Clustering
in Universe Seen as Indicator of Galaxy Evolution
Researchers at the Sloan Digital Sky Survey have
discovered surprising new information about how
galaxies cluster in space, leading to new information
about evolutions of galaxies and matter in the
universe. These findings were presented at the
American Astronomical Society meeting in Nashville,
Tennessee, on May 26, 2003.
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The spiral galaxy
NGC 1087 is found in the constellation Cetus.
(Image: SDSS Collaboration) |
June 2, 2003The
discovery of differing ways that galaxies cluster
in space has led researchers at the Sloan Digital
Sky Survey (SDSS) to new insights into the evolution
of galaxies and matter in the universe. The
SDSS is a project funded by a large collaboration
that includes the U.S. Department of Energy's
Office of Science.
"The clustering of galaxies is
directly related to the distribution of matter
in the Universe today," explained principal
investigator Tamas Budavari of Johns Hopkins
University. "How matter is distributed today
reflects conditions when the universe was less
than a second old." Mapping the distribution
of matter allows scientists to test theories
for the origin of the Universe.
Now scientists with the SDSS have
devised a method of obtaining not only a census
of newly differentiated red and blue galaxies,
but have begun to make critical findings related
to the two populations. A key finding is that
clustering properties do not appear to be continuous
from one galaxy type to another as had been
assumed.
The discovery enables progress
in understanding the connection between galaxy
properties, their environments, and their evolutionary
histories. It could also help to unravel the
mystery of the nature of dark matter.
Budavari presented the team's
findings on May 26, 2003, at the American Astronomical
Society meeting in Nashville, Tennessee.
Galaxy Densities Differentiated
SDSS investigators seek to understand
the clustering of galaxies based on their types.
Astronomers have known for years that galaxies
of different evolutionary ages have different
colors and shapes. Red elliptical galaxies today
are composed of older, less active or inactive
stars. Blue spiral galaxies are still in the
star formation stage and are evolutionarily
younger.
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These two images
show the density of red and blue galaxies
in the same area of the sky. Since red galaxies
cluster more strongly, their image (top
panel) shows larger high density regions.
Conversely, the higher density regions of
the blue galaxies are smaller and more spread
out. |
After the Big Bang 14 billion
years ago, primordial matter (mostly hydrogen
and helium) congealed into galaxies. Pockets
of matter (dark matter and the gas that forms
the stars we see) within the universe collapsed
under the force of gravity. Some of the earliest
galaxies to form are what we see today as the
red elliptical galaxies.
Over time the matter continues
to cluster via gravity so that, in the universe
we observe locally, ellipticals tend to reside
in very dense regions (i.e., regions with a
lot of galaxies that astronomers refer to as
regions that are strongly clustered). Galaxies
we see today as blue or spirals formed later
than the ellipticals so the regions they occupy
have had less time to accumulate matter and
are less clustered.
The SDSS team also reported, as
part of these new findings, is that while all
galaxies were from smaller components, elliptical
galaxies have a longer merging history than
spiral galaxies and, that the two galaxy types
clump in different ways.
|
Andrew
Connolly, University of Pittsburgh |
"As you go from red to blue you
find they cluster differently," explained Andrew
Connolly of the University of Pittsburgh. "This
is surprising because I would have expected
there to be a whole range of clustering signatures,
not just two."
The SDSS team went beyond traditional
use of spectroscopy to determine the three-dimensional
clustering of galaxies, as spectroscopy can
only be used for the brightest of objects, perhaps
one percent of all the catalogued objects in
a patch of surveyed sky.
Instead, the SDSS study carefully
evaluated the colors of galaxies to determine
their distances to create a three-dimensional
map. In this way, SDSS scientists were able
to create a uniform sample of millions of galaxies,
each with quantified physical parameters such
as their type and brightness. The result is
an evaluation based on clustering properties
of these distinct kinds of galaxies in different
environments; what SDSS investigators considered
a true apples-to-apples comparison.
|
The Sloan Digital
Sky Survey observes the sky in stripes.
Each of these eight long stripes contains
millions of galaxies. |
Budavari and Connolly have found
that red galaxies tend to cluster more tightly
and inferred that dark matter surrounding galaxies
bunches similarly. Dark matter, a non-luminous
or invisible matter that makes up as much as
27 percent of the mass of the universe, is known
by its gravitational effects on visible celestial
objects like galaxies.
The discoveries offer more questions to
contemplate: Why do different types of galaxies cluster
differently? Does differentiated clustering relate to
dark-matter contents? Or does it relate to its evolutionary
history? Are these connected?
