File:M76 (Little Dumbbell) (noao-m76block).tiff
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Size of this JPG preview of this TIF file: 800 × 539 pixels. Other resolutions: 320 × 216 pixels | 640 × 431 pixels | 1,024 × 690 pixels | 1,280 × 863 pixels | 2,184 × 1,472 pixels.
Original file (2,184 × 1,472 pixels, file size: 2.94 MB, MIME type: image/tiff)
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[edit]DescriptionM76 (Little Dumbbell) (noao-m76block).tiff |
English: M76 is a wonderful nebula to observe visually through the 20" telescope on a dark night. It displays two distinct features - the bright inner rectangle and very dim outer loops. Like most nebulae of this type, these loops of material (the rectangular part is a torus viewed edgewise) are cast off by the death of star of average mass. Stars more massive would actually explode. This process is much more non-violent and results in the convoluted bubbles shown here. The distance to M76 is uncertain, but most sources place it between 3000-5000 lightyears away. This would make the bubble of gas about a lightyear across. The full resolution image (click on image) best shows the very heart of the nebula where the central star resides. The image shows a double star - the top of which is distinctly blue. It is this hot star that is responsible for making the Little Dumbbell glow!This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014. |
Date | 18 June 2014, 14:04:00 (upload date) |
Source | M76 (Little Dumbbell) |
Author | KPNO/NOIRLab/NSF/AURA/Adam Block |
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[edit]This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public NOIRLab website, along with the texts of press releases, announcements, images of the week and captions; are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible." To the uploader: You must provide a link (URL) to the original file and the authorship information if available. | |
This file is licensed under the Creative Commons Attribution 4.0 International license.
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 17:13, 23 October 2023 | 2,184 × 1,472 (2.94 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/noao-m76block.tif via Commons:Spacemedia |
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Image title | M76 is a wonderful nebula to observe visually through the 20" telescope on a dark night. It displays two distinct features - the bright inner rectangle and very dim outer loops. Like most nebulae of this type, these loops of material (the rectangular part is a torus viewed edgewise) are cast off by the death of star of average mass. Stars more massive would actually explode. This process is much more non-violent and results in the convoluted bubbles shown here. The distance to M76 is uncertain, but most sources place it between 3000-5000 lightyears away. This would make the bubble of gas about a lightyear across. The full resolution image (click on image) best shows the very heart of the nebula where the central star resides. The image shows a double star - the top of which is distinctly blue. It is this hot star that is responsible for making the Little Dumbbell glow! This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014. |
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Width | 2,184 px |
Height | 1,472 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 | 40 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop 22.4 (Windows) |
File change date and time | 16:27, 30 August 2021 |
Exif version | 2.31 |
Color space | sRGB |