{"title":"火星Chryse Planitia和Arabia Terra构造缩短构造图","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":"{\"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}","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}
Map of tectonic shortening structures in Chryse Planitia and Arabia Terra, Mars
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.