Why normal stars can’t make gold
Stars make elements through fusion:
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Hydrogen → Helium
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Helium → Carbon, Oxygen
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Bigger stars → up to Iron
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But iron is the limit.
Making elements heavier than iron doesn’t release energy — it requires energy. So stars stop there.
Gold (atomic number 79) is far heavier than iron (26).
What can make gold: the r-process
Gold forms through something called the rapid neutron capture process (the r-process):
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A huge number of free neutrons are released.
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Atomic nuclei rapidly absorb these neutrons.
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They become extremely heavy and unstable.
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They radioactively decay into stable heavy elements like:
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Gold
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Platinum
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Uranium
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This requires:
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Insane temperatures
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Insane pressure
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A flood of neutrons
Only a few events in the universe can do this.
The main source: Neutron star collisions
When two neutron stars crash into each other:
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Matter is ripped apart
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Trillions of neutrons flood the space
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The r-process happens
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Huge amounts of gold are created in seconds
In 2017, scientists observed this happening (GW170817). The data showed that a single collision made more gold than the mass of Earth.
How gold got to Earth
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Neutron stars collided billions of years ago.
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Gold was blasted into space as dust.
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This dust became part of the cloud that formed our solar system.
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Gold was already mixed into Earth when it formed.
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Later, asteroid impacts added even more gold to Earth’s crust.
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