Institute of Geochemistry, Mineralogy and Mineral Resources, Charles University in Prague, Albertov 6, 128 43 Prague 2, Czech Republic.
Philos Trans A Math Phys Eng Sci. 2010 Jul 13;368(1922):3109-25. doi: 10.1098/rsta.2010.0075.
Organic minerals, organic acids and NH-containing organic molecules represent important target molecules for astrobiology. Here, we present the results of the evaluation of a portable hand-held Raman spectrometer to detect these organic compounds outdoors under field conditions. These measurements were carried out during the February-March 2009 winter period in Austrian Alpine sites at temperatures ranging between -5 and -25 degrees C. The compounds investigated were detected under field conditions and their main Raman spectral features were observed unambiguously at their correct reference wavenumber positions. The results obtained demonstrate that a miniaturized Raman spectrometer equipped with 785 nm excitation could be applied with advantage as a key instrument for investigating the presence of organic minerals, organic acids and nitrogen-containing organic compounds outdoors under terrestrial low-temperature conditions. Within the payload designed by ESA and NASA for several missions focusing on Mars, Titan, Europa and other extraterrestrial bodies, Raman spectroscopy can be proposed as an important non-destructive analytical tool for the in situ identification of organic compounds relevant to life detection on planetary and moon surfaces or near subsurfaces.
有机矿物质、有机酸和含 NH 的有机分子是天体生物学的重要目标分子。在这里,我们介绍了一种便携式手持拉曼光谱仪的评估结果,该光谱仪用于在野外条件下检测这些有机化合物。这些测量是在 2009 年 2 月至 3 月的冬季期间在奥地利阿尔卑斯山地区进行的,温度范围在-5 至-25°C 之间。在所研究的化合物在野外条件下进行了检测,并在其正确的参考波数位置上明确观察到了它们的主要拉曼光谱特征。所获得的结果表明,配备 785nm 激发源的小型化拉曼光谱仪可作为一种关键仪器,用于在地球低温条件下在野外探测有机矿物质、有机酸和含氮有机化合物的存在。在 ESA 和 NASA 为多个专注于火星、泰坦、木卫二和其他外星体的任务设计的有效载荷中,拉曼光谱可以作为一种重要的非破坏性分析工具,用于在行星和月球表面或近表面原位识别与生命探测相关的有机化合物。