File:E0102-72 3- Chandra X-ray Image with Scale Bar (2000-0015multi-more-2).tiff
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Chandra X-ray Image with Scale Bar Scale bar = 4.4 arcsec
Summary
editDescriptionE0102-72 3- Chandra X-ray Image with Scale Bar (2000-0015multi-more-2).tiff |
English: Chandra X-ray Image with Scale Bar Scale bar = 4.4 arcsec |
Date | 10 April 2000 (upload date) |
Source | Chandra X-ray Image with Scale Bar |
Author | (Credit: X-ray (NASA/CXC/SAO); Optical (NASA/HST); Radio: (CSIRO/ATNF/ATCA)) |
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This media is a product of the Chandra X-ray Observatory Credit and attribution belongs to the mission team, if not already specified in the "author" row |
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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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current | 21:49, 14 June 2024 | ![]() | 1,793 × 1,797 (1.86 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://chandra.si.edu/photo/2000/0015multi/E0102Comp_scale.tif via Commons:Spacemedia |
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Image title | The Chandra X-ray image (blue) shows gas that has been heated to millions of degrees Celsius by a shock wave moving into matter ejected by the supernova. This gas is rich in oxygen and neon. The radio image (red) made with the Australia Telescope Compact Array, traces the outward motion of a shock wave due to the motion of extremely high-energy electrons. The optical image (green) made with the Hubble Space Telescope, shows dense clumps of oxygen gas that have "cooled" to about 30,000 degree Celsius. |
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Author | Chandra X-ray Observatory Center |
Width | 1,793 px |
Height | 1,797 px |
Bits per component |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 1 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Exif version | 2.21 |
Color space | Uncalibrated |