Princeton astrophysicists helped Planck mission bring universe into sharp focus

This map shows the oldest light in our universe

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. (Image courtesy of ESA and the Planck Collaboration)

March 21, 2013

Princeton University researchers contributed extensively to the Planck space mission that on March 21 released the most accurate and detailed map ever made of the oldest light in the universe, revealing new information about its age, contents and origins.

The new results suggest that the universe is expanding more slowly than scientists thought, and is 13.8 billion years old, about 100 million years older than previous estimates. The data also show there is less dark energy and more matter — both normal and dark matter — in the universe than previously known. Dark matter is an invisible substance that can be seen only through the effects of its gravity, while dark energy is pushing our universe apart. The nature of both remains mysterious.

Princeton researchers helped design and implement an essential scientific instrument on the European Space Agency's Planck mission through the Agency's collaboration with NASA. Princeton astrophysicists also worked with scientists from the United States, Europe and Canada to analyze the Planck data.

"The Planck satellite has expanded the knowledge we gained from previous missions," said William Jones, a Princeton assistant professor of physics who was involved in the design of one of the two Planck detectors, the one that surveys light at high frequencies.

"Planck is able to survey the sky in greater detail than we have ever done before," Jones said.

Princeton's involvement in the project began when Jones came to Princeton from NASA's Jet Propulsion Laboratory (JPL) in Pasadena, Calif., where he had been instrumental in designing and building an instrument to image high frequencies of light. He now oversees graduate students Alexandra Rahlin and Jon Gudmundsson, as well as postdoctoral researcher Aurelien Fraisse, on the analysis of Planck data.

"Astronomers worldwide have been on the edge of their seats waiting for this map," said Joan Centrella, Planck program scientist at NASA Headquarters in Washington, D.C. "These measurements are profoundly important to many areas of science, as well as future space missions. We are so pleased to have worked with the European Space Agency on such a historic endeavor."

The three panels show 10-square-degree patches of all-sky maps
The three panels show 10-square-degree patches of all-sky maps created by space-based missions capable of detecting the cosmic microwave background. The first spacecraft, launched in 1989, is NASA's Cosmic Background Explorer, or COBE (left panel). The second is NASA's next-generation spacecraft, the Wilkinson Microwave Anisotropy Probe, or WMAP (middle panel), launched in 2001. The most advanced satellite yet of this type is Planck, a European Space Agency mission with significant NASA contributions. (Image courtesy of NASA/JPL-Caltech/ESA)

The map, based on the mission's first 15.5 months of all-sky observations, reveals tiny temperature fluctuations in the cosmic microwave background, ancient light that has traveled for billions of years from the very early universe to reach us. The patterns of light represent the seeds of galaxies and clusters of galaxies we see around us today.

"As that ancient light travels to us, matter acts like an obstacle course getting in its way and changing the patterns slightly," said Charles Lawrence, the U.S. project scientist for the JPL. "The Planck map reveals not only the very young universe, but also matter, including dark matter, everywhere in the universe."

The age, contents and other fundamental traits of our universe are described in a simple model scientists developed, called the standard model of cosmology. These new data have allowed scientists to test and improve the accuracy of this model with the greatest precision yet. At the same time, some curious features are observed that don't quite fit with the simple picture. For example, the model assumes the sky is the same everywhere, but the light patterns are asymmetrical on two halves of the sky, and there is a cold spot extending over a patch of sky that is larger than expected.

"On one hand, we have a simple model that fits our observations extremely well, but on the other hand, we see some strange features which force us to rethink some of our basic assumptions," said Jan Tauber, the European Space Agency's Planck project scientist based in the Netherlands. "This is the beginning of a new journey and we expect our continued analysis of Planck data will help shed light on this conundrum."

This full-sky map from the Planck mission
This full-sky map from the Planck mission shows matter between Earth and the edge of the observable universe. Regions with less mass show up as lighter areas while regions with more mass are darker. The grayed-out areas are where light from our own galaxy was too bright, blocking Planck's ability to map the more distant matter.
(Image courtesy of ESA/NASA/JPL-Caltech)

The findings also test theories describing inflation, a dramatic expansion of the universe that occurred immediately after its birth. In far less time than it takes to blink an eye, the universe blew up by 100 trillion trillion times in size. The new map, by showing that matter seems to be distributed randomly, suggests that random processes were at play in the very early universe on minute "quantum" scales. This allows scientists to rule out many complex inflation theories in favor of simple ones.

"Patterns over huge patches of sky tell us about what was happening on the tiniest of scales in the moments just after our universe was born," Lawrence said.

Planck launched in 2009 and has been scanning the skies ever since, mapping the cosmic microwave background, the afterglow of the theorized big bang that created our universe. This relic radiation provides scientists with a snapshot of the universe 370,000 years after the big bang. Light existed before this time, but it was locked in a hot plasma similar to a candle flame, which cooled and set the light free.

The cosmic microwave background is remarkably uniform over the sky, but tiny variations reveal the imprints of sound waves triggered by quantum fluctuations in the universe just moments after it was born. These imprints, appearing as splotches in the Planck map, are the seeds from which matter grew, forming stars and galaxies.

Prior balloon-based and space missions learned a great deal by studying these patterns, including NASA's Wilkinson Microwave Anisotropy Probe (WMAP), a joint project with Princeton named in honor of late Princeton professor and team member David Wilkinson. Since its launch in 2001, the WMAP has regularly provided new and precise data regarding the makeup of the universe by measuring temperature changes in the cosmic microwave background. Information provided by WMAP includes the proportion of the universe composed of dark matter and dark energy.

Planck is the successor to these satellites, covering a wider range of light frequencies with improved sensitivity and resolution. Its measurements reveal light patterns as small as one-twelfth of a degree on the sky.

"Planck is like the Ferrari of cosmic microwave background missions," said Krzysztof Gorski, a U.S Planck scientist at JPL. "You fine tune the technology to get more precise results. For a car, that can mean an increase in speed and winning races. For Planck, it results in giving astronomers a treasure trove of spectacular data, and bringing forth a deeper understanding of the properties and history of the universe."

The newly estimated expansion rate of the universe, known as Hubble's constant, is 67.15 plus or minus 1.2 kilometers/second/megaparsec. A megaparsec is roughly 3 million light-years. This is less than prior estimates derived from space telescopes, such as NASA's Spitzer and Hubble, using a different technique. The new estimate of dark matter content in the universe is 26.8 percent, up from 24 percent, while dark energy falls to 68.3 percent, down from 71.4 percent. Normal matter now is 4.9 percent, up from 4.6 percent.

Complete results from Planck, which still is scanning the skies, will be released in 2014.

NASA's Planck Project Office is based at JPL.

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