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  • Hydrogen and Helium: The Core Elements of Main Sequence Stars
    The two most abundant elements in a main sequence star are:

    1. Hydrogen (H): This makes up roughly 70% of the star's mass.

    2. Helium (He): This makes up about 28% of the star's mass.

    These elements are the primary fuel for nuclear fusion in the star's core, which generates the energy that makes stars shine.

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