Which carbon-bearing gases come forward in terms of abundance or importance, throughout different zones of the Protosolar Disk modeled with different pressure and C/O ratios are demonstrated in the plots and discussed in detail.
📌 3 Key Takeaways
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Objective & Hypothesis:The target of this study is analyzing chemical composition and behavior of the Protosolar Disk modeled under diverse C/O ratios from 0.1 to 10, and pressure values from 10-2 to 10-6 bar, on the basis of changes in temperature.
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Key Findings & Data:How the C/O ratio influences general patterns of chemical functions of the disk dynamics is investigated under the equilibrium conditions.
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Conclusion & Impact:Which carbon-bearing gases come forward in terms of abundance or importance, throughout different zones of the Protosolar Disk modeled with different pressure and C/O ratios are demonstrated in the plots and discussed in detail.
🔬Design:Modeling & Simulation
📍Scope:Comprehensive Sample
⚙️Variables:protoplanetary discs · solar system · abundances
Abstract
The target of this study is analyzing chemical composition and behavior of the Protosolar Disk modeled under diverse C/O ratios from 0.1 to 10, and pressure values from 10-2 to 10-6 bar, on the basis of changes in temperature. How the C/O ratio influences general patterns of chemical functions of the disk dynamics is investigated under the equilibrium conditions. Which carbon-bearing gases come forward in terms of abundance or importance, throughout different zones of the Protosolar Disk modeled with different pressure and C/O ratios are demonstrated in the plots and discussed in detail.
Pekmezci, G. S., Mousis, O., Dıb, M. A., Lunıne, J. (2020). Protosolar Disk CO-CH4 Equilibrium Chemistry. Turkish Journal of Astronomy and Astrophysics, Cilt: 1 Sayı: 1 Özel Sayı, 319–319. https://ajindex.com/articles/1555565