File:Herbig-Haro 49 50.jpg
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Original file (2,700 × 3,150 pixels, file size: 1.71 MB, MIME type: image/jpeg)
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Summary
DescriptionHerbig-Haro 49 50.jpg |
English: This "tornado," designated Herbig-Haro 49/50, is shaped by a cosmic jet packing a powerful punch as it plows through clouds of interstellar gas and dust.
The tornado-like feature is actually a shock front created by a jet of material flowing downward through the field of view. A still-forming star located off the upper edge of the image generates this outflow. The jet slams into neighboring dust clouds at a speed of more than 100 miles per second, heating the dust to incandescence and causing it to glow with infrared light detectable by Spitzer. The triangular shape results from the wake created by the jet's motion, similar to the wake behind a speeding boat. The scientists could only speculate about the source of the spiral appearance. Magnetic fields throughout the region might have shaped the object. Alternatively, the shock might have developed instabilities as it plowed into surrounding material, creating eddies that give the "tornado" its distinctive appearance. Astronomers believe that the blue color at the tornado's tip results from high molecular excitation at the head of the shock. Those high excitation levels generate more short-wavelength emission, shown as blue in this color-coded image. Molecular excitation levels decrease away from the head of the bow shock; therefore the emission is at longer wavelengths, colored red here. The star at the tip of the tornado, which appears to be surrounded by a faint halo, might be a chance superposition along our line of sight. However, the star instead might be physically associated with the tornado. In that case, the halo likely is due to the outflow running into circumstellar material. HH 49/50 is located in the Chamaeleon I star-forming complex, a region containing more than 100 young stars. Most of the new stars are smaller than the sun, although some are more massive. Visible-light observations have found a number of outflows in the region, however most of those outflows have no infrared counterpart. |
Date | |
Source | http://www.spitzer.caltech.edu/images/2311-sig06-002-Cosmic-Tornado |
Author | NASA/JPL-Caltech/J. Bally (University of Colorado) |
Image use policy: http://www.spitzer.caltech.edu/info/18-Image-Use-Policy
Licensing
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ![]() |
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12 January 2006
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 17:06, 20 June 2011 | ![]() | 2,700 × 3,150 (1.71 MB) | Spitzersteph |
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Image title | This "tornado," designated Herbig-Haro 49/50, is shaped by a cosmic jet packing a powerful punch as it plows through clouds of interstellar gas and dust.
The tornado-like feature is actually a shock front created by a jet of material flowing downward through the field of view. A still-forming star located off the upper edge of the image generates this outflow. The jet slams into neighboring dust clouds at a speed of more than 100 miles per second, heating the dust to incandescence and causing it to glow with infrared light detectable by Spitzer. The triangular shape results from the wake created by the jet's motion, similar to the wake behind a speeding boat. The scientists could only speculate about the source of the spiral appearance. Magnetic fields throughout the region might have shaped the object. Alternatively, the shock might have developed instabilities as it plowed into surrounding material, creating eddies that give the "tornado" its distinctive appearance. Astronomers believe that the blue color at the tornado's tip results from high molecular excitation at the head of the shock. Those high excitation levels generate more short-wavelength emission, shown as blue in this color-coded image. Molecular excitation levels decrease away from the head of the bow shock; therefore the emission is at longer wavelengths, colored red here. The star at the tip of the tornado, which appears to be surrounded by a faint halo, might be a chance superposition along our line of sight. However, the star instead might be physically associated with the tornado. In that case, the halo likely is due to the outflow running into circumstellar material. HH 49/50 is located in the Chamaeleon I star-forming complex, a region containing more than 100 young stars. Most of the new stars are smaller than the sun, although some are more massive. Visible-light observations have found a number of outflows in the region, however most of those outflows have no infrared counterpart. |
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Author | Spitzer Space Telescope |
Copyright holder | http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml |
Width | 2,700 px |
Height | 3,150 px |
Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CS3 Macintosh |
File change date and time | 14:33, 5 June 2009 |
Color space | Uncalibrated |