SUMMARY
The Big Bang theory describes the continuous expansion of the universe, but this expansion does not apply to galaxies or planets. Instead, only structures larger than galactic clusters experience this expansion, meaning that objects not bound by strong gravitational forces, such as different galaxy clusters, gradually move apart over time. Within galaxy clusters, the gravitational forces are sufficient to prevent expansion, keeping galaxies and planets intact. This distinction is crucial for understanding cosmic expansion.
PREREQUISITES
- Understanding of the Big Bang theory
- Knowledge of cosmic structures, specifically galactic clusters
- Familiarity with gravitational forces and their effects on celestial bodies
- Basic concepts of cosmology and the universe's expansion
NEXT STEPS
- Research the concept of cosmic expansion and its implications on large-scale structures
- Explore gravitational binding and its role in preventing expansion within galaxy clusters
- Study the differences between local and cosmic scales in the universe
- Investigate other theories of cosmic evolution and their relation to the Big Bang theory
USEFUL FOR
Astronomers, astrophysicists, students of cosmology, and anyone interested in the mechanics of the universe's expansion.