BIROn - Birkbeck Institutional Research Online

    Multiple sites of recent wet-based glaciation identified from eskers in western Tempe Terra, Mars

    Woodley, S. and Butcher, F. and Fawdon, P. and Clark, C. and Ng, F. and Davis, Joel and Gallagher, C. (2022) Multiple sites of recent wet-based glaciation identified from eskers in western Tempe Terra, Mars. Icarus 386 (115147), ISSN 0019-1035.

    [img]
    Preview
    Text
    49747.pdf - Published Version of Record
    Available under License Creative Commons Attribution.

    Download (18MB) | Preview

    Abstract

    Precipitation in Mars' mid-latitudes formed Viscous Flow Features (VFFs), landforms analogous to terrestrial debris-covered glaciers, in the last 1 Gyr. Until recently, the prevailing view was that the Amazonian environment was not conducive to basal melting of VFFs. However, recent identification of VFF-linked eskers (sedimentary ridges deposited by meltwater in sub-glacial tunnels) in Phlegra Montes and Tempe Terra suggests localized basal melting has occurred. We identify two VFF-linked sinuous ridges in western Tempe Terra, which we propose are two additional eskers. To explore this hypothesis, we produce a 1:300,000 map of the geomorphology of western Tempe Terra, use impact crater counts to constrain the age of the sinuous ridges, and analyze the morphology and morphometry of the sinuous ridges. Mapping reveals a heavily deformed Noachian massif that was embayed by younger volcanic material and subsequently glaciated. The sinuous ridges lie 3–7 km from the VFF-termini and are associated with mounds which we interpret as ice-cored moraines. After considering multiple formation hypotheses (including inverted paleochannels and volcanic features) and comparing morphometries to Martian and terrestrial eskers, we suggest that both the sinuous ridges are of glacial origin and most likely eskers. This shows that basal melting of VFFs occurred at more than one location in Tempe Terra, at least transiently. Thus, our identification of two additional candidate eskers in Tempe Terra suggests that the late Amazonian thermal environment may have been more complex than previously thought and contributes to a better characterization of the recent glacial history of the region.

    Metadata

    Item Type: Article
    Keyword(s) / Subject(s): Mars, Mars glaciation, Mars geomorphology, Sinuous ridges, Eskers
    School: Birkbeck Faculties and Schools > Faculty of Science > School of Natural Sciences
    Research Centres and Institutes: Earth and Planetary Sciences, Institute of
    Depositing User: Joel Davis
    Date Deposited: 09 Nov 2022 16:08
    Last Modified: 02 Aug 2023 18:19
    URI: https://eprints.bbk.ac.uk/id/eprint/49747

    Statistics

    Activity Overview
    6 month trend
    46Downloads
    6 month trend
    92Hits

    Additional statistics are available via IRStats2.

    Archive Staff Only (login required)

    Edit/View Item
    Edit/View Item