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Testing the ability of the ExoMars 2018 payload to document geological context and potential habitability on Mars

机译:测试ExoMars 2018有效载荷记录火星的地质背景和潜在可居住性的能力

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摘要

The future ExoMars rover mission (ESA/Roscosmos), to be launched in 2018, will investigate the habitability of the Martian surface and near subsurface, and search for traces of past life in the form of textural biosignatures and organic molecules. In support of this mission, a selection of relevant Mars analogue materials has been characterised and stored in the International Space Analogue Rockstore (ISAR), hosted in Orleans, France. Two ISAR samples were analysed by prototypes of the ExoMars rover instruments used for petrographic study. The objective was to determine whether a full interpretation of the rocks could be achieved on the basis of the data obtained by the ExoMars visible-IR imager and spectrometer (MicrOmega), the close-up imager (CLUPI), the drill infrared spectrometer (Ma_Miss) and the Raman spectrometer (RLS), first separately then in their entirety. In order to not influence the initial instrumental interpretation, the samples were sent to the different teams without any additional information. This first step was called the "Blind Test" phase. The data obtained by the instruments were then complemented with photography of the relevant outcrops (as would be available during the ExoMars mission) before being presented to two geologists tasked with the interpretation. The context data and photography of the outcrops and of the samples were sufficient for the geologists to identify the rocks. This initial identification was crucial for the subsequent, iterative interpretation of the spectroscopic data. The data from the different spectrometers was, thus, cross-calibrated against the photographic interpretations and against each other. In this way, important mineralogical details, such as evidence of aqueous alteration of the rocks, provided relevant information concerning potential habitable conditions. The final conclusion from this test is that, when processed together, the ExoMars payload instruments produce complementary data allowing reliable interpretation of the geological context and potential for habitable environments. This background information is fundamental for the analysis and interpretation of organics in the processed Martian rocks. (C) 2015 Elsevier Ltd. All rights reserved.
机译:将于2018年启动的未来ExoMars火星探测器任务(ESA / Roscosmos)将调查火星表面和近地下的可居住性,并以纹理生物签名和有机分子的形式寻找过去的生活痕迹。为了支持这一任务,对一些相关的火星模拟材料进行了表征,并将其存储在法国奥尔良举办的国际空间模拟岩石商店(ISAR)中。通过用于岩石学研究的ExoMars漫游车仪器的原型分析了两个ISAR样品。目的是根据ExoMars可见红外成像仪和光谱仪(MicrOmega),近距离成像仪(CLUPI),钻探红外光谱仪(Ma_Miss)获得的数据来确定是否可以对岩石进行全面解释)和拉曼光谱仪(RLS),然后分别将其完整。为了不影响初始乐器解释,将样本发送到不同的团队,而无需任何其他信息。第一步称为“盲测”阶段。然后,将仪器获得的数据与有关露头的照相相结合(在ExoMars任务期间将可用),然后提供给负责解释的两名地质学家。地质数据和露头以及样品的背景数据和照片足以使地质学家识别出岩石。最初的识别对于光谱数据的后续迭代解释至关重要。因此,将来自不同光谱仪的数据与照片的解释并相互进行交叉校准。这样,重要的矿物学细节(例如岩石含水变化的证据)提供了有关潜在宜居条件的相关信息。该测试的最终结论是,将ExoMars有效载荷仪器一起处理时,会产生互补数据,从而可以可靠地解释地质背景和潜在居住环境。这些背景信息对于分析和解释火星岩石中的有机物至关重要。 (C)2015 Elsevier Ltd.保留所有权利。

著录项

  • 来源
    《Planetary and space science》 |2015年第4期|87-97|共11页
  • 作者单位

    CNRS, Ctr Biophys Mol, UPR 4301, F-45071 Orleans, France|Univ Orleans, ISTO, UMR 7327, F-45071 Orleans, France|CNRS INSU, ISTO, UMR 7327, F-45071 Orleans, France|Bur Rech Geol & Minieres, ISTO, UMR 7327, F-45071 Orleans, France;

    Univ Orleans, ISTO, UMR 7327, F-45071 Orleans, France|CNRS INSU, ISTO, UMR 7327, F-45071 Orleans, France|Bur Rech Geol & Minieres, ISTO, UMR 7327, F-45071 Orleans, France;

    Univ Orleans, ISTO, UMR 7327, F-45071 Orleans, France|CNRS INSU, ISTO, UMR 7327, F-45071 Orleans, France|Bur Rech Geol & Minieres, ISTO, UMR 7327, F-45071 Orleans, France;

    CNRS, Ctr Biophys Mol, UPR 4301, F-45071 Orleans, France;

    Unidad Asociada UVa, CSIC, Ctr Astrobiol, E-47151 Valladolid, Spain;

    INAF IAPS Inst Space Astrophys & Planetol, Rome, Italy;

    Space Explorat Inst, CH-2002 Neuchatel, Switzerland;

    Unidad Asociada UVa, CSIC, Ctr Astrobiol, E-47151 Valladolid, Spain;

    Unidad Asociada UVa, CSIC, Ctr Astrobiol, E-47151 Valladolid, Spain;

    Unidad Asociada UVa, CSIC, Ctr Astrobiol, E-47151 Valladolid, Spain;

    Unidad Asociada UVa, CSIC, Ctr Astrobiol, E-47151 Valladolid, Spain;

    Space Explorat Inst, CH-2002 Neuchatel, Switzerland;

    Space Explorat Inst, CH-2002 Neuchatel, Switzerland;

    Univ Calif Los Angeles IGPP, Los Angeles, CA USA;

    INAF IAPS Inst Space Astrophys & Planetol, Rome, Italy;

    ENEA, UTMEA TER, Rome, Italy;

    INAF IAPS Inst Space Astrophys & Planetol, Rome, Italy;

    ESA ESTEC, Noordwijk, Netherlands;

    CNRS, Ctr Biophys Mol, UPR 4301, F-45071 Orleans, France;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    ExoMars; Mars; ISAR; VNIR and Raman Spectroscopy, MicrOmega; Ma_Miss and RLS; Geology;

    机译:ExoMars;Mars;ISAR;VNIR和拉曼光谱;MicrOmega;Ma_Miss和RLS;地质;

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