Cosmogenic 10Be in pyroxene: laboratory progress, production rate systematics, and application of the 10Be–3He nuclide pair in the Antarctic Dry Valleys

IF 2.7 Q2 GEOCHEMISTRY & GEOPHYSICS
A. Balter-Kennedy, J. Schaefer, R. Schwartz, J. Lamp, Laura Penrose, J. Middleton, Jeanene P. Hanley, B. Tibari, P. Blard, G. Winckler, A. Hidy, G. Balco
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Abstract

Abstract. Here, we present cosmogenic-10Be and cosmogenic-3He data from Ferrar dolerite pyroxenes in surficial rock samples and a bedrock core from the McMurdo Dry Valleys, Antarctica, with the goal of refining the laboratory methods for extracting beryllium from pyroxene, further estimating the 10Be production rate in pyroxene and demonstrating the applicability of 10Be–3He in mafic rock. The ability to routinely measure cosmogenic 10Be in pyroxene will open new opportunities for quantifying exposure durations and Earth surface processes in mafic rocks. We describe scalable laboratory methods for isolating beryllium from pyroxene, which include a simple hydrofluoric acid leaching procedure for removing meteoric 10Be and the addition of a pH 8 precipitation step to reduce the cation load prior to ion exchange chromatography. 10Be measurements in pyroxene from the surface samples have apparent 3He exposure ages of 1–6 Myr. We estimate a spallation production rate for 10Be in pyroxene, referenced to 3He, of 3.6 ± 0.2 atoms g−1 yr−1. 10Be and 3He measurements in the bedrock core yield initial estimates for parameters associated with 10Be and 3He production by negative-muon capture (f10∗=0.00183 and f3∗fCfD=0.00337). Next, we demonstrate that the 10Be–3He pair in pyroxene can be used to simultaneously resolve erosion rates and exposure ages, finding that the measured cosmogenic-nuclide concentrations in our surface samples are best explained by 2–8 Myr of exposure at erosion rates of 0–35 cm Myr−1. Finally, given the low 10Be in our laboratory blanks (average of 5.7 × 103 atoms), the reported measurement precision, and our estimated production rate, it should be possible to measure 2 g samples with 10Be concentrations of 6 × 104 and 1.5 × 104 atoms g−1 with 5 % and 15 % uncertainty, respectively. With this level of precision, Last Glacial Maximum to Late Holocene surfaces can now be dated with 10Be in pyroxene. Application of 10Be in pyroxene, alone or in combination with 3He, will expand possibilities for investigating glacial histories and landscape change in mafic rock.
辉石中宇宙成因10Be: 10Be - 3he核素对在南极干谷的实验室进展、产量系统和应用
摘要本文介绍了来自南极洲麦克默多干谷表层岩石样品和基岩岩心的ferra白云岩辉石中宇宙成因-10Be和宇宙成因- 3he的数据,目的是改进从辉石中提取铍的实验方法,进一步估计辉石中10Be的产率,并证明10Be - 3he在基性岩石中的适用性。常规测量辉石中宇宙成因10Be的能力将为量化暴露时间和基性岩石中的地球表面过程提供新的机会。我们描述了可扩展的实验室方法,用于从辉石中分离铍,其中包括一个简单的氢氟酸浸出程序,用于去除大气中的10Be,并添加pH 8沉淀步骤,以减少离子交换色谱之前的阳离子负荷。表面样品中辉石的测量结果显示,暴露年龄为1-6毫微当量。我们估计10be在辉石中(参照3He)的散裂率为3.6±0.2个原子g−1 yr−1。基岩岩心中的10Be和3He测量产生了与负介子捕获产生10Be和3He相关参数的初步估计(f10∗=0.00183和f3∗fCfD=0.00337)。接下来,我们证明了辉石中10Be-3He对可以同时用于解决侵蚀速率和暴露年龄,发现我们表面样品中测量的宇宙生成核素浓度最好解释为在0-35 cm Myr−1的侵蚀速率下2-8 Myr的暴露。最后,考虑到我们实验室空白中的低10Be(平均为5.7 × 103原子),报告的测量精度和我们估计的生产率,应该可以测量2 g样品,10Be浓度分别为6 × 104和1.5 × 104原子g−1,不确定度分别为5%和15%。在这样的精度下,末次盛冰期到全新世晚期的地表可以用辉石中的10Be测定年代。10Be在辉石中单独或与3He结合的应用,将扩大研究基性岩石的冰川历史和景观变化的可能性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Geochronology
Geochronology Earth and Planetary Sciences-Paleontology
CiteScore
6.60
自引率
0.00%
发文量
35
审稿时长
19 weeks
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