The record of baryon acoustic oscillations (white circles) in galaxy maps helps astronomers retrace the history of the expanding universe. These schematic images show the universe at three different times. The representative-color image on the right shows the "cosmic microwave background," a record of what the very young universe looked like 13.7 billion years ago. The small density variations present then have grown into the clusters, walls, and filaments of galaxies that we see today. These variations included the signal of the original baryon acoustic oscillations (white circle, right). As the universe has expanded (middle and left), evidence of the baryon oscillations has remained, visible in a "peak separation" between galaxies (the larger white circles). The SDSS-III results announced today (middle) are for galaxies 5.5 billion light-years distant, at the time when dark energy turned on. Comparing them with previous results from galaxies 3.8 billion light-years away (left) measures how the universe has expanded with time. Credit: E.M. Huff, the SDSS-III team, and the South Pole Telescope team. Graphic by Zosia Rostomian. High Resolution Image (jpg) - Low Resolution Image (jpg)
Cambridge, MA - Astronomers announced today that they have made the most accurate measurement yet of galaxy distances in the faraway universe, giving an unprecedented look at the time when dark energy turned on. Some five to seven billion years ago, the expansion of the universe stopped slowing due to gravity and started to accelerate due to dark energy. Yet the nature of dark energy remains a puzzle that astronomers are seeking to solve.
The new measurement came from the Baryon Oscillation Spectroscopic Survey (BOSS), which is part of the third Sloan Digital Sky Survey (SDSS-III).
"We see the influence of dark energy on cosmic structure, but we have no idea what it is. The data gathered by this survey will help answer that question," said Daniel Eisenstein (Harvard-Smithsonian Center for Astrophysics), the director of SDSS-III.
"There's been a lot of talk about using galaxy maps to find out what's causing accelerating expansion," said David Schlegel of the U.S. Department of Energy's Lawrence Berkeley National Laboratory, BOSS's principal investigator. "We've been making a map and now we're using it - starting to push our knowledge out to the distances when dark energy turned on."
Investigating dark energy
One of the most amazing discoveries of the last two decades in astronomy, recognized with the 2011 Nobel Prize in Physics, was that not only is our universe expanding, but it is accelerating. Galaxies are becoming farther apart from each other faster and faster with time.
The leading contender for the cause of the accelerating expansion is a postulated new property of space dubbed "dark energy." Alternatively, the universe may be accelerating because gravity deviates from Einstein's General Theory of Relativity and becomes repulsive at very large distances.
Whether the answer to the puzzle of the accelerating universe is dark energy or modified gravity, the first step to finding that answer is to measure accurate distances to as many galaxies as possible. From those measurements, astronomers can trace out the history of the universe's expansion.
BOSS is producing the most detailed map of the universe ever made by using a new custom-designed spectrograph of the SDSS 2.5-meter telescope at Apache Point Observatory in New Mexico to observe more than a million galaxies over six years.
Today's announcement is based on a map of more than 250,000 galaxies created from the first year and a half of BOSS observations. Some of these galaxies are so distant that their light has traveled more than six billion years to reach Earth - nearly half the age of the universe.
Surveying the cosmos
Maps of the universe like BOSS's show that galaxies and clusters of galaxies are clumped together into walls and filaments, with giant voids between. These structures grew out of subtle variations in density in the early universe, which bore the imprint of "baryon acoustic oscillations" - pressure-driven acoustic (sound) waves that passed through the early universe.
Billions of years later, the record of these sound waves can still be read in our universe. "Because of the regularity of the ancient sound waves, there's a slightly increased probability that any two galaxies today will be separated by about 500 million light-years, rather than 400 million or 600 million," said Eisenstein.
In a graph of the number of galaxy pairs by separation distance, that magic number of 500 million light-years shows up as a peak, so astronomers often speak of the "peak separation." The position of this peak depends on the amount of dark energy in the Universe. But measuring the distance between galaxies depends critically on having the right distances to the galaxies in the first place.
That's where BOSS comes in. "We've detected the peak separation more clearly than ever before," said Nikhil Padmanabhan of Yale University. "These measurements allow us to determine the contents of the Universe with unprecedented accuracy."
