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<dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:invenio="http://invenio-software.org/elements/1.0" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"><dc:identifier>doi:10.1016/j.icarus.2020.113680</dc:identifier><dc:language>eng</dc:language><dc:creator>Parenti, Carlota</dc:creator><dc:creator>Gutiérrez, Francisco</dc:creator><dc:creator>Baioni, Davide</dc:creator><dc:creator>García-Arnay, Ángel</dc:creator><dc:creator>Sevil, Jorge</dc:creator><dc:creator>Luzzi, Erica</dc:creator><dc:title>Closed depressions in Kotido crater, Arabia Terra, Mars. Possible evidence of evaporite dissolution-induced subsidence</dc:title><dc:identifier>ART-2020-116511</dc:identifier><dc:description>The identification of karst sinkholes in Mars may provide evidence of dissolution processes caused by liquid water and information on paleoclimatic and paleohydrological conditions. This work presents a comprehensive cartographic inventory of 513 closed depressions developed on evaporite-bearing Equatorial Layered Deposits (ELDs) within Kotido crater, Arabia Terra. Detailed mapping, morphometric analyses and spatial distribution relationships reveal a number of features supporting that the depressions correspond to collapse sinkholes related to evaporite dissolution: (1) suitable topographic and litho-structural conditions for the development of a fracture-controlled epigene evaporite karst; (2) presence of open fissures at the foot of the scarped margins; (3) dimensions and frequency-size distributions comparable with those reported on Earth; (4) spatial association with high-permeability zones (i.e., fractures). Some characteristics of the depressions indicate that they have been re-shaped and enlarged by wind erosion: (1) dominant orientation consistent with the prevalent one-directional winds; (2) differing morphological characteristics on the downwind- and upwind-sides; and (3) nested depressions associated with the upwind sector. The relatively fresh appearance of the depressions and the lack of impact craters suggest a poorly constrained Amazonian karstification phase in the region.</dc:description><dc:date>2020</dc:date><dc:source>http://zaguan.unizar.es/record/109571</dc:source><dc:doi>10.1016/j.icarus.2020.113680</dc:doi><dc:identifier>http://zaguan.unizar.es/record/109571</dc:identifier><dc:identifier>oai:zaguan.unizar.es:109571</dc:identifier><dc:relation>info:eu-repo/grantAgreement/ES/MINECO/CGL2017-85045-P</dc:relation><dc:identifier.citation>Icarus 341 (2020), 113680   [14 pp.]</dc:identifier.citation><dc:rights>by-nc-nd</dc:rights><dc:rights>http://creativecommons.org/licenses/by-nc-nd/3.0/es/</dc:rights><dc:rights>info:eu-repo/semantics/openAccess</dc:rights></dc:dc>

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