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Updated: Mar 31, 2026

A Simple, Low-cost, and Robust System to Measure the Volume of Hydrogen Evolved by Chemical Reactions with Aqueous Solutions
Published on: August 17, 2016
Experimental quantification of hydrogen content in the Earth's core
Dongyang Huang1,2, Motohiko Murakami3, Stephan Gerstl4
1SKLab-DeepMinE, MOEKLab-OBCE, School of Earth and Space Sciences, Peking University, Beijing, China. dhuang@pku.edu.cn.
Earth's core may hold vast amounts of hydrogen, equivalent to 9-45 oceans of water. This suggests Earth acquired most of its water during formation, not from comets.
Area of Science:
- Geochemistry
- Planetary Science
- High-Pressure Mineral Physics
Background:
- Earth's core is hypothesized as a major hydrogen reservoir.
- Quantifying core hydrogen is challenging due to extreme conditions.
Purpose of the Study:
- To quantify hydrogen (H) content in Earth's core.
- To investigate hydrogen sequestration mechanisms during core formation.
Main Methods:
- Superliquidus metal-silicate partitioning experiments using laser-heated diamond anvil cells.
- Atom probe tomography for direct H observation.
Main Results:
- Direct observation of hydrogen associated with silicon- and oxygen-rich nanostructures in iron alloys.
- Evidence for coupled sequestration of Si, O, and H during core formation.
- Estimated core hydrogen content of 0.07-0.36 wt.%, equivalent to 9-45 oceans of water.
Conclusions:
- Earth's core likely contains a significant amount of hydrogen.
- The observed Si/H ratio suggests a specific sequestration mechanism.
- This finding implies Earth primarily gained its water during accretion, not via cometary impacts.
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