SUMMARY
Gold is synthesized during the core-collapse phase of a supernova, specifically through the collision of neutron stars. This process occurs within three seconds, where the collapse of the stellar core generates a shock wave that produces heavy elements, including gold. Initially, gold exists as a gas and cools to form dust, which later coalesces into larger objects. The boiling point of gold is 2,856°C (5,173°F), beyond which it can exist as gas, even in the vacuum of outer space.
PREREQUISITES
- Understanding of core-collapse supernova mechanics
- Knowledge of neutron star collisions
- Familiarity with the processes of nucleosynthesis
- Basic concepts of thermodynamics related to phase changes of elements
NEXT STEPS
- Research the process of nucleosynthesis in supernovae
- Explore the role of neutrinos in stellar explosions
- Investigate the physical conditions in neutron star collisions
- Study the implications of heavy element formation in astrophysics
USEFUL FOR
Astronomers, astrophysicists, and anyone interested in the origins of heavy elements in the universe will benefit from this discussion.