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对寻找过去或现在火星生命的主要目标进行着陆式X射线衍射/荧光分析。

Landed XRD/XRF analysis of prime targets in the search for past or present Martian life.

作者信息

Vaniman D, Bish D, Blake D, Elliott S T, Sarrazin P, Collins S A, Chipera S

机构信息

Geology and Geochemistry, Los Alamos National Laboratory, New Mexico, USA.

出版信息

J Geophys Res. 1998 Dec 25;103(E13):31477-89. doi: 10.1029/98je01428.

Abstract

Mars landers seeking evidence for past or present life will be guided by information from orbital mapping and from previous surface exploration. Several target options have been proposed, including sites that may harbor extant life and sites most likely to preserve evidence of past life These sites have specific mineralogic characteristics. Extant life might be gathered around the sinters and associated mineral deposits of rare active fumaroles, or held within brine pockets and inclusions in a few evaporite-mineral deposits. Possibilities for fossilization include deltaic and lake-bottom sediments of once-flooded craters, sinters formed by ancient hot-spring deposits, and the carbonate deposits associated with some evaporite systems. However, the highly varied mineralogy of fossil occurrences on Earth leads to the inference that Mars, an equally complex planet, could host a broad variety of potential fossilizing deposits. The abundance of volcanic systems on Mars and evidence for close associations between volcanism and water release suggest possibilities of organism entrapment and mineralization in volcaniclastic deposits, as found in some instances on Earth. Thus the targets being considered for exploration include a wide variety of unique deposits that would be characterized by silica or various nonsilicate minerals. Beyond these "special" deposits and in the most general case, an ability to distinguish mineralized from uncemented volcanic detritus may be the key to success in finding possible fossil-bearing authigenic mineralogies. A prototype miniaturized X ray diffraction/X ray fluorescence (XRD/XRF) instrument has been evaluated with silica, carbonate, and sulfate minerals and with a basalt, to examine the capabilities of this tool in mineralogic and petrologic exploration for exobiological goals. This instrument. CHEMIN (chemical and mineralogical analyzer), is based on an innovative low-power X ray tube, transmission geometry, and CCD collection and discrimination of diffracted and fluoresced X rays. The ability to accumulate and integrate the entire circumference of each complete Debye diffraction ring compensates for poor powder preparations, as might be produced by robotic sampling systems. With CHEMIN, a wide range of minerals can be uniquely identified. Using Rietveld analysis of the XRD results, mineral quantification is also possible. Expanded capabilities in phase analysis and constrained data solutions using quantitative XRD and XRF are within reach.

摘要

寻找过去或现在生命证据的火星着陆器将依据轨道测绘和以往地表探测所获得的信息来指引。已经提出了几个目标选项,包括可能存在现存生命的地点以及最有可能保存过去生命证据的地点。这些地点具有特定的矿物学特征。现存生命可能聚集在稀有活跃喷气孔的泉华及相关矿床周围,或者存在于一些蒸发盐矿床中的盐水囊和包裹体之内。石化的可能性包括曾经被水淹没的陨石坑的三角洲和湖底沉积物、古代温泉沉积物形成的泉华,以及与一些蒸发盐系统相关的碳酸盐沉积物。然而,地球上化石出现的矿物学高度多样,由此推断,同样复杂的火星可能存在各种各样潜在的石化矿床。火星上丰富的火山系统以及火山活动与水释放之间紧密关联的证据表明,在火山碎屑沉积物中存在生物体被困和矿化的可能性,就像地球上某些情况那样。因此,正在考虑用于探索的目标包括各种各样以二氧化硅或各种非硅酸盐矿物为特征的独特矿床。除了这些“特殊”矿床,在最一般的情况下,区分矿化的和未胶结的火山碎屑的能力可能是成功找到可能含化石的自生矿物学的关键。一种微型X射线衍射/X射线荧光(XRD/XRF)仪器原型已针对二氧化硅、碳酸盐和硫酸盐矿物以及玄武岩进行了评估,以检验该工具在外星生物学目标的矿物学和岩石学探测中的能力。这种仪器,即化学与矿物分析仪(CHEMIN),基于一种创新的低功率X射线管、透射几何结构以及对衍射和荧光X射线的电荷耦合器件收集与鉴别。积累并整合每个完整德拜衍射环的整个圆周的能力弥补了机器人采样系统可能产生的粉末制备不佳的问题。借助CHEMIN,可以唯一地识别多种矿物。利用XRD结果的里特韦尔德分析,矿物定量也是可行的。利用定量XRD和XRF进行相分析和受限数据求解方面的扩展能力也指日可待。

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