X-ray light from the Perseus cluster of galaxies may finally reveal the true nature of one of the most mysterious substances in the cosmos: dark matter.
Dark matter is a bizarre material that does not emit light or energy, yet is thought to make up about 85 percent of the matter in the universe.
Researchers use creative and indirect observations to deduce dark matter's presence, but it remains challenging to pin down solid evidence of the substance's existence. Thanks to mounting observations by NASA's Chandra X-ray Observatory, a Japanese-led X-ray telescope known as Hitomi and the European Space Agency's (ESA) XMM-Newton, scientists may be on the verge of a groundbreaking discovery about the mysterious material, researchers said in a statement from the Chandra X-Ray Center in Cambridge, Massachusetts.
The subject of study is the Perseus cluster, a dusty region of galaxies gathered together 250 million light-years from Earth. Scientists estimate that the Perseus cluster is 11.6 million light-years across and that it may contain a whopping 660 trillion times the mass of the sun.
In 2014, an unusual spike of intensity in X-ray wavelengths caught the attention of researchers using the XMM-Newton space observatory. The waves were coming from heated gas in the Perseus galactic cluster, near the center. Researchers also found that this same wavelength of radiation, known as an emission line, was coming from 73 other galaxy clusters, according to the statement.
That 2014 observation showed radiation emanating with 3.5 kiloelectron volts (keV) of energy, and a new analysis detected an absorption of X-rays — also at 3.5 keV.
An optical image of the Perseus cluster taken using the Hubble Space Telescope.
Surrounding a supermassive black hole at the center of the Perseus cluster. Researchers have found it nearly impossible to explain why that particular wavelength is being emitted and absorbed, and because previously-seen astronomical objects don't seem to reveal clues about the wavelength emission, they suggested dark matter could be the cause.
"We expect that this result will either be hugely important or a total dud," said Joseph Conlon of the University of Oxford in the United Kingdom, lead author of the recent study. "I don't think there is a halfway point when you are looking for answers to one of the biggest questions in science." The new paper describing the team's results was published in the journal Physical Review D on Dec. 19.
If dark matter caused the atypical emission and absorption lines at that wavelength — both giving off and absorbing X-rays within the collection of galaxies — further observation could teach researchers more about the mysterious substance, the scientists said.
Fortunately, powerful X-ray telescopes currently being developed will let scientists make more-precise observations of these fascinating X-ray emission lines.
Image on the top: A composite image of X-ray and optical observations of the Perseus galaxy cluster.
This image contains X-ray data from the Chandra X-ray Observatory (blue) of the Perseus galaxy cluster. The observations have been combined with optical data from the Hubble space telescope (pink) and radio-emission data from the Very Large Array (red) in New Mexico. If these findings are confirmed with future observations, it would signal a major step forward in comprehending the nature of dark matter, researchers said in a statement. (NASA/ESA/CXO/Oxford University/NRAO/AUI/University of Montreal)
Original article on Space.com.