File:M80, NGC 6093 (noao-m80).tiff
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![File:M80, NGC 6093 (noao-m80).tiff](https://upload.wikimedia.org/wikipedia/commons/thumb/e/ec/M80%2C_NGC_6093_%28noao-m80%29.tiff/lossy-page1-600px-M80%2C_NGC_6093_%28noao-m80%29.tiff.jpg?20230917180137)
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M80, a globular cluster in the constellation Scorpius, is quite distant at over 27000 light-years, and also one of the densest globulars. It contains several hundred thousand stars within a diameter of around seventy light-years.
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[edit]DescriptionM80, NGC 6093 (noao-m80).tiff |
English: M80, a globular cluster in the constellation Scorpius, is quite distant at over 27000 light-years, and also one of the densest globulars. It contains several hundred thousand stars within a diameter of around seventy light-years. This picture was created from observations with the T2KA CCD camera at the Kitt Peak National Observatory's 0.9-meter telescope in March of 1995. |
Date | 30 June 2020, 21:53:00 (upload date) |
Source | M80, NGC 6093 |
Author | NOIRLab/NSF/AURA |
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current | 18:01, 17 September 2023 | ![]() | 1,024 × 1,024 (3.02 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/noao-m80.tif via Commons:Spacemedia |
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Image title | M80, a globular cluster in the constellation Scorpius, is quite distant at over 27000 light-years, and also one of the densest globulars. It contains several hundred thousand stars within a diameter of around seventy light-years. This picture was created from observations with the T2KA CCD camera at the Kitt Peak National Observatory's 0.9-meter telescope in March of 1995. |
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Width | 1,024 px |
Height | 1,024 px |
Bits per component |
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Compression scheme | Uncompressed |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 2 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |
Software used | ImageMagick 5.5.1 10/20/02 Q16 http://www.imagemagick.org |