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File:Saturn comp.jpg

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English: Chandra's image of Saturn (left) and Hubble optical image of Saturn (right). Saturn's X-ray spectrum is similar to that of X-rays from the Sun indicating that Saturn's X-radiation is due to the reflection of solar X-rays by Saturn's atmosphere. The optical image is much brighter, and shows the beautiful ring structures, which were not detected in X-rays. Observation period: 20 hrs, April 14-15, 2003. Color code: red (0.4 - 0.6 keV), green (0.6 - 0.8 keV), blue (0.8 - 1.0 keV).
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Source http://chandra.harvard.edu/photo/2004/saturn/saturn_comp.jpg
http://chandra.harvard.edu/photo/2004/saturn/saturn_comp.tif
Author X-ray: NASA/U. Hamburg/J.Ness et al; Optical: NASA/STScI
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Images produced by NASA are usually free of copyright [...]

Saturn at the time of Chandra observation was 1.2 billion km from Earth.

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Public domain 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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8 March 2004

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Date/TimeThumbnailDimensionsUserComment
current06:57, 7 May 2015Thumbnail for version as of 06:57, 7 May 20153,150 × 1,638 (278 KB)Jcpag2012full resolution
19:17, 11 September 2009Thumbnail for version as of 19:17, 11 September 2009756 × 405 (138 KB)Marshallsumter{{Information |Description={{en|1=Chandra's image of Saturn (left) and Hubble optical image of Saturn (right). Saturn's X-ray spectrum is similar to that of X-rays from the Sun indicating that Saturn's X-radiation is due to the reflection of solar X-rays

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