SUMMARY
The solar system rotates around the center of the Milky Way galaxy. The Milky Way itself is influenced by the gravitational pull of the local group of galaxies, primarily Andromeda, resulting in a complex motion rather than a simple orbit. Current data suggests that the Milky Way is heavier than the Andromeda Galaxy (M31), although precise measurements are challenging. Additionally, the local group is moving at approximately 600 km/s relative to the Cosmic Microwave Background, contributing to the CMB Dipole effect.
PREREQUISITES
- Understanding of basic astronomy concepts
- Familiarity with galaxy structures and dynamics
- Knowledge of gravitational interactions between celestial bodies
- Awareness of the Cosmic Microwave Background (CMB) and its significance
NEXT STEPS
- Research the gravitational dynamics of the Milky Way and Andromeda galaxies
- Explore the concept of the Cosmic Microwave Background and the CMB Dipole effect
- Study the motion of local galaxy groups and their interactions
- Investigate methods for measuring galaxy mass and gravitational influence
USEFUL FOR
Astronomy enthusiasts, astrophysicists, and students seeking to understand the dynamics of our solar system and its relationship with the Milky Way and neighboring galaxies.