Physics Institute, Space Research and Planetary Sciences, University of Bern, Bern, Switzerland.
Department of Geological Sciences, Uppsala University, Uppsala, Sweden.
J Mass Spectrom. 2020 Dec;55(12):e4660. doi: 10.1002/jms.4660.
Accurate isotope ratio measurements are of high importance in various scientific fields, ranging from radio isotope geochronology of solids to studies of element isotopes fractionated by living organisms. Instrument limitations, such as unresolved isobaric inferences in the mass spectra, or cosampling of the material of interest together with the matrix material may reduce the quality of isotope measurements. Here, we describe a method for accurate isotope ratio measurements using our laser ablation ionization time-of-flight mass spectrometer (LIMS) that is designed for in situ planetary research. The method is based on chemical depth profiling that allows for identifying micrometer scale inclusions embedded in surrounding rocks with different composition inside the bulk of the sample. The data used for precise isotope measurements are improved using a spectrum cleaning procedure that ensures removal of low quality spectra. Furthermore, correlation of isotopes of an element is used to identify and reject the data points that, for example, do not belong to the species of interest. The measurements were conducted using IR femtosecond laser irradiation focused on the sample surface to a spot size of ~12 μm. Material removal was conducted for a predefined number of laser shots, and time-of-flight mass spectra were recorded for each of the ablated layers. Measurements were conducted on NIST SRM 986 Ni isotope standard, trevorite mineral, and micrometer-sized inclusions embedded in aragonite. Our measurements demonstrate that element isotope ratios can be measured with accuracies and precision at the permille level, exemplified by the analysis of B, Mg, and Ni element isotopes. The method applied will be used for in situ investigation of samples on planetary surfaces, for accurate quantification of element fractionation induced by, for example, past or present life or by geochemical processes.
准确的同位素比测量在各个科学领域都具有重要意义,从固体的放射性同位素地质年代学到受生物影响的元素同位素分馏研究。仪器限制,如质谱中未解析的同量异位推断,或感兴趣的物质与基质材料的共采样,可能会降低同位素测量的质量。在这里,我们描述了一种使用我们设计用于原位行星研究的激光烧蚀电离飞行时间质谱仪(LIMS)进行准确同位素比测量的方法。该方法基于化学深度剖析,可以识别嵌入在样品体中不同成分的周围岩石中的微米级包裹体。使用谱线清洁程序来改善用于精确同位素测量的数据,该程序可确保去除低质量谱线。此外,通过相关同位素可以识别和剔除例如不属于感兴趣物种的数据点。测量是使用聚焦在样品表面的红外飞秒激光进行的,激光光斑尺寸约为 12 μm。材料去除是在预定义的激光射击次数内进行的,并且记录了每个烧蚀层的飞行时间质谱。在 NIST SRM 986 Ni 同位素标准品、trevorite 矿物和嵌入方解石中的微米级包裹体上进行了测量。我们的测量结果表明,可以在千分位水平上测量元素同位素比的准确度和精密度,例如 B、Mg 和 Ni 元素同位素的分析。所应用的方法将用于行星表面样品的原位研究,以准确量化例如过去或现在生命或地球化学过程引起的元素分馏。