Astrophysicists Neal Dalal of the University of California, San Diego, and Christopher Kochanek of the Harvard-Smithsonian Center for Astrophysics in Cambridge, MA, based their conclusion on an analysis of the gravitational lensing of light from distant galaxies by intervening galaxies. 

According to Einstein's theory of gravity, large concentrations of matter such as galaxies can warp the surrounding space and bend the light from distant galaxies in much the same way that a glass lens can bend light.

In particular, if a lensing galaxy is surrounded by many smaller dwarf galaxies, the brightness of one of the lensed images could be significantly enhanced if it were aligned with one of the dwarf galaxies. 

Dalal and Kochanek performed a statistical analysis of 7 different lensing galaxies which had each split the light of a background galaxy into 4 images of varying brightness. 

They found that about 2 percent of the mass of the lensing galaxies must be in the form of dwarf galaxies in order to explain the observed brightness variations among the multiple images of the background galaxies.

A growing body of evidence indicates that from 80 to 90 percent of the matter in the universe is in the form of an as yet unknown type of elementary particle that contributes to gravity through its mass but otherwise interacts weakly with normal matter composed of protons and neutrons. 

The currently favored form of dark matter is cold dark matter, so-called because the particles are assumed to move slowly, making it easier for gravity to pull them together to form galaxies. A firm prediction of this model is that large galaxies such as our Milky Way Galaxy should have numerous small satellite galaxies around them. 

The failure of astronomers to find the predicted swarms of dwarf galaxies around large galaxies has led a number of scientists to call for the abandonment of the cold dark matter model.

One puzzle remains as to why the dark dwarf galaxies contain few or no stars, if 10 to 20 percent of their mass is in the form of normal matter. 

"It's difficult to hide that much material," said Dalal. "Perhaps most of the gas was stripped from the dwarfs when the galaxy was formed." 

Their research was supported by the National Aeronautics and Space Administration, U.S. Department of Energy, Smithsonian Institution and the ARCS Foundation.