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January 5, 2004
Volume 82, Number 1
CENEAR 82 1 p. 12
ISSN 0009-2347


ASTROCHEMISTRY

STARS, CELESTIAL MOLECULES ON VIEW
IR telescope lifts the cosmic veil to reveal galactic chemical composition

MITCH JACOBY

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EYE IN THE SKY Newly acquired IR images and spectra reveal material outflow in the vicinity of a newborn star from a region of space that appears dark and featureless when probed with visible light.
COURTESY OF NASA
P
eering deep into space with a suite of infrared-sensitive instruments, NASA's orbiting IR observatory has begun beaming down images and spectra that reveal cosmic features never before seen. Showcasing the Spitzer Space Telescope's capabilities at a recent press conference, NASA displayed dazzling IR images of stars and galaxies that appear nearly featureless in the visible-wavelength region.

Launched this past August, the IR observatory joins the X-ray and gamma-ray observatories and the Hubble Space Telescope that orbit Earth while probing galactic secrets using wavelength-specific instruments.

One of the newly acquired Spitzer images shows material flowing out of a newborn star in a region of space that's shrouded by a dust cloud and appears dark and featureless in previous images recorded in visible light. Training the observatory's IR spectrometer on the same point in space, astronomers detected carbon dioxide, water, methanol, and other compounds.

Referred to as an "outflow," the object in the IR image results from interactions between interstellar matter and high speed gas jets ejected from young stars. The data provide scientists with new opportunities to study processes involved in the formation of low-mass stars, such as the sun.

The IR observatory also recorded images and spectra from a galaxy some 3 billion light years from Earth. The spectra reveal the presence of CO, CO2, silicates, hydrocarbons, molecular hydrogen, and other species. The distant object is one of the brightest galaxies ever imaged, according to NASA researchers.

Cornell University astronomy professor James R. Houck, who heads the scientific team, noted that the spectrum "gives evidence for organic chemistry in a distant galaxy shortly after the formation of Earth."



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