| Literature DB >> 32466668 |
Nicolas Mangold1, Gilles Dromart2, Veronique Ansan1, Francesco Salese3,4, Maarten G Kleinhans3, Marion Massé1, Cathy Quantin-Nataf2, Kathryn M Stack5.
Abstract
Jezero crater has been selected as the landing site for the Mars 2020 Perseverance rover, because it contains a paleolake with two fan-deltas, inlet and outlet valleys. Using the data from the High Resolution Stereo Camera (HRSC) and the High Resolution Imaging Science Experiment (HiRISE), we conducted a quantitative geomorphological study of the inlet valleys of the Jezero paleolake. Results show that the strongest erosion is related to a network of deep valleys that cut into the highland bedrock well upstream of the Jezero crater and likely formed before the formation of the regional olivine-rich unit. In contrast, the lower sections of valleys display poor bedrock erosion and a lack of tributaries but are characterized by the presence of pristine landforms interpreted as fluvial bars from preserved channels, the discharge rates of which have been estimated at 103-104 m3s-1. The valleys' lower sections postdate the olivine-rich unit, are linked directly to the fan-deltas, and are thus formed in an energetic, late stage of activity. Although a Late Noachian age for the fan-deltas' formation is not excluded based on crosscutting relationships and crater counts, this indicates evidence of a Hesperian age with significant implications for exobiology.Entities:
Keywords: Fluvial landforms; HRSC; HiRISE; Landing site; Mars; Perseverance rover
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Year: 2020 PMID: 32466668 DOI: 10.1089/ast.2019.2132
Source DB: PubMed Journal: Astrobiology ISSN: 1557-8070 Impact factor: 4.335