SUMMARY
Neutron star collisions are responsible for the creation of heavy elements, including gold, which are ejected into the InterStellar Medium (ISM) rather than falling back into the newly formed black hole. The neutron star merger event GW170817 provided estimates that approximately 0.01 solar masses of heavy elements were ejected during the collision. These ejected elements later contribute to the formation of new stars and planets. Additionally, heavy elements are also produced during supernova events, further enriching the ISM.
PREREQUISITES
- Understanding of neutron star physics
- Familiarity with the InterStellar Medium (ISM)
- Knowledge of stellar evolution and nucleosynthesis
- Awareness of gravitational wave events, specifically GW170817
NEXT STEPS
- Research the implications of neutron star mergers on cosmic element distribution
- Study the process of nucleosynthesis in supernovae
- Explore the role of gravitational waves in astrophysics
- Investigate the formation and evolution of the InterStellar Medium
USEFUL FOR
Astronomers, astrophysicists, and students interested in stellar evolution, cosmic element formation, and the dynamics of neutron star collisions.