The cosmic microwave background (CMB) as observed by Planck. The CMB is a snapshot of the oldest light in our Universe, imprinted on the sky when the Universe was just 380,000 years old. It shows tiny temperature fluctuations that correspond to regions of slightly different densities. ESA and the Planck Collaboration

A few hundred thousand years after the Big Bang, when the universe underwent recombination — the name to describe the event when the first electrons and protons came together to form hydrogen — one of the effects was the production of the cosmic microwave background, a faint omnipresent radiation left over from the time that we can observe and measure even today. As the universe expanded, the CMB began cooling from its initial temperature of about 3,000 Kelvin (almost 5,000 degrees Fahrenheit) to its present-day coolness of 2.73 Kelvin (-454.75 degrees Fahrenheit).

However, even though most irregularities were smoothed out by the universe’s ongoing expansion, some odd patches still remain. One such anomaly is the Cold Spot in the CMB, which causes problems in the standard model of cosmology. First discovered by the Wilkinson Microwave Anisotropy Probe spacecraft in 2002, and confirmed in 2013 by the Planck satellite, the Cold Spot is a large area in the region of the sky that has the Eridanus constellation.

The map of the cosmic microwave background (CMB) sky produced by the Planck satellite. Red represents slightly warmer regions, and blue slightly cooler regions. The Cold Spot is shown in the inset, with coordinates on the x- and y-axes, and the temperature difference in millionths of a degree in the scale at the bottom. ESA and Durham University

The Cold Spot is colder than its surroundings by only a fraction of a Kelvin (0.00015 Kelvin) but even that small deviation has a probability for occurrence of less than 2 percent, given the size of the area. Conventional explanations, such as a large void billions of light-years across but containing relatively few galaxies, has been disproved by new research.

Postgraduate student Ruari Mackenzie and Professor Tom Shanks of Durham University in the United Kingdom led a team of researchers who analyzed a dataset of 7,000 galaxies, collected using a spectrograph on the Anglo-Australian Telescope in Australia. The team found the Cold Spot is not one giant void, but instead, is split into smaller voids, each of which are surrounded by clusters of galaxies with the same density as other places in the universe.

The 3-D galaxy distribution in the foreground of the CMB Cold Spot, where each point is a cluster of galaxies. The galaxy distribution in the Cold Spot (black points, at right) is compared to the same in an area with no background Cold Spot (red points, at left). The number and size of low galaxy density regions in both areas are similar, making it hard to explain the existence of the CMB Cold Spot by the presence of “voids.” Durham University

In a statement Tuesday, Mackenzie said: “The voids we have detected cannot explain the Cold Spot under standard cosmology. There is the possibility that some non-standard model could be proposed to link the two in the future but our data place powerful constraints on any attempt to do that.”

While the standard model could still explain the Cold Spot — as an unlikely fluctuation — the chance of that is just about 1 in 50, according to the statement by the researchers. So what then explains this cosmic anomaly? “Exotic” origins, Shanks said, while offering some possibilities.

“Perhaps the most exciting of these is that the Cold Spot was caused by a collision between our universe and another bubble universe. If further, more detailed, analysis of CMB data proves this to be the case then the Cold Spot might be taken as the first evidence for the multiverse — and billions of other universes may exist like our own,” he said.

The researchers published a paper, titled “Evidence against a supervoid causing the CMB Cold Spot,” that appeared in the journal Monthly Notices of the Royal Astronomical Society.