3D Architecture of Kodiak Butte as Evidence of Fluvial or Shoal-Water Environments in Jezero Crater, Mars

IF 3.7 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
O. A. Kanine, M. P. Lamb, B. L. Ehlmann, J. P. Grotzinger, C. D. Tate
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Abstract

The Mars 2020 mission has explored depositional environments recorded in a fan-shaped deposit on the western side of Jezero crater. Kodiak butte is an isolated outcrop of sedimentary rock ∼1 km south of the western fan scarp and may be an erosional remnant of said fan. Sedimentary strata of Kodiak butte were first interpreted to represent Gilbert delta foresets and a lake depth of at least 10 m. Subsequent closer-range images of the northern face of Kodiak have resolved additional details of stratal geometries, permitting alternative interpretations of depositional environments. Rover visible-wavelength images, a three-dimensional digital outcrop model, and principal component analysis-based plane-fitting allow detailed facies mapping and measurements of stratal geometries in Kodiak. We observed three sets of gravel-bearing, steeply inclined beds ∼3, ∼7, and ∼10 m thick with local accretion directions ranging from ∼NW clockwise to ∼SW (covering ∼230° azimuth). These sets are interpreted as deposits from downstream-migrating bars with lobate geometries, consistent with mid-channel bars in a braided river or mouth bars in a shoal-water delta. The geometry of the inclined beds indicate channelized bankfull flow ∼4.2 m deep under persistent currents flowing south-southeast to south-southwest. The proposed hydrodynamic conditions, potentially continuous with the rest of the western fan succession, are high energy with limited settling of fine-grained sediment from suspension in a quiescent setting, indicating a lower biosignature preservation potential than previously hypothesized.

科迪亚克丘的三维建筑作为火星耶泽罗陨石坑河流或浅水环境的证据
火星2020任务已经探索了耶泽洛陨石坑西侧扇形沉积物中记录的沉积环境。Kodiak丘是西部扇崖以南约1公里处的一个孤立的沉积岩露头,可能是该扇的侵蚀残余物。科迪亚克丘的沉积地层首先被解释为吉尔伯特三角洲森林和至少10米深的湖泊。随后,科迪亚克北部的近距离图像已经解决了地层几何形状的额外细节,允许对沉积环境进行不同的解释。漫游者可见波长图像、三维数字露头模型和基于主成分分析的平面拟合,可以对Kodiak的地层几何形状进行详细的相图绘制和测量。我们观察到三组含砾石、厚度为~ 3、~ 7和~ 10 m的陡峭倾斜地层,局部吸积方向从顺时针~ NW到~ SW(覆盖~ 230°方位角)。这些组被解释为来自具有叶状几何形状的下游迁移砂坝的沉积物,与辫状河中的河道中砂坝或浅水三角洲的河口砂坝相一致。倾斜河床的几何形状表明,在南-东南至南-西南的持续水流下,河道化的河岸流约4.2 m深。所提出的水动力条件,可能与西部扇序列的其余部分连续,是高能量的,在静止环境中悬浮的细粒沉积物沉淀有限,表明生物特征保存潜力比先前假设的要低。
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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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