| Sloan Digital Sky Survey |
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The ability to record and digest immense quantities
of data in a timely way is changing the face of science. The Sloan
Digital Sky Survey, the most ambitious astronomical survey project
ever undertaken, will bring this modern practice of comprehensive and quantitative
mapping to cosmography, the science of mapping the universe and determining
our place in it.
The Sky Survey will systematically map one-quarter
of the entire sky, producing a detailed image of it and determining the
positions and absolute brightnesses of more than 100 million celestial
objects. It will also measure the distance to a million of the nearest
galaxies, giving us a three-dimensional picture of the universe through
a volume one hundred times larger than that explored to date. The Sky Survey
will also record the distances to 100,000 quasars, the most distant objects
known, giving us an unprecedented hint at the distribution of matter to
the edge of the visible universe.
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The 2.5-meter reflecting telescope of the Sloan Digital
Sky Survey. The box-like structure protects the separately mounted telescope
from being buffeted by the wind.
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As the first large-area survey to use electronic
light detectors, the image it produces will be substantially more sensitive
and accurate than earlier surveys, which relied on photographic techniques.
The results of the Sky Survey will be available to the scientific community
electronically, both as images and as precise catalogs of all the objects
discovered. The Sky Survey also represents a significant increase in scale.
The total quantity of information produced, about 15 terabytes (trillion
bytes), rivals the data content of the Library of Congress.
By systematically and sensitively observing
such a large fraction of the sky, the Sky Survey will have a significant
impact on astronomical studies as diverse as the large-scale structure
of the universe, the origin and evolution of galaxies, the relation between
dark and luminous matter, the structure of our own Milky Way, and the properties
and distribution of the dust from which stars like our sun were created.
It will represent a new reference point, a field guide to the universe
at the millenium, which will be used by scientists for decades to come.
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Redshift 5.8 Quasar: The arrow in this image points
to the most distant quasar ever observed, with a record-shattering redshift
of 5.8. SDSS astronomers identified this faint speck of light as a possible
quasar based on its distinctive red color. A spectrum of this object, obtained
with the 10-meter Keck telescope in Hawaii, showed that this was indeed
a quasar with a most impressive redshift.
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