Death of the Sun
The Death of the Sun is a phenomenon that occurs when the star at the center of our Solar System runs out of fuel, causing it to collapse and eventually die. This process takes millions of years to complete and will mark the end of our Solar System as we know it. As the Sun dies, its outer layers will be blown away by a powerful stellar wind, leaving behind a dense core of matter known as a white dwarf.
Disclaimer: This summary might be generated by an AI.