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  • Helium Flash Duration: Understanding Stellar Core Reactions
    The Helium Flash in stars with masses similar to our Sun lasts for a very short time, on the order of a few minutes.

    Here's why:

    * Rapid Energy Release: The Helium Flash is a runaway nuclear reaction where helium fuses into carbon in the core of the star. This process releases an immense amount of energy very quickly.

    * Short Duration: The energy released during the Helium Flash is so intense that it causes the core of the star to expand and cool rapidly, effectively quenching the runaway reaction within a matter of minutes.

    Important Note: While the Helium Flash itself lasts only a few minutes, the process leading up to it, known as the Helium Burning Phase, can last for hundreds of thousands of years.

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