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Material selection and its characterization for Mars environment and a study on full field strain analysis

机译:MARS环境的材料选择及其表征及全场应变分析研究

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The atmosphere of Mars consists of carbon dioxide (95.32%), nitrogen (2.70%), argon (1.60%), oxygen (0.13%), carbon monoxide (0.08%) and small amounts of water vapor and other gases. The diurnal temperature ranges from 184 K to 242 K (-89°C to -31°C). It is necessary to consider these technical attributes of the Martian environment for future endeavors in space exploration. This work aims at the selection of a material, which is most suitable for the Martian environment. The selection is carried out by defining application requirements, physical properties of the material and short-listing of possible materials. The selected material is then acquired depending on factors such as feasibility, availability and cost efficiency. Characterization of materials is carried out by conducting impact, hardness, tensile and flexural testing at room temperature following the ASTM standards for testing of plastics. Conclusively, the theoretical aspects of full-field strain analysis using Digital Image Correlation (DIC) technique is discussed as a future scope of the work.
机译:火星的气氛由二氧化碳(95.32%),氮气(2.70%),氩(1.60%),氧气(0.13%),一氧化碳(0.08%)和少量水蒸气和其他气体组成。昼夜温度范围为184k至242k(-89℃至-31°C)。有必要考虑Martian环境的这些技术属性,以便在太空探索中的未来努力。这项工作旨在选择一种最适合火星环境的材料。通过定义应用要求,材料的物理性质以及可能的材料的短列出来进行选择。然后根据可行性,可用性和成本效率等因素获取所选材料。通过在室温下进行的ASTM标准进行塑料,通过在室温下进行冲击,硬度,拉伸和弯曲测试来进行材料的表征。最后,讨论了使用数字图像相关(DIC)技术的全场应变分析的理论方面作为工作的未来范围。

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