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Last update: October 7, 2025

Quasars: Beacons of the Distant Cosmos

Artist view of a quasar emitting a relativistic jet

An Universe Illuminated by its Most Violent Cores

Discovery and Power of Quasars

Quasars (for "quasi-stellar radio source") are among the brightest and most energetic objects in the known Universe. Discovered in the early 1960s by Maarten Schmidt (1929-2022), they emit radiation capable of rivaling the light of hundreds of entire galaxies. Their power comes from accretion onto a supermassive black hole located at the center of an active galaxy.

Physical Nature of a Quasar

A quasar is neither a simple black hole nor a galaxy. It represents a state of activity of the galactic nucleus, not a separate type of object. The quasar refers to the extreme activity phenomenon observed at the center of certain galaxies, not the material object itself.

Physical Conclusion

The black hole is the energy engine, the quasar the observable phenomenon produced by this engine, and the host galaxy the gravitational framework containing the entire system.

Luminosity and Energy

The total luminosity of a quasar can reach \( L \approx 10^{40}\ \mathrm{W} \), about \(10^{13}\) times that of the Sun. Such energy can only originate from an efficient gravitational mechanism. Mass-energy conversion follows the relativistic equation \(\,E = \eta m c^2\,\), where \(\eta\) is the efficiency, typically between 0.1 and 0.4 in a relativistic accretion disk.

Note:
An active galaxy has an extremely bright nucleus powered by accretion of gas onto a supermassive black hole. This energy, around \(10^{39}\) to \(10^{41}\ \mathrm{W}\), described by \(\,E = \eta m c^2\,\) with \(\eta \approx 0.1\), makes AGN the most powerful sources in the observable Universe.

Extreme Distances and High Redshifts

Quasars are at cosmological distances, sometimes over 12 billion light-years away. Their spectra show high redshift (\(z > 6\)), indicating emission when the Universe was only a fraction of its current age.

These measurements allow astrophysicists to study the epoch of cosmic reionization, the transition of the Universe from a neutral to an ionized state. Quasars, illuminating the intergalactic medium, serve as temporal beacons of cosmic structure formation.

Redshift and Quasar Distances

Examples of Quasar Redshifts and Approximate Distances
QuasarRedshift (z)Approx. Distance (billion ly)Comment
3C 2730.1582.2Relatively nearby quasar, well studied
PG 1302-1020.2783.5Quasar with suspected periodic variability
QSO B0909+5322.0010.2Moderate redshift quasar for spectral studies
Quasar B1422+2313.6211.6High redshift, used for gravitational lens studies
SDSS J1250+31304.1012.0Distant quasar observed by the Sloan Digital Sky Survey
SDSS J1021+28035.0512.5High-redshift quasar, witness of the young Universe
SDSS J0100+28026.3012.8One of the most distant known quasars
ULAS J1120+06417.0812.9Epoch of cosmic reionization

Accretion Physics and Relativistic Jets

Around the central black hole, matter forms a rapidly rotating disk. Internal friction converts gravitational potential energy into electromagnetic radiation.

Strong magnetic fields channel part of the energy into relativistic jets, capable of propelling particles at speeds near \(c\), the speed of light. These jets, observed notably by the VLBA, are a major signature of Active Galactic Nuclei (AGN).

Quasars and Galactic Evolution

Observations suggest most massive galaxies host a supermassive black hole at their center. Quasars may represent a transitional phase in this galactic evolution: when a gas inflow triggers rapid accretion, the nucleus becomes dazzling. Once the matter reservoir is depleted, the galaxy stabilizes and the quasar shuts down.

The observed correlation between black hole mass (\(M_{\mathrm{BH}}\)) and galactic bulge mass (\(M_{\mathrm{bulge}}\)) suggests coevolution governed by energetic feedback: \( M_{\mathrm{BH}} \propto M_{\mathrm{bulge}}^{1.1} \)

Comparative Table: Quasars and Other Active Nuclei

Comparison of Main Types of Active Galactic Nuclei
Object TypeTypical Luminosity (W)Observed DistanceDominant Characteristic
Quasar1039 to 1041> 1 billion lyExtremely luminous across the spectrum, high redshift, powerful relativistic jets, witnesses of early galactic formation
Blazar1038 to 1040Up to 5 billion lyRelativistic jet pointed toward Earth, rapid variability, intense gamma-ray and X-ray emission
Seyfert galaxy1036 to 1038< 200 million lyStrong optical and UV emission lines, moderate active nucleus, host stars visible
Radio galaxy1037 to 1040Hundreds of millions to several billion lyDominant radio emission, extended lobes over hundreds of kpc, relativistic jets, often obscured nucleus
LINER1035 to 1037Often < 100 million lyLow ionization, moderate nuclear emission, often in elliptical or mature spiral galaxies
Obscured AGN / Type 21036 to 1039Variable depending on galaxyCentral radiation blocked by a dust torus, hidden nucleus, emission mostly in IR and X-rays

Source: NASA ADS Astrophysics Data System, European Southern Observatory (ESO).

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