Theory: Black hole winds allow some matter to escape
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Matter can escape from a black hole through supersonic winds originating in an accretion disk, like this one in the galaxy NGC 7052
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(CNN) -- Black holes might produce great winds that allow
some matter to escape their deadly clutches, scientists said
Wednesday. The new theory could reconcile a conflict between
theoretical models and observational data on black holes.
Black holes are thought to be so dense that not even light
can escape their gravitational pull once it crosses over its
theoretical border, known as the event horizon. But astronomical
observations have revealed unexplained outflows of matter from
the vicinity of black holes.
"We often think of black holes pulling in matter, but
actually what we observe with our current instrumentation is
matter flying out," said Timothy Kallman of NASA's Goddard
Space Flight Center in Maryland in a statement.
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This NASA movie shows a clumpy, high-velocity stream of a UV-driven particle wind emanating from a black hole accretion disk. The colors represent the density of particles that make up the
wind. Yellow is the most dense region, followed by red, green and blue (the least dense)
696 K / 6.12 sec. / 320x240
QuickTime movie
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"We couldn't explain exactly what was going on, and this led
to a certain level of uncertainty in what the data were
saying. Now we can start to explain what we've been seeing,"
added Goddard's Daniel Proga, who along with Kallan and
several other scientists presented the theory at a space
research conference in Poland.
Astronomers think that some matter escapes black holes
through particle jets shooting from the poles of the giant
collapsed stars.
The new theory, however, suggests that additional matter is
spared by supersonic winds generated in a swirling mass of
matter around the equatorial region of a black hole, the
accretion disk.
Proga and his colleagues hypothesize that intense ultraviolet
light emanating from the accretion disk region produces two
types of winds.
Together they produce a shield that allows certain types of
matter in the outer regions of the accretion disk area to
sail away to safety, according to the Greenbelt,
Maryland-based Goddard center.
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