Loizeau Damien, Pilorget Cédric, Poulet François, Lantz Cateline, Bibring Jean-Pierre, Hamm Vincent, Royer Clément, Dypvik Henning, Krzesińska Agata M, Rull Fernando, Werner Stephanie C
Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, Orsay, France.
Geosciences, University of Oslo, Oslo, Norway.
Astrobiology. 2022 Mar;22(3):263-292. doi: 10.1089/ast.2020.2420. Epub 2022 Mar 8.
The Planetary Terrestrial Analogues Library (PTAL) project aims at building and exploiting a database involving several analytical techniques, to help characterize the mineralogical evolution of terrestrial bodies, starting with Mars. Around 100 natural Earth rock samples have been collected from selected locations to gather a variety of analogs for martian geology, from volcanic to sedimentary origin with different levels of alteration. All samples are to be characterized within the PTAL project with different mineralogical and elemental analysis techniques, including techniques brought on actual and future instruments at the surface of Mars (near infrared [NIR] spectroscopy, Raman spectroscopy, and laser-induced breakdown spectroscopy). This article presents the NIR measurements and interpretations acquired with the ExoMars MicrOmega spare instrument. MicrOmega is an NIR hyperspectral microscope, mounted in the analytical laboratory of the ExoMars rover Rosalind Franklin. All PTAL samples have been observed at least once with MicrOmega using a dedicated setup. For all PTAL samples, data description and interpretation are presented. For some chosen examples, color composite images and spectra are presented as well. A comparison with characterizations by NIR and Raman spectrometry is discussed for some of the samples. In particular, the spectral imaging capacity of MicrOmega allows detections of mineral components and potential organic molecules that were not possible with other one-spot techniques. In addition, it enables estimation of heterogeneities in the spatial distribution of various mineral species. The MicrOmega/PTAL data shall support the future observations and analyses performed by MicrOmega/Rosalind Franklin instrument.
行星陆地类比物库(PTAL)项目旨在建立并利用一个包含多种分析技术的数据库,以帮助描述陆地天体的矿物学演化,首先从火星开始。已从选定地点采集了约100个天然地球岩石样本,以收集各种火星地质的类比物,从火山成因到沉积成因,具有不同程度的蚀变。所有样本将在PTAL项目中使用不同的矿物学和元素分析技术进行表征,包括火星表面实际和未来仪器所采用的技术(近红外[NIR]光谱、拉曼光谱和激光诱导击穿光谱)。本文介绍了利用ExoMars MicrOmega备用仪器获得的近红外测量结果和解释。MicrOmega是一台近红外高光谱显微镜,安装在ExoMars火星车“罗莎琳德·富兰克林”号的分析实验室中。所有PTAL样本都使用专门设置通过MicrOmega至少观测了一次。文中给出了所有PTAL样本的数据描述和解释。对于一些选定的示例,还展示了彩色合成图像和光谱。讨论了部分样本近红外光谱法和拉曼光谱法表征结果的比较。特别是,MicrOmega的光谱成像能力能够检测到其他单点技术无法检测到的矿物成分和潜在有机分子。此外,它还能估计各种矿物种类空间分布的不均匀性。MicrOmega/PTAL数据将为未来由MicrOmega/罗莎琳德·富兰克林仪器进行的观测和分析提供支持。