Credit: X-ray: NASA, CXC, SAO, E.Bulbul, et al.
Chandra X-ray Observatory
Chandra X-ray Observatory on Flickr
X-Ray Signal May Illuminate Dark Matter Mystery
By Mike Wall space.com | June 24, 2014 04:37pm ET
Two spacecraft have detected a possible signal of dark matter, the mysterious, invisible stuff that makes up most of the material universe.
NASA's Chandra X-ray Observatory and the European Space Agency's XMM-Newton satellite spotted a spike of X-ray emission coming from more than 70 different galaxy clusters. While the origin of the X-rays remains unclear at the moment, they could be generated by the decay of a certain type of dark-matter particle, scientists said.
"We know that the dark matter explanation is a long shot, but the payoff would be huge if we're right," study lead author Esra Bulbul, of the Harvard-Smithsonian Center for Astrophysics (CfA) in Cambridge, Massachusetts, said in a statement. "So we're going to keep testing this interpretation and see where it takes us."
Dark matter is so named because it neither absorbs nor emits light, making it impossible to observe directly. But astronomers know that dark matter exists because it interacts gravationally with the "normal" matter we can see and touch.
In fact, dark matter is thought to make up more than 80 percent of all matter in the universe. But scientists don't know exactly what it is.
Over the years, researchers have proposed a number of exotic particles as candidate components of dark matter, including weakly interacting massive particles (WIMPs), axions and sterile neutrinos — a hypothetical type of neutrino that emits X-rays when it decays.
It's possible that the signal observed by Chandra and XMM-Newton was produced by sterile neutrinos, researchers said. But that's far from a sure thing, they stressed, since the detection of the X-ray spike pushed both observatories to their sensitivity limits.
"We have a lot of work to do before we can claim, with any confidence, that we've found sterile neutrinos," co-author Maxim Markevitch, of NASA's Goddard Space Flight Center in Greenbelt, Maryland, said in a statement. "But just the possibility of finding them has us very excited."
"Normal" matter in the galaxy clusters may also be responsible for the emission (if it is indeed real and not an instrument artifact). But this interpretation doesn't mesh well with current thinking about galaxy clusters and the atomic physics of hot gases, researchers said.
"Our next step is to combine data from Chandra and JAXA's [the Japanese Aerospace Exploration Agency's] Suzaku mission for a large number of galaxy clusters to see if we find the same X-ray signal," said co-author Adam Foster, also of CfA.
"There are lots of ideas out there about what these data could represent," Foster added. "We may not know for certain until Astro-H launches, with a new type of X-ray detector that will be able to measure the line with more precision than currently possible."
Astro-H is an X-ray observatory being developed by JAXA. It's scheduled to be launched to Earth orbit next year.
The new paper was published in the June 20 issue of The Astrophysical Journal.
Follow Mike Wall on Twitter @michaeldwall and Google+. Originally published on Space.com.
X-ray: NASA/CXC/CfA/M.Markevitch et al.; Optical: NASA/STScI; Magellan/U.Arizona/D.Clowe et al.; Lensing Map: NASA/STScI; ESO WFI; Magellan/U.Arizona/D.Clowe et al.
Hot gas in this collision of galaxy clusters is seen as two pink clumps that contain most of the normal matter. The bullet-shaped clump on the right is hot gas from one cluster, which passed through the hot gas from the other larger cluster. Other telescopes were used to detect the bulk of the matter in the clusters, which turns out to be dark matter (highlighted in blue).
Credit: ESA/Hubble
A ghostly ring of dark matter floating in the galaxy cluster ZwCl0024+1652, one of the strongest pieces of evidence to date for the existence of dark matter. Astronomers think the dark-matter ring was produced from a collision between two gigantic clusters.
Credit: Paul Bode and Yue Shen, Princeton University
The illustration shows the distribution of dark matter, massive halos, and luminous quasars in a simulation of the early universe, shown 1.6 billion years after the Big Bang. Gray-colored filamentary structure shows the distribution of dark matter; small white circles mark concentrated "halos" of dark matter more massive than 3 trillion times the mass of the sun; larger, blue circles mark the most massive halos, more than 7 trillion times of the sun, which host the most luminous quasars. The strong clustering of the quasars in the SDSS sample demonstrates that they reside in these rare, very massive halos. The box shown is 360 million light years across.
Credit: P-A Duc/CEA-CNRS/NRAO-NASA
Galaxy NGC5291 (orange, at the center) and its ring of debris (in blue) as seen by the Very Large Array interferometer. Researchers have found evidence for the presence of dark matter in dense star-forming groups (shown in red), where 'recycled' dwarf galaxies exist.
