A new study of two Milky Way neighbors — the Fornax and Sculptor dwarf galaxies — reveals a smooth distribution of dark matter, suggesting that the standard cosmological model, showing dark matter densely packed in the centers of galaxies, may be wrong, according to an October 17, 2011, press release by the Harvard-Smithsonian Center for Astrophysics.
Like all galaxies, our Milky Way is home to a strange substance called dark matter. Dark matter is invisible, betraying its presence only through its gravitational pull. Without dark matter holding them together, our galaxy’s speedy stars would fly off in all directions. The nature of dark matter is a mystery that a new study has only deepened.
A paper by Matt Walker (Harvard-Smithsonian Center for Astrophysics) and co-author Jorge Peñarrubia (University of Cambridge, UK) describing the study was accepted for publication in the The Astrophysical Journal. Lead author Matt Walker said:
After completing this study, we know less about dark matter than we did before.
The standard cosmological model describes a universe dominated by dark energy and dark matter. Most astronomers assume that dark matter consists of “cold” (slow-moving) exotic particles that clump together gravitationally. Over time these dark matter clumps grow and attract normal matter, forming the galaxies we see today.
Cosmologists use powerful computers to simulate this process. Their simulations show that dark matter should be densely packed in the centers of galaxies.
Our measurements contradict a basic prediction about the structure of cold dark matter in dwarf galaxies. Unless or until theorists can modify that prediction, cold dark matter is inconsistent with our observational data.
Dwarf galaxies are composed of up to 99 percent dark matter and only one percent normal matter like stars. This disparity makes dwarf galaxies ideal targets for astronomers seeking to understand dark matter.
Walker and Peñarrubia analyzed the dark matter distribution in two Milky Way neighbors: the Fornax and Sculptor dwarf galaxies. These galaxies hold one million to 10 million stars, compared to about 400 billion in our galaxy. The team measured the locations, speeds and basic chemical compositions of 1,500 to 2,500 stars.
Stars in a dwarf galaxy swarm like bees in a beehive instead of moving in nice, circular orbits like a spiral galaxy. That makes it much more challenging to determine the distribution of dark matter.
Their data showed that in both cases, the dark matter is distributed uniformly over a relatively large region, several hundred light-years across. This contradicts the prediction that the density of dark matter should increase sharply toward the centers of these galaxies.
If a dwarf galaxy were a peach, the standard cosmological model says we should find a dark matter ‘pit’ at the center. Instead, the first two dwarf galaxies we studied are like pitless peaches.
Some have suggested that interactions between normal and dark matter could spread out the dark matter, but current simulations don’t indicate that this happens in dwarf galaxies. The new measurements imply that either normal matter affects dark matter more than expected, or dark matter isn’t “cold.” The team hopes to determine which is true by studying more dwarf galaxies, particularly galaxies with an even higher percentage of dark matter.
Bottom line: Matt Walker (Harvard-Smithsonian Center for Astrophysics) and co-author Jorge Peñarrubia (University of Cambridge, UK) studied the dark matter in the Fornax and Sculptor dwarf galaxies and discovered that the dark matter was not distributed as the standard cosmological model predicts. An October 17, 2011, press release by the Harvard-Smithsonian Center for Astrophysics said the new data contradict the prediction that the density of dark matter should increase sharply toward the centers of these galaxies.
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