Supernova 1604, SN 1604, Kepler's Supernova Remnant - stock photo
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Supernova 1604, SN 1604, Kepler's Supernova Remnant

This composite image represent views of Kepler's supernova remnant taken in X-rays, visible light, and infrared radiation. This Spitzer false-color image is a composite of data from the 24 micron channel of Spitzer's multiband imaging photometer (red), and three channels of its infrared array camera: 8 micron (yellow), 5.6 micron (blue), and 4.8 micron (green). Stars are most prominent in the two shorter wavelengths, causing them to show up as turquoise. The supernova remnant is most prominent at 24 microns, arising from dust that has been heated by the supernova shock wave, and re-radiated in the infrared. The 8 micron data shows infrared emission from regions closely associated with the optically emitting regions. These are the densest regions being encountered by the shock wave, and probably arose from condensations in the surrounding material that was lost by the supernova star before it exploded. Spitzer Space Telescope Mission.

Credit
Science Source / NASA/JPL-Caltech

Dimensions
3240 x 3240 pixels

Print Size @ 300 dpi
11 x 11 inches / 27 x 27 cm

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