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    Extensive Noachian fluvial systems in Arabia Terra: implications for early Martian climate

    Davis, Joel and Balme, M. and Grindrod, Peter and Williams, R. and Gupta, S. (2016) Extensive Noachian fluvial systems in Arabia Terra: implications for early Martian climate. Geology 44 (10), pp. 847-850. ISSN 0091-7613.

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    Valley networks are some of the strongest lines of evidence for extensive fluvial activity on early (Noachian; > 3.7 Ga) Mars. However, their purported absence on certain ancient terrains, such as Arabia Terra, is at variance with patterns of precipitation as predicted by ‘warm and wet’ climate models. This disagreement has contributed to the development of an alternative ‘icy highlands’ scenario, whereby valley networks were formed by the melting of highland ice-sheets. Here, we show through regional mapping that Arabia Terra shows evidence for extensive networks of sinuous ridges. We interpret these ridge features as inverted fluvial channels that formed in the Noachian, before being subject to burial and exhumation. The inverted channels developed on extensive aggrading flood plains. As the inverted channels are both sourced in, and traverse across, Arabia Terra, their formation is inconsistent with discrete, localized sources of water, such as meltwater from highland ice-sheets. Our results are instead more consistent with an early Mars that supported widespread precipitation and runoff.


    Item Type: Article
    School: Birkbeck Faculties and Schools > Faculty of Science > School of Natural Sciences
    Depositing User: Peter Grindrod
    Date Deposited: 02 Sep 2016 08:29
    Last Modified: 02 Aug 2023 17:25


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