SUMMARY
The Milky Way galaxy moves within the Local Group, which is a gravitationally bound system. This group has a common center of mass around which its galaxies orbit, but due to its relatively small size—approximately 100 times the diameter of the Milky Way—galaxies interact in complex ways. Unlike stars in a galaxy, these interactions can lead to phenomena such as galactic disruption. Consequently, the motion of galaxies in the Local Group is not purely elliptical, influenced by gravitational interactions with satellite galaxies.
PREREQUISITES
- Understanding of gravitational binding in astrophysics
- Familiarity with galaxy dynamics and motion
- Knowledge of mass distribution in astronomical systems
- Concept of satellite galaxies and their interactions
NEXT STEPS
- Research gravitational binding in galaxy clusters
- Study the dynamics of satellite galaxies in the Milky Way
- Explore the concept of mass distribution in astrophysical systems
- Learn about the interactions between galaxies in the Local Group
USEFUL FOR
Astronomers, astrophysics students, and anyone interested in the dynamics of galaxies and their interactions within the Local Group.