. Consequently, late-Amazonian glaciation has been dominated by cold-based glacier thermal regimes. However, the recent discovery of an esker (a ridge of sediment deposited by meltwater flowing through a tunnel within or beneath glacial ice) associated with a viscous flow feature in the Phlegra Montes region of Mars’ northern mid latitudes provided the first indicative evidence that wet-based glaciation occurred in at least one location during the late Amazonian.

In this thesis, I present the discovery of a second candidate esker associated with a viscous flow feature, in the NW Tempe Terra region of Mars’ northern mid latitudes. I argue that the remarkably similar geologic settings of the NW Tempe Terra and Phlegra Montes candidate eskers (both within tectonic rift/graben valleys) suggests that geothermal heating, possibly with an additional component of viscous strain heating within the basal ice, was a prerequisite for basal melting under cold climate conditions. I then characterise the 2D and 3D morphometries of these candidate eskers, undertake comparisons with the morphometries of ancient putative eskers on Mars and eskers on Earth, and develop conceptual models for the dynamics of esker formation in NW Tempe Terra. Finally, I present a geomorphic map of Chukhung crater, Mars, which hosts esker-like sinuous ridges associated with viscous flow features and provides a case study of the ongoing challenges for esker identification on Mars.

Item Type: Thesis (PhD)
Copyright Holders: 2019 The Author
Project Funding Details:
Funded Project NameProject IDFunding Body
STFC DTG 2015 - 2016 (2015 Intake)ST/N50421X/1STFC (Science & Technology Facilities Council)
Keywords: Mars; water on Mars; glacier; glaciology; esker; wet-based glaciation; meltwater; remote sensing; geomorphology; planetary geomorphology
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM)
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Research Group: Space
Item ID: 60703
Depositing User: Frances Butcher
Date Deposited: 13 May 2019 15:32
Last Modified: 23 Jan 2020 20:06
Share this page:

Download history for this item

These details should be considered as only a guide to the number of downloads performed manually. Algorithmic methods have been applied in an attempt to remove automated downloads from the displayed statistics but no guarantee can be made as to the accuracy of the figures.

Actions (login may be required)

Policies | Disclaimer

© The Open University   contact the OU