Mysterious Quasars: What We Know & Don't Know

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Quasars, particularly 3C 273, are relatively close, with a redshift of z=0.173, but some quasars are nearly as old as the universe, observed at redshifts around z=6. While quasars still exist today, 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 effects and the finite speed of light, leading to miscalculations of linear velocities. Understanding these aspects helps clarify the nature and evolution of quasars in the cosmos. The ongoing study of quasars continues to reveal insights into the early universe and cosmic expansion.
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If we calculate the distance from us to the nearest quasar, it is huge with a redshift factor nearly equal to 4. Does that make them as old as the universe itself? Do they exist today? Also, why are their 2 inner cores expanding at superluminal velocities?
 
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gaugeboson said:
If we calculate the distance from us to the nearest quasar, it is huge with a redshift factor nearly equal to 4.

The nearest quasar is much closer than that. Though it depends on the definition of "quasar", many would say that 3C 273 is the nearest, with a redshift z=0.173.


Does that make them as old as the universe itself?

Some quasars are nearly as old as the universe, yes. The highest redshift we've observed is around z=6, so at that time the universe was less than 10% of its current age.


Do they exist today?

Yes, though their numbers are greatly decreased. The peak of quasar activity was between redshifts of 2 and 3.


Also, why are their 2 inner cores expanding at superluminal velocities?

This is an illusion induced by a combination of relativistic and projection effects. We measure the angular velocities of quasar outflows and then use the distance to get the linear velocity. If you don't correct for emission delays due to the finite speed of light, then this can sometimes give you an outflow speed faster than c.
 
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