Despite the much higher quality of the measurements than any previously available, the 'concordance model universe' still matches the data well. The one significant change is that WMAP seems to detect much higher polarization on very large angular scales (> 20o) than expected. This suggests that the first stars or quasars formed, and re-ionized the Universe, much earlier than previously thought, at a redshift of about z 17, only a few hundred million years after the Big Bang.
The WMAP team got their most precise results by combining the WMAP data with other measurements of fluctuations on smaller scales: the ACBAR measurements of high-l CMB fluctuations, the 2DF Galaxy Redshift Survey for the present-day power spectrum of the large-scale structure, and data from the forest of hydrogen absorption lines found in the spectra of distant quasars, which measures fluctuations in the intergalactic gas on scales equivalent to l of several thousand. Together, these data provide remarkably tight constraints on the parameters of the Universe: for instance the age of the Universe is calculated to be 13.7±0.2 billion years (almost exactly three times the age of our Solar System). These numbers should be treated with a pinch of salt, since they rely on all the different experiments being correct within their quoted uncertainties, i.e. no systematic errors. There is tantalizing evidence that the initial spectrum of fluctuations produced by inflation (or whatever) is not a pure power law; if true this would, for the first time, allow us to go beyond the vague predictions of inflation as a scenario and begin to test some specific physical theories of how it happened.
Finally, the WMAP results confirm an earlier result from COBE, that there is surprisingly little structure in the CMB on the very largest scales, measured by the all-sky quadrupole (l = 2) and maybe octopole. This has prompted some fascinating speculation that we do indeed live in a topologically compact universe; but the smoking gun of identical circles on the sky has not (yet) been found.
This was a relatively quite year for CMB results. The VSA and the CBI have both released new, more precise measurements which continue to confirm the WMAP results, including the hint of a more complicated initial spectrum of fluctuations than a pure power law. See the VSA press release on the Jodrell Bank web site for more details. Meanwhile, a number of ground- and balloon-based experiments are beginning to take data for detailed studies of the CMB polarization.
WMAP will continue to observe until late 2005, along with more than a dozen ground and balloon-based experiments. Many new results are expected, especially on CMB polarization and the mysterious 'excess' small-scale fluctuations detected by the CBI. At a recent conference on the CMB, Professor Joe Silk of Oxford University chose to deliberately mis-quote Winston Churchill:
"This is not the end. It is not even the beginning of the end. But it is the end of the beginning."