We Are Made of Stardust from Old Supernovas
How old are the atoms in your body? Most of your body is made of hydrogen and oxygen bonded as molecules of water.
These atoms were created at the start of our universe during the Big Bang. So if you look at it this way, then you’re about 13.7 billion years old.
But your body also has heavier elements like copper and zinc. These atoms were created in the dying last stage of an exploding star called a supernova.
These elements were flung into space as dust and gas (star dust). Eventually, they coalesced to become part of a new forming solar system and our planet Earth.
Because you are made from matter from the Earth, you are made of stardust from old supernovas. So turns out, you are bits and pieces of star and cosmic dust.
Stars are element factories
As we already know, hydrogen and helium have been around since the Big Bang. So stars (like our Sun) take lighter elements like hydrogen and build heavier ones like helium, carbon and oxygen.
It’s through fusion reaction how stars build element of their own. But stars can only produce elements as heavy as iron. Anything heavier is made when the star becomes a supernova.
When a star is at the end of its life, temperature begins to increase. At about 200 million degrees, helium fuses into carbon and oxygen. Then at above 3 billion degrees, it creates silicon, iron and nickel.
If our sun was bigger, it would go through the process of a supernova. For high mass stars, they simply don’t burn out of fuel. Instead it ejects matter violently into space building heavier elements like gold and uranium.
Supernovas build heavier elements
Stars larger than our sun goes through a faster cycle with more intense pressure. But for larger stars, they have so much energy that they don’t simply die and turn into a white dwarf.
Instead they expand into a red supergiant and then explode in a dramatic event called a supernova. It blasts material dramatically into space. Eventually, they can then collapse as a neutron star or black hole.
Supernova are important because they form the more complicated elements on Earth from hydrogen to uranium. Supernovas build anything in our period table that is heavier than iron.
The process of building heavier atoms than hydrogen is called nuclearsynthesis. It happens because neutron that gets added into much larger atoms. These are the 92 natural elements, many of which that are used to create rocks and minerals.
Our sun’s fusion reaction
Fusion smashes two or more atomic nuclei together and builds a heavier nucleus. For example, our Sun constantly fuses hydrogen into helium. This process releases energy and sunlight, constantly warming our planet.
When stars like our Sun finish using hydrogen in the core, then it will begin fusing the leftover helium into carbon and oxygen. When this begins, the star will swell up into a red giant.
Based on the initial mass of the star, successive fusion reactions may follow. Starting with hydrogen, it can fuse into helium, carbon, oxygen, neon, silicon and iron.
If the star has more mass, then it will go further down the chain of reactions all the way up to iron. But if a star has enough mass to fuse iron, it will then supernova once that fusion is complete.
Our sun will never be a supernova
Like any fire, eventually they always burns out in the end. Our Sun is no different.
It’s at about halfway through its life expectancy with about 4 billion more years remaining.
Our Sun won’t become a supernova and will collapse into a white dwarf. Actually, the vast majority of stars die in a much less violent manner.
This is why we classify it in the lightweight category . Whereas heavyweight stars have the most fuel, but burns it at the fastest rate.
In general, supernova are quite rare because stars need to be massive to die this way. After they violently explode, they disperse throughout out the galaxy and become part of a new forming solar system.
For example, our solar system contains elements from different stars which died before our solar systems existence.