"Fermi sees gamma rays coming from directions in the sky where there are no obvious objects likely to produce gamma rays," says David Thompson, Fermi Deputy Project Scientist from Goddard Space Flight Center.
For two thirds of the new catalog's sources the Fermi scientists can, with at least reasonable certainty, locate a known gamma ray-producing object*, such as a pulsar or blazar, in the vicinity the gamma-rays are coming from. But the remaining third – the "mystery sources" -- have the researchers stumped, at least for now. And they are the most tantalizing.
"Some of the mystery sources could be clouds of dark matter – something that's never been seen before," speculates Thompson.
About 85% of the gravitational mass of the universe is dark matter. The stuff we see makes up the rest. Dark matter is something that pulls on things with the force of its gravity but can't be detected in any other way. It doesn't shine – doesn't emit or scatter light – hence the adjective "dark."
Astronomers cannot detect dark matter directly using optical or radio telescopes. But dark matter just might shine in gamma rays.
"We've been using Fermi to search for dark matter for a long time," says the principal investigator for the Large Area Telescope, Peter Michelson of Stanford University.
Some researchers believe that when two dark matter antiparticles bump into each other, they will annihilate, producing gamma rays. Concentrated clouds of dark matter could form a gamma ray source at specific wavelengths detectable by Fermi.
"If we see a bump in the gamma-ray spectrum -- a narrow spectral line at high energies corresponding to the energy of the annihilating particles – we could be the first to 'apprehend' dark matter,” says Michelson.
Another, less-dark possibility for some of the mystery sources is colliding galaxy clusters. According to Michelson and Thompson, clashes of such magnitude would generate super large scale shock waves that would accelerate particles. Others of the sources, they say, might be some brand new phenomenon, perhaps something involving galactic black holes.
When all is said and done, many of the mystery sources could prove to be familiar. "[They] will probably turn out to be members of known source classes – things we know but haven't recognized yet, like undiscovered pulsars, binary systems, and supernova remnants," says Michelson.
"Of course we're hoping for something really exotic like dark matter, but we have to look first at all the other options," says Thompson. "Fermi is an ongoing mission. We'll continue to search for answers to these puzzles and perhaps turn up even more surprises."
Will notorious dark matter finally be nabbed? Stay tuned!
Fermi Gamma-ray Space Telescope
Credits: NASA's Fermi Gamma-Ray Space Telescope mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the United States. The mission's main instrument, the Large Area Telescope (LAT), is making pioneering observations of gamma-ray bursts at higher energies than ever before from space. Another instrument onboard, the Fermi Gamma-Ray Burst Monitor, is monitoring gamma-ray bursts at lower energies. The combination of the GBM and the LAT provides a powerful tool for studying GRBs over a very wide range of energies. The GBM is a collaboration among scientists at the Marshall Space Flight Center, the University of Alabama in Huntsville, the Max Planck Institute for Extraterrestrial Physics in Germany, and the Los Alamos National Laboratory.