BREAKING NEWS.... the sun is going to die!
But you still have some time. Actually, you still have about 5 billion years. So while you're waiting, stick around and learn about how the sun will die.
The sun is a giant ball. It is super hot and made up mostly of hydrogen. Gravity creates energy by squeezing it and that's what makes the sun shine.
If you've ever wondered about the sun dying, don't worry. The sun has about 5 billion years of life left. The sun is only at the halfway point of its 10 billion year life.
But the sun won't last forever just like all stars. The sun will eventually run out of hydrogen in about 5 billion years. It's just like when an engine runs out of gas, except you can't refill it.
The hydrogen in the sun will eventually run out, but while the sun is using up the hydrogen, it is making helium. Then the helium will run out, so the sun will continue to keep using up bigger elements until they run out, too.
When the hydrogen, helium and other elements run out, the sun will start to turn into a red giant and engulf Mercury, Venus, and maybe even Earth. These are the three inner planets closest to the sun.
As the sun is dying, first the hydrogen will run out. Once this happens it will still take the sun about 2 to 3 billion years to finish dying.
As it's starting to die, the yellow dwarf sun will get bigger and swallow the inner planets Mercury and Venus. Earth might get swallowed too, or else turn lifeless because of the extreme heat of the red giant.
A star like the sun grows into a red giant when it's about to die. If a star has planets like our sun, it can swallow the planets when it becomes a red giant.
The sun could possibly even swallow other planets past the Earth such as Mars when the sun becomes a red giant. Even if a planet survives, it will be changed because of the extreme heat, radiation, and powerful gravity of the red giant sun.
Next, the sun is going to shrink to a very weird star called a white dwarf. A white dwarf is still super hot, but not too bright.
It's now near the end of its lifetime. When the sun changes into a white dwarf, it will lose its outer layers and shrink. White dwarfs are not as hot as our sun.
The white dwarf will fade and become a "black dwarf". When the dying sun is a black dwarf it will not put off any light or energy. The surviving parts of our solar system will become a cold, dark place without the light, life, and energy of the sun.
I got inspired to do this project because I love space and I love the sun. So that inspired me and I hope the cool facts I discovered inspire you, too.
This picture shows what the surface of the sun looks like in the modern day. Sometimes solar flares erupt from the surface of the sun.
Our sun is constantly using up hydrogen and making helium.
In its current life stage, the sun is mostly made of hydrogen. As it uses up hydrogen, it makes more helium.
Our sun will change into a red giant in about 5 billion years.
This image compares the size of our sun on the left to the size of a small red giant (in the middle) and a large red giant (on the right).
When the sun becomes a red giant, it will consume the three planets closest to the sun: Mercury, Venus, and Earth.
This image shows what the sun will look like as white dawrf. It will be smaller and dimmer that the current sun.
This drawing gives you an idea of how much SMALLER our sun will become after it changes into a white dwarf near the end of its life cycle.
Websites about the Sun:
Books about the Sun:
The Sun by Isaac Asimov
The Sun and Other Stars by Richard Harris
Our Solar System by Seymour Simon
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