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| NASA/JPL-Caltech/ J. Hora (Harvard-Smithsonian CfA) |
The Infrared Helix (Expanded View)
The Helix Nebula, which is composed of gaseous shells and disks puffed out by a dying sunlike star, exhibits complex structure on the smallest visible scales. In this new image from NASA's Spitzer Space Telescope, infrared light at wavelengths of 3.2, 4.5, and 8.0 microns has been colored blue, green, and red (respectively). The "cometary knots" show blue-green heads due to excitation of their molecular material from shocks or ultraviolet radiation. The tails of the cometary knots appear redder due to being shielded from the central star's ultraviolet radiation and wind by the heads of the knots.
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| About the Object (1) | | Object name: | Helix Nebula, NGC 7293, NGC7293 | | Object type: | Planetary Nebula | | Position (J2000): | RA: 22h 29m 38.55s Dec: -20° 49' 26.00" | | Distance: | 650 light-years (200 parsecs) | | Constellation: | Aquarius |
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About the Data
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Spitzer Data
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| Image Credit: | NASA/JPL-Caltech/ J. Hora (Harvard-Smithsonian CfA) | | Instrument: | IRAC | | Wavelength: | 3.6 microns (blue), 4.5 microns (green), 8.0 microns (red) | | Exposure Date: | October 30, 2004 | | Exposure Time: | 160 s per position | | Image scale: | 29 x 27 arcmin | | Orientation: | North is 65 deg CW from up | | Release Date: | 2007/08/24 |
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Observers
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J. L. Hora (CfA)
W. B. Latter (NASA/ Herschel Science Center)
M. Marengo (CfA)
G.G. Fazio (CfA)
H.A. Smith (CfA) |
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