首页> 外文期刊>Spectrochimica Acta, Part B. Atomic Spectroscopy >High-precision potassium measurements using laser-induced breakdown spectroscopy under high vacuum conditions for in situ K-Ar dating of planetary surfaces
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High-precision potassium measurements using laser-induced breakdown spectroscopy under high vacuum conditions for in situ K-Ar dating of planetary surfaces

机译:在高真空条件下使用激光诱导击穿光谱法进行高精度钾测量,以对行星表面进行原位K-Ar定年

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We conducted a series of laser induced breakdown spectroscopy (LIBS) experiments for K measurements under high vacuum conditions (10(-6) Pa) for the purpose of developing in-situ isochron type K-Ar dating instruments for planetary missions. Unlike whole rock measurement methods, isochron measurements require LIBS experiments in a vacuum chamber because simultaneous Ar isotopic measurements are necessary. However, detailed examination of detection limits and accuracy of this method at low pressures has not been examined extensively before. In this study, the capability of K measurements under high vacuum conditions was examined using LIBS. A compact Czerny-Turner type spectrometer equipped with a charge-coupled device (CCD) as a detector was employed. Twenty-three geologic standard samples were measured using the LIBS method. The second strongest K emission line at 769.89 nm was used for calibration because the strongest emission line at 766.49 nm may suffer from strong interference from another emission line. A calibration curve was constructed for K using internal normalization with the oxygen line at 777 nm and well fitted by a power-law function. Based on the prediction band method, the detection limit and the quantitation limit were estimated to be 300 and 800 ppm, respectively. The 1 sigma relative uncertainty of the K calibration was 20% for 1 wt.% K2O and 40% for 3000 ppm K2O. If the amount of Ar is measured with 15% error for the 3.5 billion years rocks containing 1 and 0.3 wt.% K2O, the K-Ar ages would be determined with 10% and 20% 1 sigma errors, respectively. This level of precision will significantly improve the current Martian chronology, which has uncertainty about a factor of two to four. These results indicate that the concentration of K can be measured quantitatively under high vacuum conditions using a combination of instruments that have previously been carried in planetary missions, which suggests the viability of building in situ isochron K-Ar dating instruments with LIBS. (C) 2015 Elsevier B.V. All rights reserved.
机译:我们进行了一系列激光诱导击穿光谱(LIBS)实验,以在高真空条件(10(-6)Pa)下进行K测量,目的是开发用于行星飞行任务的原位等时型K-Ar测年仪。与完整的岩石测量方法不同,等时测量需要在真空室内进行LIBS实验,因为必须同时进行Ar同位素测量。但是,以前在低压下对该方法的检测限和准确性的详细检查尚未广泛检查。在这项研究中,使用LIBS检查了在高真空条件下进行K测量的能力。使用紧凑的Czerny-Turner型光谱仪,其配备有电荷耦合器件(CCD)作为检测器。使用LIBS方法测量了23个地质标准样品。第二个最强的K发射线在769.89 nm处用于校准,因为在766.49 nm处最强的发射线可能会受到其他发射线的强烈干扰。使用内部归一化法(在777 nm处使用氧气线)针对K绘制校准曲线,并通过幂律函数很好地拟合。根据预测谱带法,检测极限和定量极限分别估计为300和800 ppm。 K校准的1 sigma相对不确定度对于1 wt。%K2O为20%,对于3000 ppm K2O为40%。如果对35亿年含1%和0.3%(重量)K2O的岩石的Ar含量进行15%误差测量,则确定的K-Ar年龄分别具有10%和20%1 sigma误差。这种精度水平将大大改善当前的火星年表,该年表的不确定性约为2到4倍。这些结果表明,可以使用先前在行星飞行任务中携带的仪器组合在高真空条件下定量测量K的浓度,这表明用LIBS构建原位等时K-Ar测年仪器的可行性。 (C)2015 Elsevier B.V.保留所有权利。

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