地球的早期大陆地是由潮湿和氧化弧形岩形成的
Rong-Feng Ge1, Simon A Wilde2, Wen-Bin Zhu3
1State Key Laboratory for Mineral Deposits Research, Institute of Continental Geodynamics, Frontiers Science Center for Critical Earth Material Cycling, School of Earth Sciences and Engineering, Nanjing University, Nanjing, People's Republic of China. gerongfeng@nju.edu.cn.
Nature
|September 27, 2023
概括
早期的地球大陆地是通过俯冲形成的,其证据是氧化,富含水的岩类似于现代的弧形. 这表明早期的板块构造和40亿年前的沉积开始.
科学领域:
- 地质科学
- 石油学
- 构造学
背景情况:
- 地球早期大陆地的形成是一个基本的地质问题.
- 了解早期地形成是资源和行星进化的关键.
- 由于分析古老的变态岩石的挑战,以前的模型受到争议.
研究的目的:
- 确定早期大陆地的岩氧气流动性 (fO2) 和水 (H2O) 含量.
- 测试潜水在早期地形成中的作用.
- 调查潜水开始的时间.
主要方法:
- 使用两台氧气计同时测量岩中的FO2和H2O含量.
- 分析了古老的花岩,它们主导着早期的大陆地.
- 与估计的岩形成深度相关的岩性质.
主要成果:
- 古代的花状岩比周围的地幔衍生的岩具有显著的氧化作用.
- 这些岩石具有高的H2O含量 (6-10%) 和高的H2O/Ce比率 (>1,000).
- 岩石中的fO2,H2O含量和H2O/Ce比率与岩石形成深度正相关.
结论:
- 观察到的岩特征强烈支持早期地形成的潜水驱动模型.
- 这些发现很难与非潜伏模型相协调.
- 在40亿至36亿年前, 岩中的二氧化和二氧化含量增加表明了沉积的开始.
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