Now, in an extensive search of the relatively recent, local universe, University of Colorado at Boulder astronomers said they have definitively found about half of the missing normal matter, called baryons, in the spaces between the galaxies.

This important component of the universe is known as the intergalactic medium and it extends essentially throughout all of space, from just outside our Milky Way galaxy to the most distant regions of space observed by astronomers.

The questions "where have the local baryons gone, and what are their properties?" are being answered with greater certainty than ever before. "We think we are seeing the strands of a web-like structure that forms the backbone of the universe," said CU-Boulder Professor Mike Shull.

"What we are confirming in detail is that intergalactic space, which intuitively might seem to be empty, is in fact the reservoir for most of the normal, baryonic matter in the universe."

Hubble observations made nearly a decade ago by Todd Tripp and colleagues first reported finding the hottest portion of this missing matter in the local universe. That study utilized spectroscopic observations of one quasar to look for absorbing intergalactic gas along the path to the quasar.

Writing in the May 20 issue of the Astrophysical Journal, postdoctoral researcher Charles Danforth and Shull of CU-Boulder's astrophysical and planetary sciences department reported on observations taken along sight-lines to 28 quasars. The analysis probably represents the most detailed look to date at the intergalactic matter within about 4 billion light-years of Earth, Shull said.

Baryons are protons, neutrons, and other subatomic particles that make up ordinary matter such as hydrogen, helium and heavier elements. Baryonic matter forms stars, planets, moons and even the interstellar gas and dust from which new stars are born, said Shull.

Astronomers caution that the missing baryonic matter is not to be confused with "dark matter," a mysterious and exotic form of matter that is only detected via its gravitational pull.

Danforth and Shull looked for the missing baryonic matter by using the light from distant quasars -- the bright cores of galaxies with active black holes -- to probe the spider web-like structure that permeates the seemingly invisible space between galaxies, much like a flashlight shining through fog.

Using the Space Telescope Imaging Spectrograph aboard NASA's Hubble Space Telescope and NASA's Far Ultraviolet Spectroscopic Explorer, the astronomers found hot gases -- mostly oxygen and hydrogen -- which provide a three-dimensional probe of intergalactic space.

The two spacecraft helped the researchers find the spectral "fingerprints" of intervening oxygen and hydrogen superimposed on the quasars' light.

The bright quasar light was measured to penetrate more than 650 filaments of hydrogen in the cosmic web. Eighty-three filaments were found laced with highly ionized oxygen in which five electrons have stripped away, said Shull.

The presence of highly ionized oxygen and other elements between the galaxies is believed to trace large quantities of invisible, hot ionized hydrogen in the universe. These vast reservoirs of hydrogen have largely escaped detection because they are too hot to be seen in visible light, yet too cool to be seen in X-rays, the researchers said.

The oxygen "tracer" was probably created when exploding stars in galaxies spewed the oxygen back into intergalactic space where it mixed with the hydrogen and then was shocked and heated to very high temperatures, Shull said. The team also found that about 20 percent of the baryons reside in the voids between the web-like filaments.

Within these voids could be dwarf galaxies or wisps of matter that could turn into stars and galaxies in billions of years, said the CU-Boulder researchers.

Probing the vast cosmic web will be a key goal for the Cosmic Origins Spectrograph, or COS, a $70 million instrument designed and built by CU-Boulder with Ball Aerospace and Technologies Corp. of Boulder to probe the nearby galaxies and the distant universe. Astronauts plan to install it on Hubble during a servicing mission later this year.

"COS will allow us to make more robust and more detailed core samples of the cosmic web," Shull said. "We predict that COS will find considerably more of the missing baryonic matter in weaker filaments.

"Our goal is to confirm the existence of the cosmic web by mapping its structure, measuring the amount of heavy metals found in it, and measuring its temperature," he said. "Studying the cosmic web gives us information on how galaxies built up over time."

The COS team hopes to observe 100 additional quasars and build up a survey of more than 10,000 hydrogen filaments in the cosmic web, many laced with heavy elements from early stars.

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