,新和同位素异质性和早期地球差异化
Richard W Carlson1, Maud Boyet, Mary Horan
1Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, NW, Washington, DC 20015, USA. carlson@dtm.ciw.edu
概括
石中的,和的同位素变化揭示了早期太阳系对恒星的各种贡献. 这项研究证实,早期的行星分化过程影响了石中的新-142 (142Nd) 水平.
科学领域:
- 太空化学 太空化学
- 同位素地球化学 同位素地球化学
- 行星科学 行星科学
背景情况:
- 碳酸保持了太阳系早期的同位素组成.
- ,和同位素提供了对恒星核合成和行星演变的见解.
- 以前的研究表明石中存在同位素异常,但它们的起源需要进一步澄清.
研究的目的:
- 为了研究碳酸中,和的同位素变异性.
- 为了确定恒星核合成对早期太阳系的贡献.
- 阐明早期行星分化的作用在塑造同位素特征中的作用.
主要方法:
- 使用148Nd/144Nd来纠正s过程的缺陷.
- 构建了一个146Sm-142Nd的同位素为chondrites.
- 混凝土中的同位素比率与陆地岩石样本进行比较.
主要成果:
- 体中的146Sm-142Nd同位素与先前对初始太阳系146Sm丰度的估计一致.
- 与陆地岩石 (21 +/- 3 ppm) 相比,测量了较低的142Nd/144Nd比率.
- 这种同位素差异归因于146Sm的衰变和早期的行星分化.
结论:
- 在Ba,Nd和Sm的同位素变化反映了新生太阳系的明星核合成输入.
- 与陆地岩石相比,在地石中观察到的142Nd缺陷是146Sm衰变的结果.
- 早期的行星分化过程在确定这些同位素差异方面发挥了重要作用.
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