Update on the 53Mn-53Cr ages of dolomite in the Ivuna CI chondrite and asteroid Ryugu sample

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Shingo Sugawara , Wataru Fujiya , Noriyuki Kawasaki , Naoya Sakamoto , Akira Yamaguchi , Hisayoshi Yurimoto
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引用次数: 0

Abstract

Aqueous alteration in planetesimals is one of the earliest geological processes in the solar system. The timing of aqueous alteration sheds light on the timescale of material evolution through water–rock interaction in small bodies. The 53Mn-53Cr decay system, where a short-lived radionuclide 53Mn decays to 53Cr with a half-life of 3.7 Myr, is a powerful tool for dating carbonates in primitive meteorites that formed during aqueous alteration. In CI chondrites and samples returned from asteroid Ryugu, a major carbonate mineral is dolomite (CaMg(CO3)2) and could be dated precisely because of their relatively high Mn abundances. However, the lack of a proper dolomite standard for secondary ion mass spectrometry (SIMS) hinders us from obtaining accurate Mn/Cr ratios of carbonates, resulting in erroneous formation ages. In this work, we synthesized Mn-, Cr-, and Fe-bearing crystalline dolomite as standard materials and evaluated the relative sensitivity factor (RSF) of Mn/Cr for SIMS analysis, namely, the ratio of Mn/Cr obtained using SIMS to true Mn/Cr. We found that the RSF values of the dolomite standards range from 0.8 to 0.9, slightly higher than that of calcite (CaCO3) (∼0.7), and increase with their Fe contents. We used the newly evaluated RSF values to date dolomite in the Ivuna CI chondrite and obtained an initial 53Mn/55Mn ratio of (3.95 ± 0.49) × 10−6 (95 % confidence interval) and the corresponding absolute age of 4564.0 + 0.6/−0.7 Ma. Our new initial 53Mn/55Mn ratio is 26 ± 19 % higher than that obtained by a previous study for the same dolomite grain using a calcite standard. This difference is consistent with the difference between the RSF values of dolomite and calcite. Based on these results, we updated the initial 53Mn/55Mn ratio previously reported for dolomite in the Ryugu sample A0058 to be (3.21 ± 0.66) × 10−6, which corresponds to an absolute age of 4562.8 + 1.0/−1.2 Ma. This age seems to be the best estimate for the formation age of dolomite in Ryugu currently available.

伊武纳CI软玉和小行星龙宫样本中白云石的53Mn-53Cr年龄的最新情况
类星体的水蚀变化是太阳系最早的地质过程之一。水蚀变的时间揭示了小天体中通过水-岩石相互作用进行物质演化的时间尺度。在锰-铬衰变系统中,短寿命放射性核素锰以 3.7 Myr 的半衰期衰变为铬,这是确定在水蚀变过程中形成的原始陨石中碳酸盐的年代的有力工具。在 CI 陨石和从小行星龙宫(Ryugu)返回的样本中,主要的碳酸盐矿物是白云石(CaMg(CO)),由于其锰丰度相对较高,因此可以对其进行精确的年代测定。然而,由于缺乏用于二次离子质谱分析(SIMS)的白云石标准,我们无法获得碳酸盐的准确锰/铬比值,从而导致错误的形成年龄。在这项工作中,我们合成了含锰、铬和铁的结晶白云石作为标准物质,并评估了用于 SIMS 分析的 Mn/Cr 相对灵敏度因子(RSF),即利用 SIMS 获得的 Mn/Cr 与真实 Mn/Cr 之比。我们发现白云石标准物质的 RSF 值在 0.8 至 0.9 之间,略高于方解石(CaCO)的 RSF 值(∼0.7),并且随着铁含量的增加而增加。我们使用新评估的RSF值来确定伊武纳CI软玉中白云石的年代,得到的初始锰/锰比值为(3.95 ± 0.49) × 10(置信区间为95%),相应的绝对年龄为4564.0 + 0.6/-0.7 Ma。我们的新初始锰/锰比值比之前使用方解石标准对同一白云岩晶粒进行研究得出的结果高出 26 ± 19 %。这一差异与白云石和方解石的 RSF 值之间的差异是一致的。根据这些结果,我们将之前报告的龙宫样本 A0058 中白云石的初始锰/锰比值更新为 (3.21 ± 0.66) × 10,对应的绝对年龄为 4562.8 + 1.0/-1.2 Ma。这个年龄似乎是目前对龙宫白云石形成年龄的最佳估计。
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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