Interesting. thanks Billy.

 

  _____  

From: [email protected]
[mailto:[email protected]] On Behalf Of [email protected]
Sent: Wednesday, January 13, 2010 12:22 PM
To: [email protected]
Subject: [RC] 99 . 9 % of the speed of light

 

 <http://www.csmonitor.com/> Christian Science Monitor


Milky Way enigma: Why galaxy's central black hole is silent


The black hole at the center of the Milky Way, called Sag A*, is much less
active than those at the center of other galaxies. A new study points to a
simple answer: heat. 

 

 

By
<http://www.csmonitor.com/layout/set/print/About/Contact/Staff-Writers/Peter
-Spotts> Peter N. Spotts Staff writer 
posted January 7, 2010 at 4:01 pm EST 

One of the Milky Way's longstanding puzzles centers on the super-massive
black hole at its core, in the constellation Sagittarius: Why is that
monstrous black hole, known as Sag A*, so much less energetic that its
counterparts in other galaxies?

The behemoth, with some 2.6 million times the sun's mass, is a cosmic dud at
the moment. Something is starving it, depriving it of material that
otherwise would plummet into it.

Roman Shcherbakov, a researcher at the Harvard-Smithsonian Center for
Astrophysics, says he's figured out what that "something" is likely to be:
heat. 

As material from surrounding stars approaches the black hole and gets
compressed by the monster's gravity, it heats up. Some of that heat gets
conducted away from the black hole, setting up a source of pressure that
sweeps material away from the voracious object.

In other words, heating around the black hole's event horizon - essentially
the boundary within which material falls into oblivion - is in effect
starving the black hole.


The challenges of studying black holes


In presenting his results during the American Astronomical Society's winter
meeting in Washington this week, Dr. Shcherbakov says that building the
process of heat conduction into models of how black holes work began a only
a couple of years ago. 

The processes are so complex that, until recently, "it's been hard to
include them in the models," he adds.

Black holes are objects so massive that their gravity is strong enough to
prevent light from escaping. Yet scientists have developed ways of detecting
them through their effects on the material around them. 

In galaxies with active black holes at their cores, strong magnetic fields
in the black hole's neighborhood accelerate electrons to speeds up to 99.9
percent of the speed of light and collect them into jets that erupt from the
poles of a central black hole. These are visible in a range of wavelengths,
from radio eaves to x-rays.

In addition, the material falling into a black hole heats to the point where
it emits x-rays.


Testing the theory


Shcherbakov and colleague Frederick Baganoff, with the Massachusetts
Institute of Technology, used data from NASA's Chandra X-Ray Observatory as
a reality check on their computer simulations testing the heat-conduction
idea.

Typically, Shcherbakov explains, roughly 1 percent of the material that
surrounding stars exhale as stellar wind reaches the event horizon of a
black hole like Sag A*. If Sag A* was receiving that banquet, it should be
100 times brighter in x-rays than it is. 

Using a long exposure from Chandra, the duo was able to observe the black
hole's activity out to a radius of about 4 light-years. They found that only
0.01 percent of the material one would expect to see ever reaches the black
hole's event horizon.

The observations, Shcherbakov says, "are in good agreement" with the model
results that take heat conduction into account. 

Sag A* hasn't always been this mellow. Last year, for instance, a team of
Japanese astrophysicists reported evidence that x-rays from superheated
material falling into Sag A* briefly flared some 300 years ago. The x-ray
signature at the time would have been a million times brighter than it is
today. 

Heat conduction is not the only explanation scientists have offered up to
explain Sag A*'s current somnolence. Another idea, for instance, involves
stellar explosions called supernovae. So many stars near the center of the
galaxy are popping off this way that the outrush of material from the
explosions in effect is pushing material away from the black hole.

Researchers now face the task of figuring out the relative roles such
mechanisms play in keeping Sag A* on its version of a Weight Watchers
program.

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