Analysis of pathways for volatile-bearing mineral formation in carbonaceous chondrites using thermodynamic simulations
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- doi:10.25911/fqg9-q561
- Authors
- Baile, Riley
- Reported year
- 2026
- Reported language
- und · en_AU
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- Thesis (MPhil)
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- 2026-11-09T19:07:42.931264+00:00
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- 2026-11-09T19:07:42.931264+00:00
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Documentary abstract — original language
Low temperature minerals in carbonaceous chondrites record volatile processes in the solar system. These processes could occur via liquid-solid or gas-solid reactions; however, few studies have considered gases. A Gibbs free energy minimization approach was used to investigate the formation of the Tagish Lake meteorite's low temperature matrix including gases and liquid water, with starting compositions of low O and high O determined from its bulk composition. The high O model predicts phyllosilicate formation at <500 Degrees C, accounting for up to 24 mol% of solids and showing a similar compositional trend to observations of Tagish Lake's carbonate-rich lithology. Carbonates reached a maximum abundance of 50 mol% of solids at the lowest simulated temperature (0 Degrees C), being the most abundant group of minerals, excluding water. The low O model also formed phyllosilicates at <500 Degrees C, reaching up to ~18 mol% of solids, however carbonates were negligible. The low O phyllosilicate compositions more closely mirror the Tagish Lake's carbonate-poor lithology. The low O composition also predicts the coexistence olivine and abundant phyllosilicate for temperatures <150 Degrees C. These models indicate the importance of O in carbonaceous chondrite alteration and confirm that high and low temperature minerals could coexist in carbonaceous chondrites in a system open to gas within the parent body. Also, this model provides a method of quantifying volatile loss due to heating on an asteroid.
Identifiers
- DOI
- 10.25911/fqg9-q561
- HANDLE
- 1885/733808735
- OAI
- oai:openresearch-repository.anu.edu.au:1885/733808735
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- Thesis (MPhil)
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- Lake
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Cite this reference
Baile, Riley. Analysis of pathways for volatile-bearing mineral formation in carbonaceous chondrites using thermodynamic simulations. 2026. https://doi.org/10.25911/fqg9-q561
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- APA
- Baile, Riley. (2026). Analysis of pathways for volatile-bearing mineral formation in carbonaceous chondrites using thermodynamic simulations. https://doi.org/10.25911/fqg9-q561
- Chicago
- Baile, Riley. Analysis of pathways for volatile-bearing mineral formation in carbonaceous chondrites using thermodynamic simulations. 2026. https://doi.org/10.25911/fqg9-q561
- ISO 690
- Baile, Riley. Analysis of pathways for volatile-bearing mineral formation in carbonaceous chondrites using thermodynamic simulations. 2026. https://doi.org/10.25911/fqg9-q561
UDTR Global Rights of Nature Legal Library. Analysis of pathways for volatile-bearing mineral formation in carbonaceous chondrites using thermodynamic simulations. Documentary record: https://www.declarationuniverselledesdroitsdelarbre.org/global-rights-of-nature-radar/reference/r-5aeeb08956de00e4d037b5f15221dbaa/ · Last HTTP verification: not performed
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Version ceae358b2d1b4b40 · udtr-reference-1.1.2
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- Repository_ANU · source · 2026-11-09T19:07:42.931264+00:00
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- Repository_ANU · source · 2026-11-09T19:07:42.931264+00:00
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3bb048483de19668 · 2026-11-09T19:07:42.931264+00:00
8cead3027525245f · 2026-11-09T19:07:42.931264+00:00
71c2d5718f9b53e5 · 2026-11-09T19:07:42.931264+00:00
ceae358b2d1b4b40 · 2026-11-09T19:07:42.931264+00:00
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Bibliographic / original publication source · https://doi.org/10.25911/fqg9-q561
Bibliographic / original publication source · https://hdl.handle.net/1885/733808735
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