Alyssa C. Pascuzzo, Ali M. Bramson, Patricio Becerra, John F. Mustard
{"title":"Development and Evolution of Icy Layer Outcrops on Mars' North Polar Ice Cap: Observations of Vertical and Lateral Variability","authors":"Alyssa C. Pascuzzo, Ali M. Bramson, Patricio Becerra, John F. Mustard","doi":"10.1029/2024JE008377","DOIUrl":null,"url":null,"abstract":"<p>Mars' north polar ice cap features troughs that cut into the ice, exposing subsurface layers of different brightness and topographic expression. Specifically, these layers represent two different stratum types: lower albedo (higher dust content) marker beds, which protrude out of the wall topographically, and higher albedo (i.e., icier) interbeds, which are recessed compared to the marker beds. Here, we investigate the role of local-scale processes by performing a detailed geomorphic characterization of variability in these strata across two sites, using a novel approach to calculating true layer protrusion which utilizes data from high-resolution Digital Terrain Models. We measure protrusions of the order of meters but find lateral variations within a single trough exposure, suggesting a role for local-scale processes in the evolution of the layers. We find that the topographic relief of protruding marker beds decreases as a function of decreasing trough slope and brightness (a proxy for dust cover/content). We also observe the presence of an insulative allochthonous dust veneer present on discrete sections of the trough wall, which we suspect plays an important role in modulating ice loss from the trough walls. A companion paper (Bramson et al., 2025, https://doi.org/10.1029/2024JE008360) models the contribution of insolation-induced sublimation to present a new framework, and potential timescales for the development of the marker bed protrusion observed here.</p>","PeriodicalId":16101,"journal":{"name":"Journal of Geophysical Research: Planets","volume":"130 1","pages":""},"PeriodicalIF":4.0000,"publicationDate":"2025-01-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Planets","FirstCategoryId":"89","ListUrlMain":"https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024JE008377","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Mars' north polar ice cap features troughs that cut into the ice, exposing subsurface layers of different brightness and topographic expression. Specifically, these layers represent two different stratum types: lower albedo (higher dust content) marker beds, which protrude out of the wall topographically, and higher albedo (i.e., icier) interbeds, which are recessed compared to the marker beds. Here, we investigate the role of local-scale processes by performing a detailed geomorphic characterization of variability in these strata across two sites, using a novel approach to calculating true layer protrusion which utilizes data from high-resolution Digital Terrain Models. We measure protrusions of the order of meters but find lateral variations within a single trough exposure, suggesting a role for local-scale processes in the evolution of the layers. We find that the topographic relief of protruding marker beds decreases as a function of decreasing trough slope and brightness (a proxy for dust cover/content). We also observe the presence of an insulative allochthonous dust veneer present on discrete sections of the trough wall, which we suspect plays an important role in modulating ice loss from the trough walls. A companion paper (Bramson et al., 2025, https://doi.org/10.1029/2024JE008360) models the contribution of insolation-induced sublimation to present a new framework, and potential timescales for the development of the marker bed protrusion observed here.
火星的北极冰帽以切入冰的槽为特征,暴露出不同亮度和地形表现的地下层。具体来说,这些层代表了两种不同的地层类型:低反照率(高含尘量)的标志层,在地形上突出于岩壁外;高反照率(即冰川)的互层,与标志层相比,它们是凹陷的。在这里,我们研究了局部尺度过程的作用,通过对两个地点的这些地层的变化进行详细的地貌表征,使用一种利用高分辨率数字地形模型数据计算真实层突出的新方法。我们测量了米数量级的突出物,但在单个槽暴露中发现了横向变化,这表明在地层演化中局部尺度过程的作用。我们发现,突出标志层的地形起伏度随着槽坡和亮度(尘盖/含量的代表)的减小而减小。我们还观察到在槽壁的离散部分存在绝缘的异质粉尘贴面,我们怀疑这在调节槽壁的冰损失方面起着重要作用。另一篇论文(Bramson et al., 2025, https://doi.org/10.1029/2024JE008360)模拟了日晒引起的升华的贡献,提出了一个新的框架,以及这里观察到的标记床突出发展的潜在时间尺度。
期刊介绍:
The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.