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  • Protostar to Star: Understanding the Ignition of Nuclear Fusion
    The onset of nuclear fusion marks the change of a protostar into a star.

    Here's why:

    * Protostars are massive clouds of gas and dust that are collapsing under their own gravity. They are very hot, but not hot enough for nuclear fusion to occur.

    * Nuclear fusion is the process where atomic nuclei combine to form heavier nuclei, releasing tremendous amounts of energy.

    * When a protostar's core reaches a temperature of about 10 million Kelvin, the pressure and density are high enough for hydrogen nuclei to fuse into helium nuclei. This process is called hydrogen burning.

    * The energy released by nuclear fusion creates outward pressure that balances the inward pull of gravity. This marks the birth of a true star.

    So, the moment nuclear fusion begins in the core of a protostar is the moment it transitions into a star.

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