- Black holes are formed from the remnants
of collapsed stars. A black hole consists of a large mass squashed so much
that not even light can escape from its force of gravity.
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- For many years scientists have speculated
that at the centre of our galaxy there may be a great concentration of
matter in the form of a supermassive black hole. Now they have some evidence
for it.
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- It has been found because of the black
holes gravitational effect on nearby stars and gas clouds.
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- Using the Keck telescope atop the Mauna
Kea extinct volcano in Hawaii, astronomers have tracked the movements of
200 stars near the galactic centre.
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- Some of them displayed signs of influence
by extreme gravitational forces.
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- These stars are spiralling around the
black hole at speeds of up to three million miles per hour - about 10 times
the speed at which stars typically move.
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- To account for these speeds it is estimated
that an object 2.6 million times more massive than the sun must be concentrated
into a single black hole.
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- The centre of our galaxy lies 30,000
light years away behind vast clouds of stars, gas and dust.
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- To peer through this obscuration the
scientists used a technique called infrared speckle interferometry. The
procedure involves taking thousands of high-speed, high-resolution snapshots.
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- Using this technique in 1995, scientists
witnessed the disappearance of a star that was, at the time, the closest
object to the black hole.
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- Whether the star was sucked into the
black hole, or simply went behind it, scientists may never know.
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