Dissection of a Galaxy
May 19, 2004
Sometimes, the best way to understand how something works is to take it apart. The same is true for galaxies like NGC 300, which NASA's Spitzer Space Telescope has divided into its various parts. NGC 300 is a face-on spiral galaxy located 7.5 million light-years away in the southern constellation Sculptor. This false-color image taken by the infrared array camera on Spitzer readily distinguishes the main star component of the galaxy (blue) from its dusty spiral arms (red). The star distribution peaks strongly in the central bulge where older stars congregate, and tapers off along the arms where younger stars reside. Thanks to Spitzer's unique ability to sense the heat or infrared emission from dust, astronomers can now clearly trace the embedded dust structures within NGC 300's arms.
Topics: Intermediate spiral galaxies, Unbarred spiral galaxies, Spiral galaxies, Technology Internet, Spitzer Space Telescope, Sculptor Galaxy, Sculptor constellation, NGC, Atlas of Peculiar Galaxies, Barred spiral galaxies, Galaxy