Earth-Like Planets & Iron: Questions Answered

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The discussion centers on the abundance of iron in Earth-like planets and the implications for planetary formation. Iron is prevalent due to its production in supernovae, particularly type Ia explosions, which generate significant amounts of nickel and iron. The initial composition of the protostellar disk was uniform, and as elements clumped together, heavier materials like iron were retained in the inner planets while lighter elements were lost. The presence of an iron core is significant for Earth's magnetic field, but other metals could potentially serve similar functions in different planetary systems. Overall, the unique abundance and properties of iron play a crucial role in the formation and characteristics of terrestrial planets.
  • #51
Bystander said:
I'm not about to speculate on the variety or properties of the adsorbing surfaces, just on the behavior of adsorbate(s) in the various layers that form.

And that behavior is hard to define

Because of the semi liquid like mobility of those adsorbates

Yes?

And that mobility is due to vacancies in the partially formed crystal lattice structure

Of those first few surface layers?

Why else would you refrain from classifying those surface layers as simply solid

Due to site hopping mobility?
 
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