A Low Albedo, Thin, Resistant Unit in Oxia Planum, Mars: Evidence for an Airfall Deposit and Late-Stage Groundwater Activity at the ExoMars Rover Landing Site

IF 3.9 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Journal of Geophysical Research: Planets Pub Date : 2024-11-22 DOI:10.1029/2024JE008527
E. Harris, J. M. Davis, P. M. Grindrod, P. Fawdon, A. L. Roberts
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Abstract

Oxia Planum, Mars, is the future landing site of the ExoMars Rosalind Franklin rover mission, which will search for preserved biosignatures in a phyllosilicate-bearing unit. Overlying the mission-important phyllosilicate-bearing rocks is a dark, capping unit—known here as the Low albedo, Thin, Resistant (LTR) unit—which may have protected the phyllosilicate-bearing unit over geologic time from solar insolation and radiation. However, little is known about the origin of the LTR unit. Here, we map the LTR unit and investigate its distribution and morphology across 50,000 km2 using a variety of orbital remote sensing data sets. The characteristics of the LTR unit include draping palaeo-topographic surfaces, deposition over a wide elevation range, and a consistent vertical thickness that can be best explained by airfall deposition including a primary or reworked volcanic palaeo-ashfall. Previous research suggests that the LTR unit was not significantly buried, and we find it to be preferentially preserved with a high mechanical strength in discrete deposits representing palaeo-topographic lows. We suggest this could be attributed to localized cementation via upwelling groundwater. This scenario suggests that most of the phyllosilicate-bearing exposures may not have been protected over geologic time, as the uncemented LTR sediment would have easily been removed by erosion. However, our observations indicate that the scarped margins of the LTR unit deposits probably exposed regions of the once protected phyllosilicate-bearing unit. These areas could be key science targets for the ExoMars Rosalind Franklin rover mission.

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火星 Oxia Planum 的低反照率、薄而坚硬的单元:ExoMars 火星漫游者着陆点空气沉积和后期地下水活动的证据
火星奥克夏普朗姆是 ExoMars 罗莎琳德-富兰克林漫游车未来的着陆点,该漫游车将在一个含植硅酸盐的单元中寻找保存下来的生物特征。在任务重要的含植物硅酸盐的岩石之上是一个深色的盖层单元--在这里被称为 "低反照率、薄、抗性(LTR)单元"--它可能在地质年代中保护了含植物硅酸盐的单元,使其免受太阳日照和辐射的影响。然而,人们对 LTR 单元的起源知之甚少。在这里,我们利用各种轨道遥感数据集绘制了 LTR 单元图,并研究了其在 50,000 平方公里范围内的分布和形态。LTR单元的特征包括悬垂古地形表面、沉积海拔范围广、垂直厚度一致,其最佳解释是气流沉积,包括原生或再造火山古瀑布。以前的研究表明,LTR 单元并没有被大量掩埋,而我们发现它被优先保存在代表古地形低点的离散沉积物中,具有很高的机械强度。我们认为这可能是由于地下水上涌造成的局部胶结。这种情况表明,由于未胶结的 LTR 沉积物很容易被侵蚀清除,因此大部分含植物硅酸盐的出露地层可能没有受到地质时间的保护。然而,我们的观察结果表明,LTR单元沉积物的瘢痕边缘很可能暴露了曾经受到保护的含硅藻土单元区域。这些区域可能是ExoMars罗莎琳德-富兰克林漫游车任务的关键科学目标。
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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
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.
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