Alex48674 said:
Also would you be able to make any sort of proof along similar lines as this as why high densities correlate with high temperatures...
I can't offer advice about how to write your paper about the history of the Earth because I don't know the teacher or class or situation, and even if I did I might not give very good advice.
On the other hand you seem to be asking good physics and cosmology questions and I can respond to those. (this may not be the best help for writing your paper because it leads to overemphasis on astrophysics and not enough attention to geology and biology)
But i am not going to worry about that. That is your responsibility.
Here you are basically asking about
how does a young planet cool?
that's a good question. It cools by radiating energy off into space.
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Someone else will correct me if I am too far off on the numbers, but I think one can say that spatial EXPANSION only drove cooling for the first few million years since it started.
The solar system formed much later, around 9 BILLION years. By that time background radiation was very cold----space was cold and dark.
At that time, the important cooling mechanism is thermal radiation-----like infrared, radiant heat.
As soon as the sky itself is cold, then material objects can begin dumping their heat radiantly into the sky.
And material objects, like planets, as they gradually collect, coagulate, condense---the little bits glomming on to make larger bits and the larger bits crashing together to make even larger lumps----they actually generate a lot of heat! A meteorite impact can melt rock. So a fair amount of that heat had to be somehow gotten rid of. And it got radiated off.
I'm sure you have thought about this.
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Maybe you should not waste time learning about it now, but there is a law called the Fourth Power Radiation Law, or else the "Stefan-Boltzmann Law" which describes the brightness with which warm objects glow.
the power density (watts per square meter surface) is proportional to T
4, the fourth power of the temperature. this is absolute temp, in kelvin.
So if you double the temperature you increase the watts per square meter by 16 fold.
And there is the Planck Black Body radiation law that shows how the wavelengths that a warm body radiates depend on the temperature. Higher temp means shorter wavelengths (higher frequency more energetic photons) and so on.
So there are these rather elegant rules that nature follows about how objects radiate.
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Before material objects can radiate their heat off into the sky, the sky itself has to cool. Otherwise, if the sky is glowing hot, it will radiate back in just as much as the object is radiating out, and no cooling will happen.
So that first part was accomplished by expansion. But very soon (I am not sure how soon, there was what was called "dark ages" when the sky was good and cold and not enough stars had condensed to brighten things up.
and then stars began to condense and galaxies collect and all that structure began to assemble itself. I think roughly speaking the first galaxies were forming at around 700 million years.
we really need a timeline don't we?. does anyone know of a good one?