File:The Hydra I cluster (potw2437b).tiff
Original file (16,201 × 13,301 pixels, file size: 278.37 MB, MIME type: image/tiff)
Captions
Summary
editWarning | The original file is very high-resolution. It might not load properly or could cause your browser to freeze when opened at full size. | Open in ZoomViewer |
---|
DescriptionThe Hydra I cluster (potw2437b).tiff |
English: This image shows a portion of the Hydra I galaxy cluster. Underneath the bright star taking the spotlight in the centre-left of the image, notice the spiral galaxy that looks almost smudged across the screen, spilling its contents into the cosmos around it. This is NGC 3312, a galaxy that is losing gas through a process known as ram pressure stripping. Check the links below for a closer look and an explanation of how this works. |
||
Date | 9 September 2024 (upload date) | ||
Source |
|
||
Author | ESO/INAF/M. Spavone, E. Iodice | ||
Other versions |
|
Licensing
editThis media was created by the European Southern Observatory (ESO).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts 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.
|
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 07:18, 10 September 2024 | 16,201 × 13,301 (278.37 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://cdn.eso.org/images/original/potw2437b.tif via Commons:Spacemedia |
You cannot overwrite this file.
File usage on Commons
The following page uses this file:
Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Image title | This image shows a portion of the Hydra I galaxy cluster. Underneath the bright star taking the spotlight in the centre-left of the image, notice the spiral galaxy that looks almost smudged across the screen, spilling its contents into the cosmos around it. This is NGC 3312, a galaxy that is losing gas through a process known as ram pressure stripping. Check the links below for a closer look and an explanation of how this works. Links Closer look on NGC 3312. Explore this image in more detail in this video. Press release by the Italian National Institute for Astrophysics. |
---|---|
Width | 16,201 px |
Height | 13,301 px |
Bits per component |
|
Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 5 |
Horizontal resolution | 10 dpc |
Vertical resolution | 10 dpc |
Data arrangement | chunky format |
Software used | Adobe Photoshop 25.9 (Windows) |
File change date and time | 16:07, 11 July 2024 |
Color space | sRGB |