The astrophysics micro-course aims to introduce various concepts of astrophysics such as stellar evolution, the fate of stars, and the HR diagram. Study the properties of a star, Hydrostatic Equilibrium, variation of pressure, temperature, and mass of a star as a function of the radial vector. Luminosity and magnitude calculations. Learn the methods of distance measurement like parallax, and distance-magnitude. Study the techniques such as spectroscopy, and photometry.

The aim of this project is to introduce Mathematical Modeling, parameterize the star formation process and analyze a star formation body, and compare the theoretical results with the actual data. We perform techniques such as stationary point analysis, eigenvector analysis, etc. to study the star-forming body through some reasonable assumptions and obtain the results. Toward the end, we will show how the data obtained through the equations match with the current data.