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Seeing red: a cool revival of Hubble's infrared camera. (Science News This Week).


After 3 years of blindness, the Hubble Space Telescope's near-infrared vision has been restored. Prematurely running out of its nitrogen-ice coolant in 1999, Hubble's Near Infrared Camera and Multi-Object Spectrometer The Near Infrared Camera and Multi-Object Spectrometer (NICMOS) is a scientific instrument for infrared astronomy, installed on the Hubble Space Telescope (HST), operating from 1997 to 1999, and from 2002 to the present.  (NICMOS NICMOS: see infrared astronomy. ) was brought back to life in March when astronauts installed a neon-gas refrigerator (SN: 3/16/02, p. 163).

Cooled to a temperature that gives the detector 10 to 30 times greater sensitivity than before, NICMOS is once again peering through dust-shrouded regions that can't be seen in visible and ultraviolet light. It can also scan for objects so distant that cosmic expansion has shifted their light out of the range of every other detector on Hubble.

The rejuvenated NICMOS teamed with Hubble's newly installed Advanced Camera for Surveys The Advanced Camera for Surveys (ACS) is a third generation axial instrument aboard the Hubble Space Telescope (HST). The initial design and scientific capabilities of ACS were defined by a team based at Johns Hopkins University.  to observe a four-galaxy collision a billion light-years from Earth. The infrared-bright regions at the collision's center produce the equivalent of 200 new suns each year, 100 times more than the Milky Ways output. Although new stars primarily radiate ultraviolet light, the dust they generate absorbs that light and reemits it in the near-infrared.

In another study, NICMOS peered through the dusty disk of the spiral galaxy NGC NGC New General Catalogue (of Nebulae and Star Clusters; astronomy)
NGC National Geographic Channel (TV)
NGC National Guideline Clearinghouse
 4013 to discover what appears to be a ring of newborn stars at the galaxy's core. Such rings are relatively common in spiral galaxies, but this is the first time a telescope has found one by looking through dust in a galaxy with an edge-on orientation, says Daniela Calzetti of the Space Telescope Science Institute The Space Telescope Science Institute (STScI) is the science operations center for the Hubble Space Telescope (HST; in orbit since 1990) and for the James Webb Space Telescope (JWST; scheduled to be launched in 2013).  in Baltimore.

Calzetti and her colleagues unveiled the images this week at a meeting of the American Astronomical Society The American Astronomical Society (AAS, sometimes pronounced "double-A-S") is a US society of professional astronomers and other interested individuals, headquartered in Washington, DC.  in Albuquerque.
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Author:Cowen, R.
Publication:Science News
Article Type:Brief Article
Date:Jun 8, 2002
Words:264
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