File:NGC 3319 (noao-n3319block).tiff
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![File:NGC 3319 (noao-n3319block).tiff](https://upload.wikimedia.org/wikipedia/commons/thumb/4/4a/NGC_3319_%28noao-n3319block%29.tiff/lossy-page1-800px-NGC_3319_%28noao-n3319block%29.tiff.jpg?20231023174557)
Size of this JPG preview of this TIF file: 800 × 540 pixels. Other resolutions: 320 × 216 pixels | 640 × 432 pixels | 1,024 × 691 pixels | 1,441 × 972 pixels.
Original file (1,441 × 972 pixels, file size: 1.62 MB, MIME type: image/tiff)
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At a distance of 32 million light years, NGC 3319 is a relatively nearby galaxy. Much of the activity in this galaxy is resigned to the central bar- the rest of the galaxy is seemingly quiet (and *very* dim).
Summary
[edit]DescriptionNGC 3319 (noao-n3319block).tiff |
English: At a distance of 32 million light years, NGC 3319 is a relatively nearby galaxy. Much of the activity in this galaxy is resigned to the central bar- the rest of the galaxy is seemingly quiet (and *very* dim). A few star forming regions punctuate the ends of the bar and the bends in the spiral arms. Astronomers have wondered why this particular barred-spiral seems to lack much gas (and thereby much star formation). The distribution of hydrogen gas in this galaxy is also significantly asymmetric. The reason for this is unknown as normally interaction with another galaxy would cause this effect; but there are no perturbers in the vicinity.This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014. |
Date | 27 March 2014, 14:06:00 (upload date) |
Source | NGC 3319 |
Author | KPNO/NOIRLab/NSF/AURA/Adam Block |
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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. |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 17:45, 23 October 2023 | ![]() | 1,441 × 972 (1.62 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/noao-n3319block.tif via Commons:Spacemedia |
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Image title | At a distance of 32 million light years, NGC 3319 is a relatively nearby galaxy. Much of the activity in this galaxy is resigned to the central bar- the rest of the galaxy is seemingly quiet (and *very* dim). A few star forming regions punctuate the ends of the bar and the bends in the spiral arms. Astronomers have wondered why this particular barred-spiral seems to lack much gas (and thereby much star formation). The distribution of hydrogen gas in this galaxy is also significantly asymmetric. The reason for this is unknown as normally interaction with another galaxy would cause this effect; but there are no perturbers in the vicinity. This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014. |
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Camera manufacturer | ST-10 w/ AO7 |
Width | 1,441 px |
Height | 972 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 | 60 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop 21.0 (Windows) |
File change date and time | 16:07, 15 September 2021 |
Exif version | 2.31 |
Color space | sRGB |