Black Holes
Within our galaxy alone, there are millions
upon millions of stars. Within our
universe, there are millions upon millions
of galaxies. Humans have known the
existence of stars since they have had
eyes. Although interpretations may have
differed on what they were, they were
always thought of as white glowing specks
in the sky, but the mystery does
not lie within what we can see, but what we can
not see. There are billions
of stars lighting the darkness of our universe, but
the question lies in what
happens when one of these enormous lamps burns out.
Upon many
speculations, one of the most fascinating is the black hole theory.
Not
any star can become a Black Hole. For instance, the possibility of our
sun
becoming a black hole is highly unlikely, simply because it is too small.
Only a
very large star has the potential to become a black hole. The
definitions of
black boles are somewhat skeptical. Generally, a black hole is
an area of
super-concentrated mass. So concentrated, that no object can
escape its
gravitational pull. In other words, once you get caught by it's
gravitational
pull, you aren't getting out again. The velocity you need to
break away from a
gravitational pull is called the "escape velocity".
Roughly, earth's
escape velocity is about 25,000 M.P.H. (11.2
kilometers/second). Earth's mass is
nothing compared to the mass of a star
that has the potential to become a black
hole. A black hole has so much mass
in such a small area, that its escape
velocity is greater than the speed of
light. So if were all living on earth, and
earth was a black hole, we would
need to go at the speed of light in order to
get to the moon. Even though a
black hole's gravitational pull is enormous, it
does have its boundary. This
boundary is called the "event horizon".
This event horizon is the point
where the black hole's gravitational pull
begins. Once you cross the event
horizon, there is no turning back. As stated
before, the escape velocity of a
black hole exceeds the speed of light, and
since going faster than the speed
of light is impossible, so is escaping a black
hole's gravitational pull.
Inside the event horizon is where the major
speculation begins. Just what
happens once you cross the event horizon? Well,
once you cross the event
horizon, you'll be spinning around the center at the
speed of light. As you
get closer to the center, or what scientists call the
"singularity", the
theory of the spaghetti effect comes into play.
That is, the
gravitational pull of the center of the black hole is greater at
your feet
than your head, thus pulling stronger at your feet, and stretching you
out to
a point of infinite thinness. This same force is what causes the tides in
our
ocean, hence the name "tidal forces". The time in which it takes
you to
witness this effect depends on the size of the black hole. A smaller
black
hole means that its singularity is not far away, thus killing you
quicker.
If you could somehow get into a horizon safely and look around,
images around
you would be distorted. And since light can go into a black
hole, you can see
outside images fine. But light won't be able to bounce of
you and back, so no
one would be able to see you. Although living long enough
to reach the
singularity is just about impossible, if you could reach it; no
one knows what
would happen. Basically, you would be in a place where time
does not exist and
all of Einstein's laws will fail. Evidence that black
holes are real does exist.
Even though you cannot see a black hole, as
light cannot escape it, you can
measure how much mass there is in an area.
And if you have a large quantity of
mass in a small area, there is a good
chance it is a black hole. Black holes do
not live forever, and as stars,
they die. Speculation on their deaths is
extremely speculative. The theory of
black hole evaporation seems to be a
popular theory on how black holes die.
Black holes emit radiation, and the
energy to emit this radiation comes from
the black hole's mass, thus shrinking
the black hole. Gradually, a black hole
wears itself out into nothing. Stephen
Hawkings presented this idea in
the 1970’s which was a great contribution to
physics.