The Shape of the Universe
Science fiction writers have taken the liberty to describe the Universe as having all kinds of funky shapes. Hey, cosmologists are to blame, for their theories predict a wide variety of possible universes -- all of which are mathematically feasible.
For starters, there's the spherical universe, where an airplane sent in
one direction ultimately comes back around, as is the case on Earth. A triangle
in this universe has angles adding up to more than 180 degrees. Parallel
lines ultimately meet, just like two friends walking parallel to each other
on their way to the North Pole. Cowboys may fancy the hyperbolic universe,
which is saddle shaped. A triangle here adds up to less than 180 degrees.
Then there's the good, old flat universe, which obeys Euclidean geometry:
triangles add up to 180 degrees; parallel lines never meet.
MAP will be able to determine the likely shape of our Universe. So far,
the data points to things being flat. How can we tell this? MAP will measure
a great big "triangle" in the sky and see if it adds up to what a flat, Euclidean-based
universe should be.
Two-dimensional renditions of the possible shape
of our universe: spherical (top); saddle (middle);
flat (bottom). (Click on image to enlarge it.)
Two sides of the triangle are equal: they correspond to the distance that light has traveled from its creation in the Big Bang to the present day. This light is the microwave background, which has traveled about 15 billion light years, and is the afterglow of the Big Bang.
If you have ever studied trigonometry, you know that with the length
of two sides and the enclosed angle, you can determine all the sides and
angles of a triangle (Recall the "side-angle-side"
theorem!). Our angle is that created by the space
between peak temperature differences in the microwave light. MAP will
measure the angle between the peak in temperature differences.
That distance between peaks corresponds to the distance that sound waves
traveled during the first 400,000 years after the Big Bang. The early Universe
was a dense fog of electrons and protons
that didn't clear up for about 400,000 years. Some patches in the fog were
a slightly denser and hotter than others. Vibrations caused by the movement
of matter caused sound waves to ripple through the fog. The sound waves map the distance from one region of high or low density to the next.
So for our triangle, we have one distance across the sky (the sound
horizon distance, which is the distance the sound waves travel for
400,000 years), and an angle, to be determined by MAP. The unknown
distance is the distance the microwave background has traveled since
the last scattering. If the angle is one degree on the sky, as many
scientists predict, then the Universe may be flat. If the angle
between peaks in temperature differences is, say, two degrees, then
sound waves will have had to have covered twice the ground in 400,000
years. This would imply that the Universe is open or curved.
The TOCO experiment in Chile made the first detection, and balloon-borne
experiments and a South Pole telescope have all found that angle to be about
one degree. MAP, with its superior resolution and data-collecting capability,
will be the final word.