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What is Stellar Evolution about?

Stars are classified by color, temperature, and brightness, with hotter stars being blue and cooler stars red. The life cycle of stars varies based on their mass, transitioning from nebula to protostar, main sequence, and eventually to red giants or supernovae, leading to white dwarfs or black holes. The Hertzsprung-Russell diagram illustrates the relationship between a star

Author

Myuu Thit Cho

Language

EN