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- After millions of years, both of our stars are now in the main sequence phase. Junior is now starting to fuse hydrogen atoms to form helium atoms right into our star's core. Junior has an estimated 10 billion years before our star will exit the main sequence phase.
- On the other hand, there goes our second star, senior who is now bigger compared to way back millions of years. Just like junior, our star is also fusing hydrogen atoms to form helium atoms. But unlike our first star, senior is only expected to have an estimated 20 million years due to its size and extent.
- Now moving on, both of these stars, impact our society today. They provide energy, and they are also the ones responsible for having life on Earth in the first place. These stars can also be seen in the history of mankind where they are connected to superstition things.
- After we adapted to the changes and harnessed their energy, the power that they give now supplies the current technology that we have, further improving our civilization. Stars also serve as a moral inspiration for us to just shine and glow, just like Junior and Senior.
- Now that Junior had passed the estimated lifetime our star has, it will now start to expand since the hydrogen fuel in the core ran out. Its outer layers will expand drastically making junior a red-giant.
- Oh no! What will happen next?!
- On the other hand, Senior is also experiencing the same effects just like Junior due to the hydrogen fuel in their core running out. But unlike Junior, Senior will greatly expand, bigger than Junior, making Senior a red-supergiant.
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