SUMMARY
The discussion centers on quasars, specifically addressing the nearest quasar, 3C 273, which has a redshift of z=0.173. While some quasars are nearly as old as the universe, the highest observed redshift is around z=6, indicating they existed when the universe was less than 10% of its current age. Quasars still exist today, but their numbers have significantly decreased since their peak activity between redshifts of 2 and 3. The phenomenon of their inner cores appearing to expand at superluminal velocities is attributed to relativistic and projection effects, requiring corrections for emission delays due to the finite speed of light.
PREREQUISITES
- Understanding of redshift and its implications in cosmology
- Familiarity with the concept of quasars and their characteristics
- Knowledge of relativistic effects in astrophysics
- Basic principles of light propagation and emission delays
NEXT STEPS
- Research the properties and significance of redshift in cosmology
- Study the characteristics and formation of quasars
- Explore relativistic effects in astrophysics, particularly in high-velocity objects
- Investigate the methods used to measure quasar distances and velocities
USEFUL FOR
Astronomers, astrophysicists, and students interested in cosmology, particularly those studying the nature and behavior of quasars and their role in the universe's evolution.