地球深层地幔中原始水的证据
Lydia J Hallis1, Gary R Huss2, Kazuhide Nagashima3
1NASA Astrobiology Institute, Institute for Astronomy, University of Hawai'i, 2680 Woodlawn Drive, Honolulu, HI 96822-1839, USA. Hawai'i Institute of Geophysics and Planetology, Pacific Ocean Science and Technology (POST) Building, University of Hawai'i, 1680 East-West Road, Honolulu, HI 96822, USA. lydia.hallis@glasgow.ac.uk.
概括
地球的深层地幔具有较低的/ (D/H) 比率,这表明它保留了原始水的特征. 这一发现有助于限制地球水的起源,而不是表面的水库.
科学领域:
- 地质化学
- 宇宙化学
- 星球科学
背景情况:
- 地球水库中的/ (D/H) 比率对于了解地球水源至关重要.
- 地球的海洋可能不会反映原始的D/H比率,因为水在表面和深层之间循环.
- 来自一个深处的隔离水库的D/H比率需要确定地球的原始水位.
研究的目的:
- 在深层岩中研究/ (D/H) 的比率.
- 找出一个潜在的储备, 保存地球的原始D/H签名.
- 限制地球水源的使用.
主要方法:
- 在巴芬岛和冰岛的火山岩中分析同位素 (D/H) 比率.
- 在深层地幔衍生样本中测量 δD 值.
主要成果:
- 来自巴芬岛和冰岛的岩具有较低的D/H比率 (δD比-218每毫米负).
- 这些强烈负的δD值表明深层地幔成分具有独特的D/H特征.
结论:
- 深层地幔包含一个D/H比率直接从原太阳星云中继承的组成部分.
- 这种深层地幔水库比表面海洋更准确地代表了地球的原始水.
- 这些发现对地球水的积累和演化模型有重大影响.
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