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Spitzer
Sees Shining Stellar Sphere
Thursday, April 10, 2008
Hi-Res
and Full Caption
A cluster brimming with
millions of stars glistens like an irridescent opal in this
image from NASA's Spitzer Space Telescope.
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Credit:
NASA/JPL-Caltech/ NOAO/AURA/NSF
Millions of
clustered stars glisten like an iridescent opal in a new image
from NASA's Spitzer Space Telescope.
Called Omega
Centauri, this sparkling orb of stars is like a miniature galaxy.
It is the biggest and brightest of the more than 150 similar
objects, called globular clusters, that orbit around the outside
of our Milky Way galaxy. Stargazers at southern latitudes can
spot the stellar gem with the naked eye in the constellation
Centaurus.
Spitzer's new infrared view, which has been
combined with visible-light data. While the visible-light
observations highlight the cluster's millions of jam-packed
stars, Spitzer's infrared eyes reveal the dustier, more evolved
stars tossed throughout the region.
"Now we can see
which stars form dust and can begin to understand how the dust
forms and where it goes once it is expelled from a star,"
said Martha Boyer of the University of Minnesota, Twin Cities.
Boyer is lead author of a paper about Omega Centauri appearing in
the April issue of the Astronomical Journal. "Surprisingly,
Spitzer revealed fewer of these dusty stars than expected."
Globular clusters are some of the oldest objects in our
universe. Their stars are more than 12 billion years old, and, in
most cases, formed all at once when the universe was just a
toddler. Omega Centauri is unusual in that its stars are of
different ages and possess varying levels of metals, or elements
heavier than boron. Astronomers say this points to a different
origin for Omega Centauri than other globular clusters: they
think it might be the core of a dwarf galaxy that was ripped
apart and absorbed by our Milky Way long ago.
In the new
picture of Omega Centauri, the red- and yellow-colored dots
represent the stars revealed by Spitzer. These are the more
evolved, larger, dustier stars, called red giants. The stars
colored blue are less evolved, like our own sun, and were
captured by both Spitzer's infrared eyes and in visible light by
the National Science Foundation's Blanco 4-meter telescope at
Cerro Tololo Inter-American Observatory in Chile. Some of the red
spots in the picture are distant galaxies beyond our own.
"As
stars age and mature into red giants, they form dust grains,
which play a vital role in the evolution of the universe and the
formation of rocky planets," said Jacco van Loon, the
study's principal investigator at Keele University in England.
"Spitzer can see this dust, and it was able to resolve
individual red giants even in the densest central parts of the
cluster."
NASA's Hubble Space Telescope and Gemini
Observatory on Cerro Pachon in Chile recently found evidence that
Omega Centauri is home to a medium-sized black hole. See: Black
hole found in enigmatic Omega Centauri
Other authors
of the paper include Iain McDonald and Nye Evans of Keele
University; Robert Gehrz and Charles Woodward of the University
of Minnesota; and Andrea Dupree of the Harvard-Smithsonian Center
for Astrophysics, Cambridge, Mass.
NASA's Jet Propulsion
Laboratory, Pasadena, Calif., manages the Spitzer Space Telescope
mission for NASA's Science Mission Directorate, Washington.
Science operations are conducted at the Spitzer Science Center at
the California Institute of Technology, also in Pasadena. Caltech
manages JPL for NASA. Spitzer's infrared array camera, which took
the Omega Centauri picture, was built by NASA's Goddard Space
Flight Center, Greenbelt, Md. The instrument's principal
investigator is Giovanni Fazio of the Harvard-Smithsonian Center
for Astrophysics.
Cerro Tololo Inter-American Observatory
is part of the National Optical Astronomy Observatory, which is
operated by the Association of Universities for Research in
Astronomy under contract with the National Science Foundation.
Source:
NASA / JPL

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