File:M94, NGC 4736 (noao-m94).tiff
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DescriptionM94, NGC 4736 (noao-m94).tiff |
English: The Sab spiral galaxy M94 in the constellation Canes Venatici is considered by some (but not others) to be in a group including M64 and various fainter galaxies. It has an extremely bright innner region surrounded by a blue ring of young star clusters, then a fainter yellowish region of older stars also surrounded by traces of young stars, and even further out a very much fainter outer ring. All of these features are visible in this picture, due to the use of a drastically compressed intensity mapping. This stretch also reveals quite a few small faint background galaxies. This picture was taken in May 1998 at the KPNO 0.9-meter telescope. Image size 17.0 arc minutes. |
Date | 16 December 2002, 11:48:00 (upload date) |
Source | M94, NGC 4736 |
Author | Hillary Mathis, N.A.Sharp/NOIRLab/NSF/AURA/ |
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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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current | 21:31, 27 October 2023 | 3,000 × 3,000 (25.76 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/noao-m94.tif via Commons:Spacemedia |
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Image title | The Sab spiral galaxy M94 in the constellation Canes Venatici is considered by some (but not others) to be in a group including M64 and various fainter galaxies. It has an extremely bright innner region surrounded by a blue ring of young star clusters, then a fainter yellowish region of older stars also surrounded by traces of young stars, and even further out a very much fainter outer ring. All of these features are visible in this picture, due to the use of a drastically compressed intensity mapping. This stretch also reveals quite a few small faint background galaxies. This picture was taken in May 1998 at the KPNO 0.9-meter telescope. Image size 17.0 arc minutes. |
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Width | 3,000 px |
Height | 3,000 px |
Bits per component |
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Compression scheme | Uncompressed |
Pixel composition | RGB |
Image data location | 2,608 |
Number of components | 3 |
Number of rows per strip | 3,000 |
Bytes per compressed strip | 27,000,000 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |