File:Deepest, widest view of the Large Magellanic Cloud from SMASH.jpg
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Summary
[edit]DescriptionDeepest, widest view of the Large Magellanic Cloud from SMASH.jpg |
English: Part of the SMASH dataset showing an unprecedented wide-angle view of the Large Magellanic Cloud. The Large and Small Magellanic Clouds are the largest satellite galaxies of the Milky Way and, unlike the rest of the satellite galaxies, are still actively forming stars— and at a rapid pace. The depth of these survey data can be appreciated by the number of stars visible in the outer regions of the galaxy, as seen in the lower part of the image. |
Date | |
Source | https://noirlab.edu/public/images/noirlab2030a/ |
Author |
CTIO/NOIRLab/NSF/AURA/SMASH/D. Nidever (Montana State University) Acknowledgment: Image processing: Travis Rector (University of Alaska Anchorage), Mahdi Zamani & Davide de Martin |
Licensing
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current | 08:34, 13 July 2023 | 6,737 × 6,536 (35.95 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/large/noirlab2030a.jpg via Commons:Spacemedia | |
13:36, 19 December 2020 | 6,737 × 6,536 (35.95 MB) | Jmencisom (talk | contribs) | Uploaded a work by CTIO/NOIRLab/NSF/AURA/SMASH/D. Nidever (Montana State University) Acknowledgment: Image processing: Travis Rector (University of Alaska Anchorage), Mahdi Zamani & Davide de Martin from https://noirlab.edu/public/images/noirlab2030a/ with UploadWizard |
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Metadata
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Credit/Provider | CTIO/NOIRLab/NSF/AURA/SMASH/D. Nidever (Montana State University) Acknowledgment: Image processing: Travis Rector (University of Alaska Anchorage), Mahdi Zamani & Davide de Martin |
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Source | NSF's NOIRLab |
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Usage terms |
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Date and time of data generation | 08:00, 1 December 2020 |
JPEG file comment | Part of the SMASH dataset showing an unprecedented wide-angle view of the Large Magellanic Cloud. The Large and Small Magellanic Clouds are the largest satellite galaxies of the Milky Way and, unlike the rest of the satellite galaxies, are still actively forming stars — and at a rapid pace. The depth of these survey data can be appreciated by the number of stars visible in the outer regions of the galaxy, as seen in the lower part of the image. |
Software used | Adobe Photoshop 21.1 (Windows) |
Date and time of digitizing | 15:46, 31 August 2020 |
Date metadata was last modified | 18:39, 21 September 2020 |
File change date and time | 18:39, 21 September 2020 |
Unique ID of original document | xmp.did:1fdb4fef-6842-a640-a40c-54b59c948034 |
Keywords | Large Magellanic Cloud |
Contact information |
950 North Cherry Ave. Tucson, AZ, 85719 USA |