The Milky Way, Our Galaxy: Learn about other stars compared to our sun and how they will die

The video tutorial explores the lifecycle of stars, starting with our Sun, which undergoes nuclear fusion to shine. As it ages, it will become a red giant and eventually a white dwarf. More massive stars have a different path, becoming supergiants and ending in supernovae, leaving behind neutron stars or black holes. The video also highlights the role of supernovae in the galaxy, contributing to the formation of new stars and elements.

What will happen to the sun in approximately 5 billion years?

How does the fate of a massive star differ from that of a modest star like the sun?

What role do supernovae play in the creation of new stars and elements in the galaxy?