The name of the process through which stars are formed is called stellar nucleosynthesis. This process occurs in giant molecular clouds where dense regions collapse under their own gravity, leading to the formation of stars. As the core temperature rises, nuclear fusion begins, converting hydrogen into helium and releasing a vast amount of energy. This energy influences the star's lifecycle and ultimately contributes to the synthesis of heavier elements. Stellar nucleosynthesis not only accounts for the birth of stars but also plays a crucial role in enriching the universe with elements necessary for planetary and biological formation.