Clay mineralogy in west Chryse Planitia, Mars: Comparison with present and future landing sites

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Jeremy Brossier, Francesca Altieri, Maria Cristina De Sanctis, Alessandro Frigeri, Marco Ferrari, Simone De Angelis, Enrico Bruschini, The Ma_MISS team
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引用次数: 0

Abstract

On Mars, the well-known crustal dichotomy marks the boundary between the old southern highlands and the younger northern lowlands. Among these lowlands, Chryse Planitia resembles a quasi-circular basin surrounded by several highlands, and blends into Acidalia Planitia, another flat lowland located farther north. The transition area between these highlands and the Chryse basin is often designated as “circum-Chryse Planitia”, and is the terminus for many outflow channels. Infrared datasets display several sites therein with extensive clay-bearing outcrops, further testifying for aqueous activity on early Mars – notably around Mawrth Vallis, Oxia Planum and Xanthe Terra. In this study, we investigate clay-bearing outcrops identified along the western margins of circum-Chryse basin, often overlooked in the Martian literature. We also compare them with outcrops found in other regions along the crustal dichotomy and relevant in the Martian literature, such as Oxia Planum, Mawrth Vallis and Nili Fossae. Investigating such deposits is crucial for astrobiological perspectives, as they are appealing targets to search for organic compounds possibly stored throughout the rocks and soils. Fe,Mg-rich clays generally result from the interaction of liquid water with rocks under low temperatures, moderate pH levels and neutral to reducing conditions, factors favorable for life. Here, the clay minerals detected in west Chryse Planitia are consistent with either ferrosaponites or vermiculites associated with hydrobiotite, as recently inferred in Oxia Planum and north Xanthe Terra. Diverse alteration pathways might be involved based on either of these clay species. The clay-bearing rocks crop out in isolated hills in Lunae Planum, and along inverted channels and small craters in Tempe Terra. Further geologic investigations in circum-Chryse Planitia should certainly provide new clues on their origin and weathering conditions, while supporting the upcoming ExoMars rover mission and other future explorations.

火星 Chryse Planitia 西部的粘土矿物学:与现在和未来着陆点的比较
在火星上,众所周知的地壳二分法是古老的南部高地和年轻的北部低地的分界线。在这些低地中,Chryse Planitia 像一个被几个高地包围的准圆形盆地,并与 Acidalia Planitia 融合在一起,Acidalia Planitia 是位于更北部的另一个平坦低地。这些高地和 Chryse 盆地之间的过渡区域通常被称为 "环 Chryse Planitia",是许多外流通道的终点。红外数据集显示,其中几个地点有大量含粘土的露头,进一步证明了早期火星上的水体活动--特别是在 Mawrth Vallis、Oxia Planum 和 Xanthe Terra 周围。在这项研究中,我们调查了在环克里斯盆地西部边缘发现的含粘土露头,这些露头在火星文献中经常被忽略。我们还将它们与地壳二分法沿线其他地区发现的、与火星文献相关的露头(如 Oxia Planum、Mawrth Vallis 和 Nili Fossae)进行了比较。从天体生物学的角度来看,调查这些沉积物至关重要,因为它们是寻找可能储存在岩石和土壤中的有机化合物的有吸引力的目标。富含铁、镁的粘土一般是在低温、适中的pH值和中性至还原性条件下液态水与岩石相互作用的结果,这些因素都有利于生命的存在。在这里,Chryse Planitia 西部检测到的粘土矿物与最近在 Oxia Planum 和 Xanthe Terra 北部推断出的与水绿辉石相关的铁皂石或蛭石一致。基于这两种粘土,可能涉及多种不同的蚀变途径。含粘土的岩石分布在 Lunae Planum 的孤立山丘以及 Tempe Terra 的倒槽和小陨石坑中。在环Chryse Planitia的进一步地质调查肯定会为这些岩石的起源和风化条件提供新的线索,同时为即将进行的ExoMars漫游车任务和其他未来探索提供支持。
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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
期刊介绍: Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered: • Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics • Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system • Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating • Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements • Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation • Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites • Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind • Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations • Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets • History of planetary and space research
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