{"title":"Map of tectonic shortening structures in Chryse Planitia and Arabia Terra, Mars","authors":"S. Z. Woodley, P. Fawdon, M. Balme, D. Rothery","doi":"10.1080/17445647.2023.2251514","DOIUrl":null,"url":null,"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 km 2 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 fi nd evidence of widespread tectonic shortening structures across the region. The shortening structures have a dominant N-S orientation and occur in all globally identi fi ed geological units. The structural map contributes to a broader understanding of the geological history of the region and Mars ’ wider tectonic history","PeriodicalId":50151,"journal":{"name":"Journal of Maps","volume":"1 3 1","pages":""},"PeriodicalIF":1.9000,"publicationDate":"2023-08-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Maps","FirstCategoryId":"89","ListUrlMain":"https://doi.org/10.1080/17445647.2023.2251514","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"GEOGRAPHY","Score":null,"Total":0}
引用次数: 0
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 km 2 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 fi nd evidence of widespread tectonic shortening structures across the region. The shortening structures have a dominant N-S orientation and occur in all globally identi fi ed geological units. The structural map contributes to a broader understanding of the geological history of the region and Mars ’ wider tectonic history
期刊介绍:
The Journal of Maps is a peer-reviewed, inter-disciplinary, online journal that aims to provide a forum for researchers to publish maps and spatial diagrams.