Chandrasekhar made significant contributions to our understanding of how stars evolve, including:
* The Chandrasekhar limit: This limit defines the maximum mass a white dwarf star can have before collapsing under its own gravity.
* Stellar structure and evolution: He developed mathematical models to describe the internal structure and evolution of stars, taking into account factors like gravity, pressure, and nuclear fusion.
* White dwarf stars: He conducted extensive research on the properties and formation of white dwarf stars, the remnants of stars that have exhausted their nuclear fuel.
His work revolutionized our understanding of stellar evolution and laid the foundation for modern astrophysics.