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Organic and inorganic correlations for Northwest Africa 852 by synchrotron-based Fourier transform infrared microspectroscopy

机译:基于同步加速器的傅立叶变换红外光谱法与西北非洲852的有机和无机相关性

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Relationships between organic molecules and inorganic minerals are investigated in a single 34 mu m diameter grain of the CR2 chondrite Northwest Africa 852 (NWA) 852 with submicron spatial resolution using synchrotron-based imaging micro-FTIR spectroscopy. Correlations based on absorption strength for the various constituents are determined using statistical correlation analysis. The silicate band is found to be correlated with the hydration band, and the latter is highly correlated with stretching modes of aliphatic hydrocarbons. Spatial distribution maps show that water+ organic combination, silicate, OH, and C-H distributions overlap, suggesting a possible catalytic role of phyllosilicates in the formation of organics. In contrast, the carbonate band is anticorrelated with water+organic combination, however uncorrelated with any other spectral feature. The average ratio of asymmetric CH2 and CH3 band strengths (CH2/CH3 = 2.53) for NWA 852 is similar to the average ratio of interplanetary dust particles (similar to 2.40) and Wild 2 cometary dust particles (2.50), but it significantly exceeds that of interstellar medium objects (similar to 1.00) and several aqueously altered carbonaceous chondrites (similar to 1.40). This suggests organics of similar length/branching, and perhaps similar formation regions, for NWA 852, Wild 2 dust particles, and interplanetary dust particles. The heterogeneous spatial distribution of ratio values indicates the presence of a mixture of aliphatic organic material with different length/branching, and thus a wide range of parent body processes, which occurred before the considered grain was formed.
机译:使用基于同步加速器的成像微型FTIR光谱,在亚微米级空间分辨率的CR2球粒陨石西北非洲852(NWA)852的单个34微米直径晶粒中研究了有机分子与无机矿物之间的关系。使用统计相关分析确定基于各种成分吸收强度的相关性。发现硅酸盐带与水合带相关,而后者与脂族烃的拉伸模式高度相关。空间分布图显示水+有机物组合,硅酸盐,OH和C-H分布重叠,表明页硅酸盐在有机物形成中可能具有催化作用。相反,碳酸盐带与水+有机物组合不相关,但是与任何其他光谱特征均不相关。 NWA 852的不对称CH2和CH3带强度的平均比率(CH2 / CH3 = 2.53)与行星际尘埃颗粒(类似于2.40)和Wild 2彗星尘埃颗粒(2.50)的平均比率相似,但大大超过了该比例。星际中等天体(类似于1.00)和几种水蚀碳质球粒陨石(类似于1.40)。对于NWA 852,Wild 2尘埃颗粒和行星际尘埃颗粒,这表明有机物具有相似的长度/分支和可能相似的形成区域。比率值的异质空间分布表明存在具有不同长度/分支的脂肪族有机材料的混合物,因此存在广泛的母体过程,这是在所考虑的颗粒形成之前发生的。

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