Is S5 0014 81 a black hole?

The host galaxy of S5 0014+81 is an FSRQ (Flat Spectrum Radio Quasar) blazar, a giant elliptical galaxy that hosts a supermassive black hole at its center. They found it to be about 10,000 times more massive than the black hole at the center of our galaxy, or equivalent to 40 billion solar masses.

Is the black hole at the center of our galaxy a quasar?

Bottom line: Quasars are extremely bright and extremely distant objects. Their huge energy output is thought to be due to activity around the central supermassive black hole in young galaxies, near the edge of the observable universe.

Where is the black hole TON 618?

RA 12h 28m 25s | Dec +31° 28′ 38″
TON 618/Coordinates

How was the 618 formed?

It was born from a collision between two smaller galaxies. That goes to the aptly named TON 618, a quasar (an active black hole consuming material and surrounded by streams of particles) that outshines the galaxy in which it sits. TON 618 is as bright as 140 trillion suns and has a mass of about 66 billion suns.

How does a black hole power a quasar?

They are powered by supermassive black holes, weighing in at billions of solar masses. Gas falling into the black hole accumulates in a bright, whirling accretion disc; the jets are probably produced by strong magnetic fields. Quasars are most conspicuous when one of the jets is more or less aimed at the observer.

Is the Milky Way a quasar?

If such a jet at the center of a distant galaxy points towards Earth we may see it as quasar. Hence the answer is most likely yes, the Milky Way or some of its predecessor galaxies will probably have had quasars at their centers, at some period when consuming lot of material, and seen from appropriate direction.

How did we find TON 618?

In 1970, a radio survey at Bologna in Italy discovered radio emission from TON 618, indicating that it was a quasar. Marie-Helene Ulrich then obtained optical spectra of TON 618 at the McDonald Observatory which showed emission lines typical of a quasar.

How long will the supermassive black hole S5 0014+81 live?

Evolution models based on the mass of S5 0014+81’s supermassive black hole predict that it will live for roughly 1.3 × 1099 years (near the end of the Black Hole Era of the universe, when it is more than 10 88 times its current age), before it dissipates by the Hawking radiation. ^ a b c d e f g h “NED results for object S5 0014+81”.

Is S5 0014+81 the most luminous quasar ever discovered?

S5 0014+81 is a distant, compact, hyperluminous, broad-absorption line quasar or blazar located near the high declination region of the constellation It is shown that, whereas S5 0014+81 is almost certainly the most luminous quasar discovered so far, its other properties are similar to those of other high-z quasars.

What is the most massive black hole in the universe?

This makes it the most massive black hole known in the entire Universe, as massive as the Triangulum galaxy, our local group’s third largest member. Distant, massive quasars show ultramassive black holes in their cores, and their electromagnetic counterparts are easy to detect.

What type of galaxy is S5 0014+81?

The host galaxy of S5 0014+81 is an FSRQ (Flat Spectrum Radio Quasar) blazar, a giant elliptical galaxy that hosts a supermassive black hole at its center. In 2009, a team of astronomers using the Swift spacecraft used the luminosity of S5 0014+81 to measure the mass of its black hole.