Addicted to YA discussion
Games
>
The Last Person To Post Wins!
message 15051:
by
Silentmoon_8
(new)
Aug 22, 2021 09:46AM

reply
|
flag

At the core, a process called ‘nuclear fusion’ takes place. You see, stars weigh immensely more than any planet in the solar system, or in the universe, that we know of. They must weigh at least 13 times more than Jupiter, the largest planet in our solar system. That allows the gravity of the star to fuse hydrogen atoms together, forming helium.
Then it gets interesting. You see, when the star runs out of hydrogen, the whole star condenses, crushing even helium together. But, the fusion of helium atoms releases more energy than that of hydrogen. So then the star expands to tens or even hundreds of times it’s original size. That’s what awaits our star. The sun. In case you forgot. What happens next depends on the mass of the star. If it is under a certain threshold, which I believe is 8 times the mass of the sun, it will carry on fusing heavier and heavier atoms until iron. With our sun, I believe it will reach helium, then extinguish slowly until it becomes a white dwarf. With a star that has reached iron however, things get interesting-er.
With those stars, the will then not get sufficient outward energy to push the gas out, so it will collapse on itself, and then, essentially ‘bounce’ of the core in a supernova. What is left can either be an extremely dense neutron star, which is so dense that it fuse protons and electrons and your left with neutron rich material. Or it will turn into an infinitely dense black hole, that is indefinitely collapsing on itself.As star survives by being on fire. A star is a ball of burning gas. A ball of gas, that, surprisingly, needs to burn. Otherwise it goes boom.
At the core, a process called ‘nuclear fusion’ takes place. You see, stars weigh immensely more than any planet in the solar system, or in the universe, that we know of. They must weigh at least 13 times more than Jupiter, the largest planet in our solar system. That allows the gravity of the star to fuse hydrogen atoms together, forming helium.
Then it gets interesting. You see, when the star runs out of hydrogen, the whole star condenses, crushing even helium together. But, the fusion of helium atoms releases more energy than that of hydrogen. So then the star expands to tens or even hundreds of times it’s original size. That’s what awaits our star. The sun. In case you forgot. What happens next depends on the mass of the star. If it is under a certain threshold, which I believe is 8 times the mass of the sun, it will carry on fusing heavier and heavier atoms until iron. With our sun, I believe it will reach helium, then extinguish slowly until it becomes a white dwarf. With a star that has reached iron however, things get interesting-er.
With those stars, the will then not get sufficient outward energy to push the gas out, so it will collapse on itself, and then, essentially ‘bounce’ of the core in a supernova. What is left can either be an extremely dense neutron star, which is so dense that it fuse protons and electrons and your left with neutron rich material. Or it will turn into an infinitely dense black hole, that is indefinitely collapsing on itself.As star survives by being on fire. A star is a ball of burning gas. A ball of gas, that, surprisingly, needs to burn. Otherwise it goes boom.
At the core, a process called ‘nuclear fusion’ takes place. You see, stars weigh immensely more than any planet in the solar system, or in the universe, that we know of. They must weigh at least 13 times more than Jupiter, the largest planet in our solar system. That allows the gravity of the star to fuse hydrogen atoms together, forming helium.
Then it gets interesting. You see, when the star runs out of hydrogen, the whole star condenses, crushing even helium together. But, the fusion of helium atoms releases more energy than that of hydrogen. So then the star expands to tens or even hundreds of times it’s original size. That’s what awaits our star. The sun. In case you forgot. What happens next depends on the mass of the star. If it is under a certain threshold, which I believe is 8 times the mass of the sun, it will carry on fusing heavier and heavier atoms until iron. With our sun, I believe it will reach helium, then extinguish slowly until it becomes a white dwarf. With a star that has reached iron however, things get interesting-er.
With those stars, the will then not get sufficient outward energy to push the gas out, so it will collapse on itself, and then, essentially ‘bounce’ of the core in a supernova. What is left can either be an extremely dense neutron star, which is so dense that it fuse protons and electrons and your left with neutron rich material. Or it will turn into an infinitely dense black hole, that is indefinitely collapsing on itself.As star survives by being on fire. A star is a ball of burning gas. A ball of gas, that, surprisingly, needs to burn. Otherwise it goes boom.
At the core, a process called ‘nuclear fusion’ takes place. You see, stars weigh immensely more than any planet in the solar system, or in the universe, that we know of. They must weigh at least 13 times more than Jupiter, the largest planet in our solar system. That allows the gravity of the star to fuse hydrogen atoms together, forming helium.
Then it gets interesting. You see, when the star runs out of hydrogen, the whole star condenses, crushing even helium together. But, the fusion of helium atoms releases more energy than that of hydrogen. So then the star expands to tens or even hundreds of times it’s original size. That’s what awaits our star. The sun. In case you forgot. What happens next depends on the mass of the star. If it is under a certain threshold, which I believe is 8 times the mass of the sun, it will carry on fusing heavier and heavier atoms until iron. With our sun, I believe it will reach helium, then extinguish slowly until it becomes a white dwarf. With a star that has reached iron however, things get interesting-er.
