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The first is the supermassive black hole. A supermassive black hole is a black hole that is over a billion times the mass of our Sun.

Black holes have very strong gravitational pulls, so they draw in objects around them. As material falls near the black hole, it surrounds it and becomes an accretion disk.

The supermassive black hole and accretion disk are the two parts of the quasar. This accretion disk heats up due to the friction caused by the pull of the black hole.

How hot does the quasar get? Recent estimates suggest that quasars can reach over 18 trillion degrees Fahrenheit! A famous example of a quasar is the Einstein Cross.

Take a look at the image above — what do you see? It may look like there are five objects here, but this image is actually of just one quasar! How can this be?

The true quasar is at the center of this image. The other four light sources around it are not actually there. This famous picture is the composite of four separate images of the exact same quasar.

This results in a wide variety of observed phenomena from what are, in reality, physically similar sources. Because of the finite speed of light , when quasars are observed at great distances, they are observed as they were in the distant past.

Thus, the increasing density of quasars with distance means that they were more common in the past than they are now.

At earlier ages, the number density of quasars decreases sharply, corresponding to an era when the quasar population was still building up.

The most distant, and thus earliest, quasars known were formed less than a billion years after the big bang.

Individual quasars appear as their central black holes begin to accrete gas at a high rate, possibly triggered by a merger with another galaxy, building up the mass of the central black hole.

The current best estimate is that quasar activity is episodic, with individual episodes lasting around a million years and the total quasar lifetime lasting around 10 million years.

At some point, quasar activity ceases completely, leaving behind the dormant massive black holes found in most massive galaxies.

Indeed, in the current universe the remaining AGN population is made up predominantly of lower-luminosity Seyfert galaxies with relatively small supermassive black holes.

In the present-day universe there is a close relationship between the mass of a black hole and the mass of its host galaxy.

This is quite remarkable, since the central black hole accounts for only about 0. It is believed that the intense radiation, mass outflows, and jets from the black hole during its active quasar phase are responsible.

The radiation, outflows, and jets heat up and can even remove entirely the interstellar medium from the host galaxy.

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QSO, quasi-stellar radio source. Learn More in these related Britannica articles: The discovery of quasars quasi-stellar radio sources in the early s also told heavily against the steady-state theory.

Quasar s were first identified as strong radio sources that in visible light appear to be identified with small starlike objects. Further, they have large redshifts, which implies that they are….

Quasar s are objects whose spectra display very large redshifts, thus implying in accordance with the Hubble law that they lie at the greatest distances see above Determining astronomical distances.

They were discovered in but remained enigmatic for many years. They appear as starlike i. These cosmic objects have intense clouds of radio emission that extend hundreds of thousands of light-years away from a central energy source located in an active galactic nucleus AGN , or quasar.

Observations with high-resolution radio arrays show…. Although price was not the issue I have to say that the fact that it's highly cost effective is a bonus.

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KidsKnowIt Network is now part of Education. Quasar A quasar is the brightest objects in the Universe. Have you ever wondered what lies at the center of a galaxy?

If you peer at the very center of some galaxies, you may find a curious object called a quasar. These objects are extremely bright.

At that time, astronomers were pointing their radio telescopes toward the sky. They noticed radio waves coming off of celestial bodies they expected, like the sun.

This term was later shortened to quasar. Quasars are usually found billions of light-years away from Earth! We now know a lot more today about quasars than ever before.

The astronomy community has many thousands of quasars cataloged. A quasar is made up of two key parts. The first is the supermassive black hole. A supermassive black hole is a black hole that is over a billion times the mass of our Sun.

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