Sloan Digital Sky Survey

Sloan Digital Sky Survey Probes Dark Matter Theory

CONTACTS:

Dr. Francisco Prada, Instituto de Astrofisica de Canarias in Spain,+34-922425431, fprada@ing.iac.es
Dr. Anatoly Klypin, New Mexico State University at Las Cruces, (505) 646-1400, aklypin@nmsu.edu
Gary S. Ruderman, Public Information Officer, Sloan Digital Sky Survey, 312-320-4794, sdsspio@aol.com

May 21, 2003 -- A new study using the Sloan Digital Sky Survey provides the most direct evidence yet that galaxies reside at the center of giant, dark matter concentrations that may be 50 times larger than the visible galaxy itself.

The study very directly supports the generally accepted astronomical theories on dark matter and contradicts an alternative theory of gravity known as Modified Newtonian Dynamics (MOND).

Lead investigator, Francisco Prada, of the Max Planck Institute for Astronomy in Germany and the Instituto de Astrofisica de Canarias in Spain, and a team of colleagues from New Mexico State University at Las Cruces and at other Sloan Digital Sky Survey (SDSS) institutions, will present the results of the team?s research at a joint conference of the Isaac Newton Group of Telescopes and the Instituto de Astrofisica de Canarias, May 26-30 in La Palma, Canary Islands, Spain.

Prada and his colleagues studied the motion of about 3,000 satellites orbiting isolated bright galaxies and found strong evidence of dark matter gravitational effects.

The study "is important because it is a direct measurement of some of the properties predicted for dark matter," said Anatoly Klypin of New Mexico State University.

Although it cannot be observed directly, dark matter is believed to account for about 27 percent of the total mass of the universe, compared with only about 3 percent for normal, observable matter. The rest, according to standard models of the structure and evolution of the universe, consists of dark energy and radiation.

Prada and his colleagues observed 250,000 galaxies from the Sloan Digital Sky Survey (SDSS) telescope to find good candidates for a study of the gravitational effects of dark matter. From the SDDS data, they identified about 3,000 satellites -- generally small galaxies orbiting large ones ? for which they could measure velocities.

The velocity of a satellite declines predictably as the satellite moves away from the object it is orbiting, due to the effects of gravity. In the case of planets in our solar system, where there is too little dark matter to have a gravitational effect, the decline is rapid because there is no mass between the planets and the sun, he said. But in the outer reaches of galaxies, where dark matter is believed to be clustered, the decline in velocity would be much more gradual if standard cosmological models are correct.

"Our results imply the presence of dark matter," Prada said. The findings provide strong evidence against the MOND alternative theory of gravity, he said. MOND, controversial since it was proposed in 1983, eliminates the need for dark matter in explaining the nature of the universe, by changing the law of gravity in areas such as the outskirts of galaxies.

Researchers said the SDSS study probes dark matter in a way that cannot be done by any other current experiment. This type of research could not have been done without the unique capabilities of the SDSS.

The researchers determined the velocity of each satellite relative to the galaxy it orbits by measuring the redshift in the light spectra from the objects. Redshift, a change in light waves as an object moves away from an observer, is a standard means of measuring the speed of a distant object.

The next stage of the research will be to extend the sample of galaxies and satellites studied to improve the accuracy of the results.

Participating institutions in this discovery are: The Max Planck Institute for Astronomy, Germany; Centro Astronomico Hispano-Aleman; New Mexico State University; Princeton University Observatory; Apache Point Observatory; University of Michigan; Eötvös University, Budapest; and Johns Hopkins University.

Authors of the paper are:

Francisco Prada, Max Planck Institute for Astronomy, Konigstuhl 17, D-679117, Heidelberg, Germany; Centro Astronomico Hispano-Aleman, Apdo. 511, E-04080, Almeria, Spain; Instituto de Astrofisica de Canarias, E-38205, Tenerife, Spain; The Isaac Newton group of Telescopes, Apdo. 321, E-38700, La Palma, Spain; fprada@ing.iac.es
Mayrita Vitviska, Astronomy Department, New Mexico State University, Box 30001, Department 4500, Las Cruces, NM 88003 mvitvit@nmsu.edu
Anatoly Klypin, New Mexico State University, aklypin@nmsu.edu
JonA. Holtzman, New Mexico State University, holtz@nmsu.edu
David J. Schlegel, Princeton University Observatory, Peyton Hall, Princeton, NJ 08544-1001 schlegel@astro.princeton.edu
Eva K. Grebel, Max Planck Institute for Astronomy, grebel@mpia-hd.mpg.de
Hans-Walter Rix, Max Planck Institute for Astronomy rix@mpia-hd.mpg.de
Jon Brinkman, Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349 jb@apo.nmsu.edu
Tim M. McKay, Department of Physics, University of Michigan, 500 E. University Ave., Ann Arbor, MI 48109 tamckay@umich.edu

Istvan Csabai, Department of Physics, Eötvös University, Budapest, Pf. 32, Hungary, H-1518 csabai@galahad.elte.hu

Distribution of dark matter around a Milky Way - size galaxy

This image is based on a computer simulation of formation of galaxies in the expanding Universe as predicted by modern cosmological scenario. "Galaxy" is the large central object surrounded by numerous dark matter satellites. (Credit: Anatoly Klypin, SDSS)

Additional information about the conference is at: http://www.iac.es/proyect/sattail/