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Last Updated:  Monday, 3 March, 2003, 13:23 GMT
Map reveals strange cosmos
By Dr David Whitehouse
BBC News Online science editor


About 300,000 years after Big Bang, matter and radiation "decoupled"
Matter went on to form stars and galaxies; radiation spread out and cooled
Radiation now shines in microwave portion of the electromagnetic spectrum - at a very cold -270.45 deg Celsius
By mapping tiniest temperature fluctuations (mottled colours above) in CMB, astronomers can "see" distribution of matter in early Universe
The best map yet of the Cosmic Microwave Background (CMB) Radiation - the so-called echo of the Big Bang - shows the Universe may not be the same in all directions.

The image has been produced from data collected by the Wilkinson Microwave Anisotropy Probe (Map), which was launched in 2001.

"It is a photo of the most distant thing we can see; our best photo yet," said Dr Max Tegmark, of the University of Pennsylvania, US, who processed the image.

Dr Tegmark and colleagues present the CMB as a sphere: "The entire observable Universe is inside this sphere, with us at the centre of it."

In so doing, the team find something unexpected and so far unexplained in the symmetry of the CMB.

Relic radiation

In producing the image, Dr Tegmark removed all sources of contaminating foreground radiation leaving only the cosmic background itself.

Launched to obtain full-sky images of 13 billion+ year old temperature fluctuations in CMB
Temperature differences correspond to "seeds" that grew to become stars and galaxies
Data help answer questions about age and geometry of Universe
He told BBC News Online that there were many sources of radiation that could "pollute" the CMB. Dust in our galaxy radiates microwaves and electrons moving through magnetic fields give off this radiation as well.

These effects have to be removed if the CMB is to be studied properly.

The radiation that we detect as the CMB comes from a time when the Universe was less than half a million years old; from the so-called recombination era when hydrogen atoms formed in the cooling, expanding fireball of the Big Bang.

It was a time when the stars and galaxies had yet to form. There was only gas.

In general, the relic radiation from these clouds is almost isotropic - the same in all directions.

'Glowing wall'

For decades, astronomers knew there must be secrets about the Universe in the CMB, if only they could observe it at a high enough sensitivity.

Octopole, Tegmark
Octopole: Looking at the symmetry of the CMB, curious patterns emerge
The expected variations in the CMB's intensity turned out to be so hard to detect that it was only in 1992 that they were first seen - variations of about a few parts per million on scales of the same angular diameter as the apparent diameter of the Moon.

The variations in the CMB contain information about the formation of the galaxies, the composition of the Universe and its fate.

Having produced the cleanest map of the CMB yet, Dr Tegmark displayed it in an unusual manner. Instead of a flat projection on a computer screen, he showed the data as ripples on a sphere - "after all the CMB comes from a sphere", he says.

"Space continues outside the sphere but this opaque glowing wall of hydrogen plasma hides it from our view. If we could only see another 380,000 light-years we would be able to see the beginning of the Universe," he told BBC News Online.

Looking for evidence

And he added: "We found something very bizarre; there is some extra, so far unexplained structure in the CMB.

"We had expected that the microwave background would be truly isotropic, with no preferred direction in space but that may not be the case."

Looking at the symmetry of the CMB - measures technically called its octopole and quadrupole components - the researchers uncovered a curious pattern.

They had expected to see no pattern at all but what they saw was anything but random.

"The octopole and quadrupole components are arranged in a straight line across the sky, along a kind of cosmic equator. That's weird.

"We don't think this is due to foreground contamination," Dr Tegmark said. "It could be telling us something about the shape of space on the largest scales. We did not expect this and we cannot yet explain it."

It may mean that the CMB is clumpier in some directions than others. Some theories of the structure of the Universe predict this but observational evidence to support it would be a major discovery.

Universe to expand for ever
14 Feb 03 |  Science/Nature
Telescope finds Big Bang evidence
20 Sep 02 |  Science/Nature
Astronomers hear 'music of creation'
30 Apr 01 |  Science/Nature
Pictures of the early Universe
28 Apr 00 |  Science/Nature

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