SUMMARY
Humanity has only observed approximately 3% of the observable universe, primarily due to limitations in our telescopes and observational technology. The observable universe is defined by the Cosmic Microwave Background (CMB) at a redshift of z~1000, with galaxies becoming visible at around z=6. A significant portion of the universe, often referred to as the "dark ages," remains largely unobserved. Current research focuses on understanding this region through the study of 21cm radiation, which is emitted and absorbed during that epoch.
PREREQUISITES
- Understanding of Cosmic Microwave Background (CMB)
- Familiarity with redshift concepts in astronomy
- Knowledge of comoving coordinates in cosmology
- Basic principles of 21cm radiation and its significance
NEXT STEPS
- Research the implications of the Cosmic Microwave Background (CMB) on cosmology
- Study the methods used to measure redshift and its applications
- Explore the significance of comoving coordinates in understanding cosmic expansion
- Investigate current research on 21cm radiation and its role in probing the "dark ages"
USEFUL FOR
Astronomers, astrophysicists, and anyone interested in cosmology and the limits of human observation of the universe.