Please use this identifier to cite or link to this item:
https://hdl.handle.net/10316/112166
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Vaz, David A. | - |
dc.contributor.author | Silvestro, Simone | - |
dc.contributor.author | Chojnacki, Matthew | - |
dc.contributor.author | Silva, David C. A. | - |
dc.date.accessioned | 2024-01-23T11:43:18Z | - |
dc.date.available | 2024-01-23T11:43:18Z | - |
dc.date.issued | 2023 | - |
dc.identifier.issn | 0012821X | - |
dc.identifier.uri | https://hdl.handle.net/10316/112166 | - |
dc.description.abstract | Aeolian processes on Mars form a distinct class of meter-scale ripples, whose mechanisms of formation are debated. We present a global morphometric survey of Martian bedforms, adding relevant observational constraints to the ongoing debate. We compare our results with previous surveys, highlighting inconsistencies in data used in previous studies, namely for the bedforms located in the Tharsis highlands. We show that the bedforms located in the Tharsis region form a distinct group, not akin to the large dark-toned ripples which cover dune fields elsewhere on the planet. Tharsis bedforms form unique patterns, present distinct thermophysical characteristics and have higher albedos, suggesting they are formed and/or covered by finer materials. The relation between wavelength and atmospheric density derived from the new data is consistent with the predictions of a wind-drag mechanism, favoring the model that uses a saltation saturation length. Regardless of the mechanism that limits the size of bedforms, these results confirm the existence of a robust relationship between the wavelength of large ripples and atmospheric density (ripples’ spacing increases with decreasing atmospheric density). This provides further support to the interpretation of paleoatmospheric conditions on Mars through the analysis of its aeolian sedimentary record. | pt |
dc.language.iso | eng | pt |
dc.publisher | Elsevier | pt |
dc.relation | CITEUC (UID/Multi/00611/2021&POCI-01-0145-FEDER-006922) | pt |
dc.relation | FCT - grant CEECIND/02981/2017 | pt |
dc.relation | NASA Mars Data Analysis Program Grant 80NSSC20K1066 | pt |
dc.rights | openAccess | pt |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | pt |
dc.subject | large Martian ripples | pt |
dc.subject | transverse aeolian ridges | pt |
dc.subject | bedform wavelength | pt |
dc.subject | aeolian | pt |
dc.subject | Mars | pt |
dc.subject | remote sensing | pt |
dc.title | Constraining the mechanisms of aeolian bedform formation on Mars through a global morphometric survey | pt |
dc.type | article | pt |
degois.publication.firstPage | 118196 | pt |
degois.publication.title | Earth and Planetary Science Letters | pt |
dc.peerreviewed | yes | pt |
dc.identifier.doi | 10.1016/j.epsl.2023.118196 | - |
degois.publication.volume | 614 | pt |
dc.date.embargo | 2023-01-01 | * |
uc.date.periodoEmbargo | 0 | pt |
item.fulltext | Com Texto completo | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.languageiso639-1 | en | - |
item.openairetype | article | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.project.grantno | Centre for Earth and Space Research of the University of Coimbra | - |
crisitem.author.researchunit | CITEUC - Centre for Earth and Space Research of the University of Coimbra | - |
crisitem.author.parentresearchunit | University of Coimbra | - |
crisitem.author.orcid | 0000-0002-3196-6620 | - |
Appears in Collections: | I&D CITEUC - Artigos em Revistas Internacionais |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Constraining the mechanisms of aeolian bedform formation on Mars through a global morphometric survey.pdf | 2.13 MB | Adobe PDF | View/Open |
Page view(s)
78
checked on Oct 16, 2024
Download(s)
56
checked on Oct 16, 2024
Google ScholarTM
Check
Altmetric
Altmetric
This item is licensed under a Creative Commons License