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HIGH GRAVITY FROM BLACK HOLES
The science article in the last issue of
Homeward (entitled "Black Holes in Outer Space") explained how
science uses a body of ideas (in scientific terms, a mathematical model) for accurately
describing nature. This body of ideas is termed 'theoretical physics', or
'physical theory' for short. The article explained further how real and genuine
science chooses to use this body of ideas for explaining and when applicable,
for manipulating nature, because of the very simple reason that physical theory
'works' every time it is ever used, error free (although the applications of
our interpretations of it certainly don’t seem to be).
To date, this body of ideas we
call physical theory is absolutely failure free. This is why, among countless
other applications, it - AND NO OTHER BODY OF IDEAS - is used for designing
television sets, microwave ovens, radar, computers, and oh yes, for launching
space craft into precise orbit and keeping them there for decade after
decade. Theoretical physics makes these
achievements possible and every one of these achievements would be flatly
impossible without the tool of theoretical physics.
Physical theory has two sides.
One side is a description of the space and time of nature. This is the theory
of gravity (the subject of this article), which is the Theory of Relativity.
Relativity describes how space and time 'tilt' (special relativity) and 'bend'
(general relativity) as a consequence of motion and mass (effectively,
'weight'), which introduces the other physical theory that describes everything
that isn’t gravity, which includes, among other things, any physical entity
with mass (again, mass is effectively 'weight'). This theory is the theory of
energy, the Theory of Quantum Mechanics, which, to say the least, makes some
remarkable (to the point of being counterintuitive) statements about nature.
But, this article deals with gravity, which is the realm of relativity, not
quantum mechanics, so we will have to wait to examine this other theory (for
energy) in subsequent editions of Homeward and deal strictly with gravity for
the moment.
The description of how (among
other effects still yet to be mentioned) the pace of time slows, compared to
how someone experiencing less gravity measures that same pace (of time), as a
consequence of the effects of gravity - the greater the gravity, the more
pronounced the slowing of time - is a direct outcome of equations and
fundamental assumptions (called axioms) of relativity (the Lorentz
transformations and derivations thereof). We explored this effect of time
slowing with gravity at its most extreme limit by exploring the effects of
gravity at the surface of what are the bodies in the universe where the effects
of gravity are greatest: on black holes.
Black holes are so called
because a black hole's 'weight' (meaning its mass) and the density of that
weight (of that mass) is so great that a black hole's gravity prevents it from
emitting any light at all, directly. In short, a black hole is a "dark
star" - a star that emits no light (again, directly). In short, a black
hole is a super dense and 'heavy' (massive) apparently former star that is
darker than the darkest night. It is called a "hole" instead of a
star though, because this kind of dark object is like a one-way
"exit" from the universe around it (hence the term, 'hole').
A black hole seems as though it
is formed as the result of an enormous star "burning up" (that is,
exhausting) all the nuclear fuel that is constantly "holding it up",
keeping it big and thus preventing its material from collapsing upon itself and
concentrating into a smaller volume.
The energy of the star and its
capacity to resist collapse against gravity are finite, which is to say that
they are limited. This energy lasts for only so long. Eventually, this energy
will become depleted to the point that the force of gravity will overcome the
energy of the star to resist it. Without sufficient energy being released to
counterbalance the immense gravity that is the outcome of the black hole's
immense weight (immense mass), gravity overcomes energy and the star collapses
inwardly, shrinking into a smaller volume.
Upon, collapsing, if a star is
heavy (i.e. massive) enough, then it collapses into a black hole, in this way
placing its contents in the closest proximity physically possible;
concentrating matter to the absolute limit that it can be concentrated in our
universe. As a consequence, black holes literally "sink" into space
and time, thus "separating" from the rest of the universe, leaving
behind afterward, only a one-way, gravity-powered "exit" from the
universe as we know it, like the drain at the bottom of an infinitely deep
(bottomless) sink.
What is left after a star
collapses into a black hole is a body that is so heavy (massive) and its
enormous weight (enormous mass) so concentrated that it exerts at its surface
more gravitational force than any other kind of body in the universe - in fact,
as much force as gravity is capable of exerting. Now, returning again to the
fact that time slows as the force of gravity increases, and the force of
gravity at a black hole's surface being as great as it can physically ever be
in the universe means that time slows there, as much as it can ever slow in the
universe - again, according to relativity's failure free description of nature:
infinitely, which means time slowing to the point of 'stopping' altogether.
As a consequence of time at a
black hole's surface slowing infinitely to the point of stopping altogether, a
black hole's surface is always 'locked' into a single moment, a moment that
'never' has enough time to pass, and that is, from the perspective of anyone
removed from the black hole's surface, a 'frozen' moment that is seemingly
eternal in duration. On the other hand, if you are 'there' at the surface,
where, according to the fundamental assumption of relativity the pace of time
never changes, except according to the perspective of another subject to
different gravity (though different motion accomplishes a different
perspective), time would be passing no differently at the surface from how it
would be passing anywhere else, even if a moment requires, again, according to
a perspective outside, an eternity for any single moment to pass.
So, it would appear that,
although it might take an eternity to approach a black hole's surface with the
laws of physics remaining the same all the while, it would seem possible to
make a journey toward such a surface, at least in principle - except for a
single yet extremely significant detail. Entering feet first, at some point
your toes would begin falling (accelerating) toward the surface faster than
your ankles, which would be falling faster than your calves, which would be
falling faster than your knees, and so on up your body. Each individual part of
the body falling faster than that attached above it would tear one’s body limb
from limb, from the bottom up, one atomic particle at a time, starting at your
toes and ending at you head, just as would be the case for any craft that you
might be a passenger aboard at the time, no matter how well made the it might
be. No material exists (or could ever be fabricated – there exists a physical
limit) would be able to resist the force.
Understanding black holes is
worthwhile because black holes are examples of the most extreme expression of
(i.e. a limit condition for) relativity. Black holes are interesting because
they capture our imagination with phenomena that (ordinarily) we can only
barely imagine (unless we practice imagining altogether new concepts, as
physicists do). But, interesting as it might be to study, a black hole is no
place that you would ever want to even try
to visit. Their overwhelming gravity makes them as unlikely place for life
surviving as could ever be imagined. Besides, the nearest one is trillions upon
trillions of miles away and a lifetime would not be long enough to make a dent
in the journey - but you never know, because by virtue of the fact that black
holes emit no light, were one approaching our solar system, we could never
'see' it coming, though we might happen to notice its arrival when our
neighbor’s clock started running a little slower than our own. Upon getting
near however, we would begin feeling its gravity more and more, reeking widespread
havoc on local planetary motion, which would spell certain doom for us, the
very “discoverers” of black hole phenomena, who, as a final note, would learn
the unquestionable validity of the conclusions of their physical theory, with
regard to black hole dark stars.
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© 2007 Chongo
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