Winnipeg, June 16, 2004 – Two University of Toronto (U of T) astronomers and a U.S. colleague have measured the sizes and shapes of massive dark matter halos that surround galaxies.
"Our findings give us the clearest picture yet of a very mysterious part of our universe," says principal investigator Henk Hoekstra, a post-doctoral fellow at U of T's Canadian Institute for Theoretical Astrophysics. "Using relatively simple physics, we can get our first direct glimpse of the size and shape of these halos which are more than fifty times more massive than the light-producing part of galaxies that we can see."
In recent years ever more detailed observations have provided convincing astrophysical evidence for the existence of dark matter, although it has not been detected directly in ongoing experiments. Dark matter emits no light and, therefore, cannot be seen directly, Hoekstra explains. The only evidence for its existence comes from its gravitational pull on stars, gas and light rays. Dark matter is believed to account for approximately 25 per cent of the total mass in the universe, with the rest of the universe composed of normal matter (five per cent) and dark energy (70 per cent).
To date, most information about dark matter has come from measurements of the motion of gas and stars in the inner regions of galaxies. Other important data have come from computer simulations of the formation of the universe's structure. However, scientists can explain their findings about dark matter only if it is true that galaxies are surrounded by massive, three-dimensional halos.
Using a magnifying glass-like effect called 'gravitational lensing', U of T scientists have found that 'dark matter' halos more than five times further than the visible stars in a galaxy, says Hoekstra. In the case of our Milky Way galaxy, he says, the halo extends to more than 500,000 light-years away and weighs approximately 880 billion times more than the sun. The findings also provide strong support for the popular "cold dark matter" model of the universe.
The majority of astronomers believe in the so-called cold dark matter theory of the universe, which suggests these halos are slightly flattened. Hoekstra's findings corroborate this. Using the relatively new technique of weak gravitational lensing which allows astronomers to study the size and shape of dark matter, the team measured the shapes of more than 1.5 million distant galaxies using the Canada-France-Hawaii Telescope in Hawaii. "The small changes in the shapes of the galaxies offered a strong indication to us that the halos are flattened, like a rubber ball compressed to half its size," Hoekstra says.
Their findings can also be applied to a larger scientific debate about the nature of the universe. Some scientists have developed theories about the universe using the assumption that dark matter does not exist and, as a result, they have proposed changes to the law of gravity. However, Hoekstra is confident that his team's findings will refute these theories.
Hoekstra will review the astrophysical evidence for dark matter and present his team's findings on June 16 at the annual meeting of the Canadian Astronomical Society (CASCA) in Winnipeg.
The research was conducted with Professor Howard Yee of U of T's Department of Astronomy and Astrophysics and Michael Gladders, a former U of T graduate student now at the Observatories of the Carnegie Institution of Washington in Pasadena, Calif. It was funded by the Natural Sciences and Engineering Research Council of Canada and U of T.
For more information, contact:
Dr. Henk Hoekstra
Canadian Institute for Theoretical Astrophysics
Professor Howard K.C. Yee
Department of Astronomy and Astrophysics
University of Toronto
Phone: (416) 978-1771