This map shows the oldest light in our universe, as detected with the greatest precision yet by the Planck mission. The ancient light, called the cosmic microwave background, was imprinted on the sky when the universe was 370,000 years old. It shows tiny temperature fluctuations that correspond to regions of slightly different densities, representing the seeds of all future structure: the stars and galaxies of today.
An odd dense spot in the universe populated by a surprising amount of matter has been puzzling scientists since it was revealed in March in an all-sky map made by the European Planck satellite. This feature and other mysteries in the observations may point the way toward new theories of physics, say scientists who met recently to discuss the implications of the findings.
Three Planck team members will answer public questions about the Planck data during a Google+ Hangout on Wednesday at 3 p.m. EDT, sponsored by the Kavli Foundation. You can watch the Hangout live here on Space.com. Questions for the researchers can be submitted in advance by emailing firstname.lastname@example.org or posting on Twitter with hashtag #KavliAstro.
Planck measures ancient light pervading the universe called the cosmic microwave background (CMB), which dates from just a few hundred thousand years old. This light records a record of what the universe was like shortly after its birth in the Big Bang, and thus offers a test of theories of how the cosmos came to be. [Gallery: Planck Spacecraft Sees Big Bang Relics]
Ultimately, the spread of matter throughout space is thought to be due to slight variations in the energy density of the young universe that are evident as temperature variations in the cosmic microwave background light. Mostly, these density variations are evenly spread throughout the sky, but one anomalous spot is particularly dense, which shows up in the data as a particularly cold area.
"(T)his is very strange," George Efstathiou, a professor of astrophysics at the U.K.'s University of Cambridge and director of the Kavli Institute for Cosmology at Cambridge, said in a statement. "And I think that if there really is anything to this, you have to question how that fits in with inflation … It’s really puzzling."
Inflation is a leading theory suggesting that within the first fraction of a second after the Big Bang, the universe grew exponentially in size.
"(T)he theory of inflation predicts that today’s universe should appear uniform at the largest scales in all directions," Efstathiou said. "That uniformity should also characterize the distribution of fluctuations at the largest scales within the CMB. But these anomalies, which Planck confirmed, such as the cold spot, suggest that this isn’t the case."
By investigating the cold spot and other mysteries in the CMB, physicists hope to discriminate between different versions of inflation theory, and perhaps open the door to further theories.
"Perhaps we may still eliminate these anomalies with more precise analysis; on the other hand, they may open the door to something much more grand — a reinvestigation of how the whole structure of the universe should be," Krzysztof Gorski, a Planck Collaboration scientist and senior research scientist at the Jet Propulsion Laboratory in Pasadena, Calif., said in a statement.
You can also watch Wednesday's Planck webcast directly at the Kavli website here.
Follow Clara Moskowitz on Twitter and Google+. Follow us @Spacedotcom, Facebook and Google+. Original article on Space.com.
First published July 30 2013, 9:29 AM