The Milky Way Galaxy is at the center of an enormous ‘halo’ of hot gas extending for hundreds of thousands of light years, according to new evidence gathered by NASA’s Chandra X-ray Observatory. The mass of the halo is estimated to be similar to the mass of all the stars in the Milky Way combined.
Once confirmed, this will be the first explanation for the “missing baryon problem,” as it’s known to astronomers.
From the NASA/Harvard press release:
“Baryons are particles, such as protons and neutrons, that make up more than 99.9 percent of the mass of atoms found in the cosmos. Measurements of extremely distant gas halos and galaxies indicate the baryonic matter present when the universe was only a few billion years old represented about one-sixth the mass and density of the existing unobservable, or dark, matter. In the current epoch, about 10 billion years later, a census of the baryons present in stars and gas in our galaxy and nearby galaxies shows at least half the baryons are unaccounted for.”
“In a recent study, a team of five astronomers used data from Chandra, the European Space Agency’s XMM-Newton space observatory and Japan’s Suzaku satellite to set limits on the temperature, extent and mass of the hot gas halo. Chandra observed eight bright X-ray sources located far beyond the galaxy at distances of hundreds of millions of light-years. The data revealed X-rays from these distant sources are absorbed selectively by oxygen ions in the vicinity of the galaxy. The scientists determined the temperature of the absorbing halo is between 1 million and 2.5 million kelvins, or a few hundred times hotter than the surface of the sun.”
There have been other studies done that have measured the Milky Way and other galaxies as being “embedded in warm gas with temperatures between 100,000 and 1 million kelvins. Studies have indicated the presence of a hotter gas with a temperature greater than 1 million kelvins.” The new research is providing good evidence that the warm gas halo around the Milky Way is greatly eclipsed in size by the massive hot gas halo.
“We know the gas is around the galaxy, and we know how hot it is,” said Anjali Gupta, lead author of the The Astrophysical Journal paper describing the research. “The big question is, how large is the halo, and how massive is it?”
Here’s more from the press release:
“To begin to answer this question, the authors supplemented Chandra data on the amount of absorption produced by the oxygen ions with XMM-Newton and Suzaku data on the X-rays emitted by the gas halo. They concluded that the mass of the gas is equivalent to the mass in more than 10 billion suns, perhaps as large as 60 billion suns.
“‘Our work shows that, for reasonable values of parameters and with reasonable assumptions, the Chandra observations imply a huge reservoir of hot gas around the Milky Way,’ said co-author Smita Mathur of Ohio State University in Columbus. ‘It may extend for a few hundred thousand light-years around the Milky Way or it may extend farther into the surrounding local group of galaxies. Either way, its mass appears to be very large.’
“The estimated mass depends on factors such as the amount of oxygen relative to hydrogen, which is the dominant element in the gas. Nevertheless, the estimation represents an important step in solving the case of the missing baryons, a mystery that has puzzled astronomers for more than a decade.
“Although there are uncertainties, the work by Gupta and colleagues provides the best evidence yet that the galaxy’s missing baryons have been hiding in a halo of million-kelvin gas that envelopes the galaxy. The estimated density of this halo is so low that similar halos around other galaxies would have escaped detection.”
The new research paper was just published in the September 1st issue of The Astrophysical Journal.
Image Credits: NASA/CXC/M.Weiss; NASA/CXC/Ohio State/A Gupta et al; X-ray: NASA/CXC/U.Mich./S.Oey, IR: NASA/JPL, Optical: ESO/WFI/2.2-m