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Star Life Cycle: Sun-like and Massive Stars by Adnan Khan is a document available to read on EtoBox.

The life cycle of stars similar in mass to the Sun begins in a nebula, evolves into a main sequence star, becomes a red giant, and finally ends as a white dwarf. In contrast, more massive stars also start in a nebula but progress to a red supergiant, undergo a supernova explosion, and can end as either a neutron star or a black hole. The key differences include the rate of nuclear fusion and the duration of each phase, with massive stars having shorter lifespans and more dramatic endings.

Author
Adnan Khan
Language
EN