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Based on the latest WMAP data analysis, most astronomers think that the universe is perhaps finite – or at least that there is a slight statistical bias towards being finite. Finite here could still mean extremely large though, approaching infinite size.
There is however a group that suggest that the universe could be finite and relatively small. Indeed, as Jean-Pierre Luminet describes, we could be living in an exotic universe shaped rather like a soccer ball! This "soccer ball universe" could even be playing tricks on us and create the illusion of a very large universe. Here's how.
Fig. 1: Dodecahedron 
If you look carefully at Figure 1, you will see an Earth-like object at the center, with some images of this object in a number of places. It is somewhat like when you stand at the center of a dodecahedron formed with mirrors as interior sides. As you look around in all directions, you will see a dozen or more images of yourself.
Essentially, this theory says that we may be seeing a dozen copies of our dodecahedron universe, just slightly rotated and slanted. Actually, it does not say that we see reflections. It's more like in computer games where when an object disappears off your screen on one side, it immediately appears on the diametrically opposite side of the screen.
In this case, it is not objects that instantly jumps to a position on diametrically opposite sides of the screen, but light (photons) that leaves the screen and does this reappearing trick. Sounds silly? You bet, but read on...
Figure 2 shows the WMAP data as a solid line and the so-called "concordance data" from three different cosmological model variations. Concordance here means that it is the flat ΛCDM model with different effects factored in. The specific models are not important, but note the general agreement and also disagreement of all three models with the WMAP measurements.
Fig. 2[1] 
The x-axis is angular scale in degrees and the y-axis the temperature two-point correlation function in micro-Kelvin squared. The models give a good overall fit to the CMB anisotropy on small and medium scales, but there remains a strange discrepancy at larger scales, as first observed by COBE and later confirmed by WMAP.[1]
Enter the "dodecahedron model" as described above. Given that the universe is just closed, with Omega = 1.020, this is how the model fits the observational data:
Fig: 3[1]
The solid line again represents the WMAP data (with Omega = 1.020), the blue-gray shading the one-sigma deviation of the observed data and the dotted line the dodecahedron model's plot. Amazing!
Does this mean that the standard ΛCDM model is overturned? Not quite, but it is very intriguing! What do you think?
Reference:
[1] http://arxiv.org/abs/astro-ph/0412569 v2, Feb. 2005
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