The History of Atoms
The History of our Atoms
The steps for making Atoms
Big Bang
Energy = matter times the speed of light squared E=mc2
E = mc2
Energy slows down and condenses into Matter in the form of Protons and Electrons
A single proton is the Atom Hydrogen
Some Hydrogens also have an electron or two
Hydrogen clouds condense into Nebula. These Nebula only have Hydrogen in them
These Hydrogen Nebula further condense into the very first stars
Generation 1 Stars are also called Population III Stars
These are 1000's of times larger than our sun, burn extremely hot, and exist for only a short time - In fact none are left
These stars are so large and hot that they turn Hydrogen into Helium, then Helium into everything else: Lithium, Beryllium, Boron, Carbon, Nitrogen, Oxygen... Iron
This is Nucleosynthesis - aka the synthesis of atoms
They then collapse on themselves, and then explode outwards - This is a super nova explosion - This slams the atoms together fusing them into the final super heavy elements, such as uranium
This makes a new nebula called Molecular Nebula - these nebula have all the elements in it
Inside this Molecular Nebula, the big elements like Iron are attracted to each other, making dust, then sand, then pebbles, then rocks, then Meteorites
New stars are created from this Molecular Nebula
The dust around these new stars form planets
Our Sun is a Generation 3 Star, or a Population 1 Star
Our Sun contains Iron that it got from the supernova explosion of Generation 1 stars
Our planets atoms, Carbon, Oxygen, Iron, come from the explosion of Generation 1 stars
This means, that the origin for the atoms in your body, are from Super Nova Explosions
This means, that the atoms that make up your body are older than the planet itself is
You are built of the Universe, you are the Universe experiencing itself