File:Cassiopeia A -MIRI Image- (weic2311a).jpg
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DescriptionCassiopeia A -MIRI Image- (weic2311a).jpg |
English: Cassiopeia A (Cas A) is a supernova remnant located about 11,000 light-years from Earth in the constellation Cassiopeia. It spans approximately 10 light-years. This new image uses data from Webb’s Mid-Infrared Instrument (MIRI) to reveal Cas A in a new light. On the remnant’s exterior, particularly at the top and left, lie curtains of material appearing orange and red due to emission from warm dust. This marks where ejected material from the exploded star is ramming into surrounding circumstellar material. Interior to this outer shell lie mottled filaments of bright pink studded with clumps and knots. This represents material from the star itself, and likely shines due to a mix of various heavy elements and dust emission. The stellar material can also be seen as fainter wisps near the cavity’s interior. A loop represented in green extends across the right side of the central cavity. Its shape and complexity are unexpected and challenging for scientists to understand. This image combines various filters with the colour red assigned to 25.5 microns (F2550W), orange-red to21 microns (F2100W), orange to 18 microns (F1800W), yellow to 12.8 microns (F1280W), green to 11.3 microns (F1130W), cyan to 10 microns (F1000W), light blue to 7.7 microns (F770W), and blue to 5.6 microns (F560W). The data comes from the general observer program 1947. [Image description: A roughlysquare image is rotated clockwise about 45 degrees. Within the image is a circular-shaped nebula with complex structure. On the circle’s exterior lie curtains of material glowing orange. Interior to this outer shell lies a ring of mottled filaments of bright pink studded with clumps and knots. Atcenter right, a greenish loop extends from the right side of the ring into the central cavity. Translucent wisps of blue, green, and red appear throughout the image.] |
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Source | https://esawebb.org/images/weic2311a/ |
Author | NASA, ESA, CSA, D. Milisavljevic (Purdue University), T. Temim (Princeton University), I. De Looze (UGent), J. DePasquale (STScI) |
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current | 19:48, 18 January 2024 | 1,280 × 1,280 (247 KB) | Laensom (talk | contribs) | Uploaded a work by NASA, ESA, CSA, D. Milisavljevic (Purdue University), T. Temim (Princeton University), I. De Looze (UGent), J. DePasquale (STScI) from https://esawebb.org/images/weic2311a/ with UploadWizard |
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Author | Space Telescope Science Institute Office of Public Outreach |
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Source | ESA/Webb |
Credit/Provider | NASA, ESA, CSA, D. Milisavljevic (Purdue University), T. Temim (Princeton University), I. De Looze (UGent), J. DePasquale (STScI) |
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Date and time of data generation | 16:00, 7 April 2023 |
JPEG file comment | The explosion of a star is a dramatic event, but the remains that the star leaves behind can be even more dramatic. A new mid-infrared image from NASA’s James Webb Space Telescope provides one stunning example. It shows the supernova remnant Cassiopeia A (Cas A), created by a stellar explosion 340 years ago. The image displays vivid colors and intricate structures begging to be examined more closely. Cas A is the youngest known remnant from an exploding, massive star in our galaxy, offering astronomers an opportunity to perform stellar forensics to understand the star’s death. |
Software used | Adobe Photoshop 24.1 (Macintosh) |
File change date and time | 10:54, 29 March 2023 |
Date and time of digitizing | 16:08, 25 March 2023 |
Date metadata was last modified | 07:50, 29 March 2023 |
Unique ID of original document | xmp.did:d8b4e69a-e41c-4002-b6a9-395e8b82898f |
Keywords | Cas A |
Contact information | outreach@stsci.edu
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
IIM version | 4 |