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球粒陨石的钡、钕和钐同位素非均质性与早期地球分异

Chondrite barium, neodymium, and samarium isotopic heterogeneity and early Earth differentiation.

作者信息

Carlson Richard W, Boyet Maud, Horan Mary

机构信息

Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, NW, Washington, DC 20015, USA.

出版信息

Science. 2007 May 25;316(5828):1175-8. doi: 10.1126/science.1140189.

Abstract

Isotopic variability in barium, neodymium, and samarium in carbonaceous chondrites reflects the distinct stellar nucleosynthetic contributions to the early solar system. We used 148Nd/144Nd to correct for the observed s-process deficiency, which produced a chondrite 146Sm-142Nd isochron consistent with previous estimates of the initial solar system abundance of 146Sm and a 142Nd/144Nd at average chondrite Sm/Nd ratio that is lower than that measured in terrestrial rocks by 21 +/- 3 parts per million. This result strengthens the conclusion that the deficiency in 142Nd in chondrites relative to terrestrial rocks reflects 146Sm decayand earlyplanetary differentiation processes.

摘要

碳质球粒陨石中钡、钕和钐的同位素变化反映了不同恒星核合成对早期太阳系的贡献。我们使用148Nd/144Nd来校正观测到的s过程亏损,这产生了一个球粒陨石146Sm-142Nd等时线,与先前对太阳系初始146Sm丰度的估计一致,并且在平均球粒陨石Sm/Nd比下的142Nd/144Nd低于在地球岩石中测量值21±3 ppm。这一结果强化了以下结论:球粒陨石中相对于地球岩石的142Nd亏损反映了146Sm衰变和早期行星分化过程。

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