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Hubble reveals cosmic framework

The first 3-D map of dark matter reveals the "scaffolding" for building the universe we know.
Cosmos volume
Hubble, XMM-Newton, and powerful ground-based telescopes provided data that let astronomers create this 3-D map of dark matter. Clumping of the dark matter is more pronounced in the more recent times (left) than in the early universe (right).
NASA / ESA / R. Massey (Caltech)
January 8, 2007
An international team of astronomers has created the first three-dimensional map of dark matter. The project, the largest ever undertaken with the Hubble Space Telescope, provides the first direct look at the large-scale distribution of dark matter in the universe.

"For the first time, we've been able to map out this invisible and mysterious dark matter," says Caltech's Richard Massey. Dark matter — a substance known only by its gravitational effect on normal matter, like stars, planets, and galaxies — accounts for most of the universe's mass.

The milestone study required nearly 1,000 hours of Hubble time over 2 years, 400 hours of observations with the European Space Agency's XMM-Newton X-ray satellite, and galaxy color data from the Subaru, Keck, and CFHT telescopes in Hawaii and the European Southern Observatory's Very Large Telescope in Chile.
COSMOS results
By measuring how dark matter bent light from distant galaxies, the COSMOS team created this false-color plot of the distribution of dark matter.
NASA / ESA / R. Massey (Caltech)
Astronomers acquired 575 images using Hubble's Advanced Camera for Surveys covering a 2-square-degree patch in Sextans. "This is 9 times larger than any previous Hubble survey," says Caltech's Nick Scoville, who led the Cosmic Evolution Survey (COSMOS) project.

XMM-Newton mapped the hot gas in the survey region's galaxy clusters. This X-ray-emitting gas constitutes about 4 times the mass of a galaxy cluster's stars. Ground-based telescopes provide the color information that allowed astronomers to determine how distant the galaxies are.

But the detailed Hubble images allowed the team to glimpse weak gravitational lensing — distortions in the shapes of background galaxies caused by intervening dark matter.
visible COSMOS
This false-color image shows the distribution of normal matter in the COSMOS map. The brightest clumps correspond to the greatest density of matter.
NASA / ESA / R. Massey (Caltech)
"If you place some dark matter in the way, this dark matter — through its gravity — bends the path of light," explains Massey. The result is a 1- to 2-percent distortion of a galaxy's shape. "We understand statistically what those galaxies are supposed to look like," he says. "As the light gets deflected, it distorts the shapes of the background galaxies. So, we end up seeing them in a distorted way, as if through lots of little lenses — and each of those lenses is a bit of dark matter."

"This is the first clear view of the cosmic web," says team member Richard Ellis of Caltech. The largest visible structures are filaments spanning 60 million light-years and containing some 2 trillion times our Sun's mass. But because the COSMOS map includes information about the distance of objects, it's also the first direct measure of the growth of galaxies in dark matter over time.

More distant "slices" of the map show the state of the universe at earlier times. The astronomers termed this "cosmopaleontology."

"Dark matter collapsed first," says Massey. "Without it, the universe as we know it today wouldn't exist." The map shows visible galaxies then formed within the framework established by dark matter.

"This is a tremendously exciting time," says Ellis, noting that the weak-lensing technique is only about 6 years old. "This is now a fundamental tool of cosmologists."

The astronomers presented their findings yesterday at the American Astronomical Society meeting in Seattle.
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