3-D map of 1.2 million galaxies sheds light on dark energy


Hundreds of scientists have collaborated in an ambitious project to chart the accelerating expansion of the universe.


A slice through the map of the large-scale structure of the universe from the Sloan Digital Sky Survey. Each dot indicates the position of a galaxy six billion years into the past. The image covers 5% of the sky, a slice of the universe six billion light-years wide, 4.5 billion light-years high, and 500 million light-years thick. Colour indicates distance from Earth, ranging from yellow (nearer) to purple (further). This image contains 48,741 galaxies, about 3% of the full survey dataset.
Daniel Eisenstein and the SDSS-III collaboration

Astronomers have created the largest-ever three-dimensional map of distant galaxies in the hope of making more precise measurements of the dark energy driving the accelerated expansion of the universe.

“We have spent a decade collecting measurements of 1.2 million galaxies over one quarter of the sky to map out the structure of the Universe over a volume of 650 cubic billion light-years,” says Jeremy Tinker of New York University, a co-leader of the team from the Sloan Digital Sky Survey III (SDSS-III).

“This map has allowed us to make the best measurements yet of the effects of dark energy in the expansion of the universe. We are making our results and map available to the world.”

New measurements included in the map were carried out by the Baryon Oscillation Spectroscopic Survey (BOSS) program of SDSS-III.

The map allows astronomers to measure the expansion rate of the universe along with the amount of dark matter and dark energy there.

The project is documented in a series of papers in the Monthly Notices of the Royal Astronomical Society.

BOSS works by determining the size of the baryon acoustic oscillations (BAO) – fluctuations in the density of visible matter in the universe.

The rectangle on the far left shows a cut-out of 1,000 sq. degrees in the sky containing nearly 120,000 galaxies, or roughly 10% of the total survey. The brighter regions correspond to regions with more galaxies and therefore more dark matter.
Jeremy Tinker and the SDSS-III collaboration

The original BAO size is determined by pressure waves up to when the universe was just 400,000 years old. That is used as a yardstick to measure the distance separating galaxies, that astronomers call the acoustic scale.

Measuring the distribution of galaxies since that time 13.48 billion years ago allows astronomers to measure how dark matter and dark energy have governed the rate of expansion of the universe.

“Measuring the acoustic scale across cosmic history gives a direct ruler with which to measure the universe’s expansion rate,” says Ariel Sanchez of the Max-Planck Institute of Extraterrestrial Physics.

“With BOSS, we have traced the BAO’s subtle imprint on the distribution of galaxies spanning a range of time from two to seven billion years ago.”

Dark energy began to significantly influence the expansion of the universe about five billion years ago, scientists say, and BOSS was designed to measure the BAO from seven billion years ago to two billion years ago – recent times in astronomical terms.

“If dark energy has been driving the expansion of the universe over that time, our maps tell us that it is evolving very slowly if at all: the change is at most 20% over the past seven billion years,” says Florian Beutler of University of Portsmouth, who led two of the papers on the project.

The map also reveals galaxies moving towards regions of the universe with more matter, due to the attractive force of gravity.

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