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I–Xe systematics of the impact plume produced chondrules from the CB carbonaceous chondrites: Implications for the half-life value of 129I and absolute age normalization of 129I–129Xe chronometer

机译:炭黑球粒陨石产生的撞击羽状结构的I–Xe系统学:对129I半衰期值和129I–129Xe天文钟的绝对年龄归一化的含义

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摘要

It is inferred that magnesian non-porphyritic chondrules in the CB (Bencubbin-type) carbonaceous chondrites formed in an impact generated plume of gas and melt at 4562.49 ± 0.21 Ma () and could be suitable for the absolute age normalization of relative chronometers. Here xenon isotopic compositions of neutron irradiated chondrules from the CB chondrites Gujba and Hammadah al Hamra (HH) 237 have been analyzed in an attempt to determine closure time of their I–Xe isotope systematics. One of the HH 237 chondrules, #1, yielded a well-defined I–Xe isochron that corresponds to a closure time of 0.29 ± 0.16 Ma after the Shallowater aubrite standard. Release profiles and diffusion properties of radiogenic 129*Xe and 128*Xe, extracted from this chondrule by step-wise pyrolysis, indicate presence of two iodine host phases with distinct activation energies of 73 and 120 kcal/mol. In spite of the activation energy differences, the I–Xe isotope systematics of these two phases closed simultaneously, suggesting rapid heating and cooling (possibly quenching) of the CB chondrules. The release profiles of U-fission Xe and I-derived Xe correlate in the high temperature host phase supporting simultaneous closure of 129I–129Xe and 207Pb–206Pb systematics.The absolute I–Xe age of Shallowater standard is derived from the observed correlation between I–Xe and Pb–Pb ages in a number of samples. It is re-evaluated here using Pb–Pb ages adjusted for an updated 238U/235U ratio of 137.794 and meteorite specific U-isotope ratios. With the addition of the new data for HH 237 chondrule #1, the re-evaluated absolute I–Xe age of Shallowater is 4562.4 ± 0.2 Ma. The absolute I–Xe age of the HH 237 chondrule #1 is 4562.1 ± 0.3 Ma, in good agreement with U-corrected Pb–Pb ages of the Gujba chondrules () and HH 237 silicates ().All I–Xe data used here, and in previous estimates of the absolute age of Shallowater, are calculated using 15.7 ± 0.6 Ma value for 129I half-life. The slopes of I–Xe – Pb–Pb correlation lines plotted for different sets of samples for Shallowater normalization are always ≤1. Assuming uranium half-life values are correct; this restricts the half-life of 129I to ≤15.7 Ma.
机译:可以推断,在撞击中形成的CB(本邦宾型)碳质球粒陨石中的镁质非斑状球状陨石产生的气体羽流在4562.49±0.21 Ma()处熔化,并且可能适合相对时计的绝对年龄归一化。在这里,已经对来自CB球粒陨石Gujba和Hammadah al Hamra(HH)237的中子辐照球粒的氙同位素组成进行了分析,试图确定它们的I–Xe同位素系统的闭合时间。一种HH 237弦线,#1,产生了明确定义的I–Xe等时线,对应于hallowater aubrite标准后的关闭时间0.29±0.16 Ma。通过逐步热解从该球藻中提取的放射源 129 * Xe和 128 * Xe的释放曲线和扩散特性表明存在两个具有不同活化能的碘主体相73和120 kcal / mol。尽管活化能存在差异,但这两相的I–Xe同位素系统同时关闭,表明CB球状晶体快速加热和冷却(可能会淬灭)。 U裂变Xe和I衍生的Xe的释放曲线在高温宿主相中相关,支持同时关闭 129 I– 129 Xe和 207 Pb– 206 Pb是系统性的。Shallowater标准品的绝对I–Xe年龄是根据在多个样本中观察到的I–Xe与Pb–Pb年龄之间的相关性得出的。在此使用重新调整的 238 U / 235 U比137.794和陨石特定的U同位素比调整的Pb–Pb年龄进行重新评估。加上HH 237准则#1的新数据,重新评估的Shallowater的绝对I–Xe年龄为4562.4±0.2 Ma。 HH 237软骨#1的绝对I–Xe年龄为4562.1±0.3 Ma,与Gujba软骨()和HH 237硅酸盐()的U校正Pb–Pb年龄高度吻合。此处使用的所有I–Xe数据,并在以前对Shallowater绝对年龄的估计中,使用 129 I半衰期的15.7±0.6 Ma值进行计算。为沙洛沃特水标准化而绘制的不同样本集的I–Xe – Pb–Pb相关线的斜率始终≤1。假设铀半衰期值正确;这将 129 I的半衰期限制为≤15.7Ma。

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