stjärnutvecklingen
Stjärnutvecklingen, or stellar evolution, is the process by which a star changes over time, from its formation to its death. This process is governed by the principles of nuclear physics, astrophysics, and fluid dynamics.
The life of a star begins with the collapse of a molecular cloud, triggered by the gravitational
As the star ages, it begins to fuse helium into heavier elements, such as carbon and oxygen.
Eventually, the star's core will run out of fuel, and it will no longer be able to
Stellar evolution is a complex process that is influenced by a star's initial mass, composition, and other