| 1 | To provide a working knowledge of stellar energy sources |
| 2 | To provide a working knowledge of stellar parameters and direct and indirect derived stellar parameters |
| 3 | To provide a working knowledge of formation process of stellar spectra |
| 4 | To develop a practical understanding of how to calculate the wavelengths of Balmer lines |
| 5 | To equip students with practical skills in calculating the life time of mainsequence stars |
| 6 | A practical understanding of how to calculate solar constant |
| 7 | Explaining the differences between open and global clusters |
| 8 | To provide students with a knowledge of interstellar reddening and Practical proficiency in calculating its effects on distance modulus |
| 9 | To provide a working knowledge of Secchi and Harvard classification |
| 10 | To provide a working knowledge of Hertzsprung Russell Diagram, and color-color versus magnitudes diagram |