File:Cassiopeia A (1999-0237 - 0237 radio).tiff
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![File:Cassiopeia A (1999-0237 - 0237 radio).tiff](https://upload.wikimedia.org/wikipedia/commons/thumb/9/9b/Cassiopeia_A_%281999-0237_-_0237_radio%29.tiff/lossy-page1-600px-Cassiopeia_A_%281999-0237_-_0237_radio%29.tiff.jpg?20240527231136)
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Original file (1,800 × 1,800 pixels, file size: 1.98 MB, MIME type: image/tiff)
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Captions
Cas A is the remnant of a star that exploded about 300 years ago.
Summary
[edit]DescriptionCassiopeia A (1999-0237 - 0237 radio).tiff |
English: Cas A is the remnant of a star that exploded about 300 years ago. The radio image shows an expanding shell of hot gas produced by the explosion. This gaseous shell is about 10 light years in diameter, and has a temperature of about 50 million degrees. |
Date | 26 August 1999 (upload date) |
Source | Cassiopeia A: First Light |
Author | NRAO/AUI/NSF |
Other versions |
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Licensing
[edit]Public domainPublic domainfalsefalse |
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This image is a work of a National Science Foundation employee, taken or made as part of that person's official duties. As a work of the U.S. federal government, the image is in the public domain. | ![]() |
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current | 23:11, 27 May 2024 | ![]() | 1,800 × 1,800 (1.98 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://chandra.si.edu/photo/1999/0237/0237_radio.tif via Commons:Spacemedia |
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This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Image title | This X-ray image of the Cassiopeia A (Cas A) supernova remnant is the official first light image of the Chandra X-ray Observatory. The 5,000 second image was made with the Advanced CCD Imaging Spectrometer (ACIS). Two shock waves are visible: a fast outer shock and a slower inner shock. The inner shock wave is believed to be due to the collision of the ejecta from the supernova explosion with a circumstellar shell of material, heating it to a temperature of ten million degrees Celsius. The outer shock wave is analogous to an awesome sonic boom resulting from this collision. The bright object near the center may be the long sought neutron star or black hole that remained after the explosion that produced Cas A. |
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Author | Chandra X-ray Observatory Center |
Width | 1,800 px |
Height | 1,800 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 | sRGB |