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  • Understanding Stellar Lifecycles: The Main Sequence Explained
    A star spends most of its lifetime on the main sequence of the Hertzsprung-Russell (H-R) diagram.

    Here's why:

    * Main Sequence: This is the stage where a star fuses hydrogen into helium in its core, generating energy and producing light and heat. This is a stable and long-lasting process.

    * Other Stages: The time spent in other stages, like red giant, white dwarf, or supernova, is relatively short compared to the main sequence.

    Think of it like this: Imagine a star's life as a journey. The main sequence is the long, steady highway, while the other stages are brief detours or destinations at the end of the journey.

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