But
since 1915, when Albert Einstein developed his theory of relativity,
scientists have known that black holes may exist. Einstein's theory
proved that if gravity could become strong enough, it would rob light
of all its energy, trapping it in the same way in which it traps a planet's
atmosphere. For gravity to be that strong, however, its source would
have to be an extremely dense object, one with a very large mass compressed
into a very small space.
In
1916 the German astronomer Karl Schwarzschild calculated just how compressed
a star would have to be for its gravity to trap light. According to
Schwarzschild's calculations, a star the size of the sun - 864,950 miles
(1,392,000 kilometers) in diameter - would have to shrink to less than
1.9 miles (3 kilometers) wide.
In
1939 the United States physicists J. Robert Oppenheimer and Hartland
S. Snyder discovered that it is possible for stars much larger than
the sun to become this small. For most of their lives, stars remain
a constant size because they contain a balance of forces: heat generated
by burning fuel expands the star outward, while the force of gravity
pulls it in. Eventually, in billions of years, the star exhausts its
nuclear fuel and collapses under its own weight.Oppenheimer
and Snyder proved that if the star is more than 3.2 times as massive
as the sun, nothing could stop the collapse.
Scientists
believe that the Earth's galaxy, the Milky Way, may harbor as many as
100 million black holes left behind by collapsed stars. In 1990 the
Very Large Array radiotelescope in New Mexico obtained detailed images
of the center of the Milky Way showing tremendous bursts of energy emanating
from its center. Some scientists believe this confirms the existence
of a black hole with four million times the mass of the sun at the center
of the Milky Way.
Scientists
using the Hubble Space Telescope in 1992 found promising signs of a
black hole with three million times the mass of the sun in a nearby
galaxy. Because black holes are invisible, astronomers have been trying
to locate them by observing their effects. Matter swirling toward the
center of a black hole should emit rapidly pulsating and detectable
X-rays. In 1965 astronomers observed intense X-rays radiating from the
constellation Cygnus, nearly 10,000 light-years away. In 1971 the world's
first X-ray satellite pinpointed the exact location of these X-rays,
a massive but invisible object that astronomers have named Cygnus X-1.
Cygnus X-1 may prove to be the first identified black hole.
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