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Updated: Dec 8, 2025

Simulation of Early Earth Hydrothermal Chimneys in a Thermal Gradient Environment
Published on: February 27, 2021
Fumarolic-like activity on carbonaceous chondrite parent body.
Clément Ganino1, Guy Libourel2,3
1Université Côte d'Azur, OCA, CNRS, IRD, Géoazur, 250 rue Albert Einstein, Sophia-Antipolis, 06560 Valbonne, France. ganino@unice.fr.
The Kudryavy volcano environment mirrors asteroid metasomatism, revealing how early solar system materials formed. This study links terrestrial volcanic processes to the origins of carbonaceous chondrite asteroids.
Area of Science:
- Comparative planetology
- Planetary science
- Geochemistry
Background:
- Comparative planetology is crucial for understanding planetary formation and evolution.
- Pristine asteroids are difficult to study due to collisional comminution over billions of years.
Purpose of the Study:
- To identify a terrestrial analog for metasomatic processes on asteroid parent bodies.
- To understand the formation of secondary silicates in carbonaceous chondrites.
Main Methods:
- Analysis of textural, mineralogical, chemical, and thermodynamic similarities.
- Comparison between Kudryavy volcano fumarolic environment and CV/CO carbonaceous chondrites.
Main Results:
- The Kudryavy volcano's high-temperature fumarolic environment is a likely proxy for Fe-alkali-halogen metasomatism on CV and CO chondrite parent bodies.
- Secondary silicates in CV and CO chondrites are inferred to be fumarolic-like incrustations.
- These incrustations precipitated from hydrothermal vapors interacting with wallrocks.
Conclusions:
- Terrestrial volcanic environments can serve as analogs for understanding early solar system processes.
- Hydrothermal vapor interactions are key to the formation of secondary minerals in carbonaceous chondrites.
- The origin of these vapors is linked to devolatilization of chondritic material or cooling nebular gases.
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