Largest Age Map Reveals How Our Galaxy Grew Up

Proud parents chart the growth of their children, but astronomers from the Sloan Digital Sky Survey (SDSS) have taken on a bigger task: charting the growth of our own Milky Way.
In a result presented today at the American Astronomical Society meeting in Kissimmee, Florida, a team led by Melissa Ness of the Max Planck Institute for Astronomy in Heidelberg, Germany created the first-ever “growth chart” for our Milky Way Galaxy. Their chart, which uses the ages of more than 70,000 stars and extends halfway across our galaxy to 50,000 light-years away, helps us read the story of how our galaxy grew from its infancy to the bright spiral galaxy we see today.

“Close to the center of our galaxy, we see old stars that were formed when it was young and small. Farther out, we see young stars. We conclude that our galaxy grew up by growing out,” says Ness, lead author of the study. “To see this, we needed an age map spanning large distances, and that’s what this new discovery gives us.”

The researchers mapped the galaxy by observing red giants, bright stars in the final stages of their lives that can be observed out to large distances from our Sun, into the very inner and outer reaches of the Milky Way. “If we know the mass of a red giant star, we know its age by using the fusion clock inside every star,” says Marie Martig, lead author of a related study and a co-author of Ness’s study. “Finding masses of red giant stars has historically been very difficult, but surveys of the galaxy have made new, revolutionary techniques possible.”

The team started with spectra taken from one of the SDSS’s component surveys, the Apache Point Observatory Galaxy Evolution Experiment (APOGEE). “APOGEE is the ideal survey for this work because it can get high-quality spectra for 300 stars simultaneously over a large area of sky,” says Steve Majewski of the University of Virginia and Principal Investigator of the APOGEE survey. “Seeing so many stars at once means getting spectra of 70,000 red giants is actually possible with a single telescope in a few years’ time.”

The ages of stars cannot be measured with APOGEE spectra alone, but the APOGEE team realized that light curves from the Kepler satellite, a NASA space mission whose main goal is to find planets around stars, could provide the missing link between APOGEE spectra and stellar ages. APOGEE therefore observed thousands of red giants that had also been seen by Kepler. After combining information from the APOGEE spectra and Kepler light curves, the researchers could then apply their methods to measure ages for all 70,000 red giant stars sampling all parts of the galaxy.

“In the galaxy we know best — our own — we can clearly read the story of how galaxies form in a Universe with large amounts of cold dark matter,” says Ness. “Because we can see so many individual stars in the Milky Way, we can chart its growth in unprecedented detail. This unprecedented, enormous map really is one for the ages.”

Image (1080 x 1080 pixels, 100 dpi): https://dl.dropboxusercontent.com/u/23495063/milkywayage.png This image shows the latest results as colored dots superimposed on an artist’s conception of the Milky Way. Red dots show stars that formed when the Milky Way was young and small, while blue shows stars that formed more recently, when the Milky Way was big and mature. The color scale shows how many billion years have passed since those stars formed. Credit: G. Stinson (MPIA)

Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS website is http://www.sdss.org.

SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofisica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the universe (IPMU) / University of Tokyo, Lawrence Berkeley National Laboratory, Leibniz Institut fur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-Planck-Institut fur Astrophysik (MPA Garching), Max-Planck-Institut fur Extraterrestrische Physik (MPE), National Astronomical Observatory of China, New Mexico State University, New York University, University of Notre Dame, Observatorio Nacional / MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University.