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
🎯
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.
📊
Key Findings & Data:How the C/O ratio influences general patterns of chemical functions of the disk dynamics is investigated under the equilibrium conditions.
💡
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.
PEKMEZCİ, G. S., MOUSİS, O., DIB, M. A., LUNINE, J. (2020). Protosolar Disk CO-CH4 Equilibrium Chemistry. Turkish Journal of Astronomy and Astrophysics, Cilt: 1 - Sayı: 1, 319–319. https://ajindex.com/articles/808533