SUMMARY
The Cosmic Microwave Background (CMB) radiation was emitted approximately 42.17 million light years away when the universe was about 380,000 years old. The current diameter of the observable CMB sphere is estimated to be around 90 billion light years, with a comoving distance to the last scattering surface at approximately 46 billion light years. The expansion factor since the emission of CMB photons is about 1100. The topology of the last scattering surface remains an open question in cosmology, complicating the understanding of the CMB sphere's true size.
PREREQUISITES
- Understanding of Cosmic Microwave Background (CMB) radiation
- Familiarity with comoving distance and proper distance concepts
- Knowledge of redshift calculations in cosmology
- Experience with cosmological calculators, specifically Jorrie's and Ned Wright's
NEXT STEPS
- Explore the functionality of Jorrie's cosmo-calculator for various cosmological parameters
- Learn about the implications of nonlinear geometry of spacetime on cosmological models
- Investigate the concept of the last scattering surface and its significance in cosmology
- Study the expansion of the universe and its effects on the observable universe's size
USEFUL FOR
Astronomers, cosmologists, and physics enthusiasts interested in the properties and implications of the Cosmic Microwave Background radiation and the expansion of the universe.