SUMMARY
The speed of an object standing still on Earth is relative and depends on the chosen frame of reference. When considering the Cosmic Microwave Background (CMB), the Solar System travels at approximately 390 ± 60 km/sec relative to the CMB, while the Galaxy moves at about 603 km/sec or 0.2%c. The CMB serves as a significant reference frame due to the uniformity of the universe at the time of its emission. The discussion emphasizes that without a specified reference frame, questions about speed become meaningless.
PREREQUISITES
- Understanding of Cosmic Microwave Background (CMB) and its significance in cosmology
- Familiarity with frames of reference in physics
- Knowledge of special relativity (SR) and general relativity (GR)
- Basic concepts of galactic motion and cosmological measurements
NEXT STEPS
- Research the implications of the Cosmic Microwave Background on cosmological models
- Learn about the calculations involved in determining velocities relative to the CMB
- Explore the concept of reference frames in special and general relativity
- Investigate the motion of the Solar System and its implications for astrophysics
USEFUL FOR
Astronomers, physicists, cosmologists, and students interested in the dynamics of the universe and the implications of relative motion in astrophysics.