File:The Mice (noao-n4676).tiff
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![File:The Mice (noao-n4676).tiff](https://upload.wikimedia.org/wikipedia/commons/thumb/0/03/The_Mice_%28noao-n4676%29.tiff/lossy-page1-800px-The_Mice_%28noao-n4676%29.tiff.jpg?20230917193546)
Size of this JPG preview of this TIF file: 800 × 534 pixels. Other resolutions: 320 × 213 pixels | 640 × 427 pixels | 1,024 × 683 pixels | 1,280 × 854 pixels | 2,048 × 1,366 pixels.
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An interacting galaxy system, NGC4676 is nicknamed the Mice because of the long tails of stars drawn out by the mutual gravitational effect of each galaxy on the other.
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[edit]DescriptionThe Mice (noao-n4676).tiff |
English: An interacting galaxy system, NGC4676 is nicknamed the Mice because of the long tails of stars drawn out by the mutual gravitational effect of each galaxy on the other. Perhaps the best match to the system's observed morphology comes from a numerical simulation of two identical disk galaxies interacting over a period of more than 300 million years. NGC4676 is also number 242 in the Arp atlas of peculiar galaxies and number 224 in Vorontsov-Vel'yaminov's catalog of interacting galaxies. NGC4676 is some 200 million light-years away in the direction of the constellation Coma Berenices. For convenience, this image is shown in a non-standard orientation, with north to the left and east down. This picture was obtained during the year 2000 Research Experiences for Undergraduates program, funded by the National Science Foundation, using the Kitt Peak National Observatory's 2.1-meter telescope. |
Date | 30 June 2020, 21:33:00 (upload date) |
Source | The Mice |
Author | REU program/NOIRLab/NSF/AURA |
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current | 19:35, 17 September 2023 | ![]() | 2,048 × 1,366 (8.02 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/noao-n4676.tif via Commons:Spacemedia |
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Image title | An interacting galaxy system, NGC4676 is nicknamed the Mice because of the long tails of stars drawn out by the mutual gravitational effect of each galaxy on the other. Perhaps the best match to the system's observed morphology comes from a numerical simulation of two identical disk galaxies interacting over a period of more than 300 million years. NGC4676 is also number 242 in the Arp atlas of peculiar galaxies and number 224 in Vorontsov-Vel'yaminov's catalog of interacting galaxies. NGC4676 is some 200 million light-years away in the direction of the constellation Coma Berenices. For convenience, this image is shown in a non-standard orientation, with north to the left and east down. This picture was obtained during the year 2000 Research Experiences for Undergraduates program, funded by the National Science Foundation, using the Kitt Peak National Observatory's 2.1-meter telescope. |
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Width | 2,048 px |
Height | 1,366 px |
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Compression scheme | Uncompressed |
Pixel composition | RGB |
Image data location | 2,046 |
Number of components | 3 |
Number of rows per strip | 1,366 |
Bytes per compressed strip | 8,392,704 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |
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1,366 pixel
2,048 pixel
8,404,904 byte
ea07094c62955f0f8b97f43a1c1eade600d2278e
30 June 2020
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