Astrophoto Lab
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NGC
3603
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Name:
NGC 3603 Description: Star formation nebula, star cluster Position (J2000): R.A. 11h 15m 9s.10 Dec. -61° 16' 17".00 Constellation: Carina Distance: 20,000 light-years Image Credit: NASA/JPL-Caltech/WISE Team Release Date: Feb. 17, 2010 Other images: S9920 S9946 S0734 S1004 S1005 S1022 |
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ABOUT THIS IMAGE: This dramatic image of a nebula containing young, massive stars was captured by NASA's Wide-Field Infrared Survey Explorer, or WISE, a space telescope mapping the whole sky in infrared light. The nebula, located 20,000 light-years away in the Carina spiral arm of our Milky Way Galaxy, contains a central cluster of huge, hot stars, called NGC3603. WISE, which is surveying the whole sky in infrared light, is particularly sensitive to the warm dust that permeates star-forming clouds like this one. In this way, WISE complements visible-light observations. The image was captured using all four of WISE's infrared channels, with longer infrared wavelengths shown in red and green and shorter wavelengths in blue (infrared light of 3.4 and 4.6 microns are blue; 12-micron light is green; and 22-micron light is red). The cluster contains some of the most massive stars known. Winds and radiation from the stars are evaporating and dispersing the cloud material from which they formed, warming the cold dust and gas surrounding the central nebula. This greenish "halo" of warm cloud material is seen best by WISE due to its large field of view and improved sensitivity over past all-sky infrared surveys. These WISE observations provide circumstantial evidence that the massive stars in the center of the cluster triggered the formation of younger stars in the halo, which can be seen as red dots. The dust at the center of the cluster is very hot, producing copious amounts of infrared light, which results in the bright, yellow cores of the nebulosity. Ultimately, this turbulent region will be blasted apart by supernova explosions. Other star-forming clouds in the Milky Way have experienced such eruptions, as evidenced by their pockmarked clouds of expanding cavities and bubbles. Massive
star clusters like this one are an important link to understanding the
details of the violent original epoch of massive star formation in the
early, distant universe. Astronomers also use them to study distant starbursts
that occur when galaxies collide, lighting up tremendous firestorms of
brilliant, but ephemeral, stars in the wreckage. Because NGC 3603 is so
close, it is an excellent lab for the study of such faraway and momentous
events. |
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