During some supernovae, how can nuclei grow heavier than iron?
They rapidly capture neutrons, then some of those neutrons convert into protons.
- Ordinary core fusion releases energy
- They collect electrons from surrounding gas
- Nuclei capture neutrons that later become protons ✔
Why: Some supernovae create neutron-rich conditions. Nuclei can rapidly capture neutrons, then nuclear decay converts some neutrons into protons, building heavier elements. Neutron-star mergers are another confirmed site of this process.
Huh, didn't know that: NASA observations confirmed that a 2017 neutron-star merger could have created gold, platinum and other heavy elements.
Gold asked a neutron to stick around. The answer carried a lot of weight.
References
Answer: Nuclei capture neutrons that later become protons. Some supernovae create neutron-rich conditions. Nuclei can rapidly capture neutrons, then nuclear decay converts some neutrons into protons, building heavier elements. Neutron-star mergers are another confirmed site of this process.
- Astronomy 2e, 23.2 Evolution of Massive Stars: An Explosive Finish openstax.org/books/astronomy-2e/pages/23-2-evolution-of-massive-stars-an-explosive-finish
These neutrons can be absorbed by iron and other nuclei where they can turn into protons.
Checked 2026-10-10. - NASA Science, Where Does Gold Come From? science.nasa.gov/universe/stars/neutron-stars/magnetars/where-does-gold-come-from-nasa-data-has-clues
they confirmed that this event could have created gold, platinum, and other heavy elements.
Checked 2026-10-10.
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