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  • What Happens to the Sun at the End of Its Life? (Planetary Nebula)
    When the Sun reaches the end of its life cycle, its expanded outer layers will be released into space, forming a planetary nebula.

    Here's a breakdown:

    * Red Giant Phase: As the Sun runs out of hydrogen fuel in its core, it starts fusing helium, causing it to swell into a red giant. This expansion will engulf the inner planets, including Earth.

    * Helium Fusion and Instability: The Sun will then fuse helium into carbon and oxygen. This process is unstable and causes the Sun to pulsate, eventually ejecting its outer layers.

    * Planetary Nebula: These ejected layers form a glowing cloud of gas and dust, called a planetary nebula. The name is a bit misleading, as it has nothing to do with planets. It was given by early astronomers who observed these objects through telescopes and thought they resembled planets.

    * White Dwarf: The remaining core of the Sun will become a white dwarf, a dense, hot, and incredibly small star. This white dwarf will slowly cool down over billions of years, eventually fading away completely.

    So, the Sun's death will be a spectacular event, resulting in a beautiful and fleeting planetary nebula.

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