This release is being issued jointly with the Sloan Digital Sky Survey.
Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/.
SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, University of Cambridge, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University.
Headquartered in Cambridge, Mass., the Harvard-Smithsonian Center for Astrophysics (CfA) is a joint collaboration between the Smithsonian Astrophysical Observatory and the Harvard College Observatory. CfA scientists, organized into six research divisions, study the origin, evolution and ultimate fate of the universe.
The new measurement came from the Baryon Oscillation Spectroscopic Survey (BOSS), which is part of the third Sloan Digital Sky Survey (SDSS-III).
"We see the influence of dark energy on cosmic structure, but we have no idea what it is. The data gathered by this survey will help answer that question," said Daniel Eisenstein (Harvard-Smithsonian Center for Astrophysics), the director of SDSS-III.
"There's been a lot of talk about using galaxy maps to find out what's causing accelerating expansion," said David Schlegel of the U.S. Department of Energy's Lawrence Berkeley National Laboratory, BOSS's principal investigator. "We've been making a map and now we're using it - starting to push our knowledge out to the distances when dark energy turned on."
Investigating dark energy
One of the most amazing discoveries of the last two decades in astronomy, recognized with the 2011 Nobel Prize in Physics, was that not only is our universe expanding, but it is accelerating. Galaxies are becoming farther apart from each other faster and faster with time.
The leading contender for the cause of the accelerating expansion is a postulated new property of space dubbed "dark energy." Alternatively, the universe may be accelerating because gravity deviates from Einstein's General Theory of Relativity and becomes repulsive at very large distances.
Whether the answer to the puzzle of the accelerating universe is dark energy or modified gravity, the first step to finding that answer is to measure accurate distances to as many galaxies as possible. From those measurements, astronomers can trace out the history of the universe's expansion.
BOSS is producing the most detailed map of the universe ever made by using a new custom-designed spectrograph of the SDSS 2.5-meter telescope at Apache Point Observatory in New Mexico to observe more than a million galaxies over six years.
Today's announcement is based on a map of more than 250,000 galaxies created from the first year and a half of BOSS observations. Some of these galaxies are so distant that their light has traveled more than six billion years to reach Earth - nearly half the age of the universe.
Surveying the cosmos
Maps of the universe like BOSS's show that galaxies and clusters of galaxies are clumped together into walls and filaments, with giant voids between. These structures grew out of subtle variations in density in the early universe, which bore the imprint of "baryon acoustic oscillations" - pressure-driven acoustic (sound) waves that passed through the early universe.
Billions of years later, the record of these sound waves can still be read in our universe. "Because of the regularity of the ancient sound waves, there's a slightly increased probability that any two galaxies today will be separated by about 500 million light-years, rather than 400 million or 600 million," said Eisenstein.
In a graph of the number of galaxy pairs by separation distance, that magic number of 500 million light-years shows up as a peak, so astronomers often speak of the "peak separation." The position of this peak depends on the amount of dark energy in the Universe. But measuring the distance between galaxies depends critically on having the right distances to the galaxies in the first place.
That's where BOSS comes in. "We've detected the peak separation more clearly than ever before," said Nikhil Padmanabhan of Yale University. "These measurements allow us to determine the contents of the Universe with unprecedented accuracy."
This release is being issued jointly with the Sloan Digital Sky Survey.
Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/.
SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, University of Cambridge, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University.
Headquartered in Cambridge, Mass., the Harvard-Smithsonian Center for Astrophysics (CfA) is a joint collaboration between the Smithsonian Astrophysical Observatory and the Harvard College Observatory. CfA scientists, organized into six research divisions, study the origin, evolution and ultimate fate of the universe.
For more information, contact:
David A. Aguilar
Director of Public Affairs
Harvard-Smithsonian Center for Astrophysics
617-495-7462
daguilar@cfa.harvard.edu
Christine Pulliam
Public Affairs Specialist
Harvard-Smithsonian Center for Astrophysics
617-495-7463
cpulliam@cfa.harvard.edu
