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The Mawrth Vallis Region of Mars: A Potential Landing Site for the Mars Science Laboratory (MSL) Mission

机译:火星莫洛斯·瓦利斯(Mawrth Vallis)地区:火星科学实验室(MSL)任务的潜在登陆点

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摘要

The primary objective of NASA's Mars Science Laboratory (MSL) mission, which will launch in 2011, is to characterize the habitability of a site on Mars through detailed analyses of the composition and geological context of surface materials. Within the framework of established mission goals, we have evaluated the value of a possible landing site in the Mawrth Vallis region of Mars that is targeted directly on some of the most geologically and astrobiologically enticing materials in the Solar System. The area around Mawrth Vallis contains a vast (>1×10~6km~2) deposit of phyllosilicate-rich, ancient, layered rocks. A thick (>150m) stratigraphic section that exhibits spectral evidence for nontronite, montmorillonite, amorphous silica, kaolinite, saponite, other smectite clay minerals, ferrous mica, and sulfate minerals indicates a rich geological history that may have included multiple aqueous environments. Because phyllosilicates are strong indicators of ancient aqueous activity, and the preservation potential of biosignatures within sedimentary clay deposits is high, martian phyllosilicate deposits are desirable astrobiological targets. The proposed MSL landing site at Mawrth Vallis is located directly on the largest and most phyllosilicate-rich deposit on Mars and is therefore an excellent place to explore for evidence of life or habitability.
机译:NASA火星科学实验室(MSL)任务(将于2011年启动)的主要目标是,通过对地表物质的组成和地质背景进行详细分析,以表征火星上某个地点的可居住性。在既定任务目标的框架内,我们评估了可能在火星的莫夫·瓦利斯(Mawrth Vallis)地区着陆的价值,该着陆点直接针对太阳系中某些最具有地质和生物学意义的材料。 Mawrth Vallis周围地区蕴藏着大量(> 1×10〜6km〜2)富含层状硅酸盐的古老分层岩石。厚(> 150m)的地层剖面显示了囊脱石,蒙脱石,无定形二氧化硅,高岭石,皂石,其他蒙脱石粘土矿物,亚铁云母和硫酸盐矿物的光谱证据,显示了丰富的地质历史,其中可能包括多种含水环境。由于层状硅酸盐是古代水活动的有力指标,并且沉积粘土沉积物中生物特征的保存潜力很高,因此火星状层状硅酸盐沉积物是理想的天体生物学目标。拟议的莫里斯瓦利斯(Mawrth Vallis)登陆点直接位于火星上最大,最富含页硅酸盐的矿床上,因此是探索生命或居住环境的理想场所。

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