Please use this identifier to cite or link to this item: http://hdl.handle.net/10397/91362
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dc.contributorDepartment of Land Surveying and Geo-Informaticsen_US
dc.creatorWu, Ben_US
dc.creatorDong, Jen_US
dc.creatorWang, Yen_US
dc.creatorLi, Zen_US
dc.creatorChen, Zen_US
dc.creatorLiu, WCen_US
dc.creatorZhu, Jen_US
dc.creatorChen, Len_US
dc.creatorLi, Yen_US
dc.creatorRao, Wen_US
dc.date.accessioned2021-11-03T06:53:01Z-
dc.date.available2021-11-03T06:53:01Z-
dc.identifier.urihttp://hdl.handle.net/10397/91362-
dc.language.isoenen_US
dc.publisherAmerican Geophysical Unionen_US
dc.rights© 2021. The Authors. Earth and Space Science published by Wiley Periodicals LLC on behalf of American Geophysical Union.This is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License (https://creativecommons.org/licenses/by-nc-nd/4.0/), which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made.en_US
dc.rightsThe following publication Wu, B., Dong, J., Wang, Y., Li, Z., Chen, Z., Liu, W. C., etal. (2021). Characterization of the candidate landing region for Tianwen-1—China's first mission to Mars. Earth and Space Science, 8, e2021EA001670 is available at https://doi.org/10.1029/2021EA001670en_US
dc.subjectCratersen_US
dc.subjectLanding regionen_US
dc.subjectMarsen_US
dc.subjectPitted conesen_US
dc.subjectRock abundanceen_US
dc.subjectTianwen-1en_US
dc.titleCharacterization of the candidate landing region for Tianwen-1—China's first mission to Marsen_US
dc.typeJournal/Magazine Articleen_US
dc.identifier.volume8en_US
dc.identifier.issue6en_US
dc.identifier.doi10.1029/2021EA001670en_US
dcterms.abstractThis paper presents our efforts to characterize the candidate landing region (109°–133°E, 23°–30°N) for Tianwen-1, China's first mission to Mars, in terms of engineering safety and scientific significance. Topographic analysis reveals that the region has a low elevation around −4,230 m, and 98% of the region have slopes smaller than 8°. The geomorphological mapping and analysis show that the region has an average crater density of about 28 craters (≥200 m in diameter) per 100 square kilometers, with several clusters of high crater densities distributed around the center of the region. There are also pitted cones distributed mainly in the southern part of the region, with a density of approximately 6.6 cones per 100 square kilometers in specific local areas. The region has rock abundances ranging from 1% to 23%, with local clusters of low and high rock abundances. The region comprises four main geological units, including a lowland unit formed in the Late Hesperian and a volcanic unit formed in the Amazonian and Hesperian period. Their specific surface ages are estimated through the analysis of crater size-frequency distribution. Combining the engineering constraints on surface slopes, crater density, cone density, and rock abundance, a hazard map of the candidate landing region is generated for landing site evaluation and safety assessment. Based on the results, we further discuss the potential scientific outcomes from the exploration in this region. The findings will be helpful for the mission planning and maximization of the scientific return from Tianwen-1, and complement existing Martian scientific research.en_US
dcterms.accessRightsopen accessen_US
dcterms.bibliographicCitationEarth and space science, June 2021, v. 8, no. 6, e2021EA001670en_US
dcterms.isPartOfEarth and space scienceen_US
dcterms.issued2021-06-
dc.identifier.scopus2-s2.0-85108549683-
dc.identifier.eissn2333-5084en_US
dc.identifier.artne2021EA001670en_US
dc.description.validate202110 bcvcen_US
dc.description.oaVersion of Recorden_US
dc.identifier.FolderNumberOA_Scopus/WOS-
dc.description.pubStatusPublisheden_US
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