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Amazonian chemical weathering rate derived from stony meteorite finds at Meridiani Planum on Mars

机译:来自火星Meridiani Planum的石陨石的亚马逊化学风化率

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摘要

Spacecraft exploring Mars such as the Mars Exploration Rovers Spirit and Opportunity, as well as the Mars Science Laboratory or Curiosity rover, have accumulated evidence for wet and habitable conditions on early Mars more than 3 billion years ago. Current conditions, by contrast, are cold, extremely arid and seemingly inhospitable. To evaluate exactly how dry today's environment is, it is important to understand the ongoing current weathering processes. Here we present chemical weathering rates determined for Mars. We use the oxidation of iron in stony meteorites investigated by the Mars Exploration Rover Opportunity at Meridiani Planum. Their maximum exposure age is constrained by the formation of Victoria crater and their minimum age by erosion of the meteorites. The chemical weathering rates thus derived are ∼1 to 4 orders of magnitude slower than that of similar meteorites found in Antarctica where the slowest rates are observed on Earth.
机译:探测火星的航天器,例如“火星探测漫游者精神与机遇”,以及“火星科学实验室”或“好奇号”火星车,已经积累了超过30亿年前火星早期潮湿和适宜居住条件的证据。相比之下,当前的条件是寒冷,极度干旱且看似荒凉。为了准确评估当今环境的干燥程度,重要的是要了解当前正在进行的风化过程。在这里,我们介绍了为火星确定的化学风化率。我们使用Meridiani Planum的火星探测漫游者机会调查的石质陨石中铁的氧化。它们的最大暴露年龄受到维多利亚陨石坑形成的限制,而其最小暴露年龄受到陨石侵蚀的限制。这样得出的化学风化速率比在地球上观察到的最慢速率的南极洲的类似陨石慢约1-4个数量级。

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