SUMMARY
The Milky Way and Andromeda galaxies will collide in approximately 4.5 billion years despite the universe's expansion. This is due to the gravitational attraction between the two galaxies, which outweighs the effects of cosmic expansion within their local cluster. The Hubble constant is 72 km/sec/Mpc, and the distance between the galaxies is about 2.5 million light-years, resulting in a relative velocity of 355 km/sec when accounting for gravitational attraction and expansion. Understanding the dynamics of galaxy motion within clusters is crucial for grasping this phenomenon.
PREREQUISITES
- Understanding of gravitational attraction in astrophysics
- Familiarity with the Hubble constant and its implications
- Knowledge of galaxy clusters and their dynamics
- Basic concepts of cosmic expansion and its effects
NEXT STEPS
- Research the implications of the Hubble constant on galaxy movement
- Study gravitational interactions within galaxy clusters
- Explore case studies of galaxy collisions observed by Hubble
- Learn about the methods used to measure cosmic expansion
USEFUL FOR
Astronomers, astrophysicists, students of cosmology, and anyone interested in the dynamics of galaxy interactions and cosmic expansion.