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Woodley, Savana Z.; Fawdon, Peter; Balme, Matthew R. and Rothery, David A.
(2023).
DOI: https://doi.org/10.1080/17445647.2023.2251514
Abstract
We present a 1:4,000,000 scale map of tectonic landforms in Chryse Planitia and Arabia Terra, on either side of Mars’ dichotomy. Our study area is a ∼3 million km2 region, transitional between Mars’ highlands and lowlands including Oxia Planum, the landing site of the ExoMars rover. Using a structural mapping approach, we digitised all kilometre-scale tectonic structures at a scale of 1:50,000 using high-resolution data (∼6 m/pixel). Although this region is represented as sparsely tectonised on global tectonic maps, we find evidence of widespread tectonic shortening structures across the region. The shortening structures have a dominant N-S orientation and occur in all globally identified geological units. The structural map contributes to a broader understanding of the geological history of the region and Mars’ wider tectonic history.
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- Item ORO ID
- 92315
- Item Type
- Journal Item
- ISSN
- 1744-5647
- Keywords
- Mars; planetary tectonism; shortening structures; wrinkle ridges; lobate scarps; ExoMars
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Copyright Holders
- © 2023 The Authors
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