Suppr超能文献

德卢斯辉长岩的铷-锶共振电离地质年代学:月球原位测年的概念验证。

Rb-Sr resonance ionization geochronology of the Duluth Gabbro: A proof of concept for in situ dating on the Moon.

作者信息

Anderson F Scott, Levine Jonathan, Whitaker Tom J

机构信息

Southwest Research Institute, Suite 300, 1050 Walnut St, Boulder, CO, 80302, USA.

Department of Physics and Astronomy, Colgate University, Hamilton, NY, 13346, USA.

出版信息

Rapid Commun Mass Spectrom. 2015 Aug 30;29(16):1457-64. doi: 10.1002/rcm.7253.

Abstract

RATIONALE

We report new (87) Rb-(87) Sr isochron data for the Duluth Gabbro, obtained with a laser ablation resonance ionization mass spectrometer that is a prototype spaceflight instrument. The gabbro has a Rb abundance and a range of Rb/Sr ratios that are similar to those of KREEP-rich basalts found on the nearside of the Moon. Dating of previously un-sampled young lunar basalts, which generally have a KREEP-rich composition, is critical for understanding the bombardment history of the Moon since 3.5 Ga, which in turn informs the chronology of the solar system. Measurements of lunar analogs like the Duluth Gabbro are a proof of concept for in situ dating of rocks on the Moon to constrain lunar history.

METHODS

Using the laser ablation resonance ionization mass spectrometer we ablated hundreds of locations on a sample, and at each one measured the relative abundances of the isotopes of Rb and Sr. A delay between the resonant photoionization processes separates the elements in time, eliminating the potential interference between (87) Rb and (87) Sr. This enables the determination of (87) Rb-(87) Sr isochron ages without sophisticated sample preparation that would be impractical in a spaceflight context.

RESULTS

We successfully dated the Duluth Gabbro to 800 ± 300 Ma using traditional isochron methods like those used in our earlier analysis of the Martian meteorite Zagami. However, we were able to improve this to 1100 ± 200 Ma, an accuracy of <1σ, using a novel normalization approach. Both these results agree with the age determined by Faure et al. in 1969, but our novel normalization improves our precision.

CONCLUSIONS

Demonstrating that this technique can be used for measurements at this level of difficulty makes ~32% of the lunar nearside amenable to in situ dating, which can complement or supplement a sample return program. Given these results and the scientific value of dating young lunar basalts, we have recently proposed a spaceflight mission called the Moon Age and Regolith Explorer (MARE).

摘要

原理

我们报告了德卢斯辉长岩新的(87)Rb - (87)Sr等时线数据,这些数据是用一种作为航天飞行仪器原型的激光烧蚀共振电离质谱仪获得的。该辉长岩的铷丰度以及铷/锶比值范围与在月球近侧发现的富含钾、稀土元素和磷的玄武岩相似。对以前未采样的年轻月球玄武岩进行年代测定至关重要,这些玄武岩通常富含钾、稀土元素和磷,这有助于理解自35亿年前以来月球的撞击历史,进而为太阳系的年表提供信息。对像德卢斯辉长岩这样的月球类似物进行测量是对月球岩石进行原位年代测定以约束月球历史的概念验证。

方法

使用激光烧蚀共振电离质谱仪,我们在一个样本上烧蚀了数百个位置,并在每个位置测量了铷和锶同位素的相对丰度。共振光电离过程之间的延迟在时间上分离了元素,消除了(87)Rb和(87)Sr之间的潜在干扰。这使得在无需复杂样品制备的情况下就能确定(87)Rb - (87)Sr等时线年龄,而这种复杂样品制备在航天飞行环境中是不切实际的。

结果

我们使用传统等时线方法成功测定德卢斯辉长岩的年龄为800±300百万年,就如同我们早期对火星陨石扎加米的分析中所使用的方法一样。然而,通过一种新颖的归一化方法,我们能够将其精度提高到1100±200百万年,误差小于1σ。这两个结果都与福尔等人在1969年确定的年龄一致,但我们新颖的归一化方法提高了精度。

结论

证明这种技术可用于在这种难度水平下进行测量,使得约32%的月球近侧区域适合进行原位年代测定,这可以补充或完善样本返回计划。鉴于这些结果以及对年轻月球玄武岩进行年代测定的科学价值,我们最近提出了一项名为月球年龄与风化层探测器(MARE)的航天飞行任务。

文献AI研究员

20分钟写一篇综述,助力文献阅读效率提升50倍。

立即体验

用中文搜PubMed

大模型驱动的PubMed中文搜索引擎

马上搜索

文档翻译

学术文献翻译模型,支持多种主流文档格式。

立即体验