With those stars, the will then not get sufficient outward energy to push the gas out, so it will collapse on itself, and then, essentially ‘bounce’ of the core in a supernova. What is left can either be an extremely dense neutron star, which is so dense that it fuse protons and electrons and your left with neutron rich material. Or it will turn into an infinitely dense black hole, that is indefinitely collapsing on itself.As star survives by being on fire. A star is a ball of burning gas. A ball of gas, that, surprisingly, needs to burn. Otherwise it goes boom.
At the core, a process called ‘nuclear fusion’ takes place. You see, stars weigh immensely more than any planet in the solar system, or in the universe, that we know of. They must weigh at least 13 times more than Jupiter, the largest planet in our solar system. That allows the gravity of the star to fuse hydrogen atoms together, forming helium.
Then it gets interesting. You see, when the star runs out of hydrogen, the whole star condenses, crushing even helium together. But, the fusion of helium atoms releases more energy than that of hydrogen. So then the star expands to tens or even hundreds of times it’s original size. That’s what awaits our star. The sun. In case you forgot. What happens next depends on the mass of the star. If it is under a certain threshold, which I believe is 8 times the mass of the sun, it will carry on fusing heavier and heavier atoms until iron. With our sun, I believe it will reach helium, then extinguish slowly until it becomes a white dwarf. With a star that has reached iron however, things get interesting-er.
With those stars, the will then not get sufficient outward energy to push the gas out, so it will collapse on itself, and then, essentially ‘bounce’ of the core in a supernova. What is left can either be an extremely dense neutron star, which is so dense that it fuse protons and electrons and your left with neutron rich material. Or it will turn into an infinitely dense black hole, that is indefinitely collapsing on itself.As star survives by being on fire. A star is a ball of burning gas. A ball of gas, that, surprisingly, needs to burn. Otherwise it goes boom.
At the core, a process called ‘nuclear fusion’ takes place. You see, stars weigh immensely more than any planet in the solar system, or in the universe, that we know of. They must weigh at least 13 times more than Jupiter, the largest planet in our solar system. That allows the gravity of the star to fuse hydrogen atoms together, forming helium.
Then it gets interesting. You see, when the star runs out of hydrogen, the whole star condenses, crushing even helium together. But, the fusion of helium atoms releases more energy than that of hydrogen. So then the star expands to tens or even hundreds of times it’s original size. That’s what awaits our star. The sun. In case you forgot. What happens next depends on the mass of the star. If it is under a certain threshold, which I believe is 8 times the mass of the sun, it will carry on fusing heavier and heavier atoms until iron. With our sun, I believe it will reach helium, then extinguish slowly until it becomes a white dwarf. With a star that has reached iron however, things get interesting-er.
With those stars, the will then not get sufficient outward energy to push the gas out, so it will collapse on itself, and then, essentially ‘bounce’ of the core in a supernova. What is left can either be an extremely dense neutron star, which is so dense that it fuse protons and electrons and your left with neutron rich material. Or it will turn into an infinitely dense black hole, that is indefinitely collapsing on itself.As star survives by being on fire. A star is a ball of burning gas. A ball of gas, that, surprisingly, needs to burn. Otherwise it goes boom.
At the core, a process called ‘nuclear fusion’ takes place. You see, stars weigh immensely more than any planet in the solar system, or in the universe, that we know of. They must weigh at least 13 times more than Jupiter, the largest planet in our solar system. That allows the gravity of the star to fuse hydrogen atoms together, forming helium.
Then it gets interesting. You see, when the star runs out of hydrogen, the whole star condenses, crushing even helium together. But, the fusion of helium atoms releases more energy than that of hydrogen. So then the star expands to tens or even hundreds of times it’s original size. That’s what awaits our star. The sun. In case you forgot. What happens next depends on the mass of the star. If it is under a certain threshold, which I believe is 8 times the mass of the sun, it will carry on fusing heavier and heavier atoms until iron. With our sun, I believe it will reach helium, then extinguish slowly until it becomes a white dwarf. With a star that has reached iron however, things get interesting-er.
With those stars, the will then not get sufficient outward energy to push the gas out, so it will collapse on itself, and then, essentially ‘bounce’ of the core in a supernova. What is left can either be an extremely dense neutron star, which is so dense that it fuse protons and electrons and your left with neutron rich material. Or it will turn into an infinitely dense black hole, that is indefinitely collapsing on itself.As star survives by being on fire. A star is a ball of burning gas. A ball of gas, that, surprisingly, needs to burn. Otherwise it goes boom.
At the core, a process called ‘nuclear fusion’ takes place. You see, stars weigh immensely more than any planet in the solar system, or in the universe, that we know of. They must weigh at least 13 times more than Jupiter, the largest planet in our solar system. That allows the gravity of the star to fuse hydrogen atoms together, forming helium.
Anyways, I’ve been winning waaaaaay longer

Haha....now who's the one winning?
Oh, I have not.... Beacuse it's clearly not u who's winning.
I WON. Thank you very much!!
I WON. Thank you very much!!

I won.
Books mentioned in this topic
Divine Rivals (other topics)Gorgeous Gruesome Faces (other topics)
Hunting Prince Dracula (other topics)
The Ballad of Songbirds and Snakes (other topics)
The Maze Runner (other topics)
More...