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Atomic Force Microscopy of Extraterrestrial Samples

机译:地外样品的原子力显微镜

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Atomic force microscopy (AFM) has been employed to perform morphological analyses of extraterrestrial dust and soil particles. This work presents a review of the first in-situ images at the nanometer scale of Martian dust recently reported by NASA/Phoenix mission. Although such AFM images cannot provide more chemical evidence than the topographical data, from an engineering point of view, the operation of AFM in-flight instrument by itself is considered as a biggest challenge. Moreover, the development and building of AFM technique for planetary (including meteorites, comets, and lunar samples) science research is discussed and compared herein with previous laboratory testing results. This work also collects the results of a relatively small number of AFM experiments (ESA/MIDAS Rosetta missions, Allan Hill 84001 and Apollo 11) in an effort to provide the reader a general idea about the related technology to use AFMs in the field of space exploration. Finally, the strengths and weakness of AFM as incorporated on planetary spacecrafts for in-situ investigations is presented leading to recognize the limiting operational constrains that exists when attempting to characterize high aspect ratio extraterrestrial particles.
机译:原子力显微镜(AFM)已被用于对地外灰尘和土壤颗粒进行形态分析。这项工作是对美国国家航空航天局/凤凰城特派团最近报告的火星尘埃纳米级的第一批原位图像的回顾。尽管此类AFM图像不能提供比地形数据更多的化学证据,但从工程角度来看,AFM机载仪器本身的操作被认为是最大的挑战。此外,本文还讨论了用于行星(包括陨石,彗星和月球样品)科学研究的AFM技术的开发和构建,并将其与以前的实验室测试结果进行了比较。这项工作还收集了相对少量的原子力显微镜实验的结果(ESA / MIDAS Rosetta任务,艾伦·希尔84001和阿波罗11号),旨在为读者提供有关在太空领域使用原子力显微镜的相关技术的一般思路。勘探。最后,提出了原子力显微镜的优点和缺点,这些优点结合在行星飞船上进行原位研究,从而使人们认识到试图表征高深宽比的地球外粒子时存在的局限性操作约束。

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