File:Webb Explores a Pair of Merging Galaxies (scaled) (potm2210d).tiff
From Wikimedia Commons, the free media repository
Jump to navigation
Jump to search
![File:Webb Explores a Pair of Merging Galaxies (scaled) (potm2210d).tiff](https://upload.wikimedia.org/wikipedia/commons/thumb/d/d3/Webb_Explores_a_Pair_of_Merging_Galaxies_%28scaled%29_%28potm2210d%29.tiff/lossy-page1-686px-Webb_Explores_a_Pair_of_Merging_Galaxies_%28scaled%29_%28potm2210d%29.tiff.jpg?20221121215047)
Size of this JPG preview of this TIF file: 686 × 600 pixels. Other resolutions: 275 × 240 pixels | 549 × 480 pixels | 879 × 768 pixels | 1,172 × 1,024 pixels | 1,716 × 1,500 pixels.
Original file (1,716 × 1,500 pixels, file size: 14.76 MB, MIME type: image/tiff)
File information
Structured data
Captions
Captions
Add a one-line explanation of what this file represents
Summary
[edit]DescriptionWebb Explores a Pair of Merging Galaxies (scaled) (potm2210d).tiff |
English: This image from the NASA/ESA/CSA James Webb Space Telescope depicts IC 1623, an entwined pair of interacting galaxies which lies around 270 million light-years from Earth in the constellation Cetus. The two galaxies in IC 1623 are plunging headlong into one another in a process known as a galaxy merger. Their collision has ignited a frenzied spate of star formation known as a starburst, creating new stars at a rate more than twenty times that of the Milky Way galaxy.In Webb’s combined MIRI and NIRCam view of the galaxies, the gas being used as fuel by the stellar nurseries is especially apparent. Webb’s ability to pierce the gaseous veil obscuring the bright galactic cores also causes prominent diffraction spikes to appear.[Image description: The two galaxies swirl into a single chaotic object in the centre. Long, blue spiral arms stretch vertically, faint at the edges. Hot gas spreads horizontally over that, mainly bright red with many small gold spots of star formation. The core of the merging galaxies is very bright and radiates eight large, golden diffraction spikes. The background is black, with many tiny galaxies in orange and blue.] |
Date | 25 October 2022 (upload date) |
Source | Webb Explores a Pair of Merging Galaxies (scaled) |
Author | ESA/Webb, NASA & CSA, L. Armus & A. Evans Acknowledgement: R. Colombari |
Other versions |
|
Licensing
[edit]![]() ![]() |
ESA/Webb images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the webbtelescope.org website, use the {{PD-Webb}} tag.
Conditions:
Notes:
|
![]() |
![w:en:Creative Commons](https://upload.wikimedia.org/wikipedia/commons/thumb/7/79/CC_some_rights_reserved.svg/90px-CC_some_rights_reserved.svg.png)
![attribution](https://upload.wikimedia.org/wikipedia/commons/thumb/1/11/Cc-by_new_white.svg/24px-Cc-by_new_white.svg.png)
This file is licensed under the Creative Commons Attribution 4.0 International license.
Attribution: ESA/Webb, NASA & CSA, L. Armus & A. Evans Acknowledgement: R. Colombari
- You are free:
- to share – to copy, distribute and transmit the work
- to remix – to adapt the work
- Under the following conditions:
- attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 21:50, 21 November 2022 | ![]() | 1,716 × 1,500 (14.76 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://esawebb.org/media/archives/images/original/potm2210d.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.
Width | 1,716 px |
---|---|
Height | 1,500 px |
Bits per component |
|
Compression scheme | Uncompressed |
Pixel composition | RGB |
Image data location | 24,972 |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 1,500 |
Bytes per compressed strip | 15,444,000 |
Horizontal resolution | 25.4 dpi |
Vertical resolution | 25.4 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop 23.5 (Windows) |
File change date and time | 14:56, 17 October 2022 |
Color space | Uncalibrated |