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  • Nuclear Fusion: Combining Atomic Nuclei for Energy
    The reaction in which small nuclei combine to form a heavier nucleus is called nuclear fusion.

    Here's a breakdown:

    * Fusion: The process of combining two or more atomic nuclei to form one or more different atomic nuclei and subatomic particles (neutrons or protons).

    * Small nuclei: Typically refers to isotopes of light elements like hydrogen (deuterium and tritium) or helium.

    * Heavier nucleus: The resulting nucleus is larger and heavier than the original nuclei.

    Key characteristics of nuclear fusion:

    * Releases enormous energy: This is due to the conversion of mass into energy, as described by Einstein's famous equation E=mc².

    * Requires extremely high temperatures and pressures: These conditions are necessary to overcome the electrostatic repulsion between positively charged nuclei.

    * Occurs naturally in stars: Fusion is the energy source of stars, including our Sun.

    Examples of fusion reactions:

    * Deuterium-tritium fusion: This reaction is used in experimental fusion reactors and is the most promising for future energy production.

    * Proton-proton chain: This is the primary fusion reaction occurring in the Sun.

    Let me know if you would like more information about nuclear fusion or specific aspects of it!

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