1-Dec-2010 
                  --New Haven, Conn.—Because red dwarfs are relatively small and 
                  dim compared to stars like our Sun, astronomers hadn't been 
                  able to detect them in galaxies other than our own Milky Way 
                  and its nearest neighbors before now. As such, they did not 
                  know how much of the total stellar population of the universe 
                  is made up of red dwarfs.
                Now astronomers 
                  have used powerful instruments on the Keck Observatory in Hawaii 
                  to detect the faint signature of red dwarfs in eight massive, 
                  relatively nearby galaxies called elliptical galaxies, which 
                  are located between about 50 million and 300 million light years 
                  away. They discovered that the red dwarfs, which are only between 
                  10 and 20 percent as massive as the Sun, were much more bountiful 
                  than expected. 
                "No one 
                  knew how many of these stars there were," said Pieter van Dokkum, 
                  a Yale University astronomer who led the research, which is 
                  described in Nature's Dec.1 Advanced Online Publication. "Different 
                  theoretical models predicted a wide range of possibilities, 
                  so this answers a longstanding question about just how abundant 
                  these stars are."
                The team 
                  discovered that there are about 20 times more red dwarfs in 
                  elliptical galaxies than in the Milky Way, said Charlie Conroy 
                  of the Harvard-Smithsonian Center for Astrophysics, who was 
                  also involved in the research. 
                "We usually 
                  assume other galaxies look like our own. But this suggests other 
                  conditions are possible in other galaxies," Conroy said. "So 
                  this discovery could have a major impact on our understanding 
                  of galaxy formation and evolution."
                For instance, 
                  Conroy said, galaxies might contain less dark matter—a mysterious 
                  substance that has mass but cannot be directly observed—than 
                  previous measurements of their masses might have indicated. 
                  Instead, the abundant red dwarfs could contribute more mass 
                  than realized. 
                In addition 
                  to boosting the total number of stars in the universe, the discovery 
                  also increases the number of planets orbiting those stars, which 
                  in turn elevates the number of planets that might harbor life, 
                  van Dokkum said. In fact, a recently discovered exoplanet that 
                  astronomers believe could potentially support life orbits a 
                  red dwarf star, called Gliese 581. 
                "There are 
                  possibly trillions of Earths orbiting these stars," van Dokkum 
                  said, adding that the red dwarfs they discovered, which are 
                  typically more than 10 billion years old, have been around long 
                  enough for complex life to evolve. "It's one reason why people 
                  are interested in this type of star."
                Contact: 
                  Suzanne Taylor Muzzin
                  suzanne.taylormuzzin@yale.edu
                  203-432-8555