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  • The Sun's Evolution: Understanding the Red Giant Phase
    The next stage in our Sun's evolution is the red giant phase. This will happen in about 5 billion years. Here's a breakdown of what will happen:

    * Hydrogen Fuel Depletion: As the Sun continues to fuse hydrogen into helium in its core, the core will eventually run out of hydrogen fuel.

    * Core Contraction: Without the outward pressure of hydrogen fusion, the Sun's core will begin to contract under its own gravity.

    * Helium Fusion: The core's contraction will increase temperature and pressure, eventually reaching a point where helium fusion can begin.

    * Expansion and Cooling: The helium fusion will cause the outer layers of the Sun to expand dramatically, transforming it into a red giant. The Sun will become much larger and cooler, its surface temperature dropping to about 3,000 K (compared to its current 5,500 K).

    * Swallowing Planets: The Sun will expand so much that it will engulf Mercury, Venus, and likely Earth.

    Important note: The red giant phase is just the beginning of a series of changes. The Sun will eventually shed its outer layers, forming a planetary nebula. The remaining core will become a white dwarf, a dense, hot object that slowly cools over billions of years.

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