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Updated: Jun 10, 2025

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Simulation of the Planetary Interior Differentiation Processes in the Laboratory
Published on: November 15, 2013
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Primitive asteroids as a major source of terrestrial volatiles
Rayssa Martins1,2, Elin M Morton1, Sven Kuthning1
1Department of Earth Science & Engineering, Imperial College London, London, UK.
Science Advances
|October 11, 2024
Summary
Earth
Area of Science:
- Planetary Science
- Geochemistry
- Isotope Cosmochemistry
Background:
- The origin of Earth's volatile elements, such as zinc (Zn), is a significant scientific debate.
- Previous studies on meteorite zinc isotope compositions suggested extraterrestrial origins but often excluded key planetary building blocks.
Purpose of the Study:
- To investigate the mass-independent zinc isotope compositions of meteorites from differentiated planetesimals.
- To model the contribution of different meteorite types to Earth's zinc budget and isotopic signature.
Main Methods:
- Analysis of mass-independent zinc isotope compositions in meteorites from differentiated planetesimals.
- Development and application of mixing models to simulate Earth's volatile element accretion.
Main Results:
- Meteorites from differentiated planetesimals, despite forming ~70% of Earth's mass, contributed only ~10% of its zinc.
- Primitive, unmelted materials were the primary source of Earth's zinc and other volatile elements.
Conclusions:
- Differentiated planetesimals were not the main source of Earth's zinc.
- Accretion of unmelted, primitive materials is crucial for establishing the volatile element inventories of terrestrial planets.
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