Stellar Evolution Modelling using MESA
Analysis of pre-main sequence contraction and stellar mass distributions using MESA.

Context
Detailed study of pre-main sequence stellar contraction and the impact of mass distributions, guided by the Initial Mass Function, involving Hertzsprung-Russell diagrams. Project conducted using the MESA (Modules for Experiments in Stellar Astrophysics) software suite.

Preview for Stellar Evolution Modelling
Key take-aways
- Core Feature 1 implementation
- Core Feature 2 development
- Key Technology stack integration
Conclusion
Discussion of the primary challenges encountered during the Stellar Evolution Modelling project and the valuable lessons learned throughout its lifecycle.
