Other SDSS lead investigators
were Alex Szalay, also of Johns Hopkins; Istvan
Szapudi of the University of Hawaii; Istvan
Csabai of Eotvos University, Budapest, Hungary;
and Ryan Scranton, also of the University of
Pittsburgh.
SDSS Large-Scale Undertaking
The SDSS is the most ambitious astronomical
survey ever undertaken. With more than 200 astronomers
at 13 institutions around the world, the SDSS will map
in detail one-quarter of the entire sky, determining
the positions and absolute brightness of more than 100
million celestial objects. It will also measure the
spectrographic distances to more than a million galaxies
and quasars. The SDSS telescopes are located at Apache
Point Observatory in New Mexico and operated by the
Astrophysical Research Consortium.
|
The Sloan Digital Sky Survey
will observe half of the northern hemisphere. This
figure illustrates the sky coverage of Data Release
1, the current status of the survey. |
The SDSS findings on galaxy clustering
were culled from statistical analysis of tens of millions
of galaxies. The first public data release from the
SDSS, called DR1or Data Release 1, contains about
15 million galaxies. Prior 3D sky mappings were able
to survey just a few hundred thousand galaxies.
Even further, the SDSS was conducted with
five color bands using charge coupled devices where
earlier astronomical surveys were done in just one color,
most using photographic plate images.
"Without the five-band photometry these
findings wouldn't have been possible," said Connolly.
SDSS provides a uniquely powerful 3D map
to make such studies: large in volume and numbers of
galaxies as well as detailed and accurate parameters
for each galaxy with uniform coverage.
"We're beginning to study these structures
at a level of accuracy that we've never been able to
do before. We can see in exquisite detail how the properties
of galaxies change and really map out how they change
in a great amount of detail," Budavari said.
Other SDSS collaborating institutions
in this discovery are Princeton University, Princeton,
New Jersey; Apache Point Observatory, Sunspot, New Mexico;
Steward Observatory, Tucson, Arizona; The University
of Chicago; Fermi National Accelerator Laboratory, Batavia,
Illinois; and the Institute for Cosmic Ray Research,
University of Tokyo.by Gary Ruderman
Media contact: Gary Ruderman,
SSDS Public Information Officer, (312) 320-4794, mailto:ssdspio@aol.com
Technical contacts: Tamas Budavari,
Johns Hopkins University, (410) 516-0643, mailto:budavari@jhu.edu;
Andrew Connolly, University of Pittsburgh, (412) 624-1345,
mailto:ajc@tiamat.phyast.pitt.edu
Related Links
SSDS
Data Release 1
"Sloan
Digital Sky Survey Probes Dark Matter Theory," Gary
Ruderman, SDSS, March 21, 2003.
Tamas
Budvari, Johns Hopkins University
Andrew
Connolly, University of Pittsburgh Department of Physics
and Astronomy
Apache
Point Observatory (site of SDSS telescopes)
Sloan
Digital Sky Survey at Johns Hopkins University
"Most
Distant Object Every Observed," DOE Office of Science's
Decades of Discovery
Funding:
Funding for the Sloan Digital Sky Survey
is provided by the U.S. Department of Energy's
Office of
Science's through its High
Energy and Nuclear Physics program, the Alfred
P. Sloan Foundation, the National
Aeronautics and Space Administration, the
National Science
Foundation, the Japanese
Monbukagakusho, and the Max
Planck Society.
The Sloan
Digital Sky Survey is managed by
the Astrophysical Research Consortium for the
Participating Institutions. The Participating
Institutions are The University of Chicago, DOE's
Fermi National Accelerator Laboratory, the Institute
for Advanced Study, the Japan Participation Group,
The Johns Hopkins University, DOE's Los Alamos
National Laboratory, the Max-Planck-Institute
for Astronomy (MPIA), the Max-Planck-Institute
for Astrophysics, New Mexico State University,
University of Pittsburgh, Princeton University,
the United States Naval Observatory, and the University
of Washington.
The SDSS will map in detail
one-quarter of the entire sky, determining the
positions and absolute brightness of 100 million
celestial objects. It will also measure the distances
to more than a million galaxies and quasars. The
Astrophysical Research Consortium operates Apache
Point Observatory, site of the SDSS telescopes.
Author: Gary Ruderman
is the public
information officer for the Sloan Digital Sky
Survey. For more news, see the current SDSS news
releases.
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