The Largest Black Holes in the Universe
Mass of 18 Billion Suns a Supermassive Black Hole Can Tear Apart a Star



The Largest Black Holes in the Universe
Mass of 18 Billion Suns a Supermassive Black Hole Can Tear Apart a Star


We've never seen them directly, yet we know they are there, lurking within dense star clusters or wandering the dust lanes of the galaxy, where they prey on stars, or swallow planets whole. Our Milky Way may harbor millions of these black holes, the ultra dense remnants of dead stars.


The Black Hole

Disney's movie The Black Hole is an older movie regarding super-massive black holes in the universe.


The crew of the spaceship Palamino stumbles across the ''lost'' ship U.S.S. Cygnus, hovering on the edge of an immense black hole.

Once aboard, they find the ship is manned by robots - it's only human inhabitant, one Dr. Hans Reinhardt; an eminent scientist, missing for the past twenty years.

His plan - to enter the Black Hole . . . Whether Dr. Reinhardt is a genius or a mad-man, one thing is for sure, he will not be denied his life's dream.

What lies beyond the Black Hole? Immortality . . . or, Oblivion . . . ?


Now, in the universe far beyond our galaxy, there's evidence of something even more ominous then just a regular-sized black hole: a breed of black holes that have reached incomprehensible size and destructive power.

How big can they get? What's the largest so far detected? Where does an 18 billion solar mass black hole hide? The most massive known black hole in the universe has been discovered, weighing in with the mass of 18 billion Suns.

Observing the orbit of a smaller black hole around this monster has allowed astronomers to test Einstein's theory of general relativity with stronger gravitational fields than ever before.

The black hole is about six times as massive as the previous record holder and in fact weighs as much as a small galaxy.

It lurks 3.5 billion light years away, and forms the heart of a quasar called OJ287. A quasar is an extremely bright object in which matter spiralling into a giant black hole emits copious amounts of radiation.

But rather than hosting just a single colossal black hole, the quasar appears to harbour two - a setup that has allowed astronomers to accurately 'weigh' the larger one.  


Supermassive Black Holes

A supermassive black hole is a black hole with a mass in the range of hundreds of thousands to tens of billions of solar masses.

It is currently thought that most, if not all galaxies, including the Milky Way, contain a supermassive black hole at their galactic center.

The smaller black hole, which weighs about 100 million Suns, orbits the larger one on an oval-shaped path every 12 years.

It comes close enough to punch through the disc of matter surrounding the larger black hole twice each orbit, causing a pair of outbursts that make OJ287 suddenly brighten.

General relativity predicts that the smaller hole's orbit itself should rotate, or precess, over time, so that the point at which it comes nearest its neighbor moves around in space - an effect seen in Mercury's orbit around the Sun, albeit on a smaller scale.
 



Supermassive Black Hole in the Milky Way Galaxy

From a distance, our galaxy would look like a flat spiral, some 100,000 light years across, with pockets of gas, clouds of dust, and about 400 billion stars rotating around the galaxy's center.

Thick dust and blinding starlight have long obscured our vision into the mysterious inner regions of the galactic center.

And yet, the clues have been piling up, that something important, something strange is going on in there.

Astronomers tracking stars in the center of the galaxy have found the best proof to date that black holes exist. Now, they are shooting for the first direct image of a black hole.


From a distance, our galaxy would look something like this. A flat spiral, some 100,000 light years across, with pockets of gas, clouds of dust, and about 400 billion stars rotating around the galaxy's center.

That center -- bulging up and out of the galactic disk -- is tightly packed with stars. Thick dust and blinding starlight have long obscured our vision into the mysterious inner regions of this so-called "bulge." And yet, the clues have been piling up, that something important...something strange... is going on in there.

The first to take notice was the physicist Karl Jansky back in the 1930s. He was asked by his employer, Bell Telephone Labs, to investigate sources of static that might interfere with what it saw as the killer app of its time... radio voice transmissions. Using this ungainly radio receiver... Jansky methodically scanned the airwaves.

He documented thunderstorms, near and far... and another signal he could not explain. It sounded like steam -- a hiss of radio noise. Jansky narrowed it to a spot in the constellation of Sagittarius, in the direction of the center of the galaxy. Located within a larger pattern of radio emissions... ... Jansky's sighting would become known as Sagittarius A*.

The word of Jansky's finding got out. He assured the public that it was not aliens seeking contact.But that's just about all anyone could say... for over three decades. Then Erik Becklin got on the case.Becklin is one of those rare researchers whose curiosity and determination push our understanding to a whole new level.

It was the 1960's and astronomy, like society, was in a period of ferment. Startling new observations were being made... and new interpretations were in the air. Quasars had just been discovered... extremely bright beacons of light from deep space. Were they coming from the centers of distant galaxies? And what powerful objects were generating them?

To study an event at the center of a galaxy, you have locate it.

Young Becklin first took aim at our neighboring galaxy, Andromeda. In ultraviolet light, you can see a dense glow in the middle.

Becklin found the point where the light reaches peak intensity... and marked it as the Center.


From our orientation in space, all of the Andromeda galaxy is in full view.

But our galaxy is a different story. We live inside it, of course. Becklin had to find a way to see through all the dust and gas that obscure our line of sight into the center. So he went to a military contractor......and obtained a device that reads infrared light... whose wavelengths are similar to the distances between particles in a dust cloud, allowing them to move right through.


Becklin began measuring the brightness of the light as it rose to a peak... marking the location of the galactic center. Pinpointing this site would now allow astronomers to begin probing for details with a new generation of powerful telescopes... to peer into the bright lights... the forbidden zones... deep in the heart of the Milky Way.

Becklin wasn't the only astronomer interested in the galactic center. Reinhardt Genzel, and a team based at the Max Planck Institute for Extraterrestrial Physics in Germany, began a similar campaign in 1990... from the New Technology Telescope in the mountains of Chile.

A few years later, in 1993, high atop Hawaii's Mauna Kea volcano...Eric Becklin and colleagues, including Andrea Ghez, began using the newly christened Keck Telescope.

The American and German groups shared the same goal... to pinpoint the precise location of Sagittarius A*, and find out what it is. Because the object is too small to see at 26,000 light years away... they would study it by tracking the orbits of stars around it.

Even seeing them would take the sensitivity of Keck's wide aperture; an instrument powerful enough to detect a single candle flame at the distance of the moon. Meanwhile, using a similar technique, astronomers had focused the new Hubble Space Telescope on a different galaxy... a giant elliptical cloud of nearly a billion stars, lying some 50 million light years away called M87.