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Hyperpolarized Xenon for NMR and MRI Applications
Published on: September 6, 2012
离子同位素限制了地球地幔的对流和挥发性起源
Chris J Ballentine1, Bernard Marty, Barbara Sherwood Lollar
1Department of Earth Sciences, University of Manchester, Oxford Road, Manchester M13 9LP, UK. chris.ballentine@manchester.ac.uk
Nature
|January 7, 2005
概括
地球的原始挥发物很可能起源于日光照射的积聚物质,而不是早期的太阳星云. 地幔气体中的离子同位素揭示了这一关键差异,挑战了以前的挥发性起源模型.
科学领域:
- 地质化学 地质化学
- 行星科学 行星科学
- 同位素地质学的同位素.
背景情况:
- 了解地球原始挥发物的起源是区分太阳星云和晚期积聚模型的关键.
- 虹同位素作为地球地幔中挥发性来源的关键标记物.
研究的目的:
- 为了研究地球对流地幔中原始挥发物质的起源.
- 为了测试竞争模式的挥发性输送到早期的地球.
主要方法:
- 在岩石中的二氧化碳 (CO2) 井气体中分析离子同位素.
- 同位素特征与太阳星云和晚期积聚物质来源的比较.
主要成果:
- 在对流地幔中的离子同位素与日光体辐射的来源对齐.
- 观察到的虹同位素异质性表明了不同的地幔来源,并挑战了羽主导的挥发性供应模型.
- 贵族气体度可能会减少深层地幔挥发性流量的必要性.
结论:
- 地球对流地幔中原始挥发物的主要来源可能是晚期积聚的物质,而不是早期的太阳星云.
- 和的同位素特征指向晚期积累作为主要的挥发性传递机制.
- 目前的地幔挥发物库存模型需要根据同位素证据进行修订.
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