Institute of Geochemistry, Mineralogy and Mineral Resources, Faculty of Science, Charles University, Albertov 6, 128 43 Prague 2, Czech Republic.
Institute of Geochemistry, Mineralogy and Mineral Resources, Faculty of Science, Charles University, Albertov 6, 128 43 Prague 2, Czech Republic.
Spectrochim Acta A Mol Biomol Spectrosc. 2020 Dec 15;243:118818. doi: 10.1016/j.saa.2020.118818. Epub 2020 Aug 11.
Organic minerals occur rather rarely in some types of peat bogs, sedimentary geological environments, and hydrothermal veins. Commonly, calcium oxalates are produced by several plants, terpenoids are often associated with conifers. Because of the organic precursor, these minerals, from the smallest group of the mineralogical system, are sometimes considered as biomarkers. Potential detection of these compounds has high relevance in the fields of exobiology or geobiology. Here we show the potential of four portable Raman spectrometers, using different excitation wavelengths and technologies (operating at 532, 785, and 1064nm together with an advanced spectrometer using the sequentially shifted excitation (SSE) technology), for the rapid and non-destructive identification of these phases. For the organic minerals investigated here, the most intense Raman bands are generally detected at the expected wavenumber positions ±1-4cm in the region 100-2000cm in the spectra obtained from all spectrometers. Additionally, two spectrometers (the 532nm instrument and the SSE) are capable of detecting Raman bands in the higher wavenumber shift region of 2000-3500cm, allowing the more detailed characterization and differentiation of the related phases. From this work, and on the basis of the experimental data obtained, it is clear that the longer laser excitation wavelengths are more preferable for organic minerals identification due to the better mitigation of fluorescence emission. In contrast, the Raman spectrometer equipped with the shortest excitation wavelength (532nm) gives a significantly higher spectral resolution and a more detailed discrimination of the Raman bands, provided that the conditions of general lower level of fluorescence emission are met. The results presented in the current study complement the knowledge on minerals and biomarkers of relevance for Martian environments which have been measured with mobile Raman spectrometers. The outcome creates a solid base towards the use of lightweight mobile Raman systems that can be used outdoors and on terrestrial outcrops. Moreover, these results and conclusions are of use for the further development of dedicated spectrometers destined for the instrumental suites on planetary rovers, in the frame of the forthcoming exobiology focused missions to Mars to be launched by NASA and ESA.
有机矿物质在某些类型的泥炭沼泽、沉积地质环境和热液脉中相当罕见。通常,几种植物会产生草酸盐,萜类化合物通常与针叶树有关。由于有机前体的存在,这些矿物质,来自矿物系统的最小一组,有时被认为是生物标志物。这些化合物的潜在检测在天体生物学或地球生物学领域具有很高的相关性。在这里,我们展示了四台便携式拉曼光谱仪的潜力,这些光谱仪使用不同的激发波长和技术(在 532nm、785nm 和 1064nm 下工作,以及使用顺序移位激发(SSE)技术的先进光谱仪),用于快速和非破坏性地识别这些相。对于这里研究的有机矿物质,在所有光谱仪获得的光谱中,通常在预期波数位置±1-4cm 的范围内检测到最强的拉曼带,在 100-2000cm 的区域内。此外,两台光谱仪(532nm 仪器和 SSE)能够检测到更高波数位移区域 2000-3500cm 的拉曼带,从而能够更详细地表征和区分相关相。从这项工作以及获得的实验数据来看,由于荧光发射的更好抑制,较长的激光激发波长更有利于有机矿物质的识别。相比之下,配备最短激发波长(532nm)的拉曼光谱仪在满足一般较低荧光发射水平的条件下,给出了更高的光谱分辨率和更详细的拉曼带区分。目前研究中提出的结果补充了使用移动拉曼光谱仪测量的与火星环境相关的矿物质和生物标志物的知识。研究结果为使用可在户外和陆地露头使用的轻量级移动拉曼系统奠定了坚实的基础。此外,这些结果和结论对于进一步开发专为行星漫游车仪器套件设计的专用光谱仪也具有一定的参考价值,这些光谱仪将在 NASA 和 ESA 即将开展的火星天体生物学重点任务中使用。