原始虹和Kimberlites的深层地幔起源
Andrea Giuliani1,2,3, Mark D Kurz4, Peter H Barry4
1Department of Earth and Planetary Sciences, ETH Zurich, Zurich, Switzerland. agiuliani@carnegiescience.edu.
Nature communications
|April 5, 2025
概括
金伯石,含有钻石的岩石,起源于深层地幔领域,而不是浅层. 被困液体中的离子同位素揭示了这种深层起源,为地球早期的异质性提供了洞察力.
科学领域:
- 地质化学 地质化学
- 同位素地球化学 同位素地球化学
- 地幔石化学地幔石化学
背景情况:
- 金伯石的起源,至关重要的钻石来源,仍在争论中,问题是它们来自深远的古代地幔还是浅层的对流地幔.
- 了解金伯莱特的起源对于经济钻石勘探和理解地幔动态至关重要.
研究的目的:
- 通过分析被困在橄石中的岩液体的同位素组成来调查金伯石的起源.
- 为了确定金伯利特是否进入古老的,深层地幔水库或浅层的来源.
主要方法:
- 分析 (He), (Ne) 和 (Ar) 的同位素组成.
- 从全球金石样本中检查橄石晶体内的岩液体含有物的检查.
- 评估同位素特征,以追踪地幔来源并确定潜在的污染.
主要成果:
- 岩石受到潜水或元体变化的影响较小,其核生成性Ne同位素比上层地幔少,表明其起源于深层地幔.
- 同位素被确定为板内部岩层中深层地幔贡献的强大的标记物,由于较少的重印,其性能优于同位素.
- 证据支持深层地幔来源,由W同位素异常和热点轨道位置证实.
结论:
- 金伯石主要来自深层地幔领域,挑战浅层地幔羽毛或板块构造学模型的起源.
- 这项研究强调了Ne同位素在揭示深层地幔异质性和早期地球遗迹方面的重要性.
- 这些发现有助于更精细地了解地幔过程和钻石岩的形成.
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