BLACK HOLE B lack holes are some of the most interesting pathologies in space and time delivered by Einstein's general theory of relativity. They form when matter collapses gravitationally onto itself, such as when massive stars burn out. They are a region of space where the gravitational pull is so strong that nothing--not even light--can escape. Hence John Wheeler called them "black holes." There is more. They incorporate singularities in spacetime structure: points where Einstein's theory breaks down, since the curvature of spacetime becomes infinite. And they can supply bridges to new universes. S uch a star may become a white dwarf or a neutron star, but if the star is sufficiently massive then it may continue shrinking eventually to the size of a tiny atom, known as a gravitational singularity. A black hole refers to the region in space in which the singularity’s gravitational force is so strong that not even light can escape its pull.
BLACK
HOLE
Black holes are some of the most interesting pathologies in space and time delivered by Einstein's general theory of relativity. They form when matter collapses gravitationally onto itself, such as when massive stars burn out. They are a region of space where the gravitational pull is so strong that nothing--not even light--can escape. Hence John Wheeler called them "black holes." There is more. They incorporate singularities in spacetime structure: points where Einstein's theory breaks down, since the curvature of spacetime becomes infinite. And they can supply bridges to new universes.
Such a star may become a white dwarf or a neutron star, but if the star is sufficiently massive then it may continue shrinking eventually to the size of a tiny atom, known as a gravitational singularity. A black hole refers to the region in space in which the singularity’s gravitational force is so strong that not even light can escape its pull.
Black holes are some of the most interesting pathologies in space and time delivered by Einstein's general theory of relativity. They form when matter collapses gravitationally onto itself, such as when massive stars burn out. They are a region of space where the gravitational pull is so strong that nothing--not even light--can escape. Hence John Wheeler called them "black holes." There is more. They incorporate singularities in spacetime structure: points where Einstein's theory breaks down, since the curvature of spacetime becomes infinite. And they can supply bridges to new universes.
Such a star may become a white dwarf or a neutron star, but if the star is sufficiently massive then it may continue shrinking eventually to the size of a tiny atom, known as a gravitational singularity. A black hole refers to the region in space in which the singularity’s gravitational force is so strong that not even light can escape its pull.
LET US KNOW
SOME FACTS ABOUT BLACK HOLE:
The
mass of a black hole is so dense and the gravity of its singularity so strong
that, in accordance with Einstein’s theory of general
relativity, it actually distorts the space-time around
it and not even light can escape. The boundary beyond which light cannot escape
the black hole’s gravity well is known as the event horizon, while its radius
is called the Schwarzschild radius. Once particles and light-rays go past the
event horizon their light cones “tip over” and point to the singularity, which
now represents all future-directed paths with no escape possible.
Person
falling black hole
If
a person was able to survive long enough to describe falling into a black hole,
he would at first experience weightless as he goes into free fall, but then
feel intense “tidal” gravitational forces as he got closer to the center of the
black hole. In other words, if his feet were closer to the centre than his
head, then they would feel a stronger pull until he eventually is stretched and
then ripped apart. As he falls in he may observe distorted images as the light
bends around him and he will also still be able to see beyond the black hole as
light continues to reach him from the outside.
Freezing
of time
To
an outside observer with a telescope, an object
passing the event horizon will appear to slow down then “freeze” in time without
ever seeming to pass through the event horizon. This is because the light takes
longer to escape the black hole’s gravitational pull and light signals won’t
reach the viewer for an infinitely long time. As time elapses, the
light subsequently becomes red shifted and dimmer as its wavelength becomes
longer, eventually disappearing from the sight of the observer as it becomes
infrared radiation, then radio waves.
Wormhole
Hawking
Radiation
Physicists
now believe that black holes actually radiate small numbers of mainly photon
particles and so can lose mass, shrink then ultimately vanish over time. This
unverified evaporation process is known as “”, after Professor Stephen Hawking who theorized its existence in 1974. However, it
is a staggeringly slow process and only the smallest black holes would have had
time to evaporate significantly during the 14 billion years the Universe has
existed.
It is now thought that most galaxies are held together by supermassive black holes at their centers, which cluster hundreds of solar systems around them. In fact, 30,000 light years away at the centre of our own Milky Way galaxy is a black hole with 30 million times the mass of our own sun.
It is now thought that most galaxies are held together by supermassive black holes at their centers, which cluster hundreds of solar systems around them. In fact, 30,000 light years away at the centre of our own Milky Way galaxy is a black hole with 30 million times the mass of our own sun.
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