原始太阳系物质和地球共享一个共同的初始 (142) Nd 丰度
1University of Western Ontario, Department of Earth Sciences, Centre for Planetary Science and Exploration, London, Ontario N6A 3K7, Canada.
Nature
|September 16, 2016
概括
早期地球的组成与富含的耐火性含量 (CAI) 保持一致,这表明了体的Sm/Nd比率. 这解决了新-142 (142Nd) 的偏移,而不需要隐藏的储.
科学领域:
- 宇宙化学:使用- (Sm-Nd) 系统学研究早期太阳系的同位素进化.
- 行星科学:通过同位素分析限制行星和行星的早期进化.
- 地化学:分析新-142 (142Nd) 的变化,以了解行星的形成和分化.
背景情况:
- 新-142 (142Nd) 变异提供了早期行星演变的见解,源自初始磁盘分布和短暂的-146 (146Sm) 衰变.
- 之前的研究指出,体石与地球之间存在142Nd的偏移,其中包括核合成变异或早期地球差异化.
- 富含的耐火性内含物 (CAI) 和静态是重建早期太阳系同位素组成的关键材料.
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