X-ray Discovery Points to Location of Missing Matter
Using observations with NASA's Chandra X-ray Observatory and ESA's XMM-Newton, astronomers have announced a robust detection of a vast reservoir of intergalactic gas about 400 million light years from Earth. This discovery is the strongest evidence yet that the "missing matter" in the nearby Universe is located in an enormous web of hot, diffuse gas. This missing matter - which is different from dark matter -- is composed of baryons, the particles, such as protons and electrons, that are found on the Earth, in stars, gas, galaxies, and so on. A variety of measurements of distant gas clouds and galaxies have provided a good estimate of the amount of this "normal matter" present when the universe was only a few billion years old. However, an inventory of the much older, nearby universe has turned up only about half as much normal matter, an embarrassingly large shortfall. Read more
X-ray Discovery Points to Location of Missing Matter
Using observations with NASA's Chandra X-ray Observatory and ESA's XMM-Newton, astronomers have announced a robust detection of a vast reservoir of intergalactic gas about 400 million light years from Earth. This discovery is the strongest evidence yet that the "missing matter" in the nearby Universe is located in an enormous web of hot, diffuse gas. This missing matter -- which is different from dark matter -- is composed of baryons, the particles, such as protons and electrons, that are found on the Earth, in stars, gas, galaxies, and so on. A variety of measurements of distant gas clouds and galaxies have provided a good estimate of the amount of this "normal matter" present when the universe was only a few billion years old. However, an inventory of the much older, nearby universe has turned up only about half as much normal matter, an embarrassingly large shortfall. Read more
Astronomers are claiming the detection via x-rays of a chunk of the universe's ordinary matter. Unlike the famous "dark matter" whose gravity is thought to hold the galaxies together, this more mundane form of missing matter is the stuff of normal atoms. The new observations fit well with the standard model of cosmology and could help test ideas about large-scale structures in the universe. Three ingredients make up the universe. Normal atomic matter accounts for less than 5%, according to analysis of the microwave afterglow of the big bang. About 22% of the universe consists of mysterious dark matter--weighty stuff whose gravity appears to keep the stars from flying out of galaxies and to hold clusters of galaxies together but that has never been directly observed. A whopping 73% of the universe consists of bizarre space-stretching dark energy that's accelerating the expansion of the universe.
Although the universe contains billions of galaxies, only a small amount of its matter is locked up in these behemoths. Most of the universe's matter that was cooked up during and just after the Big Bang must be found elsewhere. 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.
In the May 20 issue of The Astrophysical Journal, Charles Danforth and Mike Shull (University of Colorado, Boulder) report on NASA's Hubble Space Telescope and NASA's Far Ultraviolet Spectroscopic Explorer (FUSE) observations taken along sight-lines to 28 quasars. Their analysis represents the most detailed observations to date of how the intergalactic medium looks within about four billion light-years of Earth. The astronomers say they have definitively found about half of the missing normal matter, called baryons, in the space between the galaxies.
Astronomers detect a part of long-searched baryonic matter in a filament connecting two clusters of galaxies The composition of the Universe still puzzles the astronomers: Over 90 percent consist of unknown matter - three quarters of the mysterious Dark Energy which causes an accelerated expansion of the Universe and about 21 percent of Dark Matter, the components of which the physicists have not yet figured out. Just four percent are composed of the normal material of which we ourselves are made, the so-called baryonic matter. Even this minor part however has not yet been comprehended completely: all discovered stars, galaxies and gases in the Universe amount to less than a half of these four percent. Now a team of astrophysicists from the Max Planck Institute for extraterrestrial Physics (MPE) and the ESO, both in Garching, Germany, and of two institutes in the Netherlands has found evidence of a part of the missing baryons in a bridge-like filament connecting two clusters of galaxies (Astronomy & Astrophysics Letters, May 2008).
ESAs orbiting X-ray observatory XMM-Newton has been used by a team of international astronomers to uncover part of the missing matter in the universe. 10 years ago, scientists predicted that about half of the missing ordinary or normal matter made of atoms exists in the form of low-density gas, filling vast spaces between galaxies. All the matter in the universe is distributed in a web-like structure. At dense nodes of the cosmic web are clusters of galaxies, the largest objects in the universe. Astronomers suspected that the low-density gas permeates the filaments of the web.