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What is Stellar Evolution: Life Cycle of Stars about?

Stars do not live forever due to the depletion of nuclear fuel, with low-mass stars like red dwarfs living the longest. Astronomers study stars at various life stages to understand stellar evolution, while the Sun can burn hydrogen for about 10 billion years before becoming a red giant. High-mass stars evolve differently, fusing heavier elements and ending in supernovae, while low-mass stars become white dwarfs after shedding their outer layers.

Author

garybantangjr

Language

EN