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Dark Matter (or, May the Force be with you!)
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So far we know how old (and hence how big) our Universe is. It started
with a Big Bang about 13.7 billion years ago -- at least that is the
number we come up with using the best data and ideas we have today.
While looking far back in time (that is what telescopes do, you know)
with our nifty new high tech telescopes to come up with this data we
found some wonderful things.
Back in 1905 Albert Einstein published his first paper on the
Theory of Relativity. Einstein realized that the best way
of demonstrating that his new theory might be correct was to
measure the stars very near the Sun during a total eclipse.
Relativity predicted that the mass of the Sun would warp
or bend space/time enough that, during a total eclipse,
we should be able to see stars that were behind the Sun.
The starlight would bend around the Sun. Well the first few
times this measurement was attempted they were declared true --
the starlight was bent! We know now that these first few
tries weren't really accurate enough to prove relativity
but the measurement has been done many times since and no one
doubts that mass bends light.
While looking at distant galaxies with our spiffy new
telescopes, astronomers have found the ultimate light
bending. We have found many examples of one galaxy in front
of a much more distant galaxy (or sometimes a quasar).
When this happens the mass of the closer galaxy acts like
a lens and bends the light from the more distant galaxy
around it. We see the image of the distant galaxy as
rings, arcs or multiple images around the closer galaxy.
This is really cool! Check out Einstein's Cross
at: http://members.aol.com/anonglxy/einstein.htm
and lots more gravitational lensing pictures at:
http://hubblesite.org/newscenter/newsdesk/archive/releases/1995/43/
While demonstrating Relativity in a big way, the gravitational
images created a problem for astronomers. The light from the
distant galaxies was bent WAY more than could be explained
by totaling up all the stars in the closer galaxy. Something
massive and non-luminous (didn't give off light) was lurking
in that closer galaxy.
The Total Perspective Vortex
So, we have a problem. It is pretty easy to estimate how many stars
there are in a galaxy. We can also give a fair guess how much other
non-stellar (not stars) matter there is in a galaxy because all
the dust, gas, planets, asteroids, comets, etc. absorbs starlight and
re-emit that light as infrared (heat) and we can measure this. Still,
when we measure how much the light from a more distant galaxy is bent
by the mass of a closer galaxy, we are still off by a huge amount.
This means that the galaxies we measure seem to have lots and lots more
stuff in them than we can see!
Galaxies do another strange thing. In our solar system we see that
all the planets obey the laws of gravity as explained to us by Newton,
Einstein, and Kepler. Basically, all the planets are independent and the
more energy (speed) they have, the farther out from the Sun they orbit.
This means that all the planets influence each other but each travels
at a different speed around the Sun. Galaxies don't seem to do this.
By the laws of gravity, the stars should be moving independently in
a galaxy. But what we see is that galaxies rotate (did I mention
galaxies rotate?) more like a frisbie; as if it were a solid disk
and the stars farthest out from the center are moving WAY too fast.
It is as if the stars in the galaxy are embedded in something large,
massive and invisible. Astronomers call this stuff Dark Matter,
on the theory that if you don't know what something is, giving it a name
makes you feel better about it.
I know what you're thinking, but you're wrong. You're thinking that
this mysterious dark matter is just lots and lots of ordinary stuff
like very dim stars, comets, planets, dust, gas, etc. that we just
aren't seeing. Well, that's pretty much what astronomers thought for
lots of years. With our newer and better telescopes we are now pretty
sure that all the luminous stars we can see account for about 10% of the
ordinary matter in a galaxy.
If this were the only problem, astronomers could probably live with
it and just keep looking for hidden matter. Unfortunately, with
our new telescopes and vast computing power, astronomers were able,
in the last few decades, to make 3 dimensional maps of how galaxies
were scattered through the Universe. The huge surprise to astronomers
was that galaxies were NOT spread evenly though out the Universe -- not
even close to it. Galaxies were clumped into groups and super groups
and long, long chains, filaments, and walls of galaxies that went on and
on for millions of light years. Even stranger was that there are HUGE
bubbles of nothing; vast areas with few or no galaxies. The problem is
that all of the ordinary matter in the Universe still seems to be only
1/10th the amount necessary to cause this kind of enormous structure.
If what we think we know about the Big Bang is correct, then we can
account for pretty much all the ordinary matter in the Universe.
We must be seeing the effect of some kind of invisible exotic stuff
that we know nothing about. 90% of the mass of the Universe must be
made of something other than the electrons, protons, neutrons, and the
other particles we know and love.
Something massive and "invisible" early in the history of the Universe
used it's gravity to clump "ordinary" matter together to form stars,
galaxies, and those huge structures (walls, filaments, bubbles) of galaxies.
Physicists are pretty sure they can account for all the ordinary matter in
the universe. This invisible stuff wasn't "ordinary" and it seems
to be still around today. Astronomers call this "stuff" Dark Matter,
on the theory that if you don't know what something is, giving it a name
makes you feel better about it.