SUMMARY
Hubble's Law states that a galaxy's recessional speed is proportional to its distance from us, with no upper limit to this speed. For example, a galaxy 1 megaparsec away recedes at approximately 70 km/s, while galaxies at the edge of the observable universe can recede at speeds exceeding 3 times the speed of light (3c). The term "moves" is misleading; "receding" more accurately describes the behavior of these galaxies, especially since galaxies within the Local Group are gravitationally bound and do not recede.
PREREQUISITES
- Understanding of Hubble's Law and its implications
- Familiarity with the concept of recessional velocity in cosmology
- Knowledge of the observable universe and its boundaries
- Basic grasp of gravitational binding in galaxy clusters
NEXT STEPS
- Research the implications of Hubble's Law on cosmic expansion
- Explore the concept of gravitational binding in galaxy clusters
- Learn about the observable universe and its limitations
- Investigate the effects of relativistic speeds in cosmology
USEFUL FOR
Astronomers, astrophysicists, and students of cosmology seeking to understand the dynamics of galaxies and the expansion of the universe.