“The infrared background glow in our sky has been a huge mystery,” said Asantha Cooray of the University of California, Irvine. “We have new evidence this light is from the stars that linger between galaxies. Individually, the stars are too faint to be seen, but we think we are seeing their collective glow.”
The findings disagree with another theory explaining the same background infrared light observed by Spitzer. A group led by Alexander “Sasha” Kashlinsky of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, proposed in June that this light, which appears in Spitzer images as a blotchy pattern, is coming from the first stars and galaxies.
In the new study, Cooray and colleagues looked at data from a larger portion of the sky, called the Boötes field, covering an arc equivalent to 50 Full Moons. These observations were not as sensitive as those from the Kashlinsky group’s studies, but the larger scale allowed researchers to analyze better the pattern of the background infrared light.
“We looked at the Boötes field with Spitzer for 250 hours,” said Daniel Stern of NASA’s Jet Propulsion Laboratory in Pasadena, California. “Studying the faint infrared background was one of the core goals of our survey, and we carefully designed the observations in order to directly address the important, challenging question of what causes the background glow.”
The team concluded that the light pattern of the infrared glow is not consistent with theories and computer simulations of the first stars and galaxies. Researchers said the glow is too bright to be from the first galaxies, which are thought not to have been as large or as numerous as the galaxies we see around us today. Instead, the scientists propose a new theory to explain the blotchy light, based on theories of “intracluster” or “intrahalo” starlight.
Theories predict a diffuse smattering of stars beyond the halos, or outer reaches, of galaxies and in the spaces between clusters of galaxies. The presence of these stars can be attributed to two phenomena. Early in the history of our universe as galaxies grew in size, they collided with other galaxies and gained mass. As the colliding galaxies became tangled gravitationally, strips of stars were shredded and tossed into space. Galaxies also grow by swallowing smaller dwarf galaxies, a messy process that also results in stray stars.
“A light bulb went off when reading some research papers predicting the existence of diffuse stars,” Cooray said. “They could explain what we are seeing with Spitzer.”
More research is needed to confirm that this sprinkling of stars makes up a significant fraction of the background infrared light. For instance, it would be necessary to find a similar pattern in follow-up observations in visible light. NASA’s upcoming James Webb Space Telescope (JWST) might finally settle the matter for good.
“The keen infrared vision of the James Webb Telescope will be able to see some of the earliest stars and galaxies directly, as well as the stray stars lurking between the outskirts of nearby galaxies,” said Eric Smith, JWST’s deputy program manager at NASA Headquarters in Washington, D.C. “The mystery objects making up the background infrared light may finally be exposed.”