Svartalf wrote:Ignore this if it's been answered in the course of the thread (I am reading it) ... but do geologists have any idea why we cot so much iron an silicon when we have gas giants made mostly of hydrogen, helium, and carbon compounds?
In the case of iron, this is fairly straightforward, and it's to do with the stability of the nucleus and the lowest energy configuration.
There are two forces at play here, namely the strong nuclear force and the electromagnetic force. The strong nuclear force is, as the moniker suggests, strong, but its range is very short. The electromagnetic force is weaker, but operates over a longer range. Bear in mind that, in the electromagnetic force, like charged particles repel.
When there is a relatively small number of protons and neutrons (nucleons) in a nucleus, adding nucleons is energetically favourable, because the electromagnetic force between the nucleons on one side of the nucleus and the other are overcome by the strong force. As the nucleus gets larger, the balance between the two forces shifts, and the electromagnetic repulsion of like charges overcomes the attraction of the strong nuclear force. Beyond this point, removing nucleons becomes energetically favourable. Iron is pretty much at the centre point, which means that the attraction of the strong nuclear force and the repulsion of the electromagnetic force are reasonable equal.
The above is very loosely explained, but reasonably robust.
As for silicon, the answer is simply that it formed, along with oxygen, the majority of the protoplanetary disk from which the solar system formed. The reason for that is that silicon burning is the final stage of high-mass stars (>11 times the mass of the sun) at the end of their main sequence, and after the triple-alpha process responsible for carbon production.