首页> 外文期刊>Applied Spectroscopy: Society for Applied Spectroscopy >Quantitative Potassium Measurements with Laser-Induced Breakdown Spectroscopy Using Low-Energy Lasers: Application to In Situ K-Ar Geochronology for Planetary Exploration
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Quantitative Potassium Measurements with Laser-Induced Breakdown Spectroscopy Using Low-Energy Lasers: Application to In Situ K-Ar Geochronology for Planetary Exploration

机译:使用低能量激光激光引起的激光诱导击穿光谱的定量钾测量:应用于以行星勘探的原位K-AR地质学学。

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In situ radiogenic isotope measurements to obtain the absolute age of geologic events on planets are of great scientific value. In particular, K-Ar isochrons are useful because of their relatively high technical readiness and high accuracy. Because this isochron method involves spot-by-spot K measurements using laser-induced breakdown spectroscopy (LIBS) and simultaneous Ar measurements with mass spectrometry, LIBS measurements are conducted under a high vacuum condition in which emission intensity decreases significantly. Furthermore, using a laser power used in previous planetary missions is preferable to examine the technical feasibility of this approach. However, there have been few LIBS measurements for K under such conditions. In this study, we measured K contents in rock samples using 30mJ and 15mJ energy lasers under a vacuum condition (10(-3)Pa) to assess the feasibility of in situ K-Ar dating with lasers comparable to those used in NASA's Curiosity and Mars 2020 missions. We obtained various calibration curves for K using internal normalization with the oxygen line at 777nm and continuum emission from the laser-induced plasma. Experimental results indicate that when K2O<1.1wt%, a calibration curve using the intensity of the K emission line at 769nm normalized with that of the oxygen line yields the best results for the 30mJ laser energy, with a detection limit of 88ppm and 20% of error at 2400ppm of K2O. Futhermore, the calibration curve based on the K 769nm line intensity normalized with continuum emission yielded the best result for the 15mJ laser, giving a detection limit of 140ppm and 20% error at 3400ppm K2O. Error assessments using obtained calibration models indicate that a 4 Ga rock with 3000ppm K2O would be measured with 8% (30mJ) and 10% (15mJ) of precision in age when combined with mass spectrometry of Ar-40 with 10% of uncertainty. These results strongly suggest that high precision in situ isochron K-Ar dating is feasible with a laser used in previous and upcoming Mars rover missions.
机译:原位辐射同位素测量以获得行星上的地质事件的绝对年龄具有很大的科学价值。特别是,K-Ar等粒是有用的,因为它们的技术准备相对较高,精度高。因为这种等译等式方法涉及使用激光诱导的击穿光谱(Libs)和用质谱法同时测量的逐点κ测量,因此在高真空状态下进行Libs测量,发射强度显着降低。此外,在先前的行星任务中使用的激光功率优选考验这种方法的技术可行性。然而,在这种条件下k几乎没有LIBS测量。在本研究中,我们在真空条件下使用30MJ和15MJ能量激光测量岩石样品中的K含量(10(3)PA),以评估原位K-AR的可行性与与美国国家航空航天局的好奇心的激光器相当的激光器火星2020年任务。我们使用777nm的氧线和激光诱导的等离子体的连续发射来获得k的各种校准曲线。实验结果表明,当K2O <1.1wt%时,使用氧线的769nm的k20 <1.1wt%的校准曲线归一化,产生30mJ激光能量的最佳效果,检测限为88ppm和20% 2400ppm的K2O误差。 Futhermore,基于K 769nm线强度的校准曲线与连续发射标准化产生了15MJ激光的最佳结果,在3400ppm k2o的检出限为140ppm和20%的误差。使用获得的校准模型的错误评估表明,当与AR-40的质谱相结合时,使用8%(30MJ)和10%(15MJ)测量40ppm K2o的4Ga岩,其精度为AR-40的质谱,具有10%的不确定性。这些结果强烈表明,原位等待K-AR约会的高精度是可行的,激光器在前面的和即将到来的火星火车站任务中使用。